On the History of Unified Field Theories
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Abstract
This article is intended to give a review of the history of the classical aspects of unified field theories in the 20th century. It includes brief technical descriptions of the theories suggested, short biographical notes concerning the scientists involved, and an extensive bibliography. The present first installment covers the time span between 1914 and 1933, i.e., when Einstein was living and working in Berlin — with occasional digressions into other periods. Thus, the main theme is the unification of the electromagnetic and gravitational fields augmented by shortlived attempts to include the matter field described by Schrödinger’s or Dirac’s equations. While my focus lies on the conceptual development of the field, by also paying attention to the interaction of various schools of mathematicians with the research done by physicists, some prosopocraphical remarks are included.
1 Introduction
1.1 Preface
This historical review of classical unified field theories consists of two parts. In the first, the development of unified field theory between 1914 and 1933, i.e., during the years Einstein^{1} lived and worked in Berlin, will be covered. In the second, the very active period after 1933 until the 1960s to 1970s will be reviewed. In the first version of Part I presented here, in view of the immense amount of material, neither all shades of unified field theory nor all the contributions from the various scientific schools will be discussed with the same intensity; I apologise for the shortcoming and promise to improve on it with the next version. At least, even if I do not discuss them all in detail, as many references as are necessary for a first acquaintance with the field are listed here; completeness may be reached only (if at all) by later updates. Although I also tried to take into account the published correspondence between the main figures, my presentation, again, is far from exhaustive in this context. Eventually, unpublished correspondence will have to be worked in, and this may change some of the conclusions. Purposely I included mathematicians and also theoretical physicists of lesser rank than those who are known to be responsible for big advances. My aim is to describe the field in its full variety as it presented itself to the reader at the time.
The review is written such that physicists should be able to follow the technical aspects of the papers (cf. Section 2), while historians of science without prior knowledge of the mathematics of general relativity at least might gain an insight into the development of concepts, methods, and scientific communities involved. I should hope that readers find more than one opportunity for further indepth studies concerning the many questions left open.
I profited from earlier reviews of the field, or of parts of it, by Pauli^{2} ([246], Section V); Ludwig [212]; Whittaker ([414], pp. 188–196); Lichnerowicz [209]; Tonnelat ([356], pp. 1–14); Jordan ([176], Section III); Schmutzer ([290], Section X); Treder ([183], pp. 30–43); Bergmann ([12], pp. 62–73); Straumann [334, 335]; Vizgin [384, 385]^{3} ; Bergia [11]; Goldstein and Ritter [146]; Straumann and O’Raifeartaigh [240]; Scholz [292], and Stachel [330]. The section on Einstein’s unified field theories in Pais’ otherwise superb book presents the matter neither with the needed historical correctness nor with enough technical precision [241]. A recent contribution of van Dongen, focussing on Einstein’s methodology, was also helpful [371]. As will be seen, with regard to interpretations and conclusions, my views are different in some instances. In Einstein biographies, the subject of “unified field theories” — although keeping Einstein busy for the second half of his life — has been dealt with only in passing, e.g., in the book of Jordan [177], and in an unsatisfying way in excellent books by Fölsing [136] and by Hermann [159]. This situation is understandable; for to describe a genius stubbornly clinging to a set of ideas, sterile for physics in comparison with quantum mechanics, over a period of more than 30 years, is not very rewarding. For the short biographical notes, various editions of J. C. Poggendorff’s BiographischLiterarischem Handwörterbuch and internet sources have been used (in particular [1]).
If not indicated otherwise, all nonEnglish quotations have been translated by the author; the original text of quotations is given in footnotes.
1.2 Introduction to part I
Past experience has shown that formerly unrelated parts of physics could be fused into one single conceptual formalism by a new theoretical perspective: electricity and magnetism, optics and electromagnetism, thermodynamics and statistical mechanics, inertial and gravitational forces. In the second half of the 20th century, the electromagnetic and weak nuclear forces have been bound together as an electroweak force; a powerful scheme was devised to also include the strong interaction (chromodynamics), and led to the standard model of elementary particle physics. Unification with the fourth fundamental interaction, gravitation, is in the focus of much present research in classical general relativity, supergravity, superstring, and supermembrane theory but has not yet met with success. These types of “unifications” have increased the explanatory power of present day physical theories and must be considered as highlights of physical research.
In the historical development of the idea of unification, i.e., the joining of previously separated areas of physical investigation within one conceptual and formal framework, two closely linked yet conceptually somewhat different approaches may be recognised. In the first, the focus is on unification of representations of physical fields. An example is given by special relativity which, as a framework, must surround all phenomena dealing with velocities close to the velocity of light in vacuum. The theory thus is said to provide “a synthesis of the laws of mechanics and of electromagnetism” ([16], p. 132). Einstein’s attempts at the inclusion of the quantum area into his classical field theories belongs to this path. Nowadays, quantum field theory is such a unifying representation^{4} In the second approach, predominantly the unification of the dynamics of physical fields is aimed at, i.e., a unification of the fundamental interactions. Maxwell’s theory might be taken as an example, unifying the electrical and the magnetic field once believed to be dynamically different. Most of the unified theories described in this review belong here: Gravitational and electromagnetic fields are to be joined into a new field. Obviously, this second line of thought cannot do without the first: A new representation of fields is always necessary.
In an unsuccessful hunt for progress with the deductivehypothetical method alone, Einstein spent decades of his life on the unification of the gravitational with the electromagnetic and, possibly, other fields. Others joined him in such an endeavour, or even preceded him, including Mie, Hilbert, Ishiwara, Nordström, and others^{5}. At the time, another road was impossible because of the lack of empirical basis due to the weakness of the gravitational interaction. A similar situation obtains even today within the attempts for reaching a common representation of all four fundamental interactions. Nevertheless, in terms of mathematical and physical concepts, a lot has been learned even from failed attempts at unification, vid. the gauge idea, or dimensional reduction (KaluzaKlein), and much still might be learned in the future.“The successful development of science requires a proper balance between the method of building up from observations and the method of deducing by pure reasoning from speculative assumptions, […].” ([233], p. 1001)
In the following I shall sketch, more or less chronologically, and by trailing Einstein’s path, the history of attempts at unifying what are now called the fundamental interactions during the period from about 1914 to 1933. Until the end of the thirties, the only accepted fundamental interactions were the electromagnetic and the gravitational, plus, tentatively, something like the “mesonic” or “nuclear” interaction. The physical fields considered in the framework of “unified field theory” including, after the advent of quantum (wave) mechanics, the wave function satisfying either Schrödinger’s or Dirac’s equation, were all assumed to be classical fields. The quantum mechanical wave function was taken to represent the field of the electron, i.e., a matter field. In spite of this, the construction of quantum field theory had begun already around 1927 [52, 174, 178, 175, 179]. For the early history and the conceptual development of quantum field theory, cf. Section 1 of Schweber [322], or Section 7.2 of Cao [28]; for Dirac’s contributions, cf. [190]. Nowadays, it seems mandatory to approach unification in the framework of quantum field theory.
General relativity’s doing away with forces in exchange for a richer (and more complicated) geometry of space and time than the Euclidean remained the guiding principle throughout most of the attempts at unification discussed here. In view of this geometrization, Einstein considered the role of the stressenergy tensor T^{ ik } (the sourceterm of his field equations G^{ ik }=κT^{ ik }) a weak spot of the theory because it is a field devoid of any geometrical significance.

An inclusion of matter in the sense of a desired replacement, in Einstein’s equations and their generalisation, of the energymomentum tensor of matter by intrinsic geometrical structures, and, likewise, the removal of the electric current density vector as a nongeometrical source term in Maxwell’s equations.

The development of a unified field theory more geometrico for electromagnetism and gravitation, and in addition, later, of the “field of the electron” as a classical field of “de Brogliewaves” without explicitly taking into account further matter sources^{6}.
For the theories discussed, the representation of matter oscillated between the pointparticle concept in which particles are considered as singularities of a field, to particles as everywhere regular field configurations of a solitonic character. In a theory for continuous fields as in general relativity, the concept of pointparticle is somewhat amiss. Nevertheless, geodesics of the Riemannian geometry underlying Einstein’s theory of gravitation are identified with the worldlines of freely moving pointparticles. The field at the location of a pointparticle becomes unbounded, or “singular”, such that the derivation of equations of motion from the field equations is a nontrivial affair. The competing paradigm of a particle as a particular field configuration of the electromagnetic and gravitational fields later has been pursued by J. A. Wheeler under the names “geon” and “geometrodynamics” in both the classical and the quantum realm [412]. In our time, gravitational solitonic solutions also have been found [235, 26].
However, in connection with one of his moves, i.e., the 5vector version of Kaluza^{8}’s theory (cf. Sections 4.2, 6.3), which for him provided “a logical unity of the gravitational and the electromagnetic fields”, he regretfully acknowledged:“is in no way taking notice of the results of quantum calculation because he believes that by dealing with microscopic phenomena these will come out by themselves. Otherwise he would not support the theory.” ([91], p. 610)
“But one hope did not get fulfilled. I thought that upon succeeding to find this law, it would form a useful theory of quanta and of matter. But, this is not the case. It seems that the problem of matter and quanta makes the construction fall apart.”^{9} ([96], p. 442)
“[…] collections of positive and negative electricity which we are finding in the positive nuclei of hydrogen and in the negative electrons. The older Maxwell theory does not explain these collections, but also by the newer endeavours it has not been possible to recognise these collections as immediate consequences of the fundamental differential equations studied. However, if such an explanation should be found, we may perhaps also hope that new light is shed on the […] mysterious quantum orbits.”^{11} ([301], p. 39)
In this context, through all the years, Einstein vainly tried to derive, from the field equations of his successive unified field theories, the existence of elementary particles with opposite though otherwise equal electric charge but unequal mass. In correspondence with the state of empirical knowledge at the time (i.e., before the positron was found in 1932/33), but despite theoretical hints pointing into a different direction to be found in Dirac’s papers, he always paired electron and proton ^{12}.
Of course, by quantum field theory the dichotomy between matter and fields in the sense of a dualism is minimised as every field carries its particlelike quanta. Today’s unified field theories appear in the form of gauge theories; matter is represented by operator valued spinhalf quantum fields (fermions) while the “forces” mediated by “exchange particles” are embodied in gauge fields, i.e., quantum fields of integer spin (bosons). The spacetime geometry used is rigidly fixed, and usually taken to be Minkowski space or, within string and membrane theory, some higherdimensional manifold also loosely called “spacetime”, although its signature might not be Lorentzian and its dimension might be 10, 11, 26, or some other number larger than four. A satisfactory inclusion of gravitation into the scheme of quantum field theory still remains to be achieved.
On the other hand, those working in quantum theory may have frowned upon the wealth of objects within unified field theories uncorrelated to a convincing physical interpretation and thus, in principle, unrelated to observation. In fact, until the 1930s, attempts still were made to “geometrize” wave mechanics while, roughly at the same time, quantisation of the gravitational field had also been tried [284]. Einstein belonged to those who regarded the idea of unification as more fundamental than the idea of field quantisation [95]. His thinking is reflected very well in a remark made by Lanczos at the end of a paper in which he tried to combine Maxwell’s and Dirac’s equations:“I therefore believe that between the ‘reactionary point of view’ represented here, aiming at a complete fieldtheoretic description based on the usual spacetime structure and the probabilistic (statistical) point of view, a compromise […] no longer is possible.”^{14} ([198], p. 486, footnote)
Lanczos’ work shows that there has been also a smaller subprogram of unification as described before, i.e., the view that somehow the electron and the photon might have to be treated together. Therefore, a common representation of Maxwell’s equations and the Dirac equation was looked for (cf. Section 7.1).“If the possibilities anticipated here prove to be viable, quantum mechanics would cease to be an independent discipline. It would melt into a deepened ‘theory of matter’ which would have to be built up from regular solutions of nonlinear differential equations, — in an ultimate relationship it would dissolve in the ‘world equations’ of the Universe. Then, the dualism ‘matterfield’ would have been overcome as well as the dualism ‘corpusclewave’.”^{15} ([198], p. 493)
“It is remarkable that not only no fundamental tensor [first fundamental form] or tensordensity, but also no connection, neither Riemannian nor projective, nor conformal, is needed for writing down the [Maxwell] equations. Matter is characterised by a bivectordensity […].” ([367], p. 422, and also [363, 364, 365, 366])
If one of the fields to be united asks for less “geometry”, why to mount all the effort needed for generalising Riemannian geometry?

no electromagnetic field → Einstein’s equations in empty space;

no gravitational field → Maxwell’s equations;

“weak” gravitational and electromagnetic fields → EinsteinMaxwell equations;

no gravitational field but a “strong” electromagnetic field → some sort of nonlinear electrodynamics.
In the following Section 2, a multitude of geometrical concepts (affine, conformal, projective spaces, etc.) available for unified field theories, on the one side, and their use as tools for a description of the dynamics of the electromagnetic and gravitational field on the other will be sketched. Then, we look at the very first steps towards a unified field theory taken by Reichenbächer^{18}, Förster (alias Bach), Weyl^{19}, Eddington^{20}, and Einstein (see Section 3.1). In Section 4, the main ideas are developed. They include Weyl’s generalization of Riemannian geometry by the addition of a linear form (see Section 4.1) and the reaction to this approach. To this, Kaluza’s idea concerning a geometrization of the electromagnetic and gravitational fields within a fivedimensional space will be added (see Section 4.2) as well as the subsequent extensions of Riemannian to affine geometry by Schouten, Eddington, Einstein, and others (see Section 4.3). After a short excursion to the world of mathematicians working on differential geometry (see Section 5), the research of Einstein and his assistants is studied (see Section 6). Kaluza’s theory received a great deal of attention after O. Klein^{21} intervention and extension of Kaluza’s paper (see Section 6.3.2). Einstein’s treatment of a special case of a metricaffine geometry, i.e., “distant parallelism”, set off an avalanche of research papers (see Section 6.4.4), the more so as, at the same time, the covariant formulation of Dirac’s equation was a hot topic. The appearance of spinors in a geometrical setting, and endeavours to link quantum physics and geometry (in particular, the attempt to geometrize wave mechanics) are also discussed (see Section 7). We have included this topic although, strictly speaking, it only touches the fringes of unified field theory.
In Section 9, particular attention is given to the mutual influence exerted on each other by the Princeton (Eisenhart^{22}, Veblen^{23}), French (Cartan^{24}), and the Dutch (Schouten, Struik^{25}) schools of mathematicians, and the work of physicists such as Eddington, Einstein, their collaborators, and others. In Section 10, the reception of unified field theory at the time is briefly discussed.
2 The Possibilities of Generalizing General Relativity: A Brief Overview

by connecting an additional linear form to the metric through the concept of “gauging” (Weyl);

by introducing an additional space dimension (Kaluza);

by choosing an asymmetric Ricci tensor (Eddington);

by adding an antisymmetric tensor to the metric (Bach, Einstein);

by replacing the metric by a 4bein field (Einstein).

geometry,

dynamics (Lagrangians, field equations),

number field, and

dimension of space,
2.1 Geometry
It is very easy to get lost in the many constructive possibilities underlying the geometry of unified field theories. We briefly describe the mathematical objects occurring in an order that goes from the less structured to the more structured cases. In the following, only local differential geometry is taken into account^{26}.
The space of physical events will be described by a real, smooth manifold M_{ D } of dimension D coordinatised by local coordinates x^{ i }, and provided with smooth vector fields X, Y, … with components X^{ i }, Y^{ i }, … and linear forms ω, ν, …, (ω_{ i }, ν_{ i }) in the local coordinate system, as well as further geometrical objects such as tensors, spinors, connections^{27}. At each point, D linearly independent vectors (linear forms) form a linear space, the tangent space (cotangent space) of M_{ D }. We will assume that the manifold M_{ D } is space and timeorientable. On it, two independent fundamental structural objects will now be introduced.
2.2 Metrical structure
The first is a prescription for the definition of the distance ds between two infinitesimally close points on M_{ D }, eventually corresponding to temporal and spatial distances in the external world. For ds, we need positivity, symmetry in the two points, and the validity of the triangle equation. We know that ds must be homogeneous of degree one in the coordinate differentials dx^{ i } connecting the points. This condition is not very restrictive; it still includes Finsler geometry [281, 126, 224] to be briefly touched, below.
The manifold is called spacetime if D=4 and the metric is symmetric and Lorentzian, i.e., symmetric and with signature sig g=±2. Nevertheless, sloppy contemporaneaous usage of the term “spacetime” includes arbitrary dimension, and sometimes is applied even to metrics with arbitrary signature.
A new physical aspect will come in if the h _{ î } ^{ k } are considered to be the basic geometric variables satisfying field equations, not the metric. Such tetradtheories (for the case D=4) are described well by the concept of fibre bundle. The fibre at each point of the manifold contains, in the case of an orthonormal Dbein (tetrad), all Dbeins (tetrads) related to each other by transformations of the group O(D), or the Lorentz group, and so on.
2.2.1 Affine structure
A manifold provided with only a linear connection L is called affine space. From the point of view of group theory, the affine group (linear inhomogeneous coordinate transformations) plays a special role: With regard to it the connection transforms as a tensor (cf. Section 2.1.5).
In Part II of this article, we shall find the set of transformations \({L_{ik}}^j \to {L_{ik}}^j + {\delta ^j}_i\tfrac{{\partial \omega }}{{\partial {x^k}}}\) playing a role in versions of Einstein’s unified field theory.
2.2.2 Different types of geometry
2.2.2.1 Affine geometry
In order to shorten the presentation of affine geometry, we refrain from listing the corresponding set of equations for the other affine curvature tensor (cf., however, [356]).
In affine geometry, the simplest way to define a fundamental tensor is to set g_{ ij }:=αK_{(ij)}, or g_{ ij }:=αK̅_{(ij)}. It may be desirable to derive the metric from a Lagrangian; then the simplest scalar density that could be used as such is given by det (K_{ ij })^{42}.
2.2.2.2 Mixed geometry
A manifold carrying both structural elements, i.e., metric and connection, is called a metricaffine space. If the first fundamental form is taken to be asymmetric, i.e., to contain an antisymmetric part \({g_{[ik]}}: = \tfrac{1}{2}({g_{ij}}  {g_{ji}})\), we speak of a mixed geometry. In principle, both metricaffine space and mixed geometry may always be reinterpreted as Riemannian geometry with additional geometric objects: the 2form field φ(f) (symplectic form), the torsion S, and the nonmetricity Q (cf. Equation 41). It depends on the physical interpretation, i.e., the assumed relation between mathematical objects and physical observables, which geometry is the most suitable.
Even before Weyl, the question had been asked (and answered) as to what extent the conformal and the projective structures were determining the geometry: According to Kretschmann (and then to Weyl) they fix the metric up to a constant factor ([196]; see also [401], Appendix 1; for a modern approach, cf. [67]).
The geometry needed for the pre and nonrelativistic approaches to unified field theory will have to be dealt with separately. There, the metric tensor of space is Euclidean and not of full rank; time is described by help of a linear form (NewtonCartan geometry, cf. [65, 66]). In the following we shall deal only with relativistic unified field theories.
2.2.2.3 Projective geometry
2.2.3 Cartan’s method
2.2.4 Tensors, spinors, symmetries
2.2.4.1 Tensors
Objects that transform as in Equation (67) but with respect to a subgroup, e.g., the linear group, affine group G(D), orthonormal group O(D), or the Lorentz group \({\mathcal L}\), are tensors in a restricted sense; sometimes they are named affine or Cartesian tensors. All the subgroups mentioned are Liegroups, i.e., continuous groups with a finite number of parameters. In general relativity, both the “group” of general coordinate transformations and the Lorentz group are present. The concept of tensors used in Special Relativity is restricted to a representation of the Lorentz group; however, as soon as the theory is to be given a coordinateindependent (“generally covariant”) form, then the full tensor concept comes into play.
2.2.4.2 Spinors
2.2.4.3 Symmetries
A Riemannian space is called (locally) stationary if it admits a timelike Killing vector; it is called (locally) static if this Killing vector is hypersurface orthogonal. Thus if, in a special coordinate system, we take X^{ i }=δ _{0} ^{ i } then from Equation (91) we conclude that stationarity reduces to the condition ∂_{0}g_{ ik }= 0. If we take X to be the tangent vector field to the congruence of curves x^{ i }=x^{ i }(u), i.e., if \({X^k} = \tfrac{{d{x^k}}}{{du}}\), then a necessary and sufficient condition for hypersurfaceorthogonality is \({\epsilon^{ijkl}}{X_j}{X_{[k,l]}} = 0\).
A generalisation of Killing vectors are conformal Killing vectors for which \({{\mathcal L}_X}\;{g_{ik}} = \Phi {g_{ik}}\) with an arbitrary smooth function Φ holds. In purely affine spaces, another type of symmetry may be defined: \({{\mathcal L}_X}\;{\Gamma _{ik}}^l = 0\); they are called affine motions [425].
2.3 Dynamics
For most of the unified field theories to be discussed in the following, such identifications were made on internal, structural reasons, as no linkup to empirical data was possible. Due to the inherent wealth of constructive possibilities, unified field theory never would have come off the ground proper as a physical theory even if all the necessary formal requirements could have been satisfied. As an example, we take the identification of the electromagnetic field tensor with either the skew part of the metric, in a “mixed geometry” with metric compatible connection, or the skew part of the Ricci tensor in metricaffine theory, to list only two possibilities. The latter choice obtains likewise in a purely affine theory in which the metric is a derived secondary concept. In this case, among the many possible choices for the metric, one may take it proportional to the variational derivative of the Lagrangian with respect to the symmetric part of the Ricci tensor. This does neither guarantee the proper signature of the metric nor its full rank. Several identifications for the electromagnetic 4potential and the electric current vector density have also been suggested (cf. below and [143]).
2.4 Number field
Complex fields may also be introduced on a real manifold. Such fields have also been used for the construction of unified field theories, although mostly after the period dealt with here (cf. Part II, in preparation). In particular, manifolds with a complex fundamental form were studied, e.g., with \({g_{ik}} = {s_{ik}} + i{a_{ik}}\), where \(i = \sqrt {  1}\) [97]. Also, geometries based on Hermitian forms were studied [313]. In later periods, hypercomplex numbers, quaternions, and octonions also were used as basic number fields for gravitational or unified theories (cf. Part II, forthcoming).
In place of the real numbers, by which the concept of manifold has been defined so far, we could take other number fields and thus arrive, e.g., at complex manifolds and so on. In this part of the article we do not need to take into account this generalisation.
2.5 Dimension
Since the suggestions by Nordström and Kaluza [238, 181], manifolds with D>4 have been used for unified field theories. In most of the cases, the additional dimensions were taken to be spacelike; nevertheless, manifolds with more than one direction of time also have been studied.
3 Early Attempts at a Unified Field Theory
3.1 First steps in the development of unified field theories
^{59} Einstein replied:“Perhaps, there exists a covariant 6vector by which the appearance of electricity is explained and which springs lightly from the \({g_{\mu \nu }}\), not forced into it as an alien element.”
In his next letter, Förster gave results of his calculations with an asymmetric \({g_{\mu \nu }} = {s_{\mu \nu }} + {a_{\mu \nu }}\)introduced an asymmetric “threeindexsymbol” and a possible generalisation of the Riemannian curvature tensor as well as tentative Maxwell’s equations and interpretations for the 4potential \({A_\mu }\), and special solutions (28 December 1917) ([321], Volume 8A, Document 420, pp. 5817#x2013;587). Einstein’s next letter of 17 January 1918 is skeptical:“The aim of dealing with gravitation and electricity on the same footing by reducing both groups of phenomena to \({g_{\mu \nu }}\) has already caused me many disappointments. Perhaps, you are luckier in the search. I am totally convinced that in the end all field quantities will look alike in essence. But it is easier to suspect something than to discover it.”^{60} (16 November 1917 [321], Vol. 8A, Doc. 400, p. 557)
“Since long, I also was busy by starting from a nonsymmetric \({g_{\mu \nu }}\); however, I lost hope to get behind the secret of unity (gravitation, electromagnetism) in this way. Various reasons instilled in me strong reservations: […] your other remarks are interesting in themselves and new to me.”^{61} ([321], Volume 8B, Document 439, pp. 610–611)
The result is contained in (Hilbert 1915, p. 397)^{64}.“According to a general mathematical theorem, the electromagnetic equations (generalized Maxwell equations) appear as a consequence of the gravitational equations, such that gravitation and electrodynamics are not really different.”^{63} (letter of Hilbert to Einstein of 13 November 1915 [162])
“Your investigation is of great interest to me because I have often tortured my mind in order to bridge the gap between gravitation and electromagnetism. The hints dropped by you on your postcards bring me to expect the greatest.”^{65} [101]
By his “coordinate rotation”, or, as he calls it in ([269], p. 174), “electromagnetic rotation”, he tries to geometrize the electromagnetic field. As Weyl’s remark in RaumZeitMaterie ([398], p. 267, footnote 30) shows, he did not grasp Reichenbächer’s reasoning; I have not yet understood it either. Apparently, for Reichenbächer the metric deviation from Minkowski space is due solely to the electromagnetic field, whereas gravitation comes in by a single scalar potential connected to the velocity of light. He claims to obtain the same value for the perihelion shift of Mercury as Einstein ([269], p. 177). Reichenbächer was slow to fully accept general relativity; as late as in 1920 he had an exchange with Einstein on the foundations of general relativity [271, 71].“The disturbance, which is generated by the electrons and which forces us to adopt a coordinate system different from the usual one, is interpreted as the electromagnetic sixvector, as is known.”^{67} ([270], p. 136)
“Planck was uncertain to which of Einstein’s papers Reichenbächer appealed. He urged that Reichenbächer speak with Einstein and so dissolve their differences. The meeting was amicable. Reichenbächer’s paper appeared in 1917 as the first attempt at a unified field theory in the wake of Einstein’s covariant field equations.” ([262], p. 208)
In this context, we must also keep in mind that the generalisation of the metric tensor toward asymmetry or complex values was more or less synchronous with the development of Finsler geometry [126]. Although Finsler himself did not apply his geometry to physics it soon became used in attempts at the unification of gravitation and electromagnetism [274].
3.2 Early disagreement about how to explain elementary particles by field theory
Thus, the idea of a program for building the extended constituents of matter from the fields the source of which they are, was very much alive around 1920. However, Pauli’s remark after Weyl’s lecture in Bad Nauheim (86. Naturforscherversammlung, 19–25 September 1920) [245] showed that not everybody was a believer in it. He claimed that in bodies smaller than those carrying the elementary charge (electrons), an electric field could not be measured. There was no point of creating the “interior” of such bodies with the help of an electric field. Pauli:“Now, these objects are tremendous concentrations of energy in the smallest place; therefore, they will house huge curvatures of space or, in other words, gravitational fields. The idea that they keep together the dispersing electrical charges lies close at hand.”^{68} ([19], p. 235)
“None of the present theories of the electron, also not Einstein’s (Einstein 1919 [70]), up to now did achieve solving satisfactorily the problem of the electrical elementary quanta; it seems obvious to look for a deeper reason for this failure. I wish to see this reason in the fact that it is altogether not permitted to describe the electromagnetic field in the interior of an electron as a continuous space function. The electrical field is defined as the force on a charged test particle, and if no smaller test particles exist than the electron (vice versa the nucleus), the concept of electrical field at a certain point in the interior of the electron — with which all continuum theories are working — seems to be an empty fiction, because there are no arbitrarily small measures. Therefore, I’d like to ask Mr. Einstein whether he approves of the opinion that a solution of the problem of matter may be expected only from a modification of our perception of space (perhaps also of time) and of electricity in the sense of atomism, or whether he thinks that the mentioned reservations are unconvincing and is of the opinion that the fundaments of continuum theory must be upheld.”^{69}
In the same discussion Gustav Mie came back to Förster’s idea of an asymmetric metric but did not like it“With the progressing refinement of scientific concepts, the manner by which concepts are related to (physical) events becomes ever more complicated. If, in a certain stage of scientific investigation, it is seen that a concept can no longer be linked with a certain event, there is a choice to let the concept go, or to keep it; in the latter case, we are forced to replace the system of relations among concepts and events by a more complicated one. The same alternative obtains with respect to the concepts of timeand spacedistances. In my opinion, an answer can be given only under the aspect of feasibility; the outcome appears dubious to me.”^{71}
“[…] that an antisymmetric tensor was added to the symmetric tensor of the gravitational potential, which represented the sixvector of the electromagnetic field. But a more precise reasoning shows that in this way no reasonable world function is obtained.”^{72}
“Finally I cut loose firmly from Mie’s theory and arrived at another position with regard to the problem of matter. To me, field physics no longer appears as the key to reality; in contrary, the field, the ether, for me simply is the totally powerless transmitter of causations, yet matter is a reality beyond the field and causes its states.”^{73} (letter of Weyl to F. Klein on 28 December 1920, see [293], p. 83)
“The physical interpretation of geometry (theory of the continuum) presented here, fails in its direct application to spaces of submolecular scale. Yet it retains part of its meaning also with regard to questions concerning the constitution of elementary particles. Because one may try to ascribe to these field concepts […] a physical meaning even if a description of the electrical elementary particles which constitute matter is to be made. Only success can decide whether such a procedure finds its justification […].”^{74} [72]
“In the program, Mr. Einstein expressed during his two talks given in November 1929 at the Institut Henri Poincaré, he wished to search for the physical laws in solutions of his equations without singularities — with matter and the electromagnetic field thus being continuous. Let us move into the field chosen by him without too much surprise to see him apparently follow a road opposed to the one successfully walked by the contemporary physicists.”^{75} ([36], p. 17 (1178))
4 The Main Ideas for Unification between about 1918 and 1923
After 1915, Einstein first was busy with extracting mathematical and physical consequences from general relativity (Hamiltonian, exact solutions, the energy conservation law, cosmology, gravitational waves). Although he kept thinking about how to find elementary particles in a field theory [70] and looked closer into Weyl’s theory [72], at first he only reacted to the new ideas concerning unified field theory as advanced by others. The first such idea after Förster’s, of course, was Hermann Weyl’s gauge approach to gravitation and electromagnetism, unacceptable to Einstein and to Pauli for physical reasons [246, 292].
Next came Kaluza’s fivedimensional unification of gravitation and electromagnetism, and Eddington’s affine geometry.
4.1 Weyl’s theory
4.1.1 The geometry
In contrast to this, Riemann made the much stronger assumption that line elements may be compared not only at the same place but also at two arbitrary places at a finite distance.“If we make no further assumption, the points of a manifold remain totally isolated from each other with regard to metrical structure. A metrical relationship from point to point will only then be infused into [the manifold] if a principle for carrying the unit of length from one point to its infinitesimal neighbours is given.” ^{76}
In order to invent a purely “infinitesimal” geometry, Weyl introduced the 1dimensional, Abelian group of gauge transformations,“However, the possibility of such a comparison ‘at a distance’ in no way can be admitted in a pure infinitesimal geometry.”^{77} ([397], p. 397)
However, a little later, in his paper accepted on 8 June 1918, Weyl boldly claimed:“Again physics, now the physics of fields, is on the way to reduce the whole of natural phenomena to one single law of nature, a goal to which physics already once seemed close when the mechanics of masspoints based on Newton’s Principia did triumph. Yet, also today, the circumstances are such that our trees do not grow into the sky.”^{78} ([396], p. 170; preface dated “Easter 1918”)
“I am bold enough to believe that the whole of physical phenomena may be derived from one single universal worldlaw of greatest mathematical simplicity.”^{79} ([397], p. 385, footnote 4)
4.1.2 Physics
While Weyl’s unification of electromagnetism and gravitation looked splendid from the mathematical point of view, its physical consequences were dire: In general relativity, the line element ds had been identified with space and time intervals measurable by real clocks and real measuring rods. Now, only the equivalence class {λg_{ ik }λ arbitrary} was supposed to have a physical meaning: It was as if clocks and rulers could be arbitrarily “regauged” in each event, whereas in Einstein’s theory the same clocks and rulers had to be used everywhere. Einstein, being the first expert who could keep an eye on Weyl’s theory, immediately objected, as we infer from his correspondence with Weyl.
He then asked whether Einstein would be willing to communicate a paper on this new unified theory to the Berlin Academy ([321], Volume 8B, Document 472, pp. 663–664). At the end of March, Weyl visited Einstein in Berlin, and finally, on 5 April 1918, he mailed his note to him for the Berlin Academy. Einstein was impressed: In April 1918, he wrote four letters and two postcards to Weyl on his new unified field theory — with a tone varying between praise and criticism. His first response of 6 April 1918 on a postcard was enthusiastic:“As I believe, during these days I succeeded in deriving electricity and gravitation from the same source. There is a fully determined action principle, which, in the case of vanishing electricity, leads to your gravitational equations while, without gravity, it coincides with Maxwell’s equations in first order. In the most general case, the equations will be of 4th order, though.”^{83}
“Your note has arrived. It is a stroke of genious of first rank. Nevertheless, up to now I was not able to do away with my objection concerning the scale.”^{84} ([321], Volume 8B, Document 498, 710)
“Regrettably, the basic hypothesis of the theory seems unacceptable to me, [of a theory] the depth and audacity of which must fill every reader with admiration.”^{85} ([395], Addendum, p. 478)
Einstein’s remark concerning the pathdependence of the frequencies of spectral lines stems from the pathdependency of the integral (102) given above. Only for a vanishing electromagnetic field does this objection not hold.
“The most plausible assumption that can be made for a clock resting in a static field is this: that it measure the integral of the ds normed in this way [i.e., as in Einstein’s theory]; the task remains, in my theory as well as in Einstein’s, to derive this fact by a dynamics carried through explicitly.”^{86} ([395], p. 479)
“[Weyl] would say that clocks and rulers must appear as solutions; they do not occur in the foundation of the theory. But I find: If the ds, as measured by a clock (or a ruler), is something independent of prehistory, construction and the material, then this invariant as such must also play a fundamental role in theory. Yet, if the manner in which nature really behaves would be otherwise, then spectral lines and welldefined chemical elements would not exist. […] In any case, I am as convinced as Weyl that gravitation and electricity must let themselves be bound together to one and the same; I only believe that the right union has not yet been found.”^{87} ([321], Volume 8B, Document 565, 803)
Another famous theoretician who could not side with Weyl was H. A. Lorentz; in a paper on the measurement of lengths and time intervals in general relativity and its generalisations, he contradicted Weyl’s statement that the worldlines of lightsignals would suffice to determine the gravitational potentials [211].
However, Weyl still believed in the physical value of his theory. As further “extraordinarily strong support for our hypothesis of the essence of electricity” he considered the fact that he had obtained the conservation of electric charge from gaugeinvariance in the same way as he had linked with coordinateinvariance earlier, what at the time was considered to be “conservation of energy and momentum”, where a nontensorial object stood in for the energymomentum density of the gravitational field ([398], pp. 252–253).
Moreover, Weyl had some doubts about the general validity of Einstein’s theory which he derived from the discrepancy in value by 20 orders of magniture of the classical electron radius and the gravitational radius corresponding to the electron’s mass ([397], p. 476; [152]).
4.1.3 Reactions to Weyl’s theory I: Einstein and Weyl
There exists an intensive correspondence between Einstein and Weyl, now completely available in volume 8 of the Collected Papers of Einstein [321]. We subsume some of the relevant discussions. Even before Weyl’s note was published by the Berlin Academy on 6 June 1918, many exchanges had taken place between him and Einstein.
“Your rejection of the theory for me is weighty; […] But my own brain still keeps believing in it. And as a mathematician I must by all means hold to [the fact] that my geometry is the true geometry ‘in the near’, that Riemann happened to come to the special case F_{ ik }=0 is due only to historical reasons (its origin is the theory of surfaces), not to such that matter.”^{89} ([321], Volume 8B, Document 544, 767)
Einstein’s remark concerning “affine geometry” is referring to the affine geometry in the sense it was introduced by Weyl in the 1st and 2nd edition of his book [396], i.e., through the affine group and not as a suggestion of an affine connexion.“[Weyl’s] theoretical attempt does not fit to the fact that two originally congruent rigid bodies remain congruent independent of their respective histories. In particular, it is unimportant which value of the integral \(\int {\phi _\nu }d{x_\nu }\) is assigned to their world line. Otherwise, sodium atoms and electrons of all sizes would exist. But if the relative size of rigid bodies does not depend on past history, then a measurable distance between two (neighbouring) worldpoints exists. Then, Weyl’s fundamental hypothesis is incorrect on the molecular level, anyway. As far as I can see, there is not a single physical reason for it being valid for the gravitational field. The gravitational field equations will be of fourth order, against which speaks all experience until now […].”^{90} ([99], p. 133)
Einstein was unimpressed:“[…] by the prefixing of this factor, so to speak, the absolute norming of the unit of length is accomplished after all”^{91} ([321], Volume 8B, Document 619, 877–879)
“But the expression Rg_{ ik }dx^{ i }dx^{ k } for the measured length is not at all acceptable in my opinion because R is very dependent on the matter density. A very small change of the measuring path would strongly influence the integral of the square root of this quantity.”^{92}
The last remarks are interesting for the way in which Einstein imagined a successful unified field theory.“Of course I know that the state of the theory as I presented it is not satisfactory, not to speak of the fact that matter remains unexplained. The unconnected juxtaposition of the gravitational terms, the electromagnetic terms, and the λterms undeniably is a result of resignation.[…] In the end, things must arrange themselves such that actiondensities need not be glued together additively.”^{93} ([321], Volume 8B, Document 626, 893–894)
4.1.4 Reactions to Weyl’s theory II: Schouten, Pauli, Eddington, and others
“What you say here is really marvelous. In the same way in which Mie glued to his consequential electrodynamics a gravitation which was not organically linked to it, Einstein glued to his consequential gravitation an electrodynamics (i.e., the usual electrodynamics) which had not much to do with it. You establish a real unity.”^{94} [327]
Schouten, in his attempt in 1919 to replace the presentation of the geometrical objects used in general relativity in local coordinates by a “direct analysis”, also had noticed Weyl’s theory. In his “addendum concerning the newest theory of Weyl”, he came as far as to show that Weyl’s connection is gauge invariant, and to point to the identification of the electromagnetic 4potential. Understandably, no comments about the physics are given ([295], pp. 89–91).
“but also against every continuumtheory, also one which treats the electron as a singularity. Now as before I believe that one must look for such an overdetermination by differential equations that the solutions no longer have the character of a continuum. But how?” ([103], p. 43)
“One must pass to tensors of fourth order rather than only to those of second order, which carries with it a vast indeterminacy, because, first, there exist many more equations to be taken into account, second, because the solutions contain more arbitrary constants.”^{95} ([99], p. 153)
In his book “Space, Time, and Gravitation”, Eddington gave a nontechnical introduction into Weyl’s “welding together of electricity and gravitation into one geometry”. The idea of gauging lengths independently at different events was the central theme. He pointed out that while the fourfold freedom in the choice of coordinates had led to the conservation laws for energy and momentum, “in the new geometry is a fifth arbitrariness, namely that of the selected gaugesystem. This must also give rise to an identity; and it is found that the new identity expresses the law of conservation of electric charge.” One natural gauge was formed by the “radius of curvature of the world”; “the electron could not know how large it ought to be, unless it had something to measure itself against” ([57], pp. 174, 173, 177).
Of course, “wrong end” meant that Eddington took Weyl’s theory such“from the wrong end — as its author might consider; but I trust that my treatment has not unduly obscured the brilliance of what is unquestionably the greatest advance in the relativity theory after Einstein’s work.” ([59], p. 198)
Again, Eddington liked Weyl’s natural gauge encountered in Section 4.1.5, which made the curvature scalar a constant, i.e., K=4λ; it became a consequence of Eddington’s own natural gauge in his affine theory, K_{ ij }=λg_{ ij } (cf. Section 4.3). For Eddington, Weyl’s theory of gaugetransformation was a hybrid:“that his nonRiemannian geometry is not to be applied to actual spacetime; it refers to a graphical representation of that relationstructure which is the basis of all physics, and both electromagnetic and metrical variables appear in it as interrelated.” ([59], p. 197)
“He admits the physical comparison of length by optical methods […]; but he does not recognise physical comparison of length by material transfer, and consequently he takes λ to be a function fixed by arbitrary convention and not necessarily a constant.“ ([59], pp. 220–221)
“While it was not difficult to adapt also Maxwell’s equations of the electromagnetic field to this principle [of general relativity], it proved insufficient to reach the goal at which classical field physics is aiming: a unified field theory deriving all forces of nature from one common structure of the world and one uniquely determined law of action.[…] My book describes an attempt to attain this goal by a new principle which I called gauge invariance. (Eichinvarianz). This attempt has failed.” ([410], p. V)
4.1.5 Reactions to Weyl’s theory III: Further research
Pauli, still a student, and with his article for the Encyclopedia in front of him, pragmatically looked into the gravitational effects in the planetary system, which, as a consequence of Einstein’s field equations, had helped Einstein to his fame. He showed that Weyl’s theory had, for the static case, as a possible solution a constant Ricci scalar; thus it also admitted the Schwarzschild solution and could reproduce all desired effects [244, 243].
Reichenbächer seemingly was unhappy about Weyl’s taking the curvature scalar to be a constant before the variation; in the discussion after Weyl’s talk in 1920, he inquired whether one could not introduce Weyl’s “natural gauge” after the variation of the Lagrangian such that the field equations would show their gauge invariance first ([399], p. 651). Eddington criticised Weyl’s choice of a Lagrangian as speculative:“Moreover, this theory leads to the cosmological term in a uniform and forceful manner, [a term] which in Einstein’s theory was introduced ad hoc”^{97} ([402], p. 474)
“At the most we can only regard the assumed form of action […] as a step towards some more natural combination of electromagnetic and gravitational variables.” ([59], p. 212)
“to reconciliate Reichenbächer’s idea: matter causes a ‘deformation’ of the metrical field and Einstein’s idea: inertia and gravitation are one.” ([400], p. 561, footnote)
Eisenhart wished to partially reinterpret Weyl’s theory: In place of putting the vector potential equal to Weyl’s gauge vector, he suggested to identify it with \(\tfrac{{  F_k^i{J^k}}}{\mu }\), where J^{ i } is the electrical 4current vector (density) and μ the mass density. He referred to Weyl, Eddington’s book, and to Pauli’s article in the Encyclopedia of Mathematical Sciences [116].
“The part independent of the ‘electrical’ vector φ_{ i } is found to be \({K_{ij}}  \tfrac{1}{4}K{g_{ij}}\), a tensor which has been considered by Einstein from time to time in connection with the theory of gravitation.” ([237], p. 623)
After the Second World War, research following Weyl’s classical geometrical approach with his original 1dimensional Abelian gaugegroup was resumed. The more important development, however, was the extension to nonAbelian gaugegroups and the combination with Kaluza’s idea. We shall discuss these topics in Part II of this article. The shift in Weyl’s interpretation of the role of the gauging from the link between gravitation and electromagnetism to a link between the quantum mechanical state function and electromagnetism is touched on in Section 7.
4.2 Kaluza’s fivedimensional unification
This remark is surprising because Nordström had suggested a fivedimensional unification of his scalar gravitational theory with electromagnetism five years earlier [238], by embedding spacetime into a fivedimensional world in quite the same way as Kaluza did. In principle, Einstein could have known Nordström’s work. In the same year 1914, he and Fokker had given a covariant formulation of Nordström’s pure (scalar) theory of gravitation [104]. In a subsequent letter to Kaluza of 5 May 1919 Einstein still was impressed: “The formal unity of your theory is startling.” However, on 29 May 1919, Einstein became somewhat reserved^{102}:“The idea of achieving [a unified field theory] by means of a fivedimensional cylinder world never dawned on me. [–] At first glance I like your idea enormously.” (letter of Einstein to Kaluza of 21 April 1919)
Kaluza’s paper was communicated by Einstein to the Academy, but for reasons unknown was published only in 1921 [181]. Kaluza’s idea was to write down the Einstein field equations for empty space in a fivedimensional Riemannian manifold with metric \({g_{\alpha \beta }}\), i.e., \({R_{\alpha \beta }} = 0\), α, β=1,…, 5, where \({R_{\alpha \beta }}\) is the Ricci tensor of M_{5}, and to look at small deviations γ from Minkowski space: \({g_{\alpha \beta }} =  {\delta _{\alpha \beta }} + {\gamma _{\alpha \beta }}\).^{104}. In order to obtain a theory in spacetime, he assumed the socalled “cylinder condition”“I respect greatly the beauty and boldness of your idea. But you understand that, in view of the existing factual concerns, I cannot take sides as planned originally.”^{103}
Kaluza also showed that the geodesics of the fivedimensional space reduce to the equations of motion for a charged point particle in spacetime, if a weakness assumption is made for the components of the 5velocity \({u^\alpha }:{u^1},{u^2},{u^3},{u^5} \ll 1\), u^{4}≃1. The Lorentz force appears augmented by an additional term containing g_{55} of the order \({\left( {\tfrac{u}{c}} \right)^2}\) which thus may be neglected. From the fifth equation of motion Kaluza concluded that the fifth component of momentum p_{5}∼e, with e being the particles’ electric charge (up to a constant of proportionality). From the equations of motion, charge conservation also followed in Kaluza’s linear approximation. Kaluza was well aware that his theory broke down if applied to elementary particles like electrons or protons, and speculated about an escape in which gravitation had to be considered as some “difference effect”, and the gravitational constant given “a statistical meaning”. For him, any theory claiming universal validity was endangered by quantum theory, anyway.
It seems that at some point Einstein had set his calculational aide Grommer^{106} to work on regular spherically symmetric solutions of Kaluza’s theory. This led to a joint publication which was submitted just one month after Einstein had finally presented a rewritten manuscript of Kaluza’s to the Berlin Academy [105]. The negative result of his own paper, i.e., that no nonsingular, statical, spherically symmetric exact solution exists, did not please Einstein. He also thought that Kaluza’s assumption of general covariance in the fivedimensional manifold had no support from physics; he disliked the preference of the fifth coordinate due to Equation (109) which seemed to contradict the equivalence of all five coordinates used by Kaluza in the construction of the field equations [105]. In any case, apart from an encouraging letter to Kaluza in 1925 in which he called Kaluza’s idea the only serious attempt at unified field theory besides the WeylEddington approach, Einstein kept silent on the fivedimensional theory until 1926.“I am having second thoughts about having kept you from the publication of your idea on the unification of gravitation and electricity two years ago. I value your approach more than the one followed by H. Weyl. If you wish, I will present your paper to the Academy after all.”^{105} (letter from Einstein to Kaluza reprinted in [49], p. 454)
4.3 Eddington’s affine theory
4.3.1 Eddington’s paper
In the first, shorter, part of two, Eddington describes affine geometry; in the second he relates mathematical objects to physical variables. He distinguishes the affine geometry as the “geometry of the worldstructure” from Riemannian geometry as “the natural geometry of the world”. He starts by calculating both the curvature and Ricci tensors from the symmetric connection according to Equation (39). The Ricci tensor K^{ ij }(Γ):=*G^{ ij } is asymmetric^{107},“In passing beyond Euclidean geometry, gravitation makes its appearance; in passing beyond Riemannian geometry, electromagnetic force appears; what remains to be gained by further generalisation? Clearly, the nonMaxwellian binding forces which hold together an electron. But the problem of the electron must be difficult, and I cannot say whether the present generalisation succeeds in providing the material for its solution” ([58], p. 104)
Now, by Equation (25),“The divergence of j^{ k } will vanish identically if j^{ k } is itself the divergence of any antisymmetrical contravariant tensor.” ([64], p. 223; cf. also [58], p. 113)
While this remark certainly is true, there is no guarantee in Eddington’s approach that g_{ kl } thus defined is a Lorentzian metric, i.e., that it could describe light propagation at all. Only connections leading to a Lorentz metric can be used if a physical interpretation is wanted. Note also, that the interpretation of R_{ kl } as the metric implies that det R_{ kl }≠0.“Our gaugingequation is therefore certainly true wherever light is propagated, i.e., everywhere inside the electron. Who shall say what is the ordinary gauge inside the electron?” ([58], p. 114)
We must read Equation (118) as giving g_{ kl }(Γ) if the only basic variable in affine geometry, i.e., the connection \({\Gamma _{ij}}^k\), has been determined by help of some field equations. Thus, in general, g_{ kl } is not metriccompatible; in order to make it such, we are led to the differential equations \({R_{ij\left\ k \right.}} = 0\) for \({\Gamma _{ij}}^k\), an equation not considered by Eddington. In the absence of an electromagnetic field, Equation (118) looks like Einstein’s vacuum field equation with cosmological constant. In principle, now a fictitious “Riemannian” connection (the Christoffel symbol) can be written down which, however, is a horribly complicated function of the affine connection — as the only fundamental geometrical quantity available. This is due to the expression for the inverse of the metric, a function cubic in R_{ kl }. Eddington’s affine theory thus can also be seen as a biconnection theory. Note also that Eddington does not explicitly say how to obtain the contravariant form of the electromagnetic field F^{ ij } from F_{ ij }; we must assume that he thought of raising indices with the complicated inverse metric tensor.
“I would as soon think of reverting to Newtonian theory as of dropping the cosmic constant.” ([63], p. 35)
Now, Eddington was able to identify the energymomentum tensor T^{ ik } of the electromagnetic field by decomposing the Ricci tensor K^{ ij } formed from Equation (51) into a metric part R_{ ik } and the rest. The energymomentum tensor T^{ ik } of the electromagnetic field is then defined by Einstein’s field equations with a fictitious cosmological constant \(\kappa {T^{ik}}: = {G^{ik}}  \tfrac{1}{2}{g^{ik}}(G  2\lambda )\).
Although Eddington’s interest did not rest on finding a proper set of field equations, he nevertheless discussed the Lagrangian \({\mathcal L} = \sqrt {  g} *{G^{ik}}*{G_{ik}}\), and showed that a variation with regard to g_{ ik } did not lead to an acceptable field equation.
By “things” he meant“What we have sought is not the geometry of actual space and time, but the geometry of the worldstructure which is the common basis of space and time and things.” ([58], p. 121)
 (1)
the energymomentum tensor of matter, i.e., of the electromagnetic field,
 (2)
the tensor of the electromagnetic field, and
 (3)
the electric chargeandcurrent vector.
While Pauli liked Eddington’s distinction between “natural geometry” and “world geometry” — with the latter being only “a graphical representation” of reality — he was not sure at all whether “a point of view could be taken from which the gravitational and electromagnetical fields appear as union”. If so, then it must be a purely phenomenological one without any recourse to the nature of the charged elementary particles (cf. his letter to Eddington quoted below).
“It may well be asked whether after all it would not be preferable simply to introduce the functions that are necessary for characterising the electromagnetic and gravitational fields, without encumbering the theory with so great a number of superfluous quantities.” ([211], p. 382)
4.3.2 Einstein’s reaction and publications
He now tried to make Eddington’s theory work as a physical theory; Eddington had not given field equations:“I believe I have finally understood the connection between electricity and gravitation. Eddington has come closer to the truth than Weyl.” ([139], p. 274)
And a few days later, he was still intrigued about this sort of unified field theory, in particular about its elusiveness: “[…] Over it lingers the marble smile of inexorable nature, which has bestowed on us more longing than brains.”^{108} (letter of Einstein to Weyl of 26 May 1923; cf.[241], p. 343) And indeed Einstein published fast, even while still on the steamer returning from Japan through Palestine and Spain: The paper of February 1923 in the reports of the Berlin Academy carries, as location of the sender, the ship “Haruna Maru” of the Japanese Nippon Yushen Kaisha line^{109} [77].“I must absolutely publish since Eddington’s idea must be thought through to the end.” (letter of Einstein to Weyl of 23 May 1923; cf. [241], p. 343)
“In past years, the wish to understand the gravitational and electromagnetic field as one in essence has dominated the endeavours of theoreticians. […] From a purely logical point of view only the connection should be used as a fundamental quantity, and the metric as a quantity derived thereof […] Eddington has done this.”^{110} ([77], p. 32)
For a Lagrangian, Einstein used \({\mathcal L} = 2\sqrt {  \det \;{K_{ij}}} ;\); he claims that for vanishing electromagnetic field the vacuum field equations of general relativity, with the cosmological term included, hold. Einstein varied with regard to g_{ kl } and σ_{ kl }, not, as one might have expected, with regard to the connection \({\Gamma _{kj}}^j\). If \({\hat f^{kl}}: = \tfrac{{\delta {\mathcal L}}}{{\delta {\phi _{kl}}}}\), then the electric current density j^{ l } is defined by \({{\hat \jmath}^l}: = \tfrac{{\partial {{\hat f}^{kl}}}}{{\partial {x^k}}}\). \({\hat f^{kl}}\) is interpreted as “the contravariant tensor of the electromagnetic field”.
If no electromagnetic field is present, \({\hat s^{kl}}\) reduces to \({\hat s^{kl}} = {g^{kl}}\sqrt {  \det \;{g_{kl}}}\); the definition of themetric g_{ ij } in Equation (119) is reinterpreted by Einstein as giving his vacuum field equation with cosmological constant λ^{2}. In order that this makes sense, the identifications in Equation (119) are always to be made after the variation of the Lagrangian is performed.
Einstein went on to show that Maxwell’s vacuum equations are holding in first order approximation. Up to the same order, \({\hat f^{kl}} \simeq {\hat \phi _{kl}}\). In general however, \({{\hat \phi }_{kl}} \ne {s_{km}}{s_{ln}}{{\hat f}^{nm}}\). Also, the geometrical theory presented here is energetically closed, i.e., the current density \({\hat \jmath l}\) cannot be given arbitrarily as in the usual Maxwell theory with external sources.“But the extraordinary smallness of 1/λ^{2} implies that finite φ_{ kl } are possible only for tiny, almost vanishing current density. Except for singular positions, the current density is practically vanishing.”^{112}
“that EDDINGTON’S general idea in context with the Hamiltonian principle leads to a theory almost free of ambiguities; it does justice to our present knowledge about gravitation and electricity and unifies both kinds of fields in a truly accomplished manner.”^{114} ([77], p. 38)
“Therefore, the theory may not account for the difference in mass of positive and negative electrons.”^{115} ([74], p. 77)
4.3.3 Comments by Einstein’s colleagues
“[…] I now do not at all believe that the problem of elementary particles can be solved by any theory applying the concept of continuously varying field strengths which satisfy certain differential equations to regions in the interior of elementary particles. […] The quantities \(\Gamma _{\nu \alpha }^\mu\) cannot be measured directly, but must be obtained from the directly measured quantities by complicated calculational operations. Nobody can determine empirically an affine connection for vectors at neighbouring points if he has not obtained the line element before. Therefore, unlike you and Einstein, I deem the mathematician’s discovery of the possibility to found a geometry on an affine connection without a metric as meaningless for physics, in the first place.”^{119} (Pauli to Eddington on 20 September 1923; [251], pp. 115–119)
Also Weyl, in the 5th edition of RaumZeitMaterie ([398], Appendix 4), in discussing “worldgeometric extensions of Einstein’s theory”, found Eddington’s theory not convincing. He criticised a theory that keeps only the connection as a fundamental building block for its lack of a guarantee that it would also house the conformal structure (light cone structure). This is needed for special relativity to be incorporated in some sense, and thus must be an independent fundamental input [405].
In fact, when Eddington’s book was translated into German in 1925 [60], Einstein wrote an appendix to it in which he repeated, with minor changes, the results of his last paper on the affine theory. His outlook on the state of the theory now was rather bleak:“The theory is intensely formal as indeed all such actiontheories must be, and I cannot avoid the suspicion that the mathematical elegance is obtained by a short cut which does not lead along the direct route of real physical progress. From a recent conversation with Einstein I learn that he is of much the same opinion.” ([64], pp. 257–261)
An echo of this can be found in Einstein’s letter to Besso of 5 June 1925:“For me, the final result of this consideration regrettably consists in the impression that the deepening of the geometrical foundations by WeylEddington is unable to bring progress for our physical understanding; hopefully, future developments will show that this pessimistic opinion has been unjustified.”^{120} ([60], p. 371)
This remark shows that Einstein must have taken some notice of Schouten’s work in affine geometry. What the “special scalar” was, remains an open question.“I am firmly convinced that the entire chain of thought WeylEddingtonSchouten does not lead to something useful in physics, and I now have found another, physically better founded approach. To me, the quantumproblem seems to require something like a special scalar, for the introduction of which I have found a plausible way.”^{121} ([99], p. 204)
4.3.4 Overdetermination of partial differential equations and elementary particles
In a paper from December 1923, Einstein not only stated clearly the necessary conditions for a unified field theory to be acceptable to him, but also expressed his hope that this technique of “overdetermination” of systems of differential equations could solve the “quantum problem”.“I do not believe that the theory will be able to dispense with the continuum. But I fail to succeed in giving my pet idea a tangible form: to understand the quantumstructure through an overdetermination by differential equations.”^{122} ([103], pp. 48–49)
He then ventured the hope that a system of overdetermined differential equations is able to determine“According to the theories known until now the initial state of a system may be chosen freely; the differential equations then give the evolution in time. From our knowledge about quantum states, in particular as it developed in the wake of Bohr’s theory during the past decade, this characteristic feature of theory does not correspond to reality. The initial state of an electron moving around a hydrogen nucleus cannot be chosen freely; its choice must correspond to the quantum conditions. In general: not only the evolution in time but also the initial state obey laws.”^{123} ([75], pp. 360–361)
We note here Einstein’s emphasis on the very special problem of the quantum nature of elementary particles like the electron, as compared to the general problem of embedding matter fields into a geometrical setting.“also the mechanical behaviour of singular points (electrons) in such a way that the initial states of the field and of the singular points are subjected to constraints as well. […] If it is possible at all to solve the quantum problem by differential equations, we may hope to reach the goal in this direction.”
This attitude can also be found in a letter to M. Besso from 5 January 1924:“The system of differential equations to be found, and which overdetermines the field, in any case must admit this static, spherically symmetric solution which describes, respectively, the positive and negative electron according to the equations given above [i.e the EinsteinMaxwell equations].”^{124}
In his answer, Besso asked for more information concerning the quantum aspect of the concept of “overdetermination”, because:“The idea I am wrestling with concerns the understanding of the quantum facts; it is: overdetermination of the laws by more field equations than field variables. In such a way, the unambiguity of the initial conditions ought to be understood without leaving field theory. […] The equations of motion of material points (electrons) will be given up totally; their motion ought to be codetermined by the field laws.”^{125} ([99], p. 197)
“On the one hand, this seems to be connected only formally with a field theory; on the other, it has not yet dawned on me how in this manner something corresponding to the discrete quantum orbits may be reached.”^{126} ([99], p. 199)
5 Differential Geometry’s High Tide
 (1)
The generalisation of parallel transport in the sense of LeviCivita and Weyl. Schouten is the leading figure in this approach [300].
 (2)
The “geometry of paths” considering the lines of constant direction for a connection — with the proponents Veblen, Eisenhart [122, 114, 115, 373], J. M. Thomas [348], and T. Y. Thomas^{127}[349, 347]. Here, only symmetric connections can appear.
 (3)
The idea of mapping a manifold at one point to a manifold at a neighbouring point is central (affine, conformal, projective mappings). The names of König [192] and Cartan [29, 302] are connected with this program.
“based upon an integral whose integrand is homogeneous of the first degree in the differentials. Developments of this theory have been made by Finsler, Berwald, Synge, and J. H. Taylor. In this geometry the paths are the shortest lines, and in that sense are a generalisation of geodesics. Affine properties of these spaces are obtained from a natural generalisation of the definition of LeviCivita for Riemannian spaces.” ([121], p. V)
“Motivated by relativity theory, differential geometry received a totally novel, simple and satisfying foundation; I just refer to G. Hessenberg’s ‘Vectorial foundation…’, Math. Ann. 78, 1917, S. 187–217 and H. Weyl, RaumZeitMaterie, 2. Section, Leipzig 1918 (3. Aufl. Berlin 1920) as well as ‘Reine Infinitesimalgeometrie’ etc.^{128}. […] In the present investigation all 18 different linear connections are listed and determined in an invariant manner. The most general connection is characterised by two fields of third degree, one tensor field of second degree, and a vector field […].”^{129} ([297], p. 57)
Through footnote 5 on the same page we learn the pedagogical reason why Schouten did not use the ‘direct’ method [294, 336] in his presentation, but rather a coordinate dependent formalism^{132}:“The general connection for n=4 at least theoretically opens the door for an extension of Weyl’s theory. For such an extension an invariant fixing of the connection is needed, because a physical phenomenon can correspond only to an invariant expression.”^{131}
“As the results of the present investigation might be of interest for a wider circle of mathematicians, and also for a number of physicists […].”^{133}
Schouten criticised Einstein’s argument for using a symmetric connection^{134} as unfounded (cf. Equation (15)). He then restricted the generality of his approach; in modern parlance, he did allow for vector torsion only:“[…] we see that the electromagnetic field only depends on the curl of the electric current vector, so that the difficulty arises that the electromagnetic field cannot exist in a place with vanishing current density. In the following pages will be shown that this difficulty disappears when the more general supposition is made that the original deplacement is not necessarily symmetrical.” ([300], p. 850)
The affine connection Γ′ can then be decomposed as follows:“We will not consider the most general case, but the semisymmetric case in which the alternating part of the parameters has the form:in which S_{λ} is a general covariant vector.” ([298], p. 851)$$ 1/2({{\Gamma '}_\mu }^\nu _{\,\,\,\,\,\lambda }  {{\Gamma '}_\lambda }^\nu _{\,\,\,\,\,\mu }) = 1/2({S_\lambda }\;\delta _\mu ^\nu  {S_\mu }\;\delta _\lambda ^\nu ), $$
and“Einstein has said (in Meaning of Relativity) that ‘a theory of relativity in which the gravitational field and the electromagnetic field enter as an essential unity’ is desirable and recently has proposed such a theory.” ([117], pp. 367–368)
The spreading of knowledge about properties of differential geometric objects like connection and curvature took time, however, even in Leningrad. Seven years after Schouten’s classification of connections, Fréedericksz of Leningrad — known better for his contributions to the physics of liquid crystals — put forward a classification of his own by using both the connection and the curvature tensor [138].“His geometry also is included in the one now proposed and it may be that the latter, because of its greater generality and adaptability will serve better as the basis for the mathematical formulation of the results of physical experiments.” ([117], p. 369)
6 The Pursuit of Unified Field Theory by Einstein and His Collaborators
6.1 Affine and mixed geometry
As in general relativity, he started from the Lagrangian \({\mathcal L} = {\hat g^{ik}}{R_{ik}}\), but now with ĝ^{ ik } and the connection \({\Gamma _{kj}}^l\) being varied separately as independent variables. After some manipulations, the variation with regard to the metric and to the connection led to the following equations:“[…] Also, my opinion about my paper which appeared in these reports [i.e., Sitzungsberichte of the Prussian Academy, Nr. 17, p. 137, 1923], and which was based on Eddington’s fundamental idea, is such that it does not present the true solution of the problem. After an uninterrupted search during the past two years I now believe to have found the true solution.”^{137} ([78], p. 414)
“However, for later investigations (e.g., the problem of the electron) it is to be kept in mind that the HAMILTONian principle does not provide an argument for putting φ_{ k } equal to zero.”^{138}
After having shown that his new theory contains the vacuum field equations of general relativity for vanishing electromagnetic field, Einstein then proved that, in a firstorder approximation, Maxwell’s field equations result cum grano salis: Instead of \({F_{ik,l}} + {F_{li,k}} + {F_{kl,i}} = 0\) he only obtained \(\Sigma \tfrac{\partial }{{\partial {x^l}}}({F_{ik,l}} + {F_{li,k}} + {F_{kl,i}}) = 0\).
“they are not the components of the curl of a vector as in the classical theory, unless an additional condition is added.” ([120], p. 129)
Toward the end of the paper Einstein discussed timereversal; according to him, by it the sign of the magnetic field is changed, while the sign of the electric field vector is left unchanged^{139}. As he wanted to obtain chargesymmetric solutions from his equations, Einstein now proposed to change the roles of the magnetic fields and the electric fields in the electromagnetic field tensor. In fact, the substitutions \(\mathbf{\tilde E} \to \mathbf{\tilde B}\) and \({\mathbf{\tilde B}} \to  {\mathbf{\tilde E}}\) leave invariant Maxwell’s vacuum field equations (duality transformations)^{140}. Already Pauli had pointed to timereflection symmetry in relation with the problem of having elementary particles with charge ±e and unequal mass ([246], p. 774).
“If the assumption of symmetry^{141} is dropped, the laws of gravitation and Maxwell’s field laws for empty space are obtained in first approximation; the antisymmetric part of ĝ^{ ik } is the electromagnetic field. This is surely a magnificent possibility which likely corresponds to reality. The question now is whether this field theory is consistent with the existence of quanta and atoms. In the macroscopic realm, I do not doubt its correctness.”^{142} ([99], p. 209) We have noted before that a similar suggestion within a theory with a geometry built from an asymmetric metric had been made, in 1917, by Bach alias Förster.
“To me, the insight seems to be important that an explanation of the dissimilarity of the two electricities is possible only if time is given a preferred direction, and if this is taken into account in the definition of the decisive physical quantities. In this, electrodynamics is basically different from gravitation; therefore, the endeavour to melt electrodynamics with the law of gravitation into one unity, to me no longer seems to be justified.“^{143} [79]
The new field equation was picked up by R. N. Sen of Kalkutta who calculated “the energy of an electric particle” according to it [323].“That the equations (140) have received only little attention is due to two circumstances. First, the attempts of all of us were directed to arrive, along the path taken by Weyl and Eddington or a similar one, at a theory melting into a formal unity the gravitational and electromagnetic fields; but by lasting failure I now have laboured to convince myself that truth cannot be approached along this path.“^{145} (Einstein’s italics; [80], p. 100)
According to the commenting note by Tonnelat, the 14 variables are given by the 10 components of the symmetric part g_{(ik)}^{147} of the metric and the 4 components of the electromagnetic vector potential “the rotation of which are formed by the γ_{[ik]}”^{148}.“Regrettably, I had to throw away my work in the spirit of Eddington. Anyway, I now am convinced that, unfortunately, nothing can be made with the complex of ideas by WeylEddington. The equationsI take as the best we have nowadays. They are 9 equations for the 14 variables g_{ ik } and γ_{ ik } New calculations seem to show that these equations yield the motion of the electrons. But it appears doubtful whether there is room in them for the quanta.” ^{146} ([99], p. 216)$$ {R_{ik}}  \frac{1}{4}R\;{g_{ik}} =  \kappa {T_{ik}}\;\;\;\;\;{\rm{electromagnetic}} $$
“Also, the equation put forward by myself^{149},gives me little satisfaction. It does not allow for electrical masses free from singularities. Moreover, I cannot bring myself to gluing together two items (as the l.h.s. and the r.h.s. of an equation) which from a logicalmathematical point of view have nothing to do with each other.” ^{150} ([99], p. 230)$$ {R_{ik}} = {g_{ik}}{f_{lm}}{f^{lm}}  \frac{1}{2}{f_l}{f_{km}}{g^{lm}} $$
6.2 Further work on (metric) affine and mixed geometry
We met J. M. Thomas’ paper before in Section 6.1.“I show in the present paper that his [Einstein’s] new equations can be obtained by a direct generalisation of the equations of the gravitational field previously given by him [g_{ij;k}=0; R_{ ij }=0]. […] In the final section I show that the adoption of the ordinary definition of covariant differentiation leads to a geometry which includes as a special case that proposed by Weyl as a basis for the electric theory; further that the asymmetric connection for this special case is of the type adopted by Schouten for the geometry at the basis of his electric theory.” ([346], p. 187)
Thus, the same problem obtained as in Einstein’s theory: A field without electric current or charge density could not exist [155]^{154}.“The preceding equation shows that electrical charge and electrical current are distributed wherever an electromagnetic field exists.”^{153}
Infeld could as well have applied this admonishment to his own unified field theory discussed above. Perhaps, he became irritated by comparing his expression for the connection (142) with Hattori’s (145).“that the problem of generalising the theory of relativity cannot be solved along a purely formal way. At first, one does not see how a choice can be made among the various nonRiemannian geometries providing us with the gravitational and Maxwell’s equations. The proper world geometry which ought to lead to a unified theory of gravitation and electricity can only be found by an investigation of its physical content.”^{155} ([165], p. 811)
By a remark of Straneo, that autoparallels and geodesics have to be distinguished in an affine geometry, the Indian mathematician Kosambi^{156} felt motivated to approach affine geometry from the system of curves solving ẍ^{ i }+α^{ i }(x, x, t) with an arbitrary parameter t. He then defined two covariant “vectorderivations” along an arbitrary curve and arrived at an (asymmetric) affine connection. By this, he claimed to have made superfluous the fivevectors of Einstein and Mayer^{157} [107]. This must be read in the sense that he could obtain the Einstein.Mayer equations from his formalism without introducing a connecting quantity leading from the space of 5vectors to spacetime [195].
Einstein, in his papers, did not comment on the missing metric compatibility in his theory and its physical meaning. Due to this complication — for example even a condition of metric compatibility would not have the physical meaning of the conservation of the norm of an angle between vectors under parallel transport, and the further difficulty that much of the formalism was very clumsy to manipulate; essential work along this line was done only much later in the 10940s and 1950s (Einstein, Einstein and Strauss, Schrödinger, Lichnerowicz, Hlavaty, Tonnelat, and many others). In this work a generalisation of the equation for metric compatibility, i.e., Equation (47), will play a central role. The continuation of this research line will be presented in Part II of this article.
6.3 Kaluza’s idea taken up again
6.3.1 Kaluza: Act I
On the next day (17 February 1927), and ten days later Einstein was to give papers of his own in front of the Prussian Academy in which he pointed out the gaugegroup, wrote down the geodesic equation, and derived exactly the Einstein.Maxwell equations — not just in first order as Kaluza had done [81, 82]. He came too late: Klein had already shown the same before [185]. Einstein himself acknowledged indirectly that his two notes in the report of the Berlin Academy did not contain any new material. In his second communication, he added a postscript:“It appears that the union of gravitation and Maxwell’s theory is achieved in a completely satisfactory way by the fivedimensional theory (KaluzaKleinFock).” (Einstein to H. A. Lorentz, 16 February 1927)
He then referred to the papers of Klein [185, 186] and to “Fochs Arbeit” which is a paper by Fock^{159} 1926 [130], submitted three months later than Klein’s paper. That Klein had published another important clarifying note in Nature, in which he closed the fifth dimension, seems to have escaped Einstein^{160} [184]. Unlike in his paper with Grommer, but as in Klein’s, Einstein, in his notes, applied the “sharpened cylinder condition”, i.e., dropped the scalar field. Thus, the three of them had no chance to find out that Kaluza had made a mistake: For g_{55}≠const., even in first approximation the new field will appear in the fourdimensional Einstein.Maxwell equations ([145], p. 5).“Mr. Mandel brings to my attention that the results reported by me here are not new. The entire content can be found in the paper by O. Klein.”^{158}
“that the experimental discovery of the second term appears difficult, yet perhaps not entirely impossible.” ([216], p. 145)
Fock derived the general relativistic wave equation and the equations of motion of a charged point particle; the latter is identified with the null geodesics of M_{5}. Neither Mandel nor Fock used the “sharpened cylinder condition” (110).“The importance of the additional coordinate parameter p seems to lie in the fact that it causes the invariance of the equations [i.e., the relativistic wave equations] with respect to addition of an arbitrary gradient to the 4potential.”^{162} ([130], p. 228)
“Now, a rather laborious calculation of the fivedimensional curvature quantities in terms of a fourdimensional submanifold contained in it has shown to me also in the general case (g_{55}≠const., dependence of the components of the f u n d a m e n t a l [tensor] of x^{5} is admitted) that the c h a r a c t e r i s t i c properties of the field equations are then conserved as well, i.e., they keep the form
It is likely that Reichenbächer had been led to this excursion into fivedimensional space, an idea which he had rejected before as unphysical, because his attempt to build a unified field theory in spacetime through the ansatz for the metric \({\gamma _{ik}} = {g_{ik}}  { \epsilon ^2}{\phi _i}{\phi _k}\) with φ_{ k } the electromagnetic 4potential, had failed. Beyond incredibly complicated field equations nothing much had been gained [275]. Reichenbächer’s ansatz is well founded: As we have seen in Section 4.2, due to the violation of covariance in M_{5}, γ_{ ik } transforms as a tensor under the reduced covariance group.
Even L. de Broglie became interested in Kaluza’s “bold but very beautiful theory” and rederived Klein’s results his way [46], but not without getting into a squabble with Klein, who felt misunderstood [188, 47]. He also suggested that one should not accept the cylinder condition, a suggestion looked into by Darrieus who introduced an electrical 5potential and 5current, and deduced Maxwell’s equations from the fivedimensional homogeneous wave equation and the fivedimensional equation of continuity [43].
In 1929 Mandel tried to “axiomatise” the fivedimensional theory: His two axioms were the cylinder condition (109) and its sharpening, Equation (110). He then weakened the second assumption by assuming that “an objective meaning does not rest in the g_{ ik } proper, but only in their quotients”, an idea he ascribed to O. Klein and Einstein. He then discussed conformally invariant field equations, and tried to relate them to equations of wave mechanics [220].
Presently, the different contributions of Kaluza and O. Klein are lumped together by most physicists into what is called “KaluzaKlein theory”. An early criticism of this unhistorical attitude has been voiced in [210].
6.3.2 Kaluza: Act II
Four years later, Einstein returned to Kaluza’s idea. Perhaps, he had since absorbed Mandel’s ideas which included a projection formalism from the fivedimensional space to spacetime [216, 217, 218, 219].
In the eyes of Einstein, by avoiding the artificial cylinder condition (109), the new method removed a serious objection to Kaluza’s theory.“Psychologically, the theory presented here connects to Kaluza’s wellknown theory; however, it avoids extending the physical continuum to one of five dimensions.”^{165}
 (1)
\({U_{\iota k}}: = {P_{\iota k}}  \tfrac{1}{4}(P + R)\), where R is the Ricci scalar of the Riemannian curvature tensor of V_{4}, and
 (2)
the tensor \({N_{klm}}: = {F_{\{ kl;m\} }}\)^{169}.
After this paper Einstein wrote to Ehrenfest in a letter of 17 September 1931 that this theory “in my opinion definitively solves the problem in the macroscopic domain” ([241], p. 333). Also, in a lecture given on 14 October 1931 in the Physics Institute of the University of Wien, he still was proud of the 5vector approach. In talking about the failed endeavours to reconcile classical field theory and quantum theory (“a cemetery of buried hopes”) he is reported to have said:“From the theory presented here, the equations for the gravitational and the electromagnetic fields follow effortlessly by a unifying method; however, up to now, [the theory] does not bring any understanding for the way corpuscles are built, nor for the facts comprised by quantum theory.”^{170} ([107], p. 19)
“Since 1928 I also tried to find a bridge, yet left that road again. However, following an idea half of which came from myself and half from my collaborator, Prof. Dr. Mayer, a startlingly simple construction became successful. […] According to my and Mayer’s opinion, the fifth dimension will not show up. […] according to which relationships between a hypothetical fivedimensional space and the fourdimensional can be obtained. In this way, we succeeded to recognise the gravitational and electromagnetic fields as a logical unity.”^{171} [96]
“The only result of our investigation is the unification of gravitation and electricity, whereby the equations for the latter are just Maxwell’s equations for empty space. Hence, no physical progress is made, [if at all] at most only in the sense that one can see that Maxwell’s equations are not just first approximations but appear on as good a rational foundation as the gravitational equations of empty space. Electrical and massdensity are nonexistent; here, splendour ends; perhaps this already belongs to the quantum problem, which up to now is unattainable from the point of view of field [theory] (in the same way as relativity is from the point of view of quantum mechanics). The witty point is the introduction of 5vectors \({a^\sigma }\) in fourdimensional space, which are bound to space by a linear mechanism. Let a^{ s } be the 4vector belonging to \({a^\sigma }\); then such a relation \({a^s} = \gamma _\sigma ^s{a^\sigma }\) obtains. In the theory equations are meaningful which hold independently of the special relationship generated by \(\gamma _\sigma ^s\). Infinitesimal transport of \({a^\sigma }\) in fourdimensional space is defined, likewise the corresponding 5curvature from which spring the field equations.”^{172} ([99], pp. 274–25)
“This theory does not yet contain the conclusions of the quantum theory. It furnishes, however, clues to a natural development, from which we may anticipate further developments in this direction. In any event, the results thus far obtained represent a definite advance in knowledge of the structure of physical space.” ([94], p. 439)
By using the idea that an affine (n+1)space can be represented by a projective nspace [413], Veblen and Hoffmann avoided the five dimensions of Kaluza: There is a onetoone correspondence between the points of spacetime and a certain congruence of curves in a fivedimensional space for which the fifth coordinate is the curves’ parameter, while the coordinates of spacetime are fixed. The fivedimensional space is just a mathematical device to represent the events (points) of spacetime by these curves. Geometrically, the theory of Veblen and Hoffmann is more transparent and also more general than Einstein and Mayer’s: It can house the additional scalar field inherent in Kaluza’s original approach. Thus, Veblen and Hoffmann also gained the Klein.Gordon equation in curved space, i.e., an equation with the Ricci scalar R appearing besides its mass term. Interestingly, the curvature term reads as 5/27R ([381], p. 821). In his note, Hoffmann generalised the formalism such as to include Dirac’s equations (without gravitation), although some technical difficulties remained. Nevertheless, Hoffman remained optimistic:“But these authors choose a formulation that, due to an unnecessary specialisation of the coordinate system, prefers the fifth coordinate relative to the remaining [coordinates] in much the same way as this had happened in KaluzaKlein theory by means of the cylinder condition […].”^{174} ([249], p. 307)
In his book, Veblen emphasised“There is thus a possibility that the complete system will constitute an improved unification within the relativity theory of the gravitational, electromagnetic and quantum aspects of the field.” ([163], p. 89)
“[…] that our theory starts from a physical and geometrical point of view totally different from KALUZA’s. In particular, we do not demand a relationship between electrical charge and a fifth coordinate; our theory is strictly fourdimensional.”^{175} [379]
Shortly after Einstein’s and Mayer’s paper had appeared, Schouten and van Dantzig also proved that the 5vector formalism of this paper can be brought into a projective form [314].
“We note that Mr. Cartan, in a general and very illuminating investigation, has analysed more deeply the property of systems of differential equations that has been termed by us ‘compatibility’ in this paper and in previous papers.”^{176} [37]
Both the EinsteinMayer theory and Veblen and Hoffmann’s approach turned out to be subcases of the more general scheme of Schouten and van Dantzig intending“all advantages of the formulations of KaluzaKlein and EinsteinMayer while avoiding all their disadvantages.” ([249], p. 307)
In this paper ([318], p. 311, Figure 2), we find an early graphical representation of the parametrised set of all possible theories of a kind^{178}. The formalism of Schouten and van Dantzig allows for taking the additional dimension to be timelike; in their physical applications the metric of spacetime is taken as a Lorentz metric; torsion is also included in their geometry.“to give a unification of general relativity not only with Maxwell’s electromagnetic theory but also with Schrödinger’s and Dirac’s theory of material waves.” ([318], p. 271)
The second order wave equation iterated from their form of Dirac’s equation, besides the spin term contained a curvature term 1/4R, with the numerical factor different from Veblen’s and Hoffmann’s. In a sequel to this publication, Pauli and Solomon corrected an error:“[…] even in the absence of gravitation we must pay attention to a difference between Dirac’s equation in the theory of Einstein and Mayer, and Dirac’s equation as it is written out, usually.”^{181} ([253], p. 458)
“We examine from a general point of view the theory of spinors in a fivedimensional space. Then we discuss the form of the energymomentum tensor and of the current vector in the theory of EinsteinMayer.[…] Unfortunately, it turned out that the considerations of §in the first part are marred by a calculational error… This has made it necessary to introduce a new expression for the energymomentum tensor and […] likewise for the current vector […].”^{182} ([254], p. 582)
Michal had come from Cartan and Schouten’s papers on group manifolds and the distant parallelisms defined on them [227]. H. P. Robertson found a new way of applying distant parallelism: He studied groups of motion admitted by such spaces, e.g., by Einstein’s and Mayer’s spherically symmetric exact solution [282] (cf. Section 6.4.3).“The geometry considered by Einstein and Mayer in their ‘Unified field theory’ leads to the consideration of an ndimensional Riemannian space V_{ n } with a metric tensor g_{ ij }, to each point of which is associated an mdimensional linear vector space V_{ m }, (m>n), for which vector spaces a general linear connection is defined. For the general case (m−n≠1) we find that the calculation of the m−n ‘exceptional directions’ is not unique, and that an additional postulate on the linear connection is necessary. Several of the new theorems give new results even for n=4, m=5, the EinsteinMayer case.“ [228]
Cartan wrote a paper on the EinsteinMayer theory as well ([39], an article published only posthumously) in which he showed that this could be interpreted as a fivedimensional flat geometry with torsion, in which spacetime is embedded as a totally geodesic subspace.
6.4 Distant parallelism
The next geometry Einstein took as a fundament for unified field theory was a geometry with Riemannian metric, vanishing curvature, and nonvanishing torsion, named “absolute parallelism”, “distant parallelism”, “teleparallelism, or “Fernparallelismus”. The contributions from the LeviCivita connection and from contorsion^{183} in the curvature tensor cancel. In place of the metric, tetrads are introduced as the basic variables. As in Euclidean space, in the new geometry these 4beins can be parallely translated to retain the same fixed directions everywhere. Thus, again, a degree of absoluteness is reintroduced into geometry in contrast to Weyl’s first attempt at unification which tried to soften the “rigidity” of Riemannian geometry.
The geometric concept of “fields of parallel vectors” had been introduced on the level of advanced textbooks by Eisenhart as early as 1925–1927 [119, 121] without use of the concept of a metric. In particular, the vanishing of the (affine) curvature tensor was given as a necessary and sufficient condition for the existence of D linearly independent fields of parallel vectors in a Ddimensional affine space ([121], p. 19).
6.4.1 Cartan and Einstein
This remark refers to Einstein’s visit in Paris in March/April 1922. Einstein had believed to have found the idea of distant parallelism by himself. In this regard, Pais may be correct. Every researcher knows how an idea, heard or read someplace, can subconsciously work for years and then surface all of a sudden as his or her own new idea without the slightest remembrance as to where it came from. It seems that this happened also to Einstein. It is quite understandable that he did not remember what had happened six years earlier; perhaps, he had not even fully followed then what Cartan wanted to explain to him. In any case, Einstein’s motivation came from the wish to generalise Riemannian geometry such that the electromagnetic field could be geometrized:“appeared at the moment at which you gave your talks at the Collège de France. I even remember having tried, at Hadamard’s place, to give you the most simple example of a Riemannian space with Fernparallelismus by taking a sphere and by treating as parallels two vectors forming the same angle with the meridians going through their two origins: the corresponding geodesics are the rhumb lines.”^{184} (letter of Cartan to Einstein on 8 May 1929; cf. [50], p. 4)
“Therefore, the endeavour of the theoreticians is directed toward finding natural generalisations of, or supplements to, Riemannian geometry in the hope of reaching a logical building in which all physical field concepts are unified by one single viewpoint.”^{185} ([84], p. 217)
In an investigation concerning spaces with simply transitive continuous groups, Eisenhart already in 1925 had found the connection for a manifold with distant parallelism given 3 years later by Einstein [118]. He also had taken up Cartan’s idea and, in 1926, produced a joint paper with Cartan on “Riemannian geometries admitting absolute parallelism” [40], and Cartan also had written about absolute parallelism in Riemannian spaces [33]. Einstein, of course, could not have been expected to react to these and other purely mathematical papers by Cartan and Schouten, focussed on group manifolds as spaces with torsion and vanishing curvature ([41, 34], pp. 50–54). No physical application had been envisaged by these two mathematicians.
Nevertheless, this story of distant parallelism raises the question of whether Einstein kept up on mathematical developments himself, or whether, at the least, he demanded of his assistants to read the mathematical literature. Against his familiarity with mathematical papers speaks the fact that he did not use the name “torsion” in his publications to be described in the following section. In the area of unified field theory including spinor theory, Einstein just loved to do the mathematics himself, irrespective of whether others had done it before — and done so even better (cf. Section 7.3).
The embarrassing situation was solved by Einstein’s suggestion that he had submitted a comprehensive paper on the subject to Zeitschrift für Physik, and he invited Cartan to add his description of the historical record in another paper (Einstein to Cartan on 10 May 1929). After Cartan had sent his historical review to Einstein on 24 May 1929, the latter answered three months later:“[…] he indicates in his bibliography a note by Bortolotti in which he several times refers to my papers.”^{186} (Cartan to Einstein on 15 May 1929; [50], p. 14)
In his article, Cartan made it very clear that it was not Weitzenböck who had introduced the concept of distant parallelism, as valuable as his results were after the concept had become known. Also, he took Einstein’s treatment of Fernparallelism as a special case of his more general considerations. Interestingly, he permitted himself to interpet the physical meaning of geometrical structures^{188}:“I am now writing up the work for the Mathematische Annalen and should like to add yours […]. The publication should appear in the Mathematische Annalen because, at present, only the mathematical implications are explored and not their applications to physics.”^{187} (letter of Einstein to Cartan on 25 August 1929 [50, 35, 89])
Einstein explained:“Let us say simply that mechanical phenomena are of a purely affine nature whereas electromagnetic phenomena are essentially metric; therefore it is rather natural to try to represent the electromagnetic potential by a not purely affine vector.”^{189} ([35], p. 703)
For Einstein, the attraction of his theory consisted“In particular, I learned from Mr. Weitzenböck and Mr. Cartan that the treatment of continua of the species which is of import here, is not really new.[…] In any case, what is most important in the paper, and new in any case, is the discovery of the simplest field laws that can be imposed on a Riemannian manifold with Fernparallelismus.”^{190} ([89], p. 685)
The split, in first approximation, of the tetrad field h_{ ab } according to \({h_{ab}} = {\eta _{ab}} + {\bar h_{ab}}\) lead to homogeneous wave equations and divergence relations for both the symmetric and the antisymmetric part identified as metric and electromagnetic field tensors, respectively.“For me, the great attraction of the theory presented here lies in its unity and in the allowed highly overdetermined field variables. I also could show that the field equations, in first approximation, lead to equations that correspond to the NewtonPoisson theory of gravitation and to Maxwell’s theory. Nevertheless, I still am far from being able to claim that the derived equations have a physical meaning. The reason is that I could not derive the equations of motion for the corpuscles.”^{191} ([89], p. 697)
6.4.2 How the word spread
Nature then went on to quote from an interview of Einstein of 26 January 1929 in a newspaper, the Daily Chronicle. According to the newspaper, among other statements Einstein made, in his wonderful language, was the following:“For some time it has been rumoured that Prof. Einstein has been about to publish the results of a protracted investigation into the possibility of generalising the theory of relativity so as to include the phenomena of electromagnetism. It is now announced that he has submitted to the Prussian Academy of Sciences a short paper in which the laws of gravitation and of electromagnetism are expressed in a single statement.”
Whether Einstein used this as a metaphorical language or, whether he at this time still believed that the system “nucleus and electrons” is dominated by the electromagnetic force, remains open.“Now, but only now, we know that the force which moves electrons in their ellipses about the nuclei of atoms is the same force which moves our earth in its annual course about the sun, and it is the same force which brings to us the rays of light and heat which make life possible upon this planet.” [2]
“Which are the simplest and most natural conditions to which a continuum of this kind can be subjected? The answer to this question which I have attempted to give in a new paper yields unitary field laws for gravitation and electromagnetism.” ([86], p. 118)
The use of the concept “graph” had its origin in Eddington’s interpretation of his and other peoples’ unified field theories to be only graphs of the world; the true geometry remained the Riemannian geometry underlying Einstein’s general relativity.“Of course the ultimate test of the theory must be by experiment. It may succeed in predicting some interaction between gravitation and electromagnetism which can be confirmed by observation. On the other hand, it may be only a ‘graph’ and so outside the ken of the ordinary physicist.” ([258], p. 879)
“Einstein, in his last publications comments to which are still to appear, again brings us mathematical formulae which are applicable to both gravitation and electricity, as if these two forces seemingly governing the universe were identical and subject to the same law. If this were true it would be impossible to calculate the consequences.”^{194} ([214], p. 68)
6.4.3 Einstein’s research papers
We are dealing here with Einstein’s, and Einstein and Mayer’s joint papers on distant parallelism in the reports of the Berlin Academy and Mathematische Annalen, which were taken as the starting point by other researchers following suit with further calculations. Indeed, there was a lot of work to do, only in part because Einstein, from one paper to the next, had changed his field equations^{195}.
“Fernparallelism” now means that if the components referred to the local nbein of a vector \({A^{\hat k}} = h_l^{\hat k}{A^l}\) at a point p, and of a vector \({B^{\hat k}}\) at a different point q are the same, i.e., \({A^{\hat k}} = {B^{\hat k}}\), then the vectors are to be considered as “parallel”. There is an underlying symmetry, called “rotational invariance” by Einstein: joint rotations of each nbein by the same angle. All relations with a physical meaning must be “rotationally invariant”. Of course, in spacetime with a Lorentz metric, the 4beintransformations do form the proper Lorentz group.
The (Riemannian) curvature tensor calculated from Equation (161) turns out to vanish. As Einstein noted, by g_{ ij } from Equation (160) also the usual Riemannian connection \({\Gamma _{lm}}^k(g)\) may be formed. Moreover, \({Y_{lm}}^k: = {\Gamma _{lm}}^k(g)  {\Delta _{lm}}^k\) is a tensor that could be used for building invariants. In principle, distant parallelism is a particular biconnection theory. The connection \({\Gamma _{lm}}^k(g)\) does not play a role in the following (cf., however, de Donder^{198}’s paper [48]).
From Equation (161), obviously the torsion tensor \({S_{lm}}^k = \tfrac{1}{2}({\Delta _{lm}}^k  {\Delta _{ml}}^k) \ne 0\) follows (cf. Equation (21)). Einstein denoted it by \({\Lambda _{lm}}^k\) and, in comparison with the curvature tensor, considered it as the “formally simplest” tensor of the theory for building invariants by help of the linear form \({\Lambda _{lj}}^jd{x^l}\) and of the scalars \({g^{ij}}{\Lambda _{im}}^l{\Lambda _{jl}}^m\) and \({g_{ij}}\;{g^{lr}}{g^{ms}}{\Lambda _{lm}}^i{\Lambda _{rs}}^{j.}\). He indicated how a Lagrangian could be built and the 16 field equations for the field variables h_{ lj } obtained.

WEYL: Comparison at a distance neither of lengths nor of directions;

RIEMANN: Comparison at a distance of lengths but not of directions;

Present theory: Comparison at a distance of both lengths and directions.
In a postscript, Einstein noted that he could have obtained similar results by using the second scalar invariant of his previous note, and that there was a certain indeterminacy as to the choice of the Lagrangian.“The separation of the gravitational and the electromagnetic field appears artificial in this theory. […] Furthermore, it is remarkable that, according to this theory, the electromagnetic field does not enter the field equations quadratically.”^{200} ([83], p. 6)
He still was not entirely sure that the theory was physically acceptable:“The field equations suggested in this paper may be characterised with regard to other such possible ones in the following way. By staying close to the identity (167), it has been accomplished that not only 16, but 20 independent equations can be imposed on the 16 quantities h _{ i } ^{ k̂ } By ‘independent’ we understand that none of these equations can be derived from the remaining ones, even if there exist 8 identical (differential) relations among them.”^{203} ([88], p. 8)
“A deeper investigation of the consequences of the field equations (170) will have to show whether the Riemannian metric, together with distant parallelism, really gives an adequate representation of the physical qualities of space.”^{204}
 (1)
\(\hat H = {\tfrac{1}{2}}{{\hat \jmath }_1} + {\tfrac{1}{4}}{{\hat \jmath }_2}  {{\hat \jmath }_3},\)
 (2)
\(\hat H* = {\tfrac{1}{2}}{\hat \jmath _1}  {\tfrac{1}{4}}{\hat \jmath _2},\)
 (3)
\(\hat H** = {{\hat \jmath }_3},\)
with the proviso that the specialisation of the constants A, B, C must be made only after the variation of the Lagrangian, not before. Also, together with Müntz, he had shown that for an uncharged mass point the Schwarzschild solution again obtained [87].“[…] that coincide in first approximation with the known laws for the gravitational and electromagnetic field […]”^{208}
“In fact, in the new theory of Mr. Einstein, it is natural to call a universe homogeneous if the torsion vectors that are associated to two parallel surface elements are parallel themselves; this means that parallel transport conserves torsion.”^{210} ([35], p. 703)
“But I am very grateful to you for the identitywhich, astonishingly, had escaped me. […] In a new presentation in the Sitzungsberichten, I used this identity while taking the liberty of pointing to you as its source.” ^{211} (letter of Einstein to Cartan from 18 December 1929, Document X of [50], p. 72)$$ {G^{ik}}_{\left\ i \right.}  {S_{lm}}^{\;k}{G^{lm}} = 0, $$
In order to show that his field equations were compatible he counted the number of equations, identities, and field quantities (in ndimensional space) to find, in the end, n^{2}+n equations for the same number of variables. To do so, he had to introduce an additional variable ψ via \({F_k} = {\phi _k}  \tfrac{{\partial \log \psi }}{{\partial {x^k}}}\). Here, F_{ k } is introduced by \({F_{ik}} = {\partial _k}{F_i}  {\partial _i}{F_k} = {\partial _k}{\phi _i}  {\partial _i}{\phi _k}\). Einstein then showed that \({\partial _l}{F_{ik}} + {\partial _k}{F_{li}} + {\partial _i}{F_{kl}} = 0\).
“Recently, A. Einstein ([89]), following investigations by E. Cartan ([35]), has considerably modified his teleparallelism theory such that former shortcomings (connected only to the physical identifications) vanish by themselves.“^{213} ([433], p. 410)
Note that Einstein does not say that it was Cartan who first “envisaged” these spaces before. Later in the paper, he comes closer to the point:“It is not for the first time that such spaces are envisaged. From a purely mathematical point of view they were studied previously. M. Cartan was so amiable as to write a note for the Mathematische Annalen exposing the various phases in the formal development of these concepts.”^{214} ([92], p. 4)
Again, he held back in his support of Cartan’s priority claim.“This type of space had been envisaged before me by mathematicians, notably by WEITZENBÖCK, EISENHART et CARTAN […].”^{215} [92]
Some of the material in the paper overlaps with results from other publications [85, 90, 93]. The counting of independent variables, field equations, and identities is repeated from Einstein’s paper in Mathematische Annalen [89]. For n=4, there were 20 field equations (G^{ ik }=0, F^{ l }=0) for 16+1 variables \(h_{\hat \imath}^k\) and ψ, four of which were arbitrary (coordinate choice). Hence 7 identities should exist, four of which Einstein had found previously. He now presented a derivation of the remaining three identities by a calculation of two pages’ length. The field equations are the same as in [89]; the proof of their compatibility takes up, in a slightly modified form, the one communicated by Einstein to Cartan in a letter of 18 December 1929 ([92], p. 20). It is reproduced also in [90].
Interestingly, right after Einstein’s article in the institute’s journal, a paper of C. G. Darwin, “On the wave theory of matter”, is printed, and, in the same first volume, a report of Max Born on “Some problems in Quantum Mechanics.” Thus, French readers were kept uptodate on progress made by both parties — whether they worked on classical field theory or quantum theory [45, 21].
“A great step forward has been made in the pursuit of this total synthesis of phenomena which is, right or wrong, the ideal of physicists. […] the splendid effort brought about by Einstein permits us to hope that the last theoretical difficulties will be vanquished, and that we soon will compare the consequences of the theory with [our] experience, the great stepping stone of all creations of the mind.”^{216} [260, 261]
Einstein’s next paper in the Berlin Academy, in which he reverts to his original notation h _{ l } ^{ k̂ } , consisted of a brief critical summary of the formalism used in his previous papers, and the announcement of a serious mistake in his first note in 1930, which made invalid the derivation of the field equations for the electromagnetic field ([90], p. 18). The mistake was the assumption on the kind of dependence on torsion of the quantity Ĝ*^{ ik }, which was mentioned above. Also, Einstein now found it better “to keep the concept of divergence, defined by contraction of the extension of a tensor” and not use the covariant derivative \(\nabla { * _l}\) introduced by him in his third paper in the Berlin Academy [88].
 (1)
covariant,
 (2)
of second order, and
 (3)
linear in the second derivatives of the field variable h _{ i } ^{ k } .
“Therefore equations must be postulated among which identical relations are holding. The higher the number of equations (and consequently also the number of identities among them), the more precise and stronger than mere determinism is the content; accordingly, the theory is the more valuable, if it is also consistent with the empirical facts.”^{217} ([90], p. 21)
The reader had to make out for himself what Cartan’s contribution really was.“The proof of the compatibility, as given in my paper in the Mathematische Annalen, has been somewhat simplified due to a communication which I owe to a letter of Mr. CARTAN (cf. §3, [16]).”^{218}
In linear approximation, i.e., for \({h_{ik}} = {\delta _{ik}} + {\bar h_{ik}}\), Einstein obtained d’Alembert’s equation for both the symmetric and the antisymmetric part of h̄_{ ik }, identified with the gravitational and the electromagnetic field, respectively.
Einstein’s next note of one and a half pages contained a mathematical result within teleparallelism theory: From any tensor with an antisymmetric pair of indices a vector with vanishing divergence can be derived [93].
“It now appears that Einstein has succeeded in working out the consequences of his general law of gravity and electromagnetism for two special cases just as Newton succeeded in working out the consequences of his law for several special cases. […] It is hoped that the present solutions obtained by Einstein, or if not these, then others which may later evolve, will suggest some experiments by which the theory may be tested.” ([339], p. 391)
The mentioning of Cartan resulted from the intensive correspondence of both scientists between December 1929 and February 1930: About a dozen letters were exchanged which, sometimes, contained long calculations [50] (cf. Section 6.4.6). In an address given at the University of Nottingham, England, on 6 June 1930, Einstein also must have commented on the exact solutions found and on his program concerning the elementary particles. A report of this address stated about Einstein’s program:“My field theory is progressing well. Cartan has already worked with it. I myself work with a mathematician (S. Mayer^{219} from Vienna), a marvelous chap […].“^{220} ([98], p. 56)
“The problem is nearly solved; and to the first approximations he gets laws of gravitation and electromagnetics. He does not, however, regard this as sufficient, though those laws may come out. He still wants to have the motions of ordinary particles to come out quite naturally. [The program] has been solved for what he calls the ‘quasistatical motions’, but he also wants to derive elements of matter (electrons and protons) out of the metric structure of space.” ([91], p. 610)
 (4)
the field equations must contain the first derivatives of the field variable h _{ i } ^{ k̂ } only quadratically;
 (5)
the identities for the left hand sides G^{ ik } of the field equations must be linear in G^{ ik } and contain only their first derivatives;
 (6)
torsion must occur only linearly in G^{ ik }.
“Two of these are (nontrivial) generalisations of the original gravitational field equations, one of them being known already as a consequence of the Hamiltonian principle. The remaining two types are denoted in the paper by […].”^{221}
What Cartan might have felt, after investing the forty odd pages of his calculations printed in Debever’s book, is unknown. However, the correspondence on the subject came to an end in May 1930 with a last letter by Cartan. ^{223}.“[…] In any case, I have now completely given up the method of distant parallelism. It seems that this structure has nothing to do with the true character of space […].” ([50], p. 209)
6.4.4 Reactions I: Mostly critical
About half a year after Einstein’s two papers on distant parallelism of 1928 had appeared, Reichenbach^{224}, who always tended to defend Einstein against criticism, classified the new theory [268] according to the lines set out in his book [267] as “having already its precisely fixed logical position in the edifice of WeylEddington geometry” ([267], p. 683). He mentioned as a possible generalization an idea of Einstein’s, in which the operation of parallel transport might be taken as integrable not with regard to length but with regard to direction: “a generalisation which already has been conceived by Einstein as I learned from him” ([267], p. 687)^{225}.
A first reaction from a competing colleague came from Eddington, who, on 23 February 1929, gave a cautious but distinct review of Einstein’s first three publications on distant parallelism [84, 83, 88] in Nature. After having explained the theory and having pointed out the differences to his own affine unified field theory of 1921, he confessed:“[…] it is the aim of Einstein’s new theory to find such an entanglement between gravitation and electricity that it splits into the separate equations of the existing theory only in first approximation; in higher approximation, however, a mutual influence of both fields is brought in, which, possibly, leads to an understanding of questions unanswered up to now as [is the case] for the quantum riddle. But this aim seems to be in reach only if a direct physical interpretation of the operation of transport, even of the immediate field quantities, is given up. From the geometrical point of view, such a path [of approach] must seem very unsatisfactory; its justifications will only be reached if the mentioned link does encompass more physical facts than have been brought into it for building it up.”^{226} ([267], p. 689)
“For my own part I cannot readily give up the affine picture, where gravitational and electric quantities supplement one another as belonging respectively to the symmetrical and antisymmetrical features of world measurement; it is difficult to imagine a neater kind of dovetailing. Perhaps one who believes that Weyl’s theory and its affine generalisation afford considerable enlightenment, may be excused for doubting whether the new theory offers sufficient inducement to make an exchange.” [62]
“[…] my approach is radically different, because I reject distant parallelism and keep to Einstein’s general relativity. […] Various reasons hold me back from believing in parallelism at a distance. First, my mathematical intuition a priori resists to accept such an artificial geometry; I have difficulties to understand the might who has frozen into rigid togetherness the local frames in different events in their twisted positions. Two weighty physical arguments join in […] only by this loosening [of the relationship between the local frames] the existing gaugeinvariance becomes intelligible. Second, the possibility to rotate the frames independently, in the different events, […] is equivalent to the s y m m e t r y o f t h e e n e r g y  m o m e n t u m t e n s o r, or to the validity of the conservation law for angular momentum.”^{227} ([407], pp. 330–332.)
“First let me emphasize that side of the matter about which I fully agree with you: Your approach for incorporating gravitation into Dirac’s theory of the spinning electron […] I am as adverse with regard to Fernparallelismus as you are […] (And here I must do justice to your work in physics. When you made your theory with g′_{ ik }=λg_{ ik } this was pure mathematics and unphysical; Einstein rightly criticised and scolded you. Now the hour of revenge has come for you, now Einstein has made the blunder of distant parallelism which is nothing but mathematics unrelated to physics, now you may scold [him].)”^{228} ([251], pp. 518–519)
Pauli’s remark shows the importance of ideology in this field: As long as no empirical basis exists, beliefs, hopes, expectations, and rationally guided guesses abound. Pauli’s letter to Weyl from 1 July 1929 used nonstandard language (in terms of science):“By the way, I now no longer believe in one syllable of teleparallelism; Einstein seems to have been abandoned by the dear Lord.”^{229} (Pauli to Ehrenfest 29 September 1929; [251], p. 524)
while the wealth of empirical data supporting Heisenberg’s and Schrödinger’s quantum theory would have justified the use of a word like “uninformed” or even “not up to date” for the description of Einstein’s position, use of “reactionary” meant a definite devaluation.“I share completely your skeptical position with regard to Einstein’s 4bein geometry. During the Easter holidays I have visited Einstein in Berlin and found his opinion on modern quantum theory reactionary.”^{230} ([251], p. 506)
Einstein answered on 24 December 1929:“I thank you so much for letting be sent to me your new paper from the Mathematische Annalen [89], which gives such a comfortable and beautiful review of the mathematical properties of a continuum with Riemannian metric and distant parallelism […]. Unlike what I told you in spring, from the point of view of quantum theory, now an argument in favour of distant parallelism can no longer be put forward […]. It just remains […] to congratulate you (or should I rather say condole you?) that you have passed over to the mathematicians. Also, I am not so naive as to believe that you would change your opinion because of whatever criticism. But I would bet with you that, at the latest after one year, you will have given up the entire distant parallelism in the same way as you have given up the affine theory earlier. And, I do not wish to provoke you to contradict me by continuing this letter, because I do not want to delay the approach of this natural end of the theory of distant parallelism.”^{231} (letter to Einstein of 19 December 1929; [251], 526–527)
Before he had written to Einstein, Pauli, with lesser reservations, complained visavis Jordan:“Your letter is quite amusing, but your statement seems rather superficial to me. Only someone who is certain of seeing through the unity of natural forces in the right way ought to write in this way. Before the mathematical consequences have not been thought through properly, is not at all justified to make a negative judgement. […] That the system of equations established by myself forms a consequential relationship with the space structure taken, you would probably accept by a deeper study — more so because, in the meantime, the proof of the compatibility of the equations could be simplified.”^{232} ([251], p. 582)
Of course, Pauli’s spells of rudeness are well known; in this particular case they might have been induced by Einstein’s unfounded hopes for eventually replacing the SchrödingerHeisenbergDirac quantum mechanics by one of his unified field theories.“Einstein is said to have poured out, at the Berlin colloquium, horrible nonsense about new parallelism at a distance. The mere fact that his equations are not in the least similar to Maxwell’s theory is employed by him as an argument that they are somehow related to quantum theory. With such rubbish he may impress only American journalists, not even American physicists, not to speak of European physicists.”^{233} (letter of 30 November 1929, [251], p. 525)
The question of the compatibility of the field equations played a very important role because Einstein hoped to gain, eventually, the quantum laws from the extra equations (cf. his extended correspondence on the subject with Cartan ([50] and Section 6.4.6).
That Pauli had been right (except for the time span envisaged by him) was expressly admitted by Einstein when he had given up his unified field theory based on distant parallelism in 1931 (see letter of Einstein to Pauli on 22 January 1932; cf. [241], p. 347).
Born, however, was not yet a player in unified field theory, and it turned out that Einstein’s theory of distant parallelism became as involved as the previous ones.“Your report on progress in the theory of Fernparallelism did interest me very much, particularly because the new field equations are of unique simplicity. Until now, I had been uncomfortable with the fact that, aside from the tremendously simple and transparent geometry, the field theory did look so very involved”^{235} ([154], p. 307)
When Pauli reviewed this review, he started with the scathing remark“To be critical with regard to the creation of a man who has long since obtained a place in eternity does not suit us and is far from us. Not as a criticism but only as an impression do we point out why the new field theory does not house the same degree of conviction, nor the amount of inner consistency and suggestive necessity in which the former theory excelled.[…] The metric is a sufficient basis for the construction of geometry, and perhaps the idea of complementing RIEMANNian geometry by distant parallelism would not occur if there were the wish to implant something new into RIEMANNian geometry in order to geometrically interpret electromagnetism.”^{236} ([201], p. 126)
For the remainder, Pauli engaged in a discussion with the philosophical background of Lanczos and criticised his support for Mie’s theory of matter of 1913 according to which“It is indeed a courageous deed of the editors to accept an essay on a new field theory of Einstein for the ‘Results in the Exact Sciences’ [literal translation of the journal’s title]. His neverending gift for invention, his persistent energy in the pursuit of a fixed aim in recent years surprise us with, on the average, one such theory per year. Psychologically interesting is that the author normally considers his actual theory for a while as the ‘definite solution’. Hence, […] one could cry out: ’Einstein’s new field theory is dead. Long live Einstein’s new field theory!’”^{237} ([248], p. 186)
Thus, Pauli lightly pushed aside as untenable one of Einstein’s repeated motivations and hopedfor tests for his unified field theories.“the atomism of electricity and matter, fully separated from the existence of the quantum of action, is to be reduced to the properties of (singularityfree) eigensolutions of stilltobefound nonlinear differential equations for the field variables.”^{238}
Lanczos, being dissatisfied with Einstein’s distant parallelism, then tried to explain “electromagnetism as a natural property of Riemannian geometry” by starting from the Lagrangian quadratic in the components of the Ricci tensor: \({\mathcal L} = {R_{ik}}{R_{lm}}{g^{il}}{g^{km}} + C{({R_{ik}}{g^{ik}})^2}\) with an arbitrary constant C. He varied g_{ ik } and R_{ ik } independently [202]. (For Lanczos see J. Stachel’s essay “Lanczos’ early contributions to relativity and his relation to Einstein” in [330], pp. 499–518.)
6.4.5 Reactions II: Further research on distant parallelism
“We may say that A. Einstein built a plane world which is no longer waste like the Euclidean spacetimeworld of H. Minkowski, but, on the contrary, contains in it all that we usually call physical reality.”^{240} ([428], p. 724)
“If the law of motion of elementary particles could be derived from the overdetermined field equation, one could imagine that this law of motion permit only discrete orbits, in the sense of quantum theory.”^{241} ([153], p. 646)
“Einstein’s new gravitational theory is intimately linked to the known theory of the orthogonal congruences of curves due to Ricci. In order to ease a comparison between both theories, we may bring together here the notations of R i c c i and L e v i  C i v i t a […] with those of Einstein.”^{242}
A little after the publication of LeviCivita’s papers, Heinrich Mandel embarked on an application of Kaluza’s fivedimensional approach to Einstein’s theory of distant parallelism [218]. Einstein had sent him the corrected proof sheets of his fourth paper [85]. The basic idea was to consider the points of M_{4} as equivalent to the ensemble of congruences with tangent vector X _{5} ^{ i } in M_{5} (with cylindricity condition) werden.”^{243}. The spacetime interval is defined as the distance of two lines of the congruence on \({M_5}:d{\tau ^2} = ({\gamma _{il}}  {X_{5i}}\;{X_{5l}})(\delta _k^l  {X_5}^l{X_{5k}})d{x^i}d{x^k}\). Mandel did not identify the torsion vector with the electromagnetic 4potential, but introduced the covariant derivative \({\Delta _k}{A^i}: = \tfrac{{\partial {A^i}}}{{\partial {x^k}}} + \{ _{kj}^i\} {A^j} + \tfrac{e}{c}{X_{5k}}{\mathcal M}_l^i{A^l}\), where the tensor \({\mathcal M}\) is skewsymmetric. We may look at this paper also as a forerunner of some sort to the Einstein.Mayer 5vector formalism (cf. Section 6.3.2).
Before Einstein dropped the subject of distant parallelism, many more papers were written by a baker’s dozen of physicists. Some were more interested in the geometrical foundations, in exact solutions to the field equations, or in the variational principle.
He then goes on to find a rigourous solution and obtains the metric \(d{s^2} = {e^{a{x_1}}}dx_4^2  {e^{  2a{x_1}}}dx_1^2  {e^{  a{x_1}}}dx_2^2  {e^{  a{x_1}}}dx_3^2\) and the 4potential \({\phi _4} = \tfrac{1}{{2\sqrt \pi }}{e^{\tfrac{1}{2}a{x_1}}}\) [225]. He also wrote a paper on exact axially symmetric solutions of Einstein’s teleparallelism theory [226].“[…] we test whether the new equations proposed by Einstein are satisfied. It is shown that the new equations are satisfied to the first order but not exactly.”
Tamm and Leontowich treated the field equations given in Einstein’s fourth paper on distant parallelism [85]. They found that these field equations did not have a spherically symmetric solution corresponding to a charged point particle at rest^{244}. The corresponding solution for the uncharged particle was the same as in general relativity, i.e., Schwarzschild’s solution. Tamm and Leontowitch therefore guessed that a charged point particle at rest would lead to an axiallysymmetric solution and pointed to the spin for support of this hypothesis [342, 342].
In footnote 4, they added:“[…] electromagnetic field is incompatible in the new Einstein theory with the assumption of static spherical symmetry and symmetry of the past and the future. […] the new Einstein theory lacks at present all experimental confirmation.”
Müntz is mentioned in [88, 85].“Since writing this paper the authors have learned from Dr. H. Müntz that the new Einstein field equations of the 1929 paper do not yield the vanishing of the gravitational field in the case of spherical symmetry and time symmetry. In this case he has been able to obtain results checking the observed perihelion of mercury” ([416], p. 356)
Again, two months later in his next paper, “Unified field theory and Hamiltonian principle”, Einstein remarks:“I am pleased to dutifully thank Mr. Dr. H. Müntz for the laborious exact calculation of the centrallysymmetric problem based on the Hamiltonian principle; by the results of this investigation I was led to the discovery of the road following here.”^{247}
and, by deriving field equations from a Lagrangian shows that the objection can be overcome. In his paper in July 1929, the physicist Zaycoff had some details:“Mr. Lanczos and Müntz have raised doubt about the compatibility of the field equations obtained in the previous paper […].”
In the same paper, he states: “I did not see the papers of Lanczos and Müntz.” Even before this, in the same year, in a footnote to the paper of Wiener and Vallarta, we read:“Solutions of the field equations on the basis of the original formulation of unified field theory to first approximation for the spherically symmetric case were already obtained by Müntz.”
The latter remark refers to a constant query Pauli had about what would happen, within unified field theory, to the gravitational effects in the planetary system, described so well by general relativity^{248}.“Since writing this paper the authors have learned from Dr. H. Müntz that the new Einstein field equations of the 1929 paper do not yield the vanishing of the gravitational field in the case of spherical symmetry and time symmetry. In this case he has been able to obtain results checking the observed perihelion of mercury.”
And they hasten to reassure the reader:“In a previous paper the authors of the present note have treated the case of a spherically symmetrical statical field, and stated the conclusions: first, that under Einstein’s definition of the electromagnetic potential an electromagnetic field is incompatible with the assumption of static spherical symmetry and symmetry of the past and future; second, that if one uses the Hamiltonian suggested in Einstein’s second 1928 paper, the electromagnetic potential vanishes and the gravitational field also vanishes.”
“None of the conclusions of the previous paper are vitiated by this investigation, although some of the final formulas are supplemented by an additional term.” ([417], p. 802)
He also claims“In recent papers Wiener and the author have determined the tensors \(^s{h_\lambda }\) of Einstein’s unified theory of electricity and gravitation under the assumption of static spherical symmetry and of symmetry of past and future. It was there shown that the field equations suggested in Einstein’s second 1928 paper [83] lead in this case to a vanishing gravitational field. The purpose of this paper is to investigate, for the same case, the nature of the gravitational field obtained from the field equations suggested by Einstein in his first 1929 paper [88].”
Finally, Rosen and Vallarta [283] got together for a systematic investigation of the spherically symmetric, static field in Einstein’s unified field theory of the electromagnetic and gravitational fields [93].“that Wiener has shown in a paper to be published elsewhere soon that the Schwarzschild solution satisfies exactly the field equations suggested by Einstein in his second 1929 paper ([85]).”
Further papers on Einstein’s teleparallelism theory were written in Italy by Bortolotti in Cagliari, Italy [22, 23, 25, 24], and by Palatini [242].
This looks as if he had introduced four vector potentials for the electromagnetic field, and this, in fact, T. Y. Thomas does: “the components h _{ i } ^{ k̂ } will play the role of electromagnetic potentials in the present theory.” The field equations are just the four wave equations \(\sum {{e_{\hat k}}h_{\hat \jmath,\hat k\hat k}^{\hat \imath}}\) where the summation extends over k̂, with k̂= 1,…4, and the comma denotes an absolute derivative he has introduced. The gravitational potentials are still g_{ ik }. In his next note, T. Y. Thomas changed his field equations on the grounds that he wanted them to give a conservation law.“In a number of notes in the Berlin Sitzungsberichte followed by a revised account in the Mathematische Annalen, Einstein has attempted to develop a unified theory of the gravitational and electromagnetic field by introducing into the scheme of Riemannian geometry the possibility of distant parallelism. […] we are led to the construction of a system of wave equations as the equations of the combined gravitational and electromagnetic field. This system is composed of 16 equations for the determination of the 16 quantities h _{ i } ^{ k̂ } and is closely analogous to the system of 10 equations for the determination of the 10 components g_{ ik } in the original theory of gravitation. It is an interesting fact that the covariant components h _{ i } ^{ k̂ } of the fundamental vectors, when considered as electromagnetic potential vectors, satisfy in the local coordinate system the universally recognised laws of Maxwell for the electromagnetic field in free space, as a consequence of the field equations.” [350]
The third paper contains a remark as to the content of the concept “unified field theory”:“This latter point of view is made the basis for the construction of a system of field equations in the present note — and the equations so obtained differ from those of note I only by the appearance of terms quadratic in the quantities \(h_{j,k}^{\hat \imath}\). It would thus appear that we can carry over the interpretation of the h _{ i } ^{ k̂ } as electromagnetic potentials; doing this, we can say that Maxwell’s equations hold approximately in the local coordinate system in the presence of weak electromagnetic fields.” [351]
In his three further installments, T. Y. Thomas moved away from unified field theory to the discussion of mathematical details of the theory he had advanced [353, 354, 355].“It is the objective of the present note to deduce the general existence theorem of the CauchyKowalewsky type for the system of field equations of the unified field theory. […] Einstein (Sitzber. 1930, 18–23) has pointed out that the vanishing of the invariant \(h_{j,k}^{\hat \imath }\) is the condition for the fourdimensional world to be Euclidean, or more properly, pseudoEuclidean. From the point of view of our previous notes this fact has its interpretation in the statement that the world will be pseudoEuclidean only in the absence of electric and magnetic forces. This means that gravitational and electromagnetic phenomena must be intimately related since the existence of gravitation becomes dependent on the electromagnetic field. Thus we secure a real physical unification of gravitation and electricity in the sense that these concepts become but different manifestations of the same fundamental entity — provided, of course, that the theory shows itself to be tenable as a theory in agreement with experience.” [352].
The Hermitian tensor referred to leads to a linear integrable connection that, in the special case that it “is real in the real”, coincides with Einstein’s teleparallel connection.“[…] we were able to show that the metric geometry used by Einstein in his most recent approach to relativity theory [84, 83] coincides with the geometry of a Hermitian tensor of highest rank, which is real on the real axis and satisfies certain differential equations.” ([313], p. 319)
Distant parallelism was revived four decades later within the framework of Poincaré gauge theory; the corresponding theories will be treated in the second part of this review.
6.4.6 Overdetermination and compatibility of systems of differential equations
In the course of Einstein’s thinking about distant parallelism, his ideas about overdetermined systems of differential equations gradually changed. At first, the possibility of gaining hold on the paths of elementary particles — described as singular worldlines of point particles — was central. He combined this with the idea of quantisation, although Planck’s constant h could not possibly surface by such an approach. But somehow, for Einstein, discretisation and quantisation must have been too close to bother about a fundamental constant.
“The demand for the existence of an ‘overdetermined’ system of equations does provide us with the means for the discovery of the field equations”^{249} ([90], p. 21)
Einstein’s rapid answer of 9 December 1929 referred to the letter only; he had not been able to study Cartan’s note. As the further correspondence shows, he had difficulties in following Cartan:“I was not able to completely solve the problem of determining if there are systems of 22 equations other than yours and the one I just indicated […] and it still astonishes me that you managed to find your 22 equations! There are other possibilities giving rise to richer geometrical schemes while remaining deterministic. First, one can take a system of 15 equations […]. Finally, maybe there are also solutions with 16 equations; but the study of this case leads to calculations as complicated as in the case of 22 equations, and I was not fortunate enough to come across a possible system […].” ([50], pp. 25–26)
It would be a task of its own to closely study this correspondence; in our context, it suffices to note that Cartan wrote a special note^{252}“For you have exactly that which I lack: an enviable facility in mathematics. Your explanation of the indice de généralité I have not yet fully understood, at least not the proof. I beg you to send me those of your papers from which I can properly study the theory.” ([50], p. 73)
which was better suited to physicists. Through this note, Einstein came to understand Cartan’s theory of systems in involution:“[…] edited such that I took the point of view of systems of partial differential equations and not, as in my papers, the point of view of systems of equations for total differentials […]”^{253}
“I have read your manuscript, and this enthusiastically. Now, everything is clear to me. Previously, my assistant Prof. Müntz and I had sought something similar — but we were unsuccessful.”^{254} ([50], pp. 87, 94)
Although Einstein was grateful for Cartan’s help, he abandoned the geometry with distant parallelism.“It now is my conviction that for rigourous field theories to be taken seriously everywhere a complete absence of singularities of the field must be demanded. This probably will restrict the free choice of solutions in a region in a farreaching way — more strongly than the restrictions corresponding to your degrees of determination.”^{255} ([50], p. 92)
7 Geometrization of the Electron Field as an Additional Element of Unified Field Theory
After the advent of Schrödinger’s and Dirac’s equations describing the electron nonrelativistically and relativistically, a unification of only the electromagnetic and gravitational fields was considered unconvincing by many theoretical physicists. Hence, in the period 1927–1933, quite a few attempts were made to include Schrödinger’s, Dirac’s, or the KleinGordon equation as a classical oneparticle equation into a geometrical framework by relating the quantum mechanical wave function with some geometrical object. Such an approach then was believed to constitute a unification, up to a degree, of gravitation and/or electricity and quantum theory. In this section, we loosely collect some of these approaches.
A further example for the new program is given by J. M. Whittaker at the University of Edinburgh [415] who wished to introduce the wave function via the matter terms:“It is the purpose of the present paper to develop a form of the theory of relativity which shall contain the theory of quanta, as embodied in Schrödingers wave mechanics, not merely as an afterthought, but as an essential and intrinsic part.” [338]
“In addition to the wave equations a complete scheme must include electromagnetic and gravitational equations. These will differ from the equations of Maxwell and Einstein in having ‘wave’ terms instead of ‘particle’ terms for the current vector and material energy tensor. The object of the present paper is to find these equations […].” ([415], p. 543)
In fact, in a short note, Zaycoff presented his version of Whittaker’s theory with 8 coupled secondorder linear field equations for two “wave vectors” that, in a suitable combination, were to represent “the Dirac’s wave equations”; they contain the Ricci tensor and both the electromagnetic 4potential and field [432]. Thus, what is described is Dirac’s equation in external gravitational and electromagnetic fields, not a unified field theory. Whittaker had expressed himself more clearly:“It neglects the existence of wavemechanical phenomena. By the work of Dirac, wavemechanics has reached an independent status; the only attempt to bring together this new group of phenomena with the other two is J. M. Whittaker’s theory [415].”^{256} [428]
Whittaker also had written down a variational principle by which the gravitational and electromagnetic field equations were also gained. However, as the terms for the various fields were just added up in his Lagrangian, the theory would not have qualified as a genuine unified field theory in the spirit of Einstein.“Eight wave functions are employed instead of Dirac’s four. These are grouped together to form two fourvectors and satisfy wave equations of the second order. It is shown […] that these eight wave equations can be reduced, by addition and subtraction, to the four second order equations satisfied by Dirac’s functions taken twice over; and that, in a sense, the present theory includes Dirac’s.” ([415], p. 543)
An eminent voice was Weyl’s:“wavemechanical methods to gravitational phenomena, by which the curious structure of the spiral nebulae and spherical star systems may be readily understood.” [172]
“It seems to me that it is now hopeless to seek a unification of gravitation and electricity without taking material waves into account.” ([408], p. 325)
“It is an admitted fact that Dirac’s wave functions are not the components of a tensor and that his wave equations are not in tensorial form. It is contended here that therefore his theory cannot be upheld without abandoning the theory of relativity.” ([343], p. 352)
While this story about geometrizing wave mechanics might not be a genuine part of unified field theory at the time, it seems interesting to follow it as a last attempt for binding together classical field theory and quantum physics. Even Einstein was lured into thinking about spinors by Dirac’s equation; this equation promised more success for his program concerning elementary particles as solutions of differential equations (cf. Section 7.3. )
7.1 Unification of Maxwell’s and Dirac’s equations, of electrons and light
“There are probably readers who will share the present writer’s feeling that the methods of noncommutative algebra are harder to follow, and certainly much more difficult to invent, than are operations of types long familiar to analysis.” ([44], p. 654)
“This relation between the wavemechanical equations of a ‘quantum of electricity’ and the electromagnetic field equations, which may be looked at as wavemechanical equations for photons, ought to have a fundamental physical meaning. Therefore, I do not think it is superfluous to win the wave equation of the electron as a generalisation of M a x w e l l’s equations.”^{257} ([140], p. 357)
“unnecessary to introduce in any arbitrary way terms and operators to account for quantum phenomena.” ([128], p. 653; [127])
In this context, another unorthodox suggestion was put forward by A. Anderson who saw matter and radiation as two phases of the same substrate:“These equations may be interpreted as equations for the electromagnetic field in an electron gas whose elements are electric and magnetic dipoles.” [388]
Anderson somehow sensed that charge conservation was in his way; he meddled through by either assuming neutral matter, i.e., a mixture of electrons and protons, or by raising doubt as to “whether the usual quanta of light are strictly electrically neutral” ([3], p. 441).“We conclude that, under sufficiently large pressure, even at absolute zero normal matter and blackbody radiation (gas of light quanta) become identical in every sense. Electrons and protons cannot be distinguished from quanta of light, gas pressure not from radiation pressure.”^{258}
One of the German theorists trying to keep up with wave mechanics was Gustav Mie. He tried to reformulate electrodynamics into a Schrödingertype equation and arrived at a linear, homogeneous wave equation of the Klein.Gordontype for the ψfunction on the continuum of the components of the electromagnetic vector potential [232]. Heisenberg and Pauli, in their paper on the quantum dynamics of wave fields, although acknowledging Mie’s theory as an attempt to establish the classical side for the application of the correspondence principle, criticised it as a formal scheme not yet practically applicable [158].
7.2 Dirac’s electron with spin, Einstein’s teleparallelism, and Kaluza’s fifth dimension
In the same year 1928 in which Einstein published his theory of distant parallelism, Dirac presented his relativistic, spinorial wave equation for the electron with spin. This event gave new hope to those trying to include the electron field into a unified field theory; it induced a flood of papers in 1929 such that this year became the zenith for publications on unified field theory. Although we will first look at papers which gave a general relativistic formulation of Dirac’s equation without having recourse to a geometry with distant parallelism, Tetrode’s paper seems to be the only one not influenced by Einstein’s work with this geometry (cf. Section 6.4.5). Although, as we noted in Section 6.4.1, the technique of using nbeins (tetrads) had been developed by mathematicians before Einstein applied it, it may well have been that it became known to physicists through his work. Both Kaluza’s fivedimensional space and fourdimensional projective geometry were also applied in the general relativistic formulation of Dirac’s equation.
7.2.1 Spinors
This is a very sketchy outline with a focus on the relationship to unified field theories. An interesting study into the details of the introduction of local spinor structures by Weyl and Fock and of the early history of the general relativistic Dirac equation was given recently by Scholz [291].
Some early nomenclature reflects this unfamiliarity with spinors. For the 4component spinors or Diracspinors (cf. Section 2.1.5) the name “halfvectors” coined by Landau was in use^{260}. Podolsky even purported to show that it was unnecessary to employ this concept of “halfvector” if general curvilinear coordinates are used [259]. Although van der Waerden had written on spinor analysis as early as 1929 [368] and Weyl’s [407, 408], Fock’s [133, 131], and Schouten’s [306] treatments in the context of the general relativistic Dirac equation were available, it seems that only with van der Waerden’s book [369], Schrödinger’s and Bargmann’s papers of 1932 [319, 6], and the publication of Infeld and van der Waerden one year later [167] a better knowledge of the new representations of the Lorentz group spread out. Ehrenfest, in 1932, still complained^{261}:“has been brilliantly successful in accounting for the ‘duplexity’ phenomena of the atom, but has the defect that the wave equations are unsymmetrical and have not the tensor form.” ([415], p. 543)
In 1933, three publications of the mathematician Veblen in Princeton on spinors added to the development. He considered his first note on 2spinors “a sort of geometric commentary on the paper of Weyl” [378]. Veblen had studied Weyl’s, Fock’s, and Schouten’s papers, and now introduced a “spinor connection of the first kind” \(\Lambda _{\beta \alpha }^A\), α=1,…,4, with the usual transformation law under the linear transformation \({\bar \psi ^A} = T_D^A{\psi ^D}\;(A,D = 1,2)\) changing the spin frame:“Yet still a thin booklet is missing from which one could leasurely learn spinor and tensorcalculus combined.”^{262} ([68], p. 558)
The transformation law for spinors is the same as before^{264}:“[…] The components of still other objects, the spinors, remain partially indeterminate after coordinates and gauge are fixed and become completely determinate only when the spin frame is specified. There are several ways of embodying this invariant theory in a formal calculus. The one which is here employed has its antecedents chiefly in the work ofWeyl, van derWaerden, Fock, and Schouten. It differs from the calculus arrived at by Schouten chiefly in the treatment of gauge invariance, Schouten (in collaboration with van Dantzig) having preferred to rewrite the projective relativity in a formalism obtainable from the original one by a sort of coordinate transformation, whereas I think the original form fits in better with the classical notations of relativity theory. […] The theory of spinors is more general than the projective relativity and is reduced to the latter by the specification of certain fundamental spinors. These spinors have been recognised by several students (Pauli and Solomon, Fock) of the subject but their role has probably not been fully understood since it has quite recently been thought necessary to give special proofs of invariance.” [380]
“In a fivedimensional representation the use of the homogeneous coordinates (X^{0}, … ,X^{4}) amounts to representing the points of spacetime by the straight lines through the origin, whereas the use of x^{1}, … , x^{4}, and the gauge variable amounts to using the system of straight lines parallel to the x^{0}axis for the same purpose. The transformation (192) given above carries the system of lines into the other.“ [382]
7.2.2 General relativistic Dirac equation and unified field theory
In contrast to Einstein, Weyl did not expect to find the electron as a solution of “classical” spinorial equations:“It is natural to expect that one of the two pairs of components of D i r a c’s quantity belongs to the electron, the other to the proton.”^{265}
For many years, Weyl had given the statistical approach in the formulation of physical laws an important role. He therefore could adapt easily to the BornJordanHeisenberg statistical interpretation of the quantum state. For Weyl and statistics, cf. Section V of Sigurdsson’s dissertation ([326], pp. 180–192).“For every attempt at establishing the quantumtheoretical field equations, one must not lose sight [of the fact] that they cannot be tested empirically, but that they provide, only after their quantization, the basis for statistical assertions concerning the behaviour of material particles and light quanta.”^{266} ([407], p. 332)
“In the past two decades, endeavours have been made repeatedly to connect physical laws with geometrical concepts. In the field of gravitation and of classical mechanics, such endeavours have found their fullest accomplishment in E i n s t e i n’s general relativity. Up to now, quantum mechanics has not found its place in this geometrical picture; attempts in this direction (Klein, Fock) were unsuccessful. Only after Dirac had constructed his equations for the electron, the ground seems to have been prepared for further work in this direction.”^{267} ([135], p. 798)
In another paper [134], Fock and Ivanenko took a first step towards showing that Dirac’s equation can also be written in a generally covariant form. To this end, the matrixvalued linear form ds=γ_{ k }dx^{ k } (summation over k=1, …, 4) was introduced and interpreted as the distance between two points “in a space with four continuous and one discontinuous dimensions”; the discrete variable took only the integer values 1, 2, 3, and 4. Then the operatorvalued vectorial quantity γ_{ k }u^{ k } with the vectorial operator u^{ k } and its derivative \(\tfrac{{ds}}{{d\tau }} = {\gamma _k}{v^k}\) immediately led to Dirac’s equation by replacing v_{ k } by \(\tfrac{1}{m}\left( {\tfrac{h}{{2\pi i}}\tfrac{\partial }{{\partial {x^k}}} + \tfrac{e}{c}{A_k}} \right)\), where A_{ k } is the electromagnetic 4potential, by also assuming the velocity of light c to be the classical average of the “4velocity” v_{ k }, and by applying the operator to the wave function ψ. In the next step, instead of the Dirac γmatrices with constant entries γ _{ l } ^{(0)} .. , the coordinatedependent beincomponents \({\gamma _{\hat k}} = {h_{\hat k}}^l\gamma _l^{(0)}\) are defined; ds^{2} then gives the orthonormality relations of the 4beins.
In order that gaugeinvariance results, ψ must transform with a factor of norm 1, innocuous for observation, i.e., \(\psi \to \exp (i\tfrac{{2\pi }}{h}\tfrac{e}{c}\sigma )\) if \({A_k} \to {A_k} + \tfrac{{\partial \sigma }}{{\partial {x^k}}}\). Another note and extended presentations in both a French and a German physics journal by Fock alone followed suit [133, 131, 132]. In the first paper Fock defined an asymmetric matter tensor for the spinor field,“Thus, it is in the law for the transport of a halfvector that Weyl’s differential linear form must appear.”^{268} ([134], p. 1469)
For his calculations, Fock used Eisenhart’s book [119] and “the excellent collection of the most important formulas and facts in the paper of LeviCivita” [207]. Again, Weyl’s “principle of gauge invariance” as formulated in Weyl’s book of 1928 [406] is mentioned, and Fock stressed that he had found this principle independently and earlier^{270}:“By help of the concept of parallel transport of a halfvector, Dirac’s equations will be written in a generally invariant form. […] The appearance of the 4potential φ_{ l } besides the Riccicoefficients γ_{ ikl } in the expression for parallel transport, on the one hand provides a simple reason for the emergence of the term \({p_l}  \tfrac{e}{c}{\phi _l}\) in the wave equation and, on the other, shows that the potentials φ_{ l } have a place of their own in the geometrical worldview, contrary to Einstein’s opinion; they need not be functions of the γ_{ ikl }.”^{269} ([131], p. 261, Abstract)
The divergence of the complex energymomentum tensor \(W_k^i = T_k^i + iU_k^i\) satisfies“The appearance of Weyl’s differential form in the law for parallel transport of a half vector connects intimately to the fact, observed by the author and also by Weyl (l.c.), that addition of a gradient to the 4potential corresponds to multiplication of the ψ function with a factor of modulus 1.”^{271} ([130], p. 266)
In both of his papers, Fock thus stressed that Einstein’s teleparallel theory was not needed for the general covariant formulation of Dirac’s equation. In this regard he found himself in accord with Weyl, whose approach to the Dirac equation he nevertheless criticised:“The 4potential finds its place in Riemannian geometry, and there exists no reason for generalising it (Weyl, 1918), or for introducing distant parallelism (Einstein 1928). In this point, our theory, developed independently, agrees with the new theory by H. Weyl expounded in his memoir ‘gravitation and the electron’.”^{272} ([132], p. 405)
Weyl’s paper is seminal for the further development of the gauge idea [407].“The main subject of this paper is ‘Dirac’s difficulty’^{273}. Nevertheless, it seems to us that the theory suggested by Weyl for solving this problem is open to grave objections; a criticism of this theory is given in our article.”^{274}
Although Fock had cleared up the generally covariant formulation of Dirac’s equation, and had tried to propagate his results by reporting on them at the conference in Charkow in May 1929^{275} [169], further papers were written. Thus, Reichenbächer, in two papers on “a wavemechanical 2component theory” believed that he had found a method different from Weyl’s for obtaining Dirac’s equation in a gravitational field. As was often the case with Reichenbächer’s work, after longwinded calculations a less than transparent result emerged. His mass term contained a square root, i.e., a ± twovaluedness, which, in principle, might have been instrumental for helping to explain the mass difference of proton and electron. As he remarked, the chances for this were minimal, however [277, 278].
In two papers, Zaycoff (of Sofia) presented a unified field theory of gravitation, electromagnetism and the Dirac field for which he left behind the framework of a theory with distant parallelism used by him in other papers. By varying his Lagrangian with respect to the 4beins, the electromagnetic potential, the Dirac wave function and its complexconjugate, he obtained the 20 field equations for gravitation (of second order in the 4bein variables, assuming the role of the gravitational potentials) and the electromagnetic field (of second order in the 4potential), and 8 equations of first order in the Dirac wave function and the electromagnetic 4potential, corresponding to the generalised Dirac equation and its complex conjugate [426, 427].
Rumer’s paper is [285] (cf. Section 8). In the paper, Zaycoff introduced a sixdimensional manifold with local coordinates x_{0}, … , x_{5} where x_{0}, x_{5} belong to the additional dimensions. His local 6bein comprises, besides the 4bein, four electromagnetic potentials and a further one called “eigenpotential” of the electromagnetic field. As he used a “sharpened cylinder condition, ” no further scalar field is taken into account. For x^{0} to x^{4} he used the subgroup of coordinate transformations given in Klein’s approach, augmented by x^{5′}=x^{5}.“Recently, repeated attempts have been made to raise the number of dimensions of the world in order to explain its strange lawfulness (H. Mandel, G. Rumer, the author et al.). No doubt, there are weighty reasons for such a seemingly paradoxical view. For it is impossible to represent Poincaré’s pressure of the electron within the normal spacetime scheme. However, the introduction of such metaphysical elements is in gross contradiction with spacetime causality, although we may doubt in causality in the usual sense due to Heisenberg’s uncertainty relations. A multidimensional causality cannot be understood as long as we are unable to give the extra dimensions an intuitive meaning.”^{276} [433]
Schouten wrote down Dirac’s equation in a space with torsion; his iterated wave equation, besides the mass term, contains a contribution ∼−1/4R if torsion is set equal to zero. Whether Schouten could fully appreciate the importance of Weyl’s new idea of gauging remains open. For him an important conclusion is that“Fock has tried to make use of the indetermination of the displacement of spinvectors to introduce the electromagnetic vector potential. However the displacement of contravariant tensordensities of weight +1/2 being wholly determined and only these vectordensities playing a role, the idea of Weyl of replacing the potential vector by pseudovectors of class +1 and −1 seems much better.” ([306], p. 261, footnote 19)
“by the influence of a gravitational field the components of the potential vector change from ordinary numbers into Diracnumbers.” ([306], p. 265)
“The joining of Dirac’s theory of the electron with general relativity has been undertaken repeatedly, such as by Wigner [419], Tetrode [344], Fock [131], Weyl [407, 408], Zaycoff [434], Podolsky [259]. Most authors introduce an orthogonal frame of axes at every event, and, relative to it, numerically specialised Diracmatrices. This procedure makes it a little difficult to find out whether Einstein’s idea concerning teleparallelism, to which [authors] sometimes refer, really plays a role, or whether there is no dependence on it. To me, a fundamental advantage seems to be that the entire formalism can be built up by pure operator calculus, without consideration of the ψfunction.”^{278} ([319], p. 105)
The γmatrices were taken by Schrödinger such that their covariant derivative vanished, i.e., \({\gamma _{l\left\ m \right.}} = \tfrac{{\partial {\gamma _l}}}{{\partial {x^m}}}  \Gamma _{lm}^r(g){\gamma _r} + {\gamma _l}{\Gamma _m}  {\gamma _m}{\Gamma _l} = 0\), where Γ_{ l } is the spinconnection introduced by \({\psi _{\left\ l \right.}} = \tfrac{{\partial \psi }}{{\partial {x^l}}}  {\Gamma _l}\psi\). Schrödinger took γ_{0}, γ^{ i }, with i = 1, 2, 3, as Hermitian matrices. He introduced tensoroperators T _{ lm } ^{ ik } such that the inner product \(\psi *{\gamma _0}T_{lm}^{ik}\psi\) instead of \(\psi *T_{lm}^{ik}\psi\) stayed real under a “complemented pointsubstitution”.
The coefficient 1/4 in front of the Ricci scalar in Schrödinger’s (KleinGordon) wave equation differs from the 1/6 needed for a conformally invariant version of the scalar wave equation^{280} (cf. [257], p. 395).“To me, the second term seems to be of considerable theoretical interest. To be sure, it is much too small by many powers of ten in order to replace, say, the term on the r.h.s. For μ is the reciprocal Compton length, about 10^{11} cm^{1}. Yet it appears important that in the generalised theory a term is encountered at all which is equivalent to the enigmatic mass term.”^{279} ([319], p. 128)
Bargmann in his approach, unlike Schrödinger, did not couple “pointsubstitutions [linear coordinate transformations] and similarity transformations [in spin space]”[6]. He introduced a matrix α with \(\alpha + {\alpha ^\dag } = 0\) such that \({(\alpha {\gamma ^l})^\dag } = (\alpha {\gamma ^l})\), with l = 0, … , 3.
The last, erroneous, sentence must have made Pauli irate. In this paper, he pronounced his anathema (in a letter to Ehrenfest with the appeal “Please, copy and distribute!”):“Your fundamental memoir induced me to develop the calculational details for obtaining, from Dirac’s equations in a general gravitational field, the modified form of your four equations of second order and thus make certain the corresponding additional terms. These additional terms do depend in an essential way on the choice of the orthogonal tetrad in the spacetime manifold: It seems that without such a tetrad one cannot obtain Dirac’s equation.”^{281} [208]
Pauli really must have been enraged: Among the publications banned by him is also Weyl’s wellknown article on the electron and gravitation of 1929 [407].“The heap of corpses, behind which quite a lot of bums look for cover, has got an increment. Beware of the paper by LeviCivita: Dirac and Schrödingertype equations, in the Berlin Reports 1933. Everybody should be kept from reading this paper, or from even trying to understand it. Moreover, all articles referred to on p. 241 of this paper belong to the heap of corpses.”^{282} ([252], p. 170)
Unlike Schrödinger’s, the wave equation derived from Dirac’s equation by Infeld and Waerden contained a term +1/4R, with R the Ricci scalar.“In the end, Schouten arrives at almost the same formalism developed in this paper; only that he uses without need nbein components and theorems on sedenions^{283}, while afterwards the formalism is still burdened with auxiliary variables and pseudoquantities. We have taken over the introduction of ‘spin densities’ by Schouten.”^{284} ([168], p. 4)
It is left to an indepth investigation, how this discussion concerning teleparallelism and Dirac’s equation involving Tetrode, Wigner, Fock, Pauli, London, Schrödinger, Infeld and van derWaerden, Zaycoff, and many others influenced the acceptance of the most important result, i.e., Weyl’s transfer of the gauge idea from classical gravitational theory to quantum theory in 1929 [407, 408].
7.2.3 Parallelism at a distance and electron spin
However, he quickly must have found a flaw in his argumentation: He telephoned to stop the printing after less than a page had been typeset. He also wanted that, in the Academy’s protocol, the announcement of this paper be erased. This did not happen; thus we know of his failed attempt, and we can read how his line of thought began ([183], pp. 134–135).“Last week I presented a short paper to the Academy in which I showed that one can ascribe fully determined motions to Schrödinger’s wave mechanics without any statistical interpretation. Will appear soon in Sitz.Ber. [Reports of the Berlin Academy].”^{285} ([103], p. 136)
The correction of this misjudgement of Wiener and Vallarta by Fock and Ivanenko began only one month later [134], and was complete in the summer of 1929 [134, 133, 131, 132].“the quantities ^{ s }h_{λ}^{286} of Einstein seem to have one foot in the macromechanical world formally described by Einstein’s gravitational potentials and characterised by the index λ, and the other foot in a Minkowskian world of micromechanics characterised by the index s. That the micromechanical world of the electron is Minkowskian is shown by the theory of Dirac, in which the electron spin appears as a consequence of the fact that the world of the electron is not Euclidean, but Minkowskian. This seems to us the most important aspect of Einstein’s recent work, and by far the most hopeful portent for a unification of the divergent theories of quanta and gravitational relativity.” [418]
Tamm added a torsion term \(i\hbar \sqrt {({S_i}{S^i})} \chi\) to the Dirac equation (197) and derived from it a general relativistic (Schrödinger) wave equation in an external electromagnetic field with a contribution from the spin tensor coupled to a torsion term^{288} \({\alpha ^{[i}}{\alpha ^{k]}}{S_{ik}}^l\). As Tamm assumed for the torsion vector \({S_k} = \pm \tfrac{{ie}}{{\hbar c}}\;{\phi _k}\), his tetrads had to be complex, with the imaginary part containing the electromagnetic 4potential φ_{ k }. This induced him to see another link to quantum physics; by returning to the first of Einstein’s field equations (170) and replacing ∊ in Equation (169) by \(i\tfrac{e}{c}\hbar\) in the limit ħ→0, he obtained the laws of electricity and gravitation, separately. From this he conjectured that, for finite h, Einstein’s field equations might correctly reproduce the quantum features of “the microcosm” ([341], p. 291); cf. also [340].“that for the new field theory of Einstein [84, 88] certain quantummechanical features are characteristic, and that we may hope that the theory will enable one to seize the quantum laws of the microcosm.”^{287} ([341], p. 288)
What remained after all the attempts at geometrizing the matter field for the electron, was the conviction that the quantum mechanical “wave equations” could be brought into a covariant form, i.e., could be dealt with in the presence of a gravitational field, but that quantum mechanics, spin, and gravitation were independent subjects as seen from the goal of reaching unified field theory.
7.2.4 Kaluza’s theory and wave mechanics
It turned out that from the R_{55}component of the Einstein vacuum equations \({R_{\alpha \beta }} = 0\), α, β=1, … , 5, with the identification g_{55}=ψ made, and the assumption that ψ, \(\tfrac{{\partial \psi }}{{\partial {x^i}}}\) be “very small”, while ψ, \(\tfrac{{\partial \psi }}{{\partial {x^5}}}\) be “even smaller”, the covariant d‘Alembert equation followed, an equation that was identified by the authors with Schrödinger’s equation. Their further comment is:“The objective of this note is to formulate a fivedimensional relativity whose equations will give the laws for the gravitational field, the electromagnetic field, the laws of motion of a charged material point, and the wave equation of Mr. Schrödinger. Thus, we will have a frame in which to take the gravitational and electromagnetic laws, and in which it will be possible also for quantum theory to be included.”^{290} ([150], p. 543)
In the last note, with the changed identification g_{55}=ψ^{2} and slightly altered weakness assumptions, Gonseth and Juvet gained the relativistic wave equation with a nonlinear mass term.“We thus can see that the fiction of a fivedimensional universe provides a deep reason for Schrödinger’s equation. Obviously, this artifice will be needed if some phenomenon would force the physicists to believe in a variability of the [electric] charge.”^{291} ([149], p. 450)
At about the same time, W. Wilson of the University of London rederived the Schrödinger equation in the spirit of O. Klein and noted:“Particularly, I no longer think it to be possible to do justice to the deviations from the classical description of space and time necessitated by quantum theory through the introduction of a fifth dimension.” ([189], p. 191, footnote)
“Dr. H. T. Flint has drawn my attention to a recent paper by O. Klein [189] in which an extension to five dimensions similar to that given in the present paper is described. The corresponding part of the paper was written some time ago and without any knowledge of Klein’s work […].” ([420], p. 441)
Eddington’s “pentads” built up from sedenions later were generalised by Schouten [307].“The matrix theory leads to a very simple derivation of the first order wave equation, equivalent to Dirac’s but expressed in symmetrical form. It leads also to a wave equation which we can identify as relating to a system containing electrons with opposite spin. […] It is interesting to note the way in which the existence of electrons with opposite spins locks the ‘fifth dimension,’ so that it cannot come into play and introduce the absolute into a world of relation. The domain of either electron alone might be rotated in a fifth dimension and we could not observe any difference.” ([61], pp. 524, 542)
J. W. Fisher of King’s College reinterpreted KaluzaKlein theory as presented in Klein’s third paper [187]. He proceeded from the special relativistic homogeneous wave equation in fivedimensional space and, after dimensional reduction, compared it to the KleinGordon equation for a charged particle. By making a choice different from Klein’s for a constant he rederived the result of de Broglie and others that null geodesics in fivedimensional space generate the geodesics of massive and massless particles in spacetime [127].
He now posed the question whether this would be the same for Dirac’s theory. Seemingly, he also believed that a tensorial formulation of Dirac’s equation was handy for answering this question and availed himself of “the tensorial form given by W. Gordon [151], and by J. Frenkel”^{292} [140]. Mandel used, in fivedimensional space, the complexvalued tensorial wave function \({\Psi ^{ik}} = \psi {\gamma ^{ik}} + {\Psi ^{[ik]}}\) with a 5scalar ψ. Here, he had taken up a suggestion J. Frenkel had developed during his attempt to describe the “rotating electron,” i.e., Frenkel’s introduction of a skewsymmetric wave function proportional to the “tensor of magnetoelectric moment” m_{ ik } of the electron by m_{ ik }ψ=m_{0}ψ_{ ik } [141, 140]. Ψ^{ ik } may depend on x^{5}; by taking Ψ periodic in x^{5}, Mandel derived a wave equation “which can be understood as a generalisation of the KleinFock fivedimensional wave equation […].” He also claimed that the vanishing of ψ made M_{5} cylindrical (in the sense of Equation (109) [221]). As he had taken notice of a paper of Jordan [173] that spoke of the electromagnetic field as describing a probability amplitude for polarised photons, Mandel concluded that the amplitude of his Ψfield might then represent polarised electrons as its quanta. However, he restricted himself to the consideration of classical oneparticle wave equations because“a consideration in five dimensions has proven to be well suited for the geometrical interpretation of macroscopic electrodynamics.” ([221], p. 567)
In a later paper, Mandel came back to his wave equation with a skewsymmetric part and gave it a different interpretation [222].“in some cases one can properly speak of a quasimacroscopical onebody problem — think of a beam of monochromatic cathodrays in an arbitrary external forcefield.”^{293}
In following Klein, Mandel concluded from the Heisenberg uncertainty relations that“This completely corresponds to the procedure of the Dirac theory, with the only difference that for Dirac the coordinate ζ could assume not 2 but 4 values; from our point of view this remains unintelligible.”^{294} ([222], p. 785)
This made sense because, unlike Klein, Mandel had not compactified the fifth dimension. His understanding of quantum mechanics must have been limited, though: Only two pages later he claimed that the canonical commutation relations \([\mathbf{p},\mathbf{q}] = \tfrac{\hbar }{i}\mathbf{1}\) could not be applied to his pair of variables due to the discrete spectrum of eigenvalues. He then essentially went over to the Weyl form of the operators p, q in order to “save” his argument [222].“[…] all possible values of this quantity [x^{5}] still remain completely undetermined such that all its possible values from inf to +inf are of equal probability.”
Here α^{ b } is the set of Dirac numbers defined by α_{ (a }α^{ b) }=g^{ ab }, (α)^{ a }α^{ b })α^{ c }=α^{ a }(α^{ b }α^{ c }) with a, b, c = 0, … , 4, and ∇_{ b } the covariant spinor derivative defined by him.The Dirac equations for Riemannian spacetime with electromagnetic field and mass can be written in the form of equations without field or mass \({\alpha ^b}{\nabla _b}\psi = 0\) in an R_{5}.
“The following deductions are intended to show […] that the unifying combination of the gravitational and the electromagnetic fields, by projective differential geometry with the aid of five homogeneous coordinates, is a general method whose range reaches beyond classical fieldphysics and into quantum theory. Perhaps, the hope is not unjustified that the method will stand the test as a general framework for the laws of physics also with regard to a future physical and conceptual improvement of the foundations of Dirac’s theory.”^{296} ([250], pp. 837–838)
“more provisional character of his 5dimensionalprojective form of Dirac’s theory. […] In contrast to the joinder of the gravitational and electromagnetic fields, a direct logical coupling of the matterwavefield with these has not been achieved in the form of the theory developed here.”
7.3 Einstein, spinors, and semivectors
In this first publication on the subject, Einstein and Mayer explicitly referred to the paper by Infeld and van der Waerden, of which they had received a copy several months before publication ([167], and [110], p. 25, footnote). Apparently, Einstein found the reconstruction of the spinor concept in his paper more “clear and natural” than Infeld and van der Waerden’s. Nevertheless, the approach and notation of Infeld and van der Waerden became the accepted one by physicists.“In spite of the great importance which the spinor concept, as introduced by P a u l i and D i r a c, has obtained in molecular physics, one cannot claim that the analysis of this concept up to now satisfies all justified demands. Our efforts have lead to a derivation corresponding, according to our opinion, to all demands for clarity and naturalness and avoiding completely any not so transparent artifice. Thereby, […] the introduction of novel quantities was shown to be necessary, the ‘semivectors’, which include spinors but possess a clearly more transparent transformation character than spinors.”^{299} ([110], p. 522)
“I work with my Dr. Mayer on the theory of spinors. We already could clear up the mathematical relations. A grasp on the physics is far away, farther than one thinks at present. In particular, I still am convinced that the attempt at an essentially statistical theory will fail.”^{300} ([99], p. 291)
“Scientifically Mayer and I have found one very natural generalisation of Dirac’s equation which makes it comprehensible, that there are two understandable elementary masses, while there is only one electric charge.” [69]
In the first paper in the reports of the Berlin Academy, the mathematical foundations of the semivector formalism are developed [110]. The basic idea of Einstein and Mayer is the possibility of a decomposition of any (proper) Lorentz transformation described by a real matrix D into a product BC of a pair of complexconjugate, commuting matrices^{301} B and C. The transformations represented by B or C form a group isomorphic to the Lorentz group. In terms of infinitesimal Lorentz transformations given by an antisymmetric tensor ω_{ ik }, this amounts to the decomposition into a selfdual and an antiselfdual part: \({\omega _{ik}} = \tfrac{1}{2}\left( {{\omega _{ik}} + i\omega _{ik}^*} \right) + \tfrac{1}{2}\left( {{\omega _{ik}}  i\omega _{ik}^*} \right)\), with the dual^{302} defined by \(\omega _{ik}^*: = \tfrac{1}{2}\sqrt g { \epsilon _{ijkl}}\;{\omega ^{kl}}\).
Thus it can be used for raising and lowering indices of semivectors ([110], p. 535).“the metric tensor g_{ ik } is also a semivector of 1st kind (and of 2nd kind) with transformationinvariant components.”
In his “Spencer Lecture” of 10 June 1933 in Oxford, Einstein embedded his point of view into the development of field theory: “[…] Louis de Broglie guessed the existence of a wave field that could be used for the interpretation of certain quantum properties of matter. With the spinors, Dirac found novel field quantities whose simplest equations permitted the derivation of the properties of the electron to a great extent. With my collaborator, Dr. Walther Mayer, I now found that these spinors form a special case of a type of field, linked to fourdimensional space, which we called ‘semivectors’. The simplest equations to be satisfied by such semivectors provide a key for the understanding of the existence of two elementary particles with different ponderable mass and like, but opposite, charge. These semivectors are, besides the usual vectors, the simplest mathematical fieldobjects possible in a fourdimensional metrical continuum; it appears that they naturally describe essential properties of the electrical elementary particles.”^{304} ([100], p. 117)
In a previous paper, Schouten had geometrically explained the two approaches to spinor analysis followed by van der Waerden [368], Laporte and Uhlenbeck [203], and by himself. In the first approach, the vectors of the two invariant planes in spin space were identified; in the second, i.e., in Schouten’s, they were taken as the basis for a fourdimensional vector space [308]. Schouten had been corresponding with Pauli who “was so friendly as to allow me to quote this theorem from a not yet published manuscript.”^{306} In his second paper, Schouten placed the semivectors of Einstein and Mayer into his geometrical setting. He showed that there exist two different complexconjugated threedimensional representations of the real Lorentz group as a 6parameter subgroup of the fourdimensional orthogonal group. With the help of these he constructed four “building blocks: the special spin vectors of 1st and 2nd kind of spin space, which at the same time are special semivectors in the two preferred invariant planes in semispace. In both cases, always two vectors are joined which belong to different invariant planes, for semivectors two with same transformation law, for spin vectors two with conjugate complex transformations.” ([309], p. 106)“The space of semivectors of first and second kind is the manifold of two simple bivectors in the local spacetimeworld, which lie on the null cone in two planes of the first and second system of planes, respectively. […] In the notprojective theory as well as in the projective without an electromagnetic field, semivectors have an advantage, […]. As soon as an electromagnetic field is present, in the projective theory, calculation with spinvectors is simpler than calculation with semivectors.”^{305} [309]
and that the generalised Dirac equations of Einstein and Mayer (206)“to each semivector two 2component spinors correspond, which both satisfy the same transformation law.” ([7], p. 68)
This means that only one of these two systems is needed, and that it describes particles with opposite charge and the same mass. Thus, as van Dongen states curtly:“decompose into two separate 4component systems of Dirac’s type, which are distinguished only by the mass values.” ([7], p. 78)
“It is evident from Bargmann’s analysis that the most general semivector Dirac system of Einstein and Mayer is nothing more than just a linear superposition of two independent Dirac spinor systems and thus cannot give insight into the fundamental nature of electrons and protons.” ([371], p. 88, and [372])
In his letter to Einstein, Pauli had also mentioned his papers to be published in Annalen der Physik and discussed here in Section 7.2.3. Two more papers were written by Einstein and Mayer before Einstein quietly dropped the subject. The last paper considered semivectors as “usual vectors with a different differentiation character” [112, 113].
Of course, Einstein’s problem was quickly solved; at about the same time the electron’s antiparticle was observed.“Without further hypothesis the existence follows of particles with opposite charge and same rest mass, which can be produced or annihilated by absorption or emission of electromagnetic radiation. The frequency of these processes is shown to be of the same magnitude as the one for particles with the same charge and mass following from Dirac’s hole theory.”^{310} ([255], Abstract)
8 Less Than Unification
“to the consideration of the small oscillations of the proton and single electron forming the hydrogen atom.” [18, 17].
The unidentified parts in the decomposition of the Ricci tensor into its piece in V_{3} and the rest Rumer ascribed to “matter.” He acknowledged Born’s“We have seen that the V_{3} itself is either an F_{3} (in this case it is empty), or a subspace of an F_{4} (thus it contains a gravitational field), or a subspace of F_{5} (then also an electrical field is present). In the case in which ‘something’ exists which is neither a gravitational nor an electrical field, the V_{3} must be a subspace of F_{ n } (n≥6). However, geometry shows that every V_{3} is a subspace of a particular F_{6}, i.e., the Euclidean or pseudoEuclidean space. This shows us that transition to F_{6} is the final step.”^{311} ([285], p. 277)
^{312} Born himself was mildly skeptical^{313}:“[…] stimulation and his interest extended toward the completion of this paper.”
“[…] a young Russian surfaced here who brought with him a 6dimensional relativity theory. As I already felt frightened by the various 5dimensional theories, and had little confidence that something beautiful would result in this way, I was very skeptical.”^{314}
For his Lagrangian, he took \({\mathcal L} = {R_{ik}}{R^{ik}} + C{({R^k}_k)^2}\), with C being a constant. He first varied with respect to the metric g_{ ik } and the Ricci tensor R_{ ik } as independent variables, and then expressed the variation δR_{ ik } with δg_{ ij }. The resulting variation is then set equal to zero. In the process “spontaneously” a“[…] the basic properties of the electromagnetic field may be derived effortlessly from the general properties of Riemannian geometry by use of a variational principle characterised by a very natural demand.”^{315} ([202], p. 168)
“free vector appears for which, later, a restraining equation of the type of the equation for the [electromagnetic] potential results — as a consequence of the conservation laws for energy and momentum.”
“The only criterion for a unified field theory that these equations do not satisfy is that they are not derived from a variational principle by means of a Lagrange’s function involving geometric quantities alone.” ([422], p. 397)
This meant turning upside down Einstein’s geometrization program for matter.“metric should turn out finally to be a system of some statistical mean values of certain physical quantities.” ([363], p. 522)
9 Mutual Influences Among Mathematicians and Physicists?
A most interesting task far beyond this review would be to reconstruct, in detail, the mutual influences among researchers in the development of the various strands of unified field theory. An interesting indepthstudy for the case of Weyl has already been made [326].
Einstein is mentioned as the only theoretical physicist among seven mathematicians. The development of projective geometry did profit from the mathematician Kaluza’s idea of a fivedimensional space as the arena for unified field theory. It enticed physicists such as Pauli, O. Klein, Mandel, Fock, Infeld, and inspired mathematicians such as Veblen, Schouten, van Dantzig, Cartan, and others.“In recent years, due to their use in modern physical theories, the theory of differential forms (tensors) was elaborated extensively. We mention Ricci, LeviCivita, Hessenberg, Einstein, Hilbert, [Felix] Klein, E. Noether, Weyl.”^{317} [392]
we note that he had intensive contact with Berwald in Prague. Later, while working on spinors, Schouten interacted with Veblen in Princeton, such that the latter referred to him:“I owe thanks to Mr. L. Berwald in Prague, with whom I had an intensive exchange of ideas from September 1921, and who was so friendly as to give me his manuscripts before they went into print.”^{318} [299]
“[This note] suggested itself as a possible basis for a geometrical interpretation of Eddington’s theory of the interaction of electric charges [61] and was proposed to Prof. Schouten during his visit to America as a possible geometrical interpretation of the theory of spinquantities which he was then developing.” ([306]; Schouten had Hlavaty as a coauthor [312])
and“Mr. Pauli was so friendly as to permit me to quote this theorem from an unpublished manuscript.”^{319} ([308], p. 406, footnote 4)
We also noticed in Section 5 that Schouten wrote his papers on the classification of linear connections [297, 296] with the explicit intention of attracting readers from physics.“A correspondence with Mr. Pauli induced me to investigate this invariance.”^{320} ([308], p. 414, footnote 1)
On the one hand, Einstein must have been best informed by receiving papers, books, and the latest news, or even visits from many of his active colleagues. On the other, he rarely referred to these papers and books; as far as I am aware his extended correspondence included Eisenhart, Eddington, Kaluza, Mandel, Pauli, Veblen, A. Wenzl, Weyl, and Zaycoff, but not Schouten, J. M. Thomas, T. Y. Thomas, O. Klein, not to speak of Reichenbächer. In terms of his scientific output in the area of unified field theory, a more precise description of the balance between Einstein’s being at the receiving end and his stimulating and creative role will have to be given in the future.
10 Public Reception of Unified Field Theory at the Time
After Pauli’s handbook article, Weyl hardly could have been overlooked. Nevertheless, the 2nd volume of Laue’s book did not even mention Weyl’s theory, nor did LeviCivita’s book in its English or German versions of 1927 and 1928 [387, 205]. In contrast, Schouten’s and Eddington’s monographs treated Weyl extensively [300, 60]. Already in 1921, Fabre’s weak presentation of “Les théories d’Einstein” [125] had an admiring but irrelevant appendix on Weyl’s unified field theory, while, in 1922, J. Becquerel in Paris and E. Neumann in Marburg in their books on relativity had brief presentations of Weyl’s theory [236, 10]. One or the other philosopher of science took into account some of the developments, mostly Weyl’s theory, as did Reichenbach in 1928 [267]. In his book on “The present world view according to the natural sciences”, Wenzl discussed Einstein’s theory of distant parallelism but cautioned that this theory, as a physical theory was not on the same level as general relativity: It seemed unclear whether the new theory would predict new phenomena that could be empirically tested [394].“Hilbert, Klein [i.e., Felix Klein] and other mathematicians have taken part, have researched in depth and illuminated the formal structure of Einstein’s formulas.”^{321} ([20], p. 248)
Also, from 1930, Einstein’s yearly travels to the United States and his sojourns there brought about increased publicity for his research on unified field theory. Thus, a “preliminary announcement for the Josiah Macy, Jr., Foundation” of his paper with his assistant Mayer on the 5vector formulation of Kaluza’s theory [107] was printed in full in Science about a month before the publication appeared [94]. However, it seems safe to say that reports on Einstein’s newest unified field theory in the dailies, whether seen as an educational affair or as part of entertainment, must have strained the general public’s intellectual abilities.“[…] the typhoon of publicity crossed the Atlantic. From that point on, the American press played Einstein to the maximum.” ([42], p. 28)
11 Conclusion
Even a superficial survey such as the one made here shows clearly the dense net of mathematicians and theoretical physicists involved in the building of unified field theory and of the geometric structures underlying it. Mathematician Grossmann introduced physicist Einstein into Ricci’s calculus; Einstein influenced many mathematicians such as Hessenberg, Weyl, Schouten, Struik, Cartan, Eisenhart, and Veblen, to name a few. In return, some very influential ideas on Einstein’s path within unified field theories came from these mathematicians: Förster’s asymmetric metric^{322}, Cartan’s distant parallelism, Kaluza’s fivedimensional space, Weyl’s, Schouten’s, and Cartan’s completely general concept of connection, Veblen’s projective formulation.
This may be true, but in a sense possibly not intended by Vizgin. First, Einstein could lead only those few unaffected by the main new topic of theoretical physics at the time: quantum theory. Second, Einstein’s importance consisted in having been the central identification figure in a scientific enterprise within theoretical physics which, without his weight, fame, and obstinacy, would have been dwindling to an interesting specialty in differential geometry and become a dead end for physicists. It is interesting, though, to note how uncritically Einstein’s zigzagging path through the wealth of constructive possibilities was followed by many in the (small) body of researchers in the field.“became the recognised leader of the investigations [in unified field theory], taking over, as it were, the baton from Weyl, who had been the leading authority for the previous five years.” ([385], p. 183)
“One can see […] the variety of aspects by which unified field theory may be envisaged, and also the difficulty of the problems arising from it. But Mr. Einstein is not one of those afraid of difficulties; even if his attempt does not succeed, it will have forced us to think about the great questions at the foundation of science.”^{324} ([36], p. 1184/1185)
“At present, this new theory is nothing but a mathematical construct barely connected to physical reality by very loose cords. It has been discovered by exclusively formal considerations, and its mathematical consequences have not yet been developed sufficiently for allowing a comparison with experiment. Nevertheless, to me this attempt seems very interesting in itself; it mainly offers splendid possibilities for the [further] development, and it is with the hope that the mathematicians get interested in it that I permit myself to expose and analyse [the theory] here.”^{325} ([92], p. 1)
It may also be that general relativity, his great and lasting success in dealing with gravitation, was misleading him. In a report about his teleparallel geometry, after having described “the derivation of the complicated field law of gravitation along a logical path,” Einstein went on to say:“[…], in the end experience is the only competent judge. Yet in the meantime one thing may be said in defence of the theory. Advances in scientific knowledge must bring about the result that an increase in formal simplicity can only be won at the cost of an increased distance or gap between the fundamental hypotheses of the theory on the one hand, and the directly observed facts on the other. Theory is compelled more and more from the inductive to the deductive method, even though the most important demand to be made of every scientific theory will always remain that it must fit the facts.” ([86], pp. 114–115)
“The successful attempt to derive delicate laws of nature, along a purely mental path, by following a belief in the formal unity of the structure of reality, encourages continuation in this speculative direction, the dangers of which everyone vividly must keep in sight who dares follow it.”^{327} [87]
“This looks oldfashioned, and the dear colleagues and also you, my dear, will show me the tongue as long as they can. Because Planck’s h is not showing up in the equations. But if the limit is clearly reached of what the statistical fad can achieve they will again return full of repentance to the spacetime picture, and then these equations will form a starting point.”^{328} ([99], p. 240)
“In the present situation, neither from classical nor from quantum mechanical methods alone ‘all’ can be expected; rather, it suits us to adopt the opinion, voiced several times, that the field problem must be carried further on classical ground before it may present new anchor points for quantum mechanics. Seen precisely from this angle, it is regrettable that after these broad designs, such as the ones available in gauge theory and distant parallelism, no further attempts in the classical direction can be noticed.”^{330} ([239], p. 683)
It might be an interesting task to confront the methodology that helped Einstein to arrive at general relativity with the one used by him within unified field theory. (See the contributions of J. Renn, J. Norton, M. Janssen, T. Sauer, M. Schemmel, et al. originating from their work on Einstein’s Zürich notebook of 1912 [279, 280].) If it is the same, then it might become harder to draw general conclusions as to its importance for the gain in and development of knowledge in physics.
A report on the rich further development of the field past 1933 will be given in Part II of this review.
Footnotes
 1.
Albert Einstein (1879–1955). Born in Ulm, Württemberg (Germany). Studied physics and mathematics at the Swiss Federal Polytechnic School (ETH) Zurich and received his doctor’s degree in 1905. Lecturer at the University of Bern (Switzerland), Professor in Zurich, Prague (then belonging to Austria), Berlin (Germany) and Princeton (U.S.A.). Nobel Prize 1921 for his work on the lightelectric effect (photon concept). Best known for his special and general relativity theories. Important results in Brownian motion and the statistical foundations of radiation as a quantum phenomenon. Worked for more than 30 years on Unified Field Theory.
 2.
Wolfgang Ernst Pauli (1900–1958). Born in Vienna, Austria. Studied at the University of Munich with A. Sommerfeld who recognised his great gifts. Received his doctorate in 1921 for a thesis on the quantum theory of ionised molecular hydrogen. From October 1921 assistant of Max Born in Göttingen. After a year with Bohr, Pauli, became a lecturer at the University of Hamburg in 1923. In 1928 he was appointed professor of theoretical physics at the Federal Institute of Technology in Zürich. From 1945–1950 guest professor at the Institute for Advanced Study, Princeton. He then returned to Zürich. Did important work in quantum mechanics, quantum field theory and elementary particle theory (fourth quantum number (spin), Pauli exclusion principle, prediction of neutrino). Fellow of the Royal Society. Nobel Prize winner in 1954.
 3.
Vizgin’s book is the only one that covers the gamut of approaches during the period considered. Fortunately, he has made accessible contributions in the Russian language by scientists in the Soviet Union. Vizgin also presents and discusses attempts at unification prior to 1914.
 4.
The inclusion of the quantum corresponds to Vizgin’s maximal unification problem [385], p. 169.
 5.
See Section 1 of Vizgin’s book [385] for a treatment of the history of prerelativistic unified field theories and an exposition of Mie’s, Ishiwara’s, and Nordström’s approaches.
 6.
In presentday interpretation, the first two fields are fields mediating the interactions while the third, the electron field, really is a matter field.
 7.
This definition corresponds, in a geometrical framework, to Vizgin’s minimal unification problem ([385], p. 187).
 8.
Theodor Franz Eduard Kaluza (1885–1954). Born in Ratibor, Germany (now Raciborz, Poland). Studied mathematics at the University of K’nigsberg (now Kaliningrad, Russia) and became a lecturer there in 1910. In 1929 he received a professorship at the University of Kiel, and in 1935 was made full professor at the University of Göttingen. He wrote only a handful of mathematical papers and a textbook on “Higher mathematics for the practician” (cf. [423]).
 9.
“Eine Hoffnung ist aber nicht in Erfüllung gegangen. Ich dachte, wenn es gelingt, dieses Gesetz aufzustellen, dass es eine brauchbare Theorie der Quanten und Materie bilden würde. Aber das ist nicht der Fall. Die Konstruktion scheint am Problem der Materie und der Quanten zu scheitern.”
 10.
Jan Arnoldus Schouten (1883–1971). Born near Amsterdam in the Netherlands. Studied electrical engineering at the Technical University (Hogeschool) of Delft and then mathematics at the University of Leiden. His doctoral thesis of 1914 was on tensor analysis, a topic he worked on during his entire academic career. From 1914 until 1943 he held a professorship in mathematics at the University of Delft, and from 1948 to 1953 he was director of the Mathematical Research Centre at the University of Amsterdam. He was a prolific writer, applying tensor analysis to Lie groups, general relativity, unified field theory, and differential equations.
 11.
“[…] Anhäufungen von positiver und negativer Elektrizität, die wir in den positiven Wasserstoffkernen und in den negativen Elektronen antreffen. Die ältere Maxwellsche Theorie erklärt diese Anhäufungen nicht, aber auch den neueren Bestrebungen ist es bisher nicht gelungen, diese Anhäufungen als selbstverständliche Folgen der zugrundeliegenden Differentialgleichungen zu erkennen. Sollte aber eine solche Erklärung gefunden werden, so darf man vielleicht auch hoffen, dass die […] mysteriösen Quantenbahnen in ein neues Licht gerückt werden.”
 12.
It is true that Dirac, in his first paper, in contrast to what his “hole”theory implied, had identified the positively charged particle corresponding to the electron also with the proton [55]. However, after Weyl had pointed out that Dirac’s hole theory led to equal masses [409], he changed his mind and gave the new particle the same mass as the electron [56].
 13.
Cornelius Lanczos (Kornél Löwy) (1893–1974). Born in Székesfehérvár (Hungary). Studied physics and mathematics at the University of Budapest with Eötvös, Fejér, and Lax. Received his doctorate in 1921, became scientific assistant at the University of Freiburg (Germany) and lecturer at the University of Frankfurt am Main (Germany). Worked with Einstein in Berlin 1928–1929, then returned to Frankurt. Became a visiting professor at Purdue University in 1931 and came back on a professorship in 1932. Worked mainly in mathematical physics and numerical analysis. After 1944 he held various posts in industry and in the National Bureau of Standards. Left the U.S.A. during the McCarthy era and in 1952 followed an invitation by Schrödinger to become head of the Theoretical Physics Department of the Dublin Institute for Advanced Study.
 14.
“Ich glaube darum, dass zwischen dem hier vertretenen ‘reactionären Standpunkt’, der eine vollständige feldtheoretische Beschreibung auf Grund der normalen RaumZeitStruktur erstrebt, und dem wahrscheinlichkeitstheoretischen (statistischen) Standpunkt ein Kompromiss […] nicht mehr möglich ist.”
 15.
“Sollten sich die hier vorausgeahnten Möglichkeiten als wirklich lebensfähig erweisen, so würde die Quantenmechanik aufhören, eine selbständige Disziplin zu sein. Sie würde verschmelzen mit einer vertieften ‘Theorie der Materie’, die auf reguläre Lösungen von nichtlinearen Differentialgleichungen aufzubauen hätte, — in letztem Zusammenhang also aufgehen in den ‘Weltgleichungen’ des Universums. Der Dualismus ‘MaterieFeld’ würde dann ebenso überwunden sein, wie der Dualismus ‘KorpuskelWelle’.”
 16.
David van Dantzig (1900–1959). Born in Rotterdam, Netherlands. Studied mathematics at the University of Amsterdam. Worked first on differential geometry, electrodynamics and unified field theory. Known as cofounder, in 1946, of the Mathematical Centre in Amsterdam and by his role in establishing mathematical statistics as a subdiscipline in the Netherlands.
 17.
Thus, in a paper of 1934 really belonging to the 2nd part of this review, Schouten and Haantjes exchanged the previously assigned “induced geodesic lines” for “autogeodesical lines” [311].
 18.
Ernst Reichenbächer (1881–1944). Studied mathematics and received his doctorate from the University of Halle in 1903 under the guidance of AlbertWangerin (a student of Franz Neumann in Königsberg). At first, Reichenbächer did not enter an academic career, but started teaching in a Gymnasium in Wilhelmshaven in North Germany, then in Königsberg on the Baltic Sea. In 1929 he became a Privatdozent (lecturer) at the University of Königsberg (now Kaliningrad, Russia). His courses covered special and general relativity, the physics of fixed stars and galaxies with a touch on cosmology, and quantum mechanics. In the fifth year of World War II he finally received the title of professor at the University Königsberg, but in the same year was killed during a bombing raid on the city.
 19.
Hermann Klaus Hugo Weyl (1885–1955). Born in Elmshorn, Germany. Studied at the Universities of Munich and Göttingen where he received his doctorate in 1908 (Hilbert was his supervisor). From 1913 he held the Chair of Mathematics at the Federal Institute of Technology in Zürich, and from 1930 to 1933 a corresponding Chair at the University of Göttingen. Then until retirement he worked at the Institute for Advanced Study in Princeton. Weyl made important contributions in mathematics (integral equations, Riemannian surfaces, continuous groups, analytic number theory) and theoretical physics (differential geometry, unified field theory, gauge theory). For his papers, cf. also the Collected Works [411]
 20.
Arthur Stanley Eddington (1882–1944). Born in Kendal, England. Studied mathematics at Owens College, Manchester and Trinity College, Cambridge. After some work in physics, moved into astronomy in 1905 and was appointed to the Royal Observatory at Greenwich. From 1914 director of the Cambridge Observatory. Fellow of the Royal Society. As a Quaker he became a conscientious objector to military service during the First World War. Eddington made important contributions to general relativity and astrophysics (internal structure of stars). In 1918, he led an eclipse expedition from which the first indications resulted that Einstein’s general relativity theory was correct. Wrote also on epistemology and the philosophy of science.
 21.
Oskar Klein (1894–197). Born in Mörby, Sweden. After work with Arrhenius in physical chemistry, he met Kramers, then a student of Bohr, in 1917. Klein worked with Bohr in the field of molecular physics and received his doctorate in 1921 at Stockholm Högskola. His first research position was at the University of Michigan in Ann Arbor, where he worked on the Zeeman effect. Back in Europe from 1925, he taught at Lund University and tried to connect Kaluza’s work with quantum theory. In 1930 he became professor for mathematical physics at Stockholm Högskola until retirement. His later work included quantum theory (KleinNishina formula), superconductivity, and cosmology.
 22.
Luther Pfahler Eisenhart (1876–1965). Born in York, Pennsylvania, U.S.A. Studied mathematics at John Hopkins University, Baltimore and received his doctorate in 1900. Eisenhart taught at the University of Princeton from 1900, was promoted to professor in 1909 and remained there (as Dean of the mathematical Faculty and Dean of the Graduate School) until his retirement in 1945. All his work is in differential geometry, including Riemannian and nonRiemannian geometry and in group theory.
 23.
Oswald Veblen (1880–1960). Born in Decorah, Iowa, U.S.A. Entered the University of Iowa in 1894, receiving his B.A. in 1898. He obtained his doctorate from the University of Chicago on “a system of axioms in geometry” in 1903. He taught mathematics at Princeton (1905–1932), at Oxford in 1928–1929, and became a professor at the Institute for Advanced Study in Princeton in 1932. Veblen made important contribution to projective and differential geometry, and to topology. He gave a new treatment of spin.
 24.
Elie Joseph Cartan (1869–1951). Born in Dolomien near Chambéry, France. Student at l’École Normale since 1888, he received his Ph.D. in 1894 with a thesis in which he completed Killing’s classification of semisimple algebras. He lectured at Montpellier (1894–1903), Lyon (1896–1903), Nancy (1903–1909), and Paris (1909–1940). His following work on the representation of semisimple Lie groups combines group theory, classical geometry, differential geometry, and topology. From 1904 he worked on differential equations and differential geometry, and developed a theory of moving frames (calculus of differential forms). He also contributed to the geometry of symmetric spaces and published on general relativity and its geometric extensions as well as on the theory of spinors. For his Collected Works, cf. [38].
 25.
Dirk J. Struik (1894–2000). Born in Rotterdam in the Netherlands. Studied mathematics and physics at the University of Leiden with Lorentz and de Sitter. Received his doctorate in 1922. Then worked with Schouten at the University of Delft and, with a Rockefeller International Education Fellowship, moved to Rome and Göttingen. After a collaboration with Wiener, in 1926 he received a lectureship at the Massachusetts Institute of Technology (MIT) in Cambridge, Ma. where he became full professor in 1940. He stayed on the MIT mathematics faculty until 1960. As a professed Marxist he was suspended from teaching duties during the McCarthy period but was reinstated in 1956. In 1972, he became an honorary research associate in the History of Science Department of Harvard University.
 26.
for the following, it is assumed that readers have some prior knowledge of the mathematics underlying General Relativity.
 27.
for the precise definition of “geometrical object”, cf. Yano’s book [425].
 28.
The second fundamental form comes into play when local isometric embedding is considered, i.e., when .... is taken as a submanifold of a larger space such that the metrical relationships are conserved. In the following, all geometrical objects are supposed to be differentiable as often as is needed.
 29.
Here, the Kroneckersymbol δ^{ i }_{ k } with value +1 for i=k, and value 0 for i≠k is used. δ^{ i }_{ k } keeps its components unchanged under arbitrary coordinate transformations.
 30.
Latin indices i, j, k, … run from 1 to D, or from 0 to D−1 to point to the single timelike direction. We have used the symmetrisation bracket defined by \({A_{(ij)}}: = 1/2({A_{ij}} + {A_{ji}})\).
 31.
In physical applications, special conditions for γ and φ might be needed in order to guarantee that g is a Lorentz metric.
 32.
 33.
We have \({({L_X}Y)^k}: = {([X,Y])^k} = {X^i}{\partial _i}{Y^k}  {Y^i}{\partial _i}{X^k}\).
 34.
Eisenhart called his object “ennuple” instead of nbein [119]. In French, the expressions “npode”, “nèdre”, and “polyaxe á n dimensions” were also used.
 35.
In an arbitrary basis for the differential forms (cotangent space), the connection may be represented by a 1form.
 36.
In the literature, different notations and conventions are used. Tonnelat [356] writes \({A_{\mathop k\limits_ + ;j}}: = {A_{k,j}}  {L_{kj}}^l{A_l}\) and \({A_{\mathop {{\rm{ }}k}\limits_  ;j}}: = {A_{k,j}}  {L_{jk}}^l{A_l}\).
 37.
Many authors replace “autoparallel” by “geodesic”. We will reserve the name geodesic for curves of extreme length; cf. Riemannian geometry.
 38.
In the following we will note a symmetrical connection by \({\Gamma _{ij}}^k = {L_{(ij)}}^k\).
 39.
Schouten denotes the curvature tensor by \({K_{jkl}}^i\).
 40.
Again, we have two kinds of homothetic curvatures deriving from \(\mathop K\limits^ +\) and \(\mathop K\limits^ \). In the following, we will mostly use the \(\mathop X\limits^ +\)quantities and drop the + sign.
 41.for a threeindextensor the symmetrisation bracket is defined by$$ {A_{(ikl)}}: = \frac{1}{{3!}}({A_{ikl}} + {A_{lik}} + {A_{kli}} + {A_{kil}} + {A_{lki}} + {A_{ilk}}). $$
 42.
 43.
Tullio LeviCivita (1873–1941). Born in Padua, Italy. Studied mathematics and received his doctorate at the University of Padua. Was given the Chair of Mechanics there and, in 1918, went to the University of Rome in the same position. Together with Ricci, he developed tensor calculus and introduced covariant differentiation. He worked also in the mechanical manybody problem, in hydrodynamics, general relativity theory, and unified field theory. Strongly opposed to Fascism in Italy and dismissed from his professorship in 1938.
 44.
This definition differs from Schouten’s by an overall minus sign.
 45.
See [157]; his sign conventions are different, though.
 46.In the case of an asymmetric metric, this relation must be satisfied separately by the symmetric and antisymmetric parts of g:$$ \begin{array}{*{20}{c}} {{\nabla _k}{h_{ij}} = 0,\;\;\;}&{{\nabla _k}{\phi _{ij}} = 0.} \end{array} $$
 47.
Joseph Miller Thomas (1898–1979). Studied mathematics in Philadelphia at the University of Pennsylvania. Received his doctorate in 1923. From 1927 assistant professor at the University of Pennsylvania, from 1930 assistant and in 1935 full professor of mathematics at the Duke University in Durham, North Carolina. His fields were differential geometry and partial differential equations. He was the principle founder of Duke Mathematical Journal.
 48.
The index 0 does not refer to a timecoordinate.
 49.
Note that \({X^\alpha }\) and \(\lambda {X^\alpha }\) correspond to the same point of M_{ D }; Veblen uses \(\lambda = \exp (N{x^0})\) (see [379], Section II).
 50.
For an asymmetric connection, this corresponds to the + derivative.
 51.The external derivative d of linear forms ω, μ satisfies the following rules:
 (1)
\(d(a\omega + b\mu ) = ad\omega + bd\mu\),
 (2)
\(d(\omega \wedge \mu ) = d\omega \wedge \mu  \omega \wedge d\mu\),
 (3)
ddω=0.
 (1)
 52.
A representation of a group is defined as a map to the vectors of a linear space that is homomorphic in the group operation.
 53.
The full Lorentz group contains as further elements the temporal and spatial reflections.
 54.
\({\mathbf{X}^ + }_{AB} = {\mathbf{X}_{BA}};A,B = 1,2\).
 55.
2component spinors are also called Weylspinors.
 56.
For a contemporary exposition of the use of spinors in spacetime, see the book of Penrose and Rindler [256].
 57.
In the early papers on general relativity, Equation (96) was called a “conservation law” because, in Minkowski space, it implies the conservation laws for energy and linear momentum. For an arbitrary Riemannian manifold this no longer holds true.
 58.
Förster published under a nom de plume “R. Bach” because his employer Krupp did not like his employees using their free time on something as academical as research in gravitation and unified field theory. Bach wrote also about Weyl’s theory (Bach 1921) [4].
 59.
“Vielleicht findet sich ein kovarianter Sechservektor der das Auftreten der Elektrizität erklärt und ungezwungen aus den \({g_{\mu \nu }}\) herauskommt, nicht als fremdes Element herangetragen wird.”
 60.
“Das Ziel, Gravitation und Elektromagnetismus einheitlich zu behandeln, indem man beide Phänomengruppen auf die \({g_{\mu \nu }}\) zurückführt, hat mir schon viele erfolglose Bemühungen gekostet. Vielleicht sind Sie glücklicher im Suchen. Ich bin fest überzeugt, dass letzten Endes alle Feldgrössen sich als wesensgleich herausstellen werden. Aber leichter ist ahnen als finden.”
 61.
“Das Ausgehen von einem nichtsymmetrischen \({g_{\mu \nu }}\) hat mich auch schon lange beschäftigt; ich habe aber die Hoffnung aufgegeben, auf diese Weise hinter das Geheimnis der Einheit (Gravitation.Elektromagnetismus) zu kommen. Verschiedene Gründe flössen da schwere Bedenken ein: […] Ihre übrigen Bemerkungen sind ebenfalls an sich interessant und mir neu.”
 62.
In his textbook, M. von Laue presented and discussed Mie’s theory [387].
 63.
“In Folge eines allgem. math. Satzes erscheinen die elektrody. Gl. (verallgemeinerte Maxwellsche) als math. Folge der Gravitationsgl., so dass Gravitation und Elektrodynamik eigentlich garnicht verschiedenes sind.”
 64.
See also the Diploma thesis by König [191]. In it it is shown that from the divergence relation \({T^{\mu \nu }}{;_\nu } = 0\) and the most general Lagrangian L(u, v) with \(u = {F_{\mu \nu }}{F^{\mu \nu }}andv = *{F_{\mu \nu }}{F^{\mu \nu }}\), the field equations follow only for the generic case of full rank of the electromagnetic field tensor \({F_{\mu \nu }}\).
 65.
“Ihre Untersuchung interessiert mich gewaltig, zumal ich mir oft schon das Gehirn zermartert habe, um eine Brücke zwischen Gravitation und Elektromagnetik zu schlagen. Die Andeutungen, welche Sie auf Ihren Karten geben, lassen das Grösste erwarten.”
 66.
Reichenbächer’s solution is a special case of a huge number of spherically symmetric solutions of R=0 given in Goenner and Havas 1980 [144]. Reichenbächer published 29 papers between 1917 and 1930.
 67.
“Die Störung, die durch die Elektronen erzeugt wird und uns also zur Annahme eines von dem gewöhnlichen abweichenden Weltkoordinatensystem zwingt, wird nun bekanntlich als der elektromagnetische Sechservektor aufgefasst.”
 68.
“Nun sind diese Gebilde ungeheure Anhäufungen von Energie auf kleinsten Räumen; daher werden sie gewaltige Raumkrümmungen, oder mit anderen Worten, Gravitationsfelder, in sich bergen. Der Gedanke liegt nahe, dass diese es sind, die die auseinanderstrebenden elektrischen Ladungen zusammenhalten.”
 69.
“Keiner der bisherigen Theorien des Elektrons, auch nicht der Einsteinschen (Einstein 1919 [70]) ist es bisher gelungen, das Problem der elektrischen Elementarquante befriedigend zu lösen, und es liegt nahe, nach einem tieferen Grund für diesen Miβerfolg zu suchen. Ich möchte nun diesen Grund darin suchen, daβ es überhaupt unstatthaft ist, das elektrische Feld im Innern des Elektrons als stetige Raumfunktion zu beschreiben. Die elektrische Feldstärke ist definiert als die Kraft auf einen geladenen Probekörper und, wenn es keine kleineren Probekörper gibt als das Elektron (bzw den NKern), scheint der Begriff der elektrischen Feldstärke in einem bestimmten Punkt im Innern des Elektrons, mit welchem alle Kontinuumstheorien operieren, eine leere, inhaltslose Fiktion zu sein, da es keine beliebig kleinen Maβstäbe gibt. Ich möchte deshalb Herrn Einstein fragen, ob er der Auffassung zustimmt, daβ man die Lösung des Problems der Materie nur von einer Modifikation unserer Vorstellungen vom Raum (vielleicht auch von der Zeit) und vom elektrischen Felde im Sinne des Atomismus erwarten darf, oder ob er die angeführten Bedenken nicht für stichhaltig hält und die Ansicht vertritt, daβ man an den Grundlagen der Kontinuumstheorie festhalten muβ.”
 70.
For the evolution of Einstein’s position visavis continuum theory and shortcomings of it, cf. J. Stachel [329].
 71.
“Mit fortschreitender Verfeinerung des wissenschaftlichen Begriffssystems wird die Art undWeise der Zuordnung der Begriffe von den Erlebnissen immer komplizierter. Hat man in einem gewissen Studium der Wissenschaft gesehen, daβ einem Begriff ein bestimmtes Erlebnis nicht mehr zugeordnet werden kann, so hat man die Wahl, ob man den Begriff fallen lassen oder ihn beibehalten will; in letzterem Fall ist man aber gezwungen, das System der Zuordnung der Begriffe zu den Erlebnissen durch ein komplizierteres zu ersetzen. Vor dieser Alternative sind wir auch hinsichtlich der Begriffe der zeitlichen und räumlichen Entfernung gestellt. Die Antwort kann nach meiner Ansicht nur nach Zweckmäβigkeitsgründen gegeben werden; wie sie ausfallen wird, erscheint mir zweifelhaft.”
 72.
“[…] dass man dem symmetrischen Tensor des Gravitationspotentials einen antisymmetrischen Tensor hinzufügte, der den Sechservektor des elektromagnetischen Feldes repräsentierte. Aber eine genauere Überlegung zeigt, dass man so zu keiner vernünftigen Weltfunktion kommt.”
 73.
“Endlich habe ich mich gründlich von der Mieschen Theorie losgemacht und bin zu einer anderen Stellung zum Problem der Materie gelangt. Die Feldphysik erscheint mir keineswegs mehr als der Schlüssel zu der Wirklichkeit; sondern das Feld, der Äther, ist mir nur noch der in sich selbst völlig kraftlose Übermittler der Wirkungen, die Materie aber eine jenseits des Feldes liegende und dessen Zustände verursachende Realität.”
 74.
“Die hier vertretene physikalische Interpretation der Geometrie (Kontinuumstheorie) versagt zwar bei ihrer unmittelbaren Anwendung auf Räume von submolekularer Grössenordnung. Einen Teil ihrer Bedeutung behält sie indessen auch noch den Fragen der Konstitution der Elementarteilchen gegenüber. Denn man kann versuchen, denjenigen Feldbegriffen […] auch dann physikalische Bedeutung zuzuschreiben, wenn es sich um die Beschreibung der elektrischen Elementarteilchen handelt, die die Materie konstituieren. Nur der Erfolg kann über die Berechtigung eines solchen Verfahrens entscheiden […].”
 75.
“Dans le programme qu’a esquissé M. Einstein dans ses deux conférences faites en novembre 1929 à l’institut Henri Poncaré, il voulait chercher les lois physiques dans les solutions sans singularité de ses equations, la matière et l’electricité n’existant donc qu’à l’état continu. Placonsnous sur le terrain choisi par lui, sans trop nous étonner de le voir suivre en apparence une voie opposée à celle suivi avec succès par les physiciens contemporains.”
 76.
“Machen wir keine weitere Voraussetzung, so bleiben die einzelnen Punkte der Mannigfaltigkeit in metrischer Hinsicht vollständig gegeneinander isoliert. Ein metrischer Zusammenhang von Punkt zu Punkt wird erst dann in sie hineingetragen, wenn ein Prinzip der Übertragung der Längeneinheit von einem Punkte P zu seinem unendlich benachbarten vorliegt.”
 77.
“Die Möglichkeit einer solchen ‘ferngeometrischen’ Vergleichung kann aber in einer reinen Infinitesimalgeometrie durchaus nicht zugestanden werden.”
 78.
“Wieder ist die Physik, heute die Feldphysik, auf dem Wege, die Gesamtheit der Naturerscheinungen auf ein einziges Naturgesetz zurückzuführen, ein Ziel, dem sie schon einmal, als die durch Newtons Principia begründete mechanische MassenpunktPhysik ihre Triumphe feierte, nahe zu sein. Doch ist auch heute dafür gesorgt, dass unsere Bäume nicht in den Himmel wachsen.”
 79.
“Ich bin verwegen genug, zu glauben, dass die Gesamtheit der physikalischen Erscheinungen sich aus einem einzigen universellen Weltgesetz von höchster mathematischer Einfachheit herleiten lässt.”
 80.
In order to distinguish it from the “coordinateweight” connected with relative tensors [27]. In his book, Weyl just uses the expression “weight”.
 81.
Roland Weitzenböck (1885–1955). Studied mathematics at the University of Vienna where he obtained his doctoral degree in 1910. Became a professional officer during the First World War. He obtained professorships in Graz and Vienna and, in 1921, at the University of Amsterdam. He specialised in the theory of invariants (cf. [156]).
 82.
 83.
“Diese Tage ist es mir, wie ich glaube, gelungen, Elektrizität und Gravitation aus einer gemeinsamen Quelle herzuleiten. Es ergibt sich ein völlig bestimmtes Wirkungsprinzip, das im elektrizitätsfreien Fall auf Ihre Gravitationsgleichungen führt, im gravitationsfreien dagegen Gleichungen ergibt, die in erster Näherung mit den Maxwellschen übereinstimmen. Im allgemeinsten Fall werden die Gleichungen allerdings 4. Ordnung.”
 84.
“Ihre Abhandlung ist gekommen. Es ist ein GenieStreich ersten Ranges. Allerdings war ich nicht imstande, meinen MassstabEinwand zu erledigen.”
 85.
“[…] scheint mir die Grundhypothese der Theorie leider nicht annehmbar, deren Tiefe und Kühnheit aber jeden Leser mit Bewunderung erfüllen muss.”
 86.
“Die plausibelste Annahme, die man über ein im statischen Feld ruhende Uhr machen kann, ist die, dass sie das Integral des so normierten [d. h. so wie in der Einsteinschen Theorie] ds misst; es bleibt in meiner wie in der Einsteinschen Theorie die Aufgabe^{1}, diese Tatsache aus einer explizit durchgeführten Dynamik abzuleiten.”
 87.
“[Weyl] würde sagen, Uhren und Massstäbe müssten erst als Lösungen auftreten; im Fundament der Theorie kommen sie nicht vor. Aber ich finde: Wenn das mit einer Uhr (bzw. einem Massstab) gemessene ds ein von der Vorgeschichte, dem Bau und dem Material Unabhängiges ist, so muss diese Invariante als solche auch in der Theorie eine ganz fundamentale Rolle spielen. Wenn aber die Art des wirklichen Naturgeschehens nicht so wäre, so gäbe es keine Spektrallinien und keine wohldefinierten chemischen Elemente. […] Jedenfalls bin ich mit Weyl überzeugt, dass Gravitation und Elektrizität zu einem Einheitlichen sich verbinden lassen müssen, nur glaube ich, dass die richtige Verbindung noch nicht gefunden ist.”
 88.
“Abgesehen von der Übereinstimmung mit der Wirklichkeit ist es jedenfalls eine grandiose Leistung des Gedanken.”
 89.
“Ihre Ablehnung der Theorie fällt für mich schwer ins Gewicht; […] Aber mein eigenes Hirn bewahrt noch den Glauben an sie. Und daran muss ich als Mathematiker durchaus festhalten: Meine Geometrie ist die wahre Nahegeometrie, dass Riemann nur auf den Spezialfall F_{ ik }=0 geriet, hat lediglich historische Gründe (Entstehung aus der Flächentheorie), keine sachlichen.”
 90.
“[Weyl’s] theoretischer Versuch, passt nicht zu der Thatsache, dass zwei ursprünglich kongruente feste Körper auch kongruent bleiben, unabhängig davon, welche Schicksale sie durchmachen. Insbesondere hat es keine Bedeutung, welcher Wert des Integrals \(\int {\phi _\nu }d{x_\nu }\) ihrer Weltlinie zukommt. Sonst würde es NatriumAtome und Elektronen in allen Grössen geben müssen. Wenn aber die relative Grösse starrer Körper von der Vorgeschichte unabhängig ist, dann gibt es einen messbaren Abstand zweier (benachbarter) Weltpunkte. Dann ist die Weylsche Grundannahme jedenfalls nicht richtig für das molekulare. Dafür, dass sie für das Gravitationsfeld zutreffe, spricht, soweit ich sehe, kein einziger physikalischer Grund. Dagegen aber spricht, dass die Feldgleichungen der Gravitation von vierter Ordnung werden, wofür die bisherige Erfahrung keinerlei Anhalts bietet […].”
 91.
“[…] durch Vorsetzen dieses Faktors wird dann doch sozusagen die absolute Normierung der Längeneinheit vollzogen.”
 92.
“Der Ausdruck Rg_{ ik }dx^{ i }dx^{ k } für die gemessene Länge ist aber, wenn man für R die Krümmungsinvariante nimmt, nach meiner Meinung keineswegs akzeptabel, weil R sehr abhängig ist von der materiellen Dichte. Eine ganz kleine Änderung des Messweges würde das Integral der Quadratzwurzel dieser Grösse sehr stark beeinflussen.”
 93.
“Natürlich weiss ich, dass der Zustand der Theorie, wie ich ihn hingestellt habe, ein nicht befriedigender ist, abgesehen davon, dass die Materie unerklärt bleibt. Die zusammenhanglose Nebeneinandersetzung der Gravitationsglieder, der elektromagnetischen Glieder und der λGlieder ist unleugbar ein Produkt der Resignation. […] Endlich muss es so herauskommen, dass man nicht Wirkungsdichten additiv aneinander kleben muss.”
 94.
“Was Sie da sagen, ist wirklich wundervoll. So wie Mie seiner konsequenten Elektrodynamik eine Gravitation angeklebt hatte, die nicht organisch mit jener zusammenhing, ebenso hat Einstein seiner konsequenten Gravitation eine Elektrodynamik (d.h. die gewöhliche Elektrodynamik) angeklebt, die mit jener nicht viel zu tun hatte. Sie stellen eine wirkliche Einheit her.”
 95.
“Man muss zu Tensoren übergehen die 4. Ordnung sind statt nur zweiter Ordnung, was eine weitgehende Unbestimmtheit der Theorie mit sich bringt, erstens weil es bedeutend mehr Gleichungen gibt, die in Betracht kommen, zweitens, weil die Lösungen mehr willkürliche Konstanten enthalten.”
 96.
In fact, from Equation (104) we obtain \(K = R + 3{Q_l}{Q^l} + 3Q_{;j}^j\).
 97.
“Ausserdem führt dies Theorie auf einheitliche Weise und zwingend zu dem kosmologischen Gliede, das bei Einstein nur eine ad hoc gemachte Annahme war […].”
 98.
Wilhelm Wirtinger (1865–1945). Born in Ybbs, Austria. Studied mathematics at the University of Vienna. Received his doctorate in 1887, and continued his studies at the Universities of Berlin and of Göttingen. From 1895 a full professor at the University of Vienna, but accepted professorship at University of Innsbruck, returning to Vienna only in 1905. Wrote an important paper on the general theta function and had an exceptional range in mathematics (function theory, algebra, number theory, plane geometry, theory of invariants).
 99.
In the same year, Wirtinger sent in a paper on relativity theory published only in 1922 [421].
 100.
Paul Dienes (1982–1952). Born in Tokaj, Hungary. Studied mathematics. From 1929–1945 Reader, and from 1945–48 Professor at Birkbeck College, University of London.
 101.
A detailed investigation of this subject will appear soon, and will be included in the next update of this article [145].
 102.
 103.
“Ich habe grossen Respekt vor der Schönheit und Kühnheit Ihrer Gedanken. Aber Sie begreifen ja, dass ich bei den obwaltenden sachlichen Bedenken nicht in der ursprünglich geplanten Weise dafür Partei nehmen kann.”
 104.
Greek lettered indices run in M_{5}, Latin ones in space time; x^{4} is the time coordinate, x^{5} the new spacelike coordinate.
 105.
“Ich mache mir Gedanken darüber, dass ich Sie vor zwei Jahren von der Publikation Ihrer Idee über die Vereinigung von Gravitation und Elektrizität abgehalten habe. Ihr Weg scheint mir jedenfalls mehr für sich zu haben als der von H. Weyl beschrittene. Wenn Sie wollen, lege ich Ihre Arbeit doch der Akademie vor […].”
 106.
Jakob Grommer (1879–1933). Born near Brest, then in Russia. First a Talmud student with a keen interest in mathematics. Came to Göttingen to study mathematics and obtained his Ph.D. there. Worked with Einstein for at least a decade (1917–1927) as his calculational assistant. He held a university position in Minsk from 1929 on and later became a member of the Belorussian Academy of Sciences. From his youth he was inflicted with elephantiasis.
 107.
We use some of Eddington’s notation. His notation representing the covariant derivative by a lower index is highly ambiguous, though, and will be avoided. *G_{ kl } is not a dual.
 108.
108“[…] Darüber steht das marmorne Lächeln der unerbittlichen Natur, die uns mehr Sehnsucht als Geist verliehen hat.”
 109.
There even exist a manuscript dating from Einstein’s stopover in Singapore; it is incomplete and of little importance [223].
 110.
“Der Wunsch, das Gravitationsfeld und das elektromagnetische Feld als Wesenseinheit zu begreifen, beherrscht in den letzten Jahren das Streben der Theoretiker. […] Von einem logisch einleuchtenden Standpunkt her sollte nur die Konnektion als fundamentale Grösse benutzt werden und die Metrik eine daraus abgeleitete Grösse sein. […] Dies that Eddington.”
 111.
In place of our K_{ ik } Einstein used R_{ ik }.
 112.
“Aber die ausserordentliche Kleinheit von 1/λ^{2} bringt es mit sich, dass endliche φ_{ kl } nur bei winzigen, praktisch verschwindenden kovarianten Stromdichten möglich sind. Singuläre Stellen ausgenommen verschwindet praktisch also die Stromdichte.”
 113.
“[…] dass nach dieser Theorie die positive und die negative Elektrizität keineswegs bloss dem Vorzeichen nach verschieden sein können.”
 114.
“dass EDDINGTONS allgemeiner Gedanke in Verbindung mit dem Hamiltonschen Prinzip zu einer von Willkür fast freien Theorie führt, welche unserem bisherigen Wissen über Gravitation und Elektrizität gerecht wird und beide Feldarten in wahrhaft vollendeter Weise vereinigt.”
 115.
“Die Theorie vermag also jedenfalls von der Verschiedenheit der Masse der positiven und negativen Elektronen keine Rechenschaft zu geben.”
 116.
He exchanged g_{ ik } by γ_{ ik }, R_{ ik } by r_{ ik }.
 117.
“R bedeutet hierbei den aus den g_{ ij } gebildeten RIEMANNschen Krümmungsskalar”
 118.
This proportionality is about the simplest assumption one can make; the equation \({\nabla _l}{F^{kl}} \sim {A^k}\) corresponds, in the case of the gravitational field, to the equation R_{ ik }=λg_{ ik } leading to Einstein spaces.
 119.
“[…] Ich glaube nun überhaupt nicht, dass dieses Problem der elektrischen Elementarteilchen von irgend einer Theorie gelöst werden kann, die den Begriff der kontinuierlich variierenden Feldstärken, die gewissen Differentialgleichungen genügen, auf die Gebiete im Innern der Elementarteilchen anwendet. […] Die Grössen \(\Gamma _{\nu \;\;\alpha }^\mu\) können nicht direkt gemessen werden, sondern müssen aus den direkt gemessenen Grössen erst durch komplizierte Rechenoperationen gewonnen werden. Niemand kann empirisch einen affinen Zusammenhang zwischen Vektoren in benachbarten Punkten feststellen, wenn er nicht vorher bereits das Linienelement ermittelt hat. Deswegen halte ich im Gegensatz zu Ihnen und Einstein die Erfindung der Mathematiker, dass man auch ohne Linienelement auf einen affinen Zusammenhang eine Geometrie gründen kann, zunächst für die Physik bedeutungslos.”
 120.
“Für mich besteht das Endergebnis dieser Betrachtung leider in dem Eindruck, dass uns dieWeylEddingtonsche Vertiefung der geometrischen Grundlagen keinen Fortschritt der physikalischen Erkenntnis zu bringen vermag; hoffentlich wird die künftige Entwicklung zeigen, dass diese pessimistische Meinung unberechtigt gewesen ist.”
 121.
“Ich bin fest überzeugt, dass die ganze GedankenReihe WeylEddingtonSchouten zu nichts physikalisch brauchbarem führt und habe jetzt eine andere Spur gefunden, die mehr physikalisch fundiert ist. Das QuantenProblem scheint mir etwas wie einen besonderen Skalar zu verlangen, für dessen Einführung ich einen plausiblen Weg gefunden habe.”
 122.
“Ich glaube nicht, dass die Theorie das Kontinuum wird entbehren können. Es will mir aber nicht gelingen, meiner Lieblingsidee, die Quantenstruktur aus einer Überbestimmung durch Differentialgleichungen zu verstehen, greifbare Gestalt zu geben.”
 123.
“Nach den bisherigen Theorien kann der Anfangszustand eines Systems frei gewählt werden; die Differentialgleichungen liefern dann die zeitliche Fortsetzung. Nach unserem Wissen über die Quantenzustände, wie es sich insbesondere im Anschluss an die BOHRsche Theorie im letzten Jahrzehnt entwickelt hat, entspricht dieser Zug der Theorie nicht der Wirklichkeit. Der Anfangszustand eines um einen Wasserstoffkern bewegten Elektrons kann nicht frei gewählt werden, sondern diese Wahl muss den Quantenbedingungen entsprechen. Allgemein: nicht nur die zeitliche Fortsetzung, sondern auch der Anfangszustand unterliegt Gesetzen.”
 124.
“Das gesuchte Gleichungssystem, welches das Feld überbestimmt, muss jedenfalls jene statische, kugelsymmetrische Lösung zulassen, welche gemäss obigen Gleichungen [i.e., the EinsteinMaxwell equations] das positive bzw. negative Elektron beschreibt.”
 125.
“Die Idee, mit der ich mich herumschlage, betrifft das Verstehen der Quantentheorie und heisst: Überbestimmung der Gesetze durch mehr Gleichungen als Feldvariable. So soll die Nichtwillkürlichkeit der Anfangsbedingungen begriffen werden, ohne die Feldtheorie zu verlassen.[…] Die Bewegungsgleichungen materieller Punkte (Elektronen) wird ganz aufgegeben; das motorische Verhalten der letzteren soll durch die Feldgesetze mitbestimmt werden.”
 126.
“Einerseits scheint das nur noch formell etwas mit einer Feldtheorie gemeinsam zu haben; und andererseits schimmert mir noch nicht, wie auf diesem Wege etwas den diskreten Quantenbahnen entsprechendes zu erreichen ist.”
 127.
Tracy Yerkes Thomas (1899–1983). Born in Alton, Illinois, U.S.A.: Studied mathematics at Princeton University and received his doctorate in 1923. Professor at Princeton, then from 1938–1944 at the University of California in Los Angeles, and since 1944 professor and chairman of the mathematics department at Indiana University in Bloomington, U.S.A.
 128.
 129.
“Durch die Relativitätstheorie veranlasst, hat die Differentialgeometrie eine ganz neue, einfache und befriedigende Begründung erfahren; ich nenne nur G. Hessenberg ‘Vektorielle Begründung…’, Math. Ann. 78, 1917, S. 187–217 und H. Weyl, RaumZeitMaterie, 2. Kap., Leipzig 1918 (3. Aufl. Berlin 1920) sowie ‘Reine Infinitesimalgeometrie’ etc. […] In der vorliegenden Untersuchung sind nun alle achtzehn verschiedenen Arten der linearen Übertragung vollständig aufgezählt und in invarianter Weise festgelegt. Die allgemeinste Übertragung wird durch zwei Felder dritten Grades, ein Tensorfeld zweiten Grades und ein Vektorfeld charakterisiert, […].”
 130.
The 18 possibilities were numbered by Schouten as I, …, VI a–c; he mentioned 5 examples: Einstein (VI c), Hessenberg (VI a), Weyl (IV c) and (II c) (the latter also corresponds to Eddington’s choice) as well as König (II a) (cf. also [296]).
 131.
“Die allgemeinen Übertragungen für n=4 eröffnen für die Physik wenigstens theoretisch die Möglichkeit einer Erweiterung der Weylschen Theorie. Für eine solche Erweiterung ist eine invariante Festlegung der Übertragung notwendig, da eine physische Erscheinung nur mit einem invarianten Ausdruck korrespondieren kann.”
 132.
A summary of Schouten’s papers from 1922 is given in [300].
 133.
“Da die Resultate der vorliegenden Arbeit aber für weitere Kreise von Mathematikern und auch für manche Physiker interessant sein dürften […].”
 134.
Einstein had wished to avoid the distinction between \(\mathop \nabla \limits^ +\) and \(\mathop \nabla \limits^ \).
 135.
Henri Eyraud (1892–1994). Studied mathematics at the University of Paris and received his doctorate in 1926 with a thesis on “Metrical spaces and physicogeometrical theories”. From 1930 professor of mathematics at the University of Lyon and director of the Institute of “Financial and AssuranceSciences”. Perhaps he considered his papers on the geometry of unified field theory as a sin of his youth: In Poggendorff, among the 33 papers listed, all are from his later main interest.
 136.
The geometry of paths involves a change of connection that preserves the geodesics when vectors are displaced along themselves.
 137.
“[…] Auch von meiner in diesen Sitzungsberichten (Nr. 17, p. 137 1923) erschienenen Abhandlung, welche ganz auf Eddingtons Grundgedanke basiert war, bin ich der Ansicht, dass sie die wahre Lösung des Problems nicht gibt. Nach unablässigem Suchen in den letzten zwei Jahren glaube ich nun die wahre Lösung gefunden zu haben.”
 138.
“Man wird jedoch für spätere Untersuchungen (z. B. Problem des Elektrons) im Sinne behalten müssen, dass das HAMILTONsche Prinzip für das Verschwinden der φ_{ k } keinen Anhaltspunkt liefert.”
 139.
 140.
Einstein’s proof that chargesymmetric solutions with the same mass are unavoidable, although to him a rather negative feature of his unified field theories, later was interpreted as Einstein’s discovery of the concept of antimatter ([357, 371], p. 78, footnote 44). To me, this seems to be a case of whiggish historical hindsight. According to Bargmann, Einstein’s lasting result is that he pointed out the importance of the discrete symmetry operations [8].
 141.
i.e., the symmetry of the metrical tensor.
 142.
“Lässt man die Voraussetzung der Symmetrie fallen, so erhält man in erster Näherung die Gesetze der Gravitation und die Maxwell’schen Feldgesetze für den leeren Raum, wobei der antisymmetrische Teil der ĝ^{ ik } das elektromagnetische Feld ist. Dies ist doch eine prachtvolle Möglichkeit, die doch der Realität entsprechen dürfte. Nun ist die Frage, ob diese Feldtheorie mit der Existenz der Atome und Quanten vereinbar ist. Im Makroskopischen zweifle ich nicht an ihrer Richtigkeit.”
 143.
“Wesentlich scheint mir die Erkenntnis zu sein, dass eine Erklärung der Ungleichartigkeit der beiden Elektrizitäten nur möglich ist, wenn man der Zeit eine Ablaufrichtung zuschreibt und diese bei der Definition der massgebenden physikalischen Grössen heranzieht. Hierin unterscheidet sich die Elektrodynamik von der Gravitation; deshalb erscheint mir auch das Bestreben, die Elektrodynamik mit dem Gravitationsgesetz zu einer Einheit zu verschmelzen, nicht mehr gerechtfertigt.“
 144.
George Yuri Rainich (1886–1968). Of Russian origin. He studied mathematics at universities in Odessa, Göttingen, and Munich, taking his final exam at the University of Kazan in 1913. He then taught at Kazan and Odessa until 1922, when he came to the United States of America. He was a Johnston Scholar at Johns Hopkins University from 1923–1926 and then Professor of Mathematics at the University of Michigan in Ann Arbor, U.S.A.
 145.
“Dass die Gleichungen (140) noch wenig Beachtung gefunden haben, liegt an zwei Umständen. Erstens nämlich waren unser aller Bestrebungen darauf gerichtet, auf dem von Weyl und Eddington eingeschlagenen oder einem ähnlichen Weg zu einer Theorie zu gelangen, die das Gravitationsfeld und das elektromagnetische Feld zu einer formalen Einheit verschmilzt; durch mannigfache Misserfolge habe ich mich aber nun zu der Überzeugung durchgerungen, dass man auf diesem Wege der Wahrheit nicht näher kommt.“
 146.“Meine Arbeit im Sinne Eddington’s habe ich leider verwerfen müssen. Ueberhaupt bin ich jetzt überzeugt, dass mit dem WeylEddington’schen GedankenKomplex leider nichts zu machen ist. Ich halte die Gleichung[cf. Equation (140)] für das beste, was wir heute haben. Es sind 9 Gleichungen für die 14 Grössen g_{ ik } und γ_{ ik }. Aus den neuen Rechnungen scheint sich zu ergeben, dass diese Gleichungen die Bewegung der Elektronen liefern. Aber es erscheint zweifelhaft, ob die Quanten darin Platz haben.”$$ {R_{ik}}  \frac{1}{4}R\;{g_{ik}} =  \kappa {T_{ik}}\;\;\;\;\;{\rm{elektromagnetisch}} $$
 147.
It remains unclear how these γ_{[ik]} are embedded into the theory, possibly in the sense of Rainich. Einstein’s paper practically excludes that they form the antisymmetric part of an asymmetric metric tensor.
 148.
“dont les γ_{[ik]} forment le rotationel”
 149.
Einstein had a wrong factor: 1/2 instead of 1/4.
 150.“Auch die ja von mir selbst aufgestellte Gleichungbefriedigt mich wenig. Sie lässt keine singularitätenfreien elektrischen Massen zu. Ferner kann ich mich nicht dazu entschliessen, zwei Sachen zusammenzuleimen (wie die rechte und die linke Seite einer Gleichung), die logischmathematisch nichts miteinander zu schaffen haben.”$$ {R_{ik}} = {g_{ik}}{f_{lm}}{f^{lm}}  \frac{1}{2}{f_l}{f_{km}}{g^{lm}} $$
 151.
Leopold Infeld (1889–1968). Born in Cracow, Poland. Studied at the University of Cracow and received his doctorate in 1923. After teaching in Lwow/Lemberg, he became professor of applied mathematics at the University of Toronto in 1938. Worked on unitary field theory and quantum electrodynamics, with van der Waerden on spinors, worked with Born on nonlinear electrodynamics, and with Einstein on equations of motion (“EIH paper”).
 152.
For the correspondence between Einstein and Infeld, cf. J. Stachel’s essay in [330], pp. 477–497.
 153.
“Die obige Gleichung zeigt, dass sich die elektrische Ladung und der elektrische Strom überall verteilen, wo das elektromagnetische Feld existiert.”
 154.
 155.
“das Problem der Verallgemeinerung der Relativitätstheorie nicht auf rein formalem Wege gelöst werden kann. Man sieht zunächst nicht, wie die Wahl zwischen den verschiedenen nichtRiemannschen Geometrien, die uns die Gravitation und die Maxwellschen Gleichungen ergeben, zu treffen ist. Die eigentliche Weltgeometrie, die zu einer einheitlichen Theorie von Gravitation und Elektrizität führen soll, kann nur durch Untersuchung ihres physikalischen Inhalts gefunden werden.”
 156.
Damodar D. Kosambi (1907–1966). Of Indian origin; born in Goa he moved to America in 1918 with his learned father and graduated from Harvard University in 1926 in mathematics, history and languages. Taught at the Muslim University of Aligarh and, from 1932, at Ferguson College, Pune. Mathematician, historian, and Sanskrit scholar.
 157.
Walther Mayer (1887–1948). Studied mathematics at the Federal Institute of Technology in Zürich and at the University of Vienna where he wrote his dissertation and became a Privatdozent (lecturer) with the title “professor”. He had made himself a name in topology (“MayerVietoris sequences”), and worked also in differential geometry (wellknown textbook “DuschekMayer” on differential geometry). In 1929 he became Einstein’s assistant with the explicit understanding that he work with him on distant parallelism. It seems that Mayer was appreciated much by Einstein and, despite being in his forties, did accept this role as a collaborator of Einstein. After coming to Princeton with Einstein in 1933, he got a position at the Mathematical Institute of Princeton University and became an associate of the Institute for Advanced Study. Wrote a joint paper with T. Thomas on “Field of parallel vectors in nonanalytic manifolds in the large.” Mayer died in 1948.
 158.
“Herr Mandel macht mich darauf aufmerksam, dass die von mir hier mitgeteilten Ergebnisse nicht neu sind. Der ganze Inhalt findet sich in der Arbeit von O. Klein.”
 159.
Vladimir Aleksandrovich Fo(c)k (1898–1974). Born in St. Petersburg (renamed later Petrograd and Leningrad). Studied at Petrograd University and spent his whole carrier at this University. Member of the USSR Academy of Sciences. Fundamental contributions to quantum theory (Fock space, HartreeFock method); also worked in and defended general relativity
 160.
The correspondence is taken from Pais [241] who, in his book, expresses his lack of understanding as to why Einstein published these two papers at all.
 161.
Heinrich Mandel (1898 ). From 1928 lecturer at the University of Leningrad, and from 1931 research work at the Physics Institute of this university.
 162.
“Die Bedeutung des überzähligen Koordinatenparameters scheint nämlich gerade darin zu liegen, dass er die Invarianz der Gleichungen [i.e., the relativistic wave equations] in bezug auf die Addition eines beliebigen Gradienten zum Viererpotential bewirkt.”
 163.
My italics.
 164.“Nun hat mir die allerdings reichlich mühsehlige Umrechnung der fünfdimensionalen Krümmungsgrössen auf eine in ihr enthaltene vierdimensionale Untermannigfaltigkeit auch im allgemeinen Falle (g_{55}≠const., Abhängigkeit der F u n d a m e n t a lkomponenten auch von x^{5} zugelassen) gezeigt, dass die w e s e n t l i c h e n Eigenschaften der Feldgleichungen auch dann erhalten bleiben, d.h. diese behalten die Gestalt:nur enthalten die T^{ ik } ausser den Komponenten S^{ ik } des elektromagnetischen Energietensors noch weitere Glieder, und die zu s^{ i } zusammengefassten Grössen verschwinden nicht. […] Man könnte sogar das Auftreten der neuen Glieder auf den rechten Seiten von dem Standpunkt aus begrüssen, dass nunmehr die Feldgleichungen nicht nur für einen materie und ladungsfreien Feldpunkt geliefert werden.”$$ \begin{array}{*{20}{c}} {{R^{ik}}  \frac{1}{2}{g^{ik}}R = {T^{ik}},\;\;\;\;\;}&{\frac{{\partial \sqrt g {F^{ik}}}}{{\partial {x^k}}} = {s^i},} \end{array} $$(#)
 165.
“Die hier dargestellte Theorie knüpft psychologisch an die bekannte Theorie von KALUZA an, vermeidet es aber, das physikalische Kontinuum zu einem solchen von fünf Dimensionen zu erweitern.”
 166.
Greek indices run from 1 to 5, Latin indices from 1 to 4.
 167.
In special coordinates, \({A^\iota }\mathop = \limits^* \delta _5^\iota\).
 168.
Enea Bortolotti (1896–1934). Born in Rome. After a break during the First World War, he received his Ph.D. in 1920 at Pisa; he was particularly influenced by L. Bianchi. After teaching at the medical school, he became professor of geometry at the Univerity of Cagliari in 1928. From there he moved on to the same position at the University of Florence in 1934. Despite his premature death, Bortolotti published about a hundred papers, notably in differential geometry.
 169.
The curly bracket was introduced in Equation (29).
 170.
“Die hier dargelegte Theorie liefert die Gleichungen des Gravitationsfeldes und des elektromagnetischen Feldes zwanglos auf einheitlichem Wege; dagegen liefert sie vorläufig kein Verständnis för den Bau der Korpuskeln sowie för die in der Quantentheorie zusammengefassten Tatsachen.”
 171.
“Auch ich habe seit 1928 einen Ausgleich zu finden gesucht, diesen Weg aber wieder verlassen. Dagegen gelang eine verblüffend einfache Konstruktion auf Grund einer Idee, die zur Hälfte von mir, zur Hälfte von meinem Mitarbeiter Prof. Dr. Mayer stammt. […] Nach meiner und Mayers Auffassung tritt die fünfte Dimension nicht in Erscheinung. […] demzufolge man Beziehungen zwischen einem hypothetischen fünfdimensionalen Raum und dem vierdimensionalen aufstellen kann. Auf diese Weise gelang es, das Gravitations und das elektromagnetische Feldals logische Einheit zu erfassen.”
 172.
“Das Einzige, was in unserer Untersuchung herauskommt, ist die Vereinigung von Gravitation und Elektrizität, wobei die Gleichungen der letzteren genau die (relativistisch geschriebenen) Maxwell’schen des leeren Raumes sind. Es ist also kein physikalischer Fortschritt dabei, höchstens nur insoweit als man eben sieht, dass die Maxwell’schen Gleichungen nicht nur erste Näherungen sind, sondern ebensogut rationell begründet erscheinen wie die Gravitationsgleichungen des leeren raumes. Elektrische und Massendichte gibt es hierbei nicht; da hört die Herrlichkeit auf; dies gehört wohl schon zum Quantenproblem, das bis jetzt vom Feldstandpunkt unerreichbar ist (ebensowenig wie die Relativität vom Standpunkt der Quantenmechanik aus). Der Witz liegt in der Einführung von Fünfervektoren \({a^\sigma }\) im vierdimensionalen Raum, die an den Raum durch einen linearen Mechanismus gebunden sind. a^{ s } sei der zu \({a^\sigma }\) gehörende Vierervektor, dann gibt es eine solche Beziehung \({a^\sigma } = \gamma _\sigma ^s{a^\sigma }\). Sinnvoll sind dann in der Theorie solche Gleichungen, welche unabhängig von der durch \(\gamma _\sigma ^s\) geschaffenen besonderen Beziehung gelten. Infinitesimale Verschiebung von (\({a^\sigma }\)) im vierdim. Raum wird definiert, ebenso die dazu gehörige Fünferkrümmung und diese liefert dann die Feldgleichungen.”
 173.
Banesh Hoffmann (1906–1986). Born in Richmond, England. Studied mathematics and theoretical physics at Oxford University and received his doctorate in 1929. Became an assistant at Princeton University and worked there with Einstein in 1932–1935. (His name supplied the “H” in the EIH paper.) From 1939 professor at Queens College in New York. His scientific interests were in relativity theory, tensor analysis, and quantum theory.
 174.
“Diese Autoren wählen aber eine Formulierung, die infolge unnötiger Spezialisierung des Koordinatensystems die fünfte Koordinate in ganz ähnlicher Weise vor den übrigen auszeichnet wie dies bei KaluzaKlein durch die Zylinderbedingung geschehen war […].”
 175.
“[…] dass unsere Theorie von ganz anderen physikalischen und geometrischen Gesichtspunkten als die KALUZAsche ausgeht. Insbesondere fordern wir kein Verhältnis zwischen elektrischer Ladung und einer fünften Koordinate; unsere Theorie ist vielmehr durchaus vierdimensional.”
 176.
“Wir bemerken, dass Herr Cartan in einer allgemeinen und überaus aufklärenden Untersuchung jene Eigenschaft von Differentialgleichungssystemen tiefer analysiert hat, welche von uns in dieser Arbeit und in früheren Arbeiten als ‘Kompatibilität’ bezeichnet wurde.”
 177.
van Dantzig ventured even into physics; he wrote a paper on Miller’s repeat of Michelson’s experiment but published it in a mathematics journal [359].
 178.
A similar picture is already given in [315], p. 666, Figure 2
 179.
J. Solomon came from Copenhagen to Zürich on a Rockerfeller grant.
 180.
“la forme que prennent les équations de Dirac dans la théorie unitaire d’Einstein et Mayer”
 181.
“[…] même en l’absence de gravitation nous devons nous attendre à une différence entre l’e de Dirac dans la théorie d’Einstein et Mayer et l’équation de Dirac telle qu’elle est écrite habituellement.”
 182.
“On y examine d’un point de vue général la théorie des spinors dans l’espace à cinq dimensions. On discute ensuite la forme du tenseur énergiequantité de mouvement et du vecteur de courant dans la théorie d’Einstein et Mayer.[…] Malheureusement il s’est montré que les considérations du §7 de la première partie sont entachées d’une faute de calcul… Ceci a rendu nécessaire l’introduction d’une nouvelle expression pour le tenseur énergiequantité de mouvement et […] également pour le vecteur de courant […].”
 183.
a linear combination of torsion appearing in the connection besides the metric contribution (cf. Equation (43)).
 184.
“Parue au moment oú vous faisiez vos conférences au Collège de France; je me rappelle même avoir, chez M. Hadamard, essayé de vous donner l’exemple le plus simple d’un espace de Riemann avec Fernparallelismus en prenant une sphère et en regardand commes paralléles deux vecteurs faisant le même angle avec les méridiennes qui passent par leurs deux origines: les géodésiques correspondantes sont les loxodromies.”
 185.
“Deshalb ist das Bestreben der Theoretiker darauf gerichtet, natürliche Verallgemeinerungen oder Ergänzungen der RIEMANNschen Geometrie aufzufinden, welche begriffsreicher sind als diese, in der Hoffnung, zu einem logischen Gebäude zu gelangen, das alle physikalischen Feldbegriffe unter einem einzigen Gesichtspunkte vereinigt.”
 186.
“[…] il indique dans sa bibliographie une note de Bortolotti dans laquelle il se réfère plusieurs fois à mes travaux.”
 187.
Mathematische Annalen was a journal edited by David Hilbert with coeditors O. Blumenthal and G. Hecke which physicists usually would not read. Einstein had been coeditor for the volumes 81 (1920) to 100 (1928); thus he had easy access. The editor of Zeitschrift für Physik was Karl Scheel, an experimental physicist.
 188.
 189.
“Remarquons simplement qu’en principe les phénomènes mécaniques sont de nature purement affine, tandis que les phénomènes électromagnétiques sont de nature essentiellement métrique; il peut donc assez naturel de chercher à représenter le potentiel électromagnétique par un vecteur non purement affine.”
 190.
“Insbesondere durch die Herren Weitzenböck und Cartan erfuhr ich, dass die Behandlung von Kontinua der hier in Betracht kommenden Gattung an sich nicht neu sei. […] Was an der vorliegenden Abhandlung das Wichtigste und jedenfalls neu ist, das ist die Auffindung der einfachsten Feldgesetze, welche eine Riemannsche Mannigfaltigkeit mit Fernparallelismus unterworfen werden kann.”
 191.
“in ihrer Einheitlichkeit und der hochgradigen (erlaubten) Überbestimmung der Feldvariablen. Auch habe ich zeigen können, dass die Feldgleichungen in erster Näherung auf Gleichungen führen, welche der NewtonPoissonschen Theorie der Gravitation und der Maxwellschen Theorie des elektromagnetischen Feldes entsprechen. Trotzdem bin ich noch weit davon entfernt, die physikalische Gültigkeit der abgeleiteten Gleichungen behaupten zu können. Der Grund liegt darin, dass mir die Ableitung von Bewegungsgesetzen für die Korpuskeln noch nicht gelungen ist.”
 192.
Einstein’s policy was to permit only articles for the general reader to be printed in newspapers; he discouraged an English translation of his first teleparallelism paper of 1929 asked for by a publishing house (see [183], Documents Nr. 57 and 58, p. 141).
 193.
German edition: “Geheimnisse des Weltalls” (secrets of the universe).
 194.
“Einstein wiederum bringt uns in seiner letzten Veröffentlichung, deren Kommentare noch ausstehen, mathematische Formeln, die gleichzeitig auf die Schwerkraft und die Elektrizität anwendbar sind, als wären diese beiden Kräfte, die das Weltall zu lenken scheinen, identisch und demselben Gesetz unterworfen. Wenn dem so wäre, würden die Folgen unberechenbar sein.”
 195.
The nonspecialised reader will find this section rather technical.
 196.
“normed subdeterminants” means that the subdeterminants are divided by the determinant det \(h_{\hat \imath }^k\). Thus, the inverse matrix must be calculated.
 197.
Unlike in Einstein’s notation, which used Greek indices for the coordinate indices and Latin ones for the beins, here beinindices are noted by a hatsymbol. Consequently, Latin indices are to be moved by the metric g_{ ik }, while beinindices are raised and lowered by \({\delta _{\hat \imath k}}\) or, for real coordinates, by the Minkowski metric.
 198.
Théophile Ernest de Donder (1872–1957). Born in Brussels. Studied mathematics and physics at the University of Brussels and received his doctorate in 1899. Professor of mathematical physics at the Université libre de Bruxelles from 1911 to 1942. Member of the Royal Belgian Academy. Research on variational calculus, general relativity, electromagnetism, thermodynamics, and wave mechanics.
 199.
\(h: = \det {h_{l\hat m}}\) corresponds to \(\sqrt {  \det {g_{ij}}}\). In his next note [88] Einstein also switched his notation of the 4leg to Weitzenböck’s ^{ s }h_{ k }, where the index to the left of h counts the number of legs.
 200.
“die Trennung des Gravitationsfeldes und des elektromagnetischen Feldes erscheint aber nach dieser Theorie als künstlich. […] Bemerkenswert ist ferner, dass nach dieser Theorie das elektrische Feld nicht quadratisch in die Feldgleichungen eingeht.”
 201.
There are some misprints in the formulae of § 1 of Einstein’s paper [88]. He writes the tensor density V with an upper coordinate and two lower beinindices, i.e., as \({\hat V_{\hat k\hat l}}^j\). Einstein also introduced a new covariant derivative for which he used the symbol A_{/k}. We call it \(\nabla { * _l}\); it is given through Equation (16), i.e., by \({\nabla _k}{X^i} = \nabla { * _l}  {\Delta _{kr}}^r{\hat X^i}\).
 202.
The abbreviation \({A_{\left\ k \right.}}\) is used only in place of \({\mathop \nabla \limits^ + _k}\). If summation over indices is to be performed, it is irrelevant whether beinindices or coordinate indices are written.
 203.
“Die in dieser Arbeit vorgeschlagenen Feldgleichungen sind formal gegenüber sonst denkbaren so zu kennzeichnen. Es ist durch Anlehnung an die Identität (167) erreicht worden, dass die 16 Grössen h _{ i } ^{ k̂ } nicht nur 16, sondern 20 selbständigen Differentialgleichungen unterworfen werden können. Unter ‘selbständig’ ist dabei verstanden, dass keine dieser Gleichungen aus den übrigen gefolgert werden kann, wenn auch zwischen ihnen 8 identische (Differentiations) Relationen bestehen.”
 204.
“Eine tiefere Untersuchung der Konsequenzen der Feldgleichungen (170) wird zu zeigen haben, ob die RIEMANNMetrik in Verbindung mit dem Fernparallelismus wirklich eine adäquate Auffassung der physikalischen Qualitäten des Raumes liefert.”
 205.
As to the person of H. Müntz, it is not obvious whether he can be identified with Dr. Ch. Müntz, a possibility following from a paper of Ch. H. Müntz, presented to the Göttingen Academy by D. Hilbert in 1917. If it is the same person, then H. Müntz seems to have been a mathematics teacher, first at the Odenwaldschule in Heppenheim a.d. B. from 1918 to 1922(?), then, possibly for a short time in Göttingen (Friedländerweg 61), and from 1924 on in BerlinNikolassee, Herkrathstr. 5. I conclude this from the membership lists of the Deutsche Mathematikervereinigung, which Müntz entered in 1913, and which gives a Berlin address since July 1924 and lists him as “Prof.” in Berlin, in 1931. At the time, experienced teachers at Gymnasium could carry the title of professor. In the Einstein archive, 26 letters of Einstein to Müntz from the years 1927–1931 exist. The addresses show that Müntz went to Stockhom via Tallin. In fact, Pais [241] writes that Müntz became a professor of mathematics at the University of Leningrad but had to leave the Soviet Union in 1938 for Sweden. In fact, a document of 1931 states: “Prof. Hermann Mueninz, der einer der engeren wissenschaftlichen Mitarbeiter Albert Einsteins ist und gegenwärtig ein Lehramt für höhere Mathematik an der Leningrader Universität bekleidet […]” ([183], Dokument 144, p. 222). Sauer ([289], p.11) reports the life span of Müntz to have been 1884–1956.
 206.
The variational derivatives of Ĥ, Ĥ*, and Ĥ** are named Ĝ^{ ik }, Ĝ*^{ ik }, and Ĝ**^{ ik }, respectively, by Einstein.
 207.
Einstein’s contribution seems to have been submitted towards the end of 1928 (cf. [289], p. 21).
 208.
“[…] welche mit den bekannten Gesetzen des Gravitationsfeldes und des elektromagnetischen Feldes in erster Näherung übereinstimmen […]”
 209.
The quantity G^{ ik } defined here must be distinguished from the Einstein tensor in Section 2.2 denoted by the same symbol.
 210.
“En effet, avec la nouvelle théorie de M. Einstein, il est naturel d’appeler homogène un univers où les vecteurs de torsion associés à deux éléments de surface sont paralléles euxmêmes; c’est à dire où le transport paralléle conserve la torsion.”
 211.“Sehr dankbar bin ich Ihnen aber für die Identitätdie mir merkwürdigerweise entgangen war. […] In einer neuen Darstellung in den Sitzungsberichten habe ich von dieser Identität Gebrauch gemacht, indem ich mir erlaubte, auf Sie als Quelle aufmerksam zu machen.”$$ {G^{ik}}_{\left\ i \right.}  {S_{lm}}^{\;k}{G^{lm}} = 0, $$
 212.
Gawrilow Raschko Zaycoff (1901–1982). Born in Burgas, Bulgaria. Studied at the Universities of Sofia, Göttingen, and Berlin from 1922 to 1928. From 1928 assistant in the Physics Institute of the University of Sofia; 1931–1933 teacher at a Gymnasium in Sofia. From 1935 on mathematical statistician at the Institute for Economic Research of Sofia University. From 1961–1972 Professor at the Physics Institute of the Bulgarian Academy of Science
 213.
“Neuerdings hat A. Einstein gestützt auf Untersuchungen von E. Cartan, seine Fernparallelismustheorie wesentlich modifiziert, so dass die früheren Nachteile (es handelt sich nur um die physikalischen Identifikationen) derselben von selbst hinfällig werden.”
 214.
“Ce n’est pas la première fois qu’on envisage de tels espaces. Du point de vue purement mathématique ils ont déjà été étudié auparavant. M. CARTAN a eu l’amabilité de rédiger, pour les Mathematische Annalen, une note exposant les diverses phases du développement formel de ces conceptions.”
 215.
“Ce type d’espace à été envisagé, avant moi, par des mathématiciens, notamment par WEITZENBÖCK, EISENHART et CARTAN […].”
 216.
“Un grand pas en avant a été fait dans la poursuite de cette synthèse totale des phénomènes qui est, à tort ou à raison, l’idéal des physiciens. […] le splendide effort fourni par Einstein nous permet d’espérer que les dernières difficultés théoriques seront vaincues et que nous pourrons bientôt comparer les conséquences de la théorie à l’expérience, cette pierre d’achoppement de toutes les créations de l’esprit.”
 217.
“Es müssen also Gleichungen aufgestellt werden, zwischen denen identische Relationen bestehen. Je höher die Zahl der Gleichungen ist (und folglich auch der zwischen ihnen bestehenden Identitäten), desto bestimmtere, über die Forderung des blossen Determinismus hinausgehende Aussagen macht die Theorie; desto wertvoller ist also die Theorie, falls sie mit den Erfahrungstatsachen verträglich ist.”
 218.
“Der Kompatibilitätsbeweis ist auf Grund einer brieflichen Mitteilung, welche ich Herrn CARTAN verdanke (vgl. §3, [16]), gegenüber der in den Mathematischen Annalen gegebene Darstellung etwas vereinfacht.”
 219.
Note that Einstein used the initial “S” in place of the correct “W” (Walther)
 220.
“Meine Feldtheorie macht gute Fortschritte. Cartan hat schon darin gearbeitet. Ich selbst arbeite mit einem Mathematiker (S. Mayer aus Wien), einem prächtigen Kerl […].”
 221.
“Hiervon sind zwei (nichttriviale) Verallgemeinerungen der ursprünglichen Feldgleichungen der Gravitation, von denen eine als aus dem Hamiltonschen Prinzip hervorgehend bereits bekannt ist […]. Die beiden übrigen sind in der Arbeit durch […] bezeichnet.”
 222.
This view is supported by an (as yet unpublished) detailed investigation of Einstein’s theory of distant parallelism by T. Sauer which I received 6 month after after having submitted this review [289]. Sauer uses unpublished correspondence in the Einstein Papers Archive, and points to “some historical and systematic similarities between the Fernparallelismus episode and the Entwurf theory, i.e., the precurser theory of general relativity theory pursued by Einstein in the years 1912–1915.”
 223.
An evaluation of this correspondence has been given in [15].
 224.
Hans Reichenbach (1891–1953). Philosopher of science, neopositivist. Professor in Berlin, Istanbul, and Los Angeles. Wrote books on the foundations of relativity theory, probability, and quantum mechanics.
 225.
In fact, this generalisation was to be worked out soon by V. Bargmann in 1930 [5] (cf. below).
 226.
“[…] es ist das Ziel der neuen Theorie Einsteins, eine derartige Verkettung von Gravitation und Elektrizität zu finden, dass sie nur in erster Näherung in die getrennten Gleichungen der bisherigen Theorie zerspaltet, während sie in höherer Näherung einen gegenseitigen Einfluss der beiden Felder lehrt, der möglicherweise zum Verständnis bisher ungelöster Fragen, wie der Quantenrätsel, führt. Aber dieses Ziel scheint nur erreichbar zu sein unter Verzicht auf eine unmittelbare physikalische Interpretation der Verschiebungsoperation, ja sogar der eigentlichen Feldgrössen selbst. Vom geometrischen Standpunkt muss deshalb ein solcher Weg sehr unbefriedigend erscheinen; seine Rechtfertigung wird allein dadurch gegeben werden können, dass er durch die genannte Verkettung mehr physikalische Tatsachen umschliesst, als zu seiner Aufstellung in ihn hineingelegt wurden.”
 227.
“[…] unterscheidet sich mein Ansatz in radikaler Weise dadurch, dass ich den Fernparallelismus ablehne und an Einsteins klassischer Relativitätstheorie der Gravitation festhalte. […] An den Fernparallelismus vemag ich aus mehreren Gründen nicht zu glauben. Erstens sträubt sich mein mathematisches Gefühl a priori dagegen, eine so künstliche Geometrie zu akzeptieren; es fällt mir schwer, die Macht zu begreifen, welche die lokalen Achsenkreuze in den verschiedenen Weltpunkten in ihrer verdrehten Lage zu starrer Gebundenheit aneinander hat einfrieren lassen. Es kommen […] zwei gewichtige physikalische Gründe hinzu. […] nur durch diese Lockerung [des Zusammenhangs zwischen den lokalen Achsenkreuzen] wird die tatsächlich bestehende Eichinvarianz verständlich. Und zweitens ist die Möglichkeit, die Achsenkreuze an verschiedenen Stellen unabhängig voneinander zu drehen […] gleichbedeutend mit der S y m m e t r i e d e s E n e r g i e i m p u l s t e n s o r s oder mit der Gültigkeit des Erhaltungssatzes für das Impulsmoment.”
 228.
“Zuerst will ich diejenige Seite der Sache hervorheben, bei der ich voll und ganz mit Ihnen übereinstimme: Ihr Ansatz zur Einordnung der Gravitation in die Diracsche Theorie des Spinelektrons. […] Ich bin nämlich dem Fernparallelismus ebenso feindlich gesinnt wie Sie, […]. (Und hier muss ich Ihrer Tätigkeit in der Physik Gerechtigkeit widerfahren lassen. Als Sie früher die Theorie mit g′=λg_{ ik } machten, war dies reine Mathematik und unphysikalisch, Einstein konnte mit Recht kritisieren und schimpfen. Nun ist die Stunde der Rache für Sie gekommen; jetzt hat Einstein den Bock des Fernparallelismus geschossen, der auch nur reine Mathematik ist und nichts mit Physik zu tun hat, und Sie können schimpfen!)”
 229.
“Jetzt glaube ich übrigens vom Fernparallelismus keine Silbe mehr, den Einstein scheint der liebe Gott jetzt völlig verlassen zu haben.”
 230.
“Ihre Skepsis bezüglich der Einsteinschen 4Beingeometrie teile ich vollständig. In den Osterferien habe ich Einstein in Berlin besucht und fand seine Einstellung zur modernen Quantenphysik reaktionär.”
 231.
“Ich danke Ihnen vielmals dafür, dass Sie die Korrekturen Ihrer neuen Arbeit aus den mathematischen Annalen [89] an mich senden liessen, die eine so bequeme und schöne Übersicht über die mathematischen Eigenschaften eines Kontinuums mit RiemannMetrik und Fernparallelismus enthält. […] Entgegen dem, was ich im Frühjahr zu Ihnen sagte, lässt sich vom Standpunkt der Quantentheorie nunmehr kein Argument zu Gunsten des Fernparallelismus mehr vorbringen. […] Es bleibt […] nur übrig, Ihnen zu gratulieren (oder soll ich lieber sagen: zu kondolieren?), dass Sie zu den reinen Mathematikern übergegangen sind. Ich bin auch nicht so naiv, dass ich glauben würde, Sie würden auf Grund irgendeiner Kritik durch Andere Ihre Meinung ändern. Aber ich würde jede Wette mit Ihnen eingehen, dass Sie spätestens nach einem Jahr den ganzen Fernparallelismus aufgegeben haben werden, so wie Sie früher die Affintheorie aufgegeben haben. Und ich will Sie nicht durch Fortsetzung dieses Briefes noch weiter zum Widerspruch reizen, um das Herannahen dieses natürlichen Endes der Fernparallelismustheorie nicht zu verzögern.”
 232.
“Ihr Brief ist recht amüsant, aber Ihre Stellungnahme scheint mir doch etwas oberflächlich. So dürfte nur einer schreiben, der sicher ist, die Einheit der Naturkräfte vom richtigen Standpunkt aus zu überblicken. […] Bevor die mathematischen Konsequenzen richtig durchgedacht sind, ist es keineswegs gerechtfertigt, darüber wegwerfend zu urteilen. […] Dass das von mir aufgestellte Gleichungssystem zu der zugrundegelegten Raumstruktur in einer zwangsläufigen Beziehung steht, würden Sie bei tieferem Studium bestimmt einsehn, zumal der Kompatibilit ätsbeweis der Gleichungen sich unterdessen noch hat vereinfachen lassen.”
 233.
“Einstein soll im Berliner Kolloquium schrecklichen Quatsch über neuen Fernparallelismus verzapft haben! Die blosse Tatsache, dass seine Gleichungen nicht die geringste Ähnlichkeit mit der Maxwellschen Theorie haben, will er als Argument dafür hinstellen, dass sie etwas mit Quantentheorie zu tun haben. Mit einem solchen Kohl kann man nur amerikanischen Journalisten imponieren, nicht einmal amerikanischen Physikern, geschweige denn europäischen Physikern.”
 234.
234This letter printed in Grüning’s book is not contained in the EinsteinBorn correspondence edited by Born [103].
 235.
“Dein Bericht über die Fortschritte der FernparallelismusTheorie hat mich sehr interessiert und besonders, dass die neuen Feldgleichungen von einzigartiger Einfachheit sind. Bisher hat mich nämlich immer an der Sache gestört, dass neben der so ungeheuer einfachen und durchsichtigen Geometrie die Feldtheorie so äusserst verwickelt aussah.”
 236.
“Kritik zu üben an der Schöpfung eines Mannes, der längst der Ewigkeit verschrieben ist, kommt uns nicht zu und liegt uns auch fern. Nicht als Kritik, lediglich als Eindruck sei darauf hingewiesen, weshalb der neuen Feldtheorie nicht jene Überzeugungskraft inne zu wohnen scheint, nicht jene innere Geschlossenheit und suggestive Notwendigkeit, die die frühere Theorie ausgezeichnet hat. […] Die Metrik ist eine hinreichende Basis zum Aufbau der Geometrie und man würde wahrscheinlich nicht auf den Gedanken kommen, die RIEMANNsche Geometrie durch den Fernparallelismus zu ergänzen, wenn man nicht den Wunsch hätte, etwas Neues in die RIEMANNsche Geometrie hineinzukonstruieren, um den Elektromagnetismus geometrisch zu interpretieren.”
 237.
237“Es ist schon eine kühne Tat der Redaktion, ein Referat über eine neue Feldtheorie EINSTEINs unter die Ergebnisse der exakten Naturwissenschaften aufzunehmen. Beschert uns doch seine nie versagende Erfindungsgabe sowie seine hartnäckige Energie beim Verfolgen eines bestimmten Zieles in letzter Zeit durchschnittlich etwa eine solche Theorie pro Jahr — wobei es psychologisch interessant ist, dass die jeweilige Theorie vom Autor gewöhnlich eine Zeitlang als ’definitive’ Lösung betrachtet wird. So könnte man […] ausrufen ’Die neue Feldtheorie Einsteins ist tot. Es lebe die neue Feldtheorie Einsteins!’”
 238.
“soll der Atomismus von Elektrizität und Materie ganz losgelöst von der Existenz des Wirkungsquantums, auf die Eigenschaften von (singularitätenfreien) Eigenlösungen noch aufzufindender nichtlinearer Differentialgleichungen der Feldgrössen zurückgeführt werden.”
 239.
The paper extended a previous one within the framework of special relativity [345].
 240.
“Man kann etwa sagen, dass A. Einstein eine ebene Welt aufgebaut hat, welche nicht mehr öde ist wie die euklidische RaumZeitWelt von H. Minkowski, sondern im Gegenteil alles in sich enthält, was wir als physikalische Wirklichkeit zu bezeichnen pflegen.”
 241.
“Würde man das Bewegungsgesetz der Elementarteilchen aus den überbestimmten Feldgleichungen ableiten können, so kann man sich denken, dass dieses Bewegungsgesetz nur diskrete Bahnen, im Sinne der Quantentheorie, gestatten wird.”
 242.
“Die neue Einsteinsche Gravitationstheorie steht mit der bekannten, von Ricci herrührenden Theorie der orthogonalen Kurvenkongruenzen in engem Zusammenhang. Um den Vergleich der beiden Theorien zu erleichtern, mögen hier die Bezeichnungen von R i c c i und L e v i  C i v i t a, […] mit denjenigen von Einstein zusammengestellt werden.”
 243.
Mandel’s X _{5} ^{ i } corresponds to a 5bein vector h _{5} ^{ i } .
 244.
There is no contradiction with the result of Einstein and Mayer [106]; this paper proceeds from different field equations.
 245.
Norbert Wiener (1894–1964). Born in Columbia, Missouri, U.S.A. Studied at Tufts College and Harvard University and received his doctorate with a dissertation on mathematical logic. He continued his studies in Cambridge, England and in Göttingen. From 1918 instructor at the Massachusetts Institute of Technology where he first studied Brownian motion. Wiener had a wide range of interests, from harmonic analysis to communications theory and cybernetics.
 246.
Manuel Sandoval Vallarta (1899–1977). Born in Mexico City. He studied at the Massachusetts Institute of Technology (MIT), where he received his degree in science and specialised in theoretical physics (1924). With a scholarship from the Guggenheim Foundation (1927–1928), he studied physics in Berlin and Leipzig. From 1923 to 1946, he worked as an assistant, associate, and regular professor at the MIT, and guest professor at the Lovaina University in Belgium (Cooperation with Lemaître). From 1943, he divided his time between MIT and the School of Sciences and the Institute of Physics of the National Autonomous University of Mexico (UNAM). His main contributions were in mathematic methods, quantum mechanics, general relativity and, from 1932, cosmic rays.
 247.
“Es ist mir eine angenehme Pflicht, Hrn. Dr. H. Müntz für die mühsame strenge Berechnung des zentralsymmetrischen Problems auf Grund des Hamiltonschen Prinzips zu danken; durch die Ergebnisse jener Untersuchung wurde mir die Auffindung des hier beschrittenen Weges nahegebracht.”
 248.
See Pauli’s note of 1919 concerning Weyl’s theory [243]. So far, I have not been able to find a publication by Dr. H. Müntz reporting about his calculations for Einstein. What should we conclude if none exists? That Einstein lost his interest in this particular version of unified field theory? That the calculations were erroneous, or just not reaching far enough? Further hypotheses are possible.
 249.
“Die Forderung der Existenz eines ‘überbestimmten’ Gleichungssystems mit der erforderlichen Zahl der Identitäten gibt uns ein Mittel zur Auffindung der Feldgleichungen an die Hand.”
 250.Cartan explained the generality index like this:
“[…] the general solution of a given deterministic system in involution depends on r_{2}+2p−n arbitrary functions of three variables in the sense that the 3dimensional solution (x_{4}=0) that determines the most general solution can be obtained by arbitrarily taking r_{2}+2p−n of the unknown functions to be functions of x_{1}, x_{2}, x_{3}.”
 251.
Here, and in the sequel, I mostly take over the English translation by J. Leroy and J. Ritter used in the book.
 252.
Cartan’s note was published in a very similar form in [37].
 253.
“[…] redigée en me placant au point de vue des systèmes d’équations aux dérivées partielles et non, comme dans mes mémoires, au point de vue des systémes d’équations aux différentielles totales […]”
 254.
“Ich habe Ihr Manuskript gelesen und zwar mit Begeisterung. Nun ist mir alles klar. […] Ich hatte mit meinem Assistenten Prof. Müntz früher etwas ähnliches versucht — wir sind aber nicht durchgekommen.”
 255.
“Es ist nun meine Überzeugung, dass bei ernst zu nehmenden Feldtheorien völlig Singularitätsfreiheit des ganzen Feldes verlangt werden muss. Dies wird wohl die freie Wahl der Lösungen in einem Gebiete in einer sehr weitgehenden Weise einschränken — über die Einschränkung hinaus, die Ihren Determinationsgrade entsprechen.”
 256.
“Sie vernachlässigt die Existenz der wellenmechanischen Erscheinungen. Die Wellenmechanik ist durch die Arbeiten von Dirac in eine selbständige Phase getreten, und der einzige Versuch, diese neue Gruppe von Erscheinungen mit den übrigen beiden in Zusammenhang zu bringen, ist die Theorie von J. M. Whittaker [415].”
 257.
“Diese Beziehung zwischen den wellenmechanischen Gleichungen eines ‘Elektrizitätsquantums’ und den elektromagnetischen Feldgleichungen, die man als wellenmechanische Gleichungen von Lichtquanten ansehen darf, muss wahrscheinlich eine grundlegende physikalische Bedeutung haben. Es erscheint mir daher nicht überflüssig […], die Wellengleichung des Elektrons als Verallgemeinerung der M a x w e l lschen Gleichungen aufzustellen.”
 258.
“Wir kommen also zu dem Schluss, dass unter genügend grossem Drucke selbst beim absoluten Nullpunkt gewöhnliche Materie und Hohlraumstrahlung (Lichtquantengas) in jeder Hinsicht identisch werden. Die Elektronen und Protonen sind nicht zu unterscheiden von Lichtquanten, der Gasdruck nicht vom Strahlungsdruck.”
 259.
Although the name “spinor” seems to have been suggested by Ehrenfest, Cartan first used the concept in 1913.
 260.
Scholz uses the expression “semivectors” which is reserved here for the objects of Einstein and Mayer with same name (cf. Section 7.3).
 261.
Ehrenfest had uttered much the same complaint to van der Waerden who had tried to answer to it by this paper, obviously without satisfying Ehrenfest but nevertheless laying the ground for other physicists’ understanding.
 262.
“Noch immer fehlt ein dünnes Büchlein, aus dem man gemütlich die Spinorrechnung mit der Tensorrechnung vereinigt lernen könnte.”
 263.
While Veblen denoted the covariant derivative of ψ^{ A } by \({\psi ^A}_{,\alpha }\), we are using the nablasymbol.
 264.
Unfortunately, in his paper, in contrast to his previous and our notation, Veblen now used N for the index and k for weight.
 265.
“Es ist naheliegend, zu erwarten, dass von den beiden Komponentenpaaren der D i r a cschen Grösse das eine dem Elektron, das andere dem Proton zugehört.”
 266.
“Bei jedem Versuch zur Aufstellung der quantentheoretischen Feldgleichungen muss man im Auge haben, dass diese nicht direkt mit der Erfahrung verglichen werden können, sondern erst nach ihrer Quantisierung die Unterlage liefern für die statistischen Aussagen über das Verhalten der materiellen Teilchen und Lichtquanten.”
 267.
“In den letzten zwei Jahrzehnten sind wiederholt Bestrebungen zum Ausdruck gekommen, die physikalischen Gesetze geometrischen Begriffen zuzuordnen. Im Gebiet der Gravitation und der klassischen Mechanik und haben diese Bestrebungen in E i n s t e i ns allgemeiner Relativitätstheorie ihre höchste Vollendung gefunden. Bisher hat aber die Quantenmechanik im geometrischen Bilde keinen Platz gefunden; Versuche in dieser Richtung (Klein, Fock) hatten keinen Erfolg. Erst nachdem Dirac seine Gleichungen für das Elektron aufgestellt hat, scheint der Boden zur weiteren Arbeit in dieser Richtung geschaffen zu sein.”
 268.
“C’est donc dans la loi du déplacement d’un demivecteur que doit figurer la forme différentielle lineaire de Weyl.”
 269.
“Mit Hilfe des Begriffs der Parallelübertragung eines Halbvektors werden die Diracschen Gleichungen in allgemein invarianter Form geschrieben. […] Das Auftreten des Viererpotentials φ_{ l } neben den Riccikoefficienten γ_{ ikl } in der Formel für die Parallelübertragung gibt einerseits einen einfachen geometrischen Grund für das Auftreten des Ausdrucks \({p_l}  \tfrac{e}{c}{\phi _l}\) in der Wellengleichung und zeigt andererseits, dass die Potentiale φ_{ l }, abweichend von Einsteins Auffassung, einen selbständigen Platz im geometrischen Weltbild haben und nicht etwa Funktionen der γ_{ ikl } sein müssen.”
 270.
Fock referred to his paper of 1926 [130].
 271.
“Das Auftreten der Weylschen Differentialform im Gesetz der Parallelverschiebung eines Halbvektors steht in enger Beziehung mit der vom Verfasser und auch von Weyl (l.c.) bemerkten Tatsache, dass die Addition eines Gradienten zum Viererpotential der Multiplikation der ψFunktion mit einem Faktor vom absoluten Betrag 1 entspricht.”
 272.
“Le potentielvecteur trouve sa place dans la géométrie de Riemann, et on n’a pas besoin de la généraliser (Weyl, 1918) ou d’introduire le parallélisme à distance (Einstein 1928). Dans ce point notre théorie — développée indépendamment — s’accorde avec la nouvelle théorie de H. Weyl exposée dans son mémoire ‘Gravitation et Électron’.”
 273.
By ‘Dirac’s difficulty’ we must understand the existence of negative energy states of the electron and the nonvanishing probability that a change of electrical charge occurs.
 274.
“L’objet principal de ce mémoire est la ‘difficulté de Dirac’. La théorie proposée par Weyl pour résoudre cette difficulté nous semble, cependant, ouverte à de graves objections; une critique de cette théorie est donnée dans notre article cité au debut [this is [135]].”
 275.
During a discussion with Frenkel, he also insisted that, in Kaluza’s approach, the meaning of the fifth coordinate is to be seen in the “preservation of invariance against adding a gradient to the [electromagnetic] vector potential” (p. 651).
 276.
“Es sind kürzlich wiederholt Versuche gemacht worden (H. Mandel, G. Rumer, Verfasser u. a.), die Dimensionszahl der Welt zwecks Deutung ihrer sonderbaren Gesetzlichkeit zu erhöhen. Es gibt zwar gewichtige Gründe zu einer solchen augenscheinlich paradoxen Anschauung. Denn es ist gar nicht möglich, den Poincaréschen Druck des Elektrons in dem üblichen RaumZeitschema darzustellen. Aber die Einführung derartiger metaphysischer Elemente steht in grobem Widerspruch mit der raumzeitlichen Kausalität, obwohl wir andererseits nach der Heisenbergschen Unschärferelation eine Kausalität im üblichen Sinne bezweifeln dürfen. Ein mehrdimensionaler Determinismus ist jedoch unbegreiflich, solange wir nicht in der Lage sind, den überschüssigen Dimensionen einen anschaulichen Sinn beizulegen.”
 277.
Pseudotensors of class k are defined by help of an auxiliary variable ξ^{0} transforming like ξ^{0′}=σξ^{0}; in their transformation law the multiplicative factor σ^{ k } occurs. σ is a function of the coordinates involved in the tensor transformation law.
 278.
“Die Vereinigung der Diracschen Theorie des Elektrons mit der allgemeinen Relativitätstheorie ist schon wiederholt in Angriff genommen worden, […]. Die meisten Autoren führen in jedem Weltpunkt ein orthogonales Achsenkreuz und in bezug auf dieses numerisch spezialisierte Diracsche Matrizen ein. Bei diesem Verfahren ist es ein bisschen schwer, zu erkennen, ob die Einsteinsche Idee des Fernparallelismus, auf die teilweise Bezug genommen wird, wirklich hereinspielt oder ob man davon unabhängig ist […]. Ein grundsätzlicher Vorzug scheint es mir, dass sich der ganze Apparat fast vollständig durch reinen Operatorenkalkül aufbauen lässt, ohne auf die ψFunktion Bezug zu nehmen.”
 279.
“Das zweite Glied scheint mir von erheblichem theoretischen Interesse. Es ist freilich um viele Zehnerpotenzen zu klein, um etwa das Glied rechter Hand ersetzen zu können. Denn μ ist die reziproke ComptonWellenlänge, ungefähr 10^{11} cm^{1}. Immerhin scheint es bedeutungsvoll, dass in der verallgemeinerten Theorie überhaupt ein mit dem rätselhaften Massenglied gleichartiges angetroffen wird.”
 280.
For arbitrary dimension D≥2 of the manifold M_{ D }, the coefficient in the conformally invariant equation is \(\tfrac{{D  2}}{{4(D  1)}}\).
 281.
“Ihre grundlegende Abhandlung hat mich veranlasst, die Rechnungseinzelheiten zu entwickeln, um von den Diracschen Gleichungen im allgemeinen Schwerefeld die modifizierte Form ihrer vier Gleichungen zweiter Ordnung zu gewinnen und so die entsprechenden Zusatzglieder festzustellen. Diese Zusatzglieder hängen in wesentlicherWeise von der Wahl des orthogonalen Vierbeines der Raumzeitmannigfaltigkeit ab: ein solches Bein scheint unentbehrlich zu sein, um die Diracschen Gleichungen zu bekommen.”
 282.
“Der Leichenberg, hinter dem allerlei Gesindel Deckung sucht, hat einen Zuwachs erfahren. Es wird gewarnt vor der Arbeit von LeviCivita: Diracsche und Schrödingersche Gleichungen, Berliner Berichte 1933. Alle sollten abgehalten werden, diese Arbeit zu lesen oder gar zu versuchen, sie zu verstehen. Ferner gehören sämtliche auf S. 241 dieser Arbeit zitierten Arbeiten dem Leichenberge an.”
 283.
Sedenions or quadriquaternions form a system of 16 elements of an associative algebra; they are formed by the unit element 1, four elements E_{ i } with E_{ i }E_{ i }=1; E_{ i }E_{ j }=E_{ j }E_{ i } and their products.
 284.
“Schouten kommt am Ende nahezu zum gleichen Formalismus, der in dieser Arbeit entwickelt wird; nur benutzt er zur Einführung dieses Formalismus unnötigerweise nBeinkomponenten und Sätze über Sedenionen, während der Formalismus nachher noch durch Hilfsvariable und Pseudogrössen belastet wird. Die Einführung von ‘Spinordichten’ haben wir von Schouten übernommen.”
 285.
“Vorige Woche habe ich der Akademie eine kleine Arbeit eingereicht, in der ich zeigte, dass man der Schrödinger Wellenmechanik ganz bestimmte Bewegungen zuordnen kann, ohne jede statistische Deutung. Erscheint baldigst in den Sitz.Ber.”
 286.
The symbol ^{ s }h_{λ} for the tetrad field is due to Weitzenböck.
 287.
“dass für die neue Einsteinsche Feldtheorie gewisse quantenmechanische Züge charakteristisch sind und dass man hoffen darf, dass die Theorie die Erfassung der Quantengesetze des Mikrokosmos ermöglichen wird.”
 288.
For the alphamatrices, cf. Equation (88).
 289.
Ferdinand Gonseth (1890–1975). Born in Sonvilier, Switzerland. Mathematician teaching first at the University of Bern and then at the Federal Institute of Technology (ETH) Zurich. His interest were in the foundations of mathematics, geometry and in problems of space and time. With G. Bachelard and P. Bernays he founded the philosophical review journal Dialectica.
 290.
“L’object de cette note est de formuler une relativité à cinq dimensions dont les équations fourniront les lois du champ gravifique, du champ électromagnétique, les lois du mouvement d’un point matériel chargé et l’équation des ondes de M. Schrödinger. Nous aurons ainsi un cadre dans lequel entreront les lois de la gravitation et de l’électromagnétisme, et où il sera possible de faire entrer aussi la théorie des quanta.”
 291.
“On voit ainsi que la fiction d’un univers à cinq dimensions permet de donner une raison profonde à l’équation de Schrödinger. Il est clair que cet artifice deviendrait nécessaire si quelque phénomène obligeait les physiciens à croir à la variabilité de la charge.”
 292.
Gordon has not given a tensorial form of Dirac’s equation but his wellknown decomposition of the Dirac current into a conduction and a polarisation part.
 293.
“in manchen Fällen kann wohl eigentlich von einer quasimakroskopischen Betrachtung des Einkörperproblems die Rede sein, man denke etwa an ein Bündel von monochromatischen Kathodenstrahlen.”
 294.
“Das entspricht vollständig dem Verfahren der Diracschen Theorie, nur mit dem Unterschied, dass bei Dirac die Koordinate ξ nicht zwei, sondern vier Werte haben konnte, was von unserem Standpunkt aus unverständlich bleibt.”
 295.
Although Zaycoff does not say it, he takes ψ̃ as the complexconjugate transposed function.
 296.
“Die folgenden Ausführungen sollen […] zeigen, dass die einheitliche Zusammenfassung des Gravitations und des elektromagnetischen Feldes durch die projektive Differentialgeometrie mittels fünf homogener Koordinaten eine allgemeine Methode ist, deren Tragweite über die klassische Feldphysik hinaus und in die Quantentheorie hineinreicht. Vielleicht ist es nicht unberechtigt, zu hoffen, dass die Methode als allgemeiner Rahmen der physikalischen Gesetze sich auch gegenüber einer künftigen physikalischbegrifflichen Verbesserung der Grundlagen der Diracschen Theorie bewähren wird.”
 297.
Ψ^{⋇} is the complex conjugate and transposed object.
 298.
“schwer verständlich und unübersichtlich”
 299.
“Bei der grossen Bedeutung, welche der von P a u l i und D i r a c eingeführte SpinorBegriff in der Molekularphysik erlangt hat, kann doch nicht behauptet werden, dass die bisherige mathematische Analyse dieses Begriffs allen berechtigten Ansprüchen genüge. […] Unsere Bemühungen haben zu einer Ableitung geführt, welche nach unserer Meinung allen Ansprüchen an Klarheit und Natürlichkeit entspricht und undurchsichtige Kunstgriffe völlig vermeidet. Dabei hat sich […] die Einführung neuartiger Grössen, der ‘SemiVektoren’, als notwendig erwiesen, welche die Spinoren in sich begreifen, aber einen wesentlich durchsichtigeren Transformationscharakter besitzen als die Spinoren.”
 300.
“Ich arbeite mit meinem Dr. Mayer an der Theorie der Spinoren. Wir haben die mathematischen Zusammenhänge schon klären können. Von einer Erfassung des Physikalischen ist man noch weit entfernt, viel weiter, als man gegenwärtig denkt. Besonders bin ich nach wie vor davon überzeugt, dass der Versuch einer wesentlich statistischen Theorie scheitern wird.”
 301.
Two matrices B and C are called commuting if [B, C]:=BC−CB=0.
 302.
∊_{ ijkl }, the components of which are either ±1 or 0, is the totally antisymmetric (LeviCivita) tensor density keeping its components fixed under any coordinate transformation (cf. Section 2.1.5).
 303.
All indices run from 1 to 4.
 304.
“[…] Louis de Broglie erriet die Existenz einesWellenfeldes, das zur Deutung von gewissen Quanteneigenschaften der Materie verwendbar war. Dirac fand in den Spinoren neuartige Feldgrössen, deren einfachste Gleichungen die Eigenschaften des Elektrons weitgehend abzuleiten gestatten. Ich fand nun mit meinem Mitarbeiter, Dr. Walther Mayer, dass diese Spinoren einen Spezialfall einer, mathematisch mit dem Vierdimensionalen verknüpften Feldart bilden, die wir als ‘Semivektoren’ bezeichneten. Die einfachsten Gleichungen, welchen solche Semivektoren unterworfen werden können, geben einen Schlüssel für das Verständnis der Existenz von zweierlei Elementarteilchen verschiedener ponderabler Masse und gleicher, aber entgegengesetzter Ladung. Diese Semivektoren sind nach den gewöhnlichen Vektoren die einfachsten mathematischen Feldgebilde, die in einem metrischen Kontinuum von vier Dimensionen möglich sind, und es scheint, dass sie zwanglos wesentliche Eigenschaften der elektrischen Elementarteilchen beschreiben.”
 305.
“Der Raum der Semivektoren erster bzw. zweiter Art ist die Mannigfaltigkeit der Systeme von zwei einfachen Bivektoren der lokalen Raumzeitwelt, die in zwei Ebenen des ersten bzw. zweiten Ebenensystems auf dem Nullkegel liegen. […] In der nicht projektiven Theorie sowie in der projektiven bei fehlendem elektromagnetichen Feld haben die Semivektoren einen Vorzug, […]. Sobald in der projektiven Theorie ein elektromagnetisches Feld auftritt, ist die Rechnung mit Spinvektoren einfacher als die mit Semivektoren.”
 306.
Schouten referred to Pauli several times ([308], pp. 406, 414, 416–417).
 307.
In his letter to Einstein, Pauli had also mentioned his papers to be published in Annalen der Physik and discussed in Section 7.2.3.
 308.
 309.
Dirac had made an antiparticle to the electron appear in his theory as early as in 1930 [55].
 310.
“Dabei ergibt sich ohne weitere Hypothese die Existenz von zueinander entgegengesetzt geladenen Teilchen gleicher Ruhmasse, die unter Absorption bzw. Emission von elektromagnetischer Strahlung paarweise erzeugt bzw. vernichtet werden können. Die Häufigkeit solcher Prozesse erweist sich als von derselben Grössenordnung wie die für Teilchen derselben Ladung und Masse aus der Diracschen Löchertheorie folgende.”
 311.
“Wir haben gesehen dass ein V_{3} entweder selbst ein F_{3} ist (dann ist er leer) oder ein Unterraum von F_{4} (dann ist in ihm ein Gravitationsfeld vorhanden), oder ein Unterraum von F_{5} (dann ist in ihm auch ein reines Elektrizitätsfeld vorhanden). Wo also noch ‘etwas’ ist, das weder Gravitationsfeld noch Elektrizitätsfeld ist, muss der V_{3} ein Unterraum in F_{ n } (n≥6) sein. Nun zeigt aber die Geometrie, dass jeder V_{3} ein Unterraum eines speziellen F_{6}, nämlich des euklidischen oder pseudoeuklidischen Raumens ist. Das zeigt uns, dass der Übergang zum F_{6} auch der letzte Schritt ist.”
 312.
“[…] Anregungen und das Interesse, das er dem Werden dieser Arbeit entgegenbrachte.”
 313.
Born tried to support Rumer in various ways, as can be seen from his correspondence with Einstein [103].
 314.
“[…] tauchte hier ein junger Russe auf, der eine 6dimensionale Relativitätsheorie mitbrachte. Da ich bereits vor den verschiedenen 5dimensionalen Theorien Angstgefühle empfand und wenig Zuversicht, dass auf diesem Wege etwas Schönes herauskommen könnte, war ich sehr skeptisch.”
 315.
“[…] aus den allgemeinen Eigenschaften der Riemannschen Geometrie, unter Zugrundelegung eines durch eine sehr natürliche Forderung ausgezeichneten Wirkungsprinzips, ohne jeden besonderen Kunstgriff die Grundeigenschaften des elektromagnetischen Feldes zwanglos abgeleitet werden können.”
 316.
Ludwig Berwald (1883–1942). Born in Prague. Studied mathematics in Munich and became a full professor at the German Charles University in Prague. His scientific work is mainly in differential geometry, notably on Finsler geometry and on spray geometry, i.e., path spaces. He died in Poland after having been deported by the German authorities just because he was Jewish.
 317.
“Die Theorie der Differentialformen (Tensoren) hat mit Rücksicht auf ihre Verwendung in modernen physikalischen Theorien in den letzten Jahren eine ausführliche Bearbeitung erfahren. Wir erwähnen Ricci, LeviCivita, Hessenberg, Einstein, Hilbert, [Felix] Klein, E. Noether, Weyl.”
 318.
“Herrn L. Berwald in Prag, mit dem ich seit September 1921 in regem Gedankenaustausch stand und der mir seine Manuskripte schon vor der Drucklegung freundlichst zur Verfügung stellte, schulde ich Dank.”
 319.
“Herr Pauli hatte die Freundlichkeit, zu erlauben, diesen Satz aus einem noch nicht publizierten Manuskript zu zitieren.”
 320.
“Eine Korrespondenz mit Herrn Pauli veranlasste mich, diese Invarianz zu untersuchen.”
 321.
“Hilbert, Klein [i.e., Felix Klein], Weyl und andere Mathematiker haben dabei mitgewirkt und die formale Struktur der Einsteinschen Formeln tief durchforscht und aufgehellt.”
 322.
Förster wrote his thesis in mathematics [137].
 323.
 324.
“On voit […] la variété des aspects sous lesquels peut etre envisagée la théorie unitaire du champ et aussi la difficulté des problèmes qu‘elle soulève. Mais M. Einstein n’est pas de ceux à qui les difficultés font peur et, meme si sa tentative n‘aboutit pas, elle nous aura forcés à réfléchir sur les grandes questions qui sont à la base de la science.”
 325.
“À l’heure actuelle cette nouvelle théorie n’est qu’un édifice mathématique, à peine relié par quelques liens très lâches à la réalité physique. Elle a été découverte par des considérations exclusivement formelles et ses conséquences mathématiques n’ont pas pu être suffisamment développées pour permettre la comparaison avec l’expérience. Néanmoins, cette tentative me semble très intéressante en ellemême; elle offre surtout de magnifique possibilités de développemnet et c’est dans l’espoir que les mathématiciens s’y intéressont, que je me permets de l’exposer et de l’analyser ici.”
 326.
Compare with the fate of contemporaneaous (quantum) geometrodynamics [328].
 327.
“Das Gelingen dieses Versuches, aus der Überzeugung der formalen Einheit der Struktur des Wirklichen heraus auf rein gedanklichemWege subtile Naturgesetze abzuleiten, ermutigt zu einem Fortschreiten auf diesem spekulativen Wege, dessen Gefahren sich jeder lebhaft vor Augen halten muss, der ihn zu beschreiten wagt.”
 328.
“Das sieht altertümlich aus und die lieben Kollegen sowie auch Du, mein Lieber, werden zunächst einmal die Zunge herausstrecken solange es geht. Denn in diesen Gleichungen kommt kein Planck’sches h vor. Aber wenn man an die Leistungsgrenzen des statistischen Fimmels deutlich gelangt sein wird, wird man wieder zur zeiträumlichen Auffassung reuevoll zurückkehren und dann werden diese Gleichungen einen Ausgangspunkt bilden.”
 329.
My reservations hold only if the toolbox does not also contain quantum field theory.
 330.
“Nach dem heutigen Stand der Dinge wird man weder von klassischen noch von quantentheoretischen Methoden ‘alles’ erwarten, sondern sich eher jener mehrfach geäusserten Meinung anschliessen, dass das Feldproblem auf klassischem Boden weitergeführt werden muss, ehe es der Quantentheorie neuere Angriffspunkte zu bieten vermag. Eben deshalb ist es bedauerlich, dass nach jenen gross angelegten Entwürfen, wie sie in der Eichungstheorie und im Fernparallelismus vorliegen, weitere Versuche in klassischer Richtung nicht zu vermerken sind.”
Notes
Acknowledgements
The carefully worded and detailed comments of a referee have been helpful in improving on the original version. I would also like to thank the staff of Living Reviews, notably Mrs. Christina Weyher and Mr. Robert Forkel, for their friendly and generous assistance.
References
 [1]“MacTutor History of Mathematics Archive”, web interface to database, University of St Andrews. URL (cited on 28 January 2003): http://turnbull.mcs.stand.ac.uk/history/. 1.1
 [2]“News and Views”, Nature, 123(3092), 174–175, (1929). [DOI]. 6.4.2Google Scholar
 [3]Anderson, W., “Gewöhnliche Materie und strahlende Energie als verschiedene ‘Phasen’ eines und desselben Grundstoffes”, Z. Phys., 54, 433–444, (1929). [DOI]. 7.1ADSzbMATHCrossRefGoogle Scholar
 [4]Bach, R., “Zur Weylschen Relativitätstheorie und der Weylschen Erweiterung des Krümmungsbegriffs”, Math. Z., 9, 110–135, (1921). [DOI]. 58, 4.1.1, 9MathSciNetzbMATHCrossRefGoogle Scholar
 [5]Bargmann, V., “über eine Verallgemeinerung des Einsteinschen Raumtyps”, Z. Phys., 65, 830–847, (1930). [DOI]. 225, 6.4.5ADSzbMATHCrossRefGoogle Scholar
 [6]Bargmann, V., “Bemerkungen zur allgemeinrelativistischen Fassung der Quantentheorie”, Sitzungsber. Preuss. Akad. Wiss., 1932(XXIV), 346–354, (1932). 7.2.1, 7.2.2, 7.2.4zbMATHGoogle Scholar
 [7]Bargmann, V., “über den Zusammenhang zwischen Semivektoren und Spinoren und die Reduktion der Diracgleichungen für Semivektoren”, Helv. Phys. Acta, 7, 57–82, (1934). 7.3zbMATHGoogle Scholar
 [8]Bargmann, V., “Relativity”, in Fierz, M., and Weisskopf, V.F., eds., Theoretical Physics in the Twentieth Century: A Memorial Volume to Wolfgang Pauli, pp. 187–198, (Interscience Publishers, New York, 1960). 140Google Scholar
 [9]Beck, G., “Allgemeine Relativitätstheorie”, in Geiger, H., and Scheel, K., eds., Handbuch der Physik, Vol. 4, pp. 299–407, (Springer, Berlin, 1929). 10Google Scholar
 [10]Becquerel, J., Le Principe de relativité et la théorie de la gravitation, (GauthierVillars, Paris, 1922). 10zbMATHGoogle Scholar
 [11]Bergia, S., “Attempts at Unified Field Theories (1919–1955). Alleged Failure and Intrinsic Validation/Refutation Criteria”, in Earman, J., Janssen, M., and Norton, J.D., eds., The Attraction of Gravitation: New Studies in the History of General Relativity, Einstein Studies, vol. 5, pp. 274–307, (Birkhäuser, Boston; Basel, 1993). [Google Books]. 1.1ADSMathSciNetGoogle Scholar
 [12]Bergmann, P.G., “Unitary Field Theory: Yesterday, Today, Tomorrow”, in Treder, H.J., ed., EinsteinCentenarium 1979, Ansprachen und Vorträge auf der Festveranstaltung des EinsteinKomitees der DDR bei der Akademie der Wissenschaften der DDR vom 28.2. — 2.3. 1979 in Berlin, (AkademieVerlag, Berlin, 1979). 1.1Google Scholar
 [13]Berwald, L., “Differentialinvarianten in der Geometrie. Riemannsche Mannigfaltigkeiten und ihre Verallgemeinerungen”, in Meyer, W.F., and Mohrmann, H., eds., Enzyklopädie der Mathematischen Wissenschaften mit Einschluss ihrer Anwendungen, Band III, 3. Teil, D 11, pp. 73–181, (Teubner, Leipzig, 1923). Related online version (cited on 30 October 2009): http://gdz.sub.unigoettingen.de/dms/load/img/?PPN=PPN360610161&DMDID=dmdlog384. 9Google Scholar
 [14]Biezunski, M., La diffusion de la théorie de la relativité en France, Ph.D. Thesis, (Université VII, Département de Didactique des Sciences physiques et de la Technologie, Paris, 1981). 6.4.3Google Scholar
 [15]Biezunski, M., “Inside the coconut: The EinsteinCartan discussion”, in Howard, D., and Stachel, J., eds., Einstein and the History of General Relativity, Based on the proceedings of the 1986 Osgood Hill Conference, North Andover, Massachusetts, 8–11 May 1986, Einstein Studies, vol. 1, pp. 315–324, (Birkhäuser, Boston; Basel, 1989). 223ADSMathSciNetGoogle Scholar
 [16]Biezunski, M., Histoire de la physique moderne, (La Découverte, Paris, 1993). 1.2Google Scholar
 [17]Birkhoff, G.D., “The hydrogen atom and the Balmer formula”, Proc. Natl. Acad. Sci. USA, 13, 165–169, (1927). [DOI]. 8ADSMathSciNetzbMATHCrossRefGoogle Scholar
 [18]Birkhoff, G.D., “A theory of matter and electricity”, Proc. Natl. Acad. Sci. USA, 13, 160–165, (1927). [DOI]. 8ADSCrossRefGoogle Scholar
 [19]Born, M., Die Relativitätstheorie Einsteins und ihre physikalischen Grundlagen, (Springer, Berlin, 1920). 3.2, 10zbMATHCrossRefGoogle Scholar
 [20]Born, M., Die Relativitätstheorie Einsteins und ihre physikalischen Grundlagen, (Springer, Berlin, 1922), 2nd edition. 10zbMATHCrossRefGoogle Scholar
 [21]Born, M., “Quelques problèmes de méchanique quantique”, Ann. Inst. Henri Poincare, 1, 205–284, (1930). 6.4.3MathSciNetzbMATHGoogle Scholar
 [22]Bortolotti, E., “On metric connections with absolute parallelism”, Proc. K. Akad. Wetensch., 30, 216–218, (1927). 6.4.5zbMATHGoogle Scholar
 [23]Bortolotti, E., “Parallelismo assoluto nella varietá a connessione affine e nuove veduti sulla relativitá”, Mem. Accad. Sci. Ist. Bologna, Cl. Sci. Fis., 6, 45–58, (1928). 6.4.5Google Scholar
 [24]Bortolotti, E., “Stelle di congruenze e parallelisme assoluto: basi geometriche di una recente teoria di Einstein”, Rend. Lincei, 9, 530–538, (1929). 6.3.2, 6.4.5zbMATHGoogle Scholar
 [25]Bortolotti, E., “Stelle di congruenze e parallelisme assoluto: basi geometriche di una recente teoria di Einstein”, Rend. Lincei, 9, 530–538, (1929). 6.4.5zbMATHGoogle Scholar
 [26]Boyd, P.T., Centrella, J.M., and Klasky, S.A., “Properties of gravitational ‘solitons’”, Phys. Rev. D, 43, 379–90, (1991). 1.2ADSMathSciNetCrossRefGoogle Scholar
 [27]Buchdahl, H.A., “Gaugeinvariant generalization of field theories with asymmetric fundamental tensor”, Quart. J. Math., 8, 89–96, (1957). [DOI]. 80ADSMathSciNetzbMATHCrossRefGoogle Scholar
 [28]Cao, T.Y., Conceptual developments of 20th century field theories, (Cambridge University Press, Cambridge, 1997). 1.2zbMATHCrossRefGoogle Scholar
 [29]Cartan, é., “Sur les équations de structure des espaces généralisés et l‘Univers optique”, C. R. Acad. Sci., 174, 857–859, (1922). 3zbMATHGoogle Scholar
 [30]Cartan, é., “Sur les espaces généralisés et la théorie de la relativité”, C. R. Acad. Sci., 174, 734–737, (1922). 6.4.1zbMATHGoogle Scholar
 [31]Cartan, é., “Sur les variétés à connexion affine courbure de Riemann et les espaces à torsion”, C. R. Acad. Sci., 174, 593–595, (1922). 6.4.1zbMATHGoogle Scholar
 [32]Cartan, é., “Sur les variétés à connexion affine et la théorie de la relativité généralisée”, Ann. Sci. Ecole Norm. Sup., 40, 325–412, (1923). 5, 6.4.1MathSciNetzbMATHGoogle Scholar
 [33]Cartan, é., “Sur les espaces de Riemann dans lesquels le transport par parallélism conserve la courbure”, Rend. Lincei, 3(6), 544–547, (1926). 6.4.1zbMATHGoogle Scholar
 [34]Cartan, é., “La Géométrie des groupes de transformations”, J. Math. Pures Appl., 6, 1–119, (1927). 6.4.1MathSciNetzbMATHGoogle Scholar
 [35]Cartan, é., “Notice historique sur la notion de parallélisme absolu”, Math. Ann., 102, 698–706, (1930). [DOI]. 6.4.1, 6.4.3MathSciNetzbMATHCrossRefGoogle Scholar
 [36]Cartan, é., “Le parallelisme absolu et la théorie unitaire du champ”, Rev. Metaphys. Morale, 38, 13–28, (1931). Oeuvres Complètes, tome III, 2 pp. 1167–1185. 3.2, 11zbMATHGoogle Scholar
 [37]Cartan, é., “Sur la théorie des systèmes en involution et ses applications à la Relativité”, Bull. Soc. Math. France, 59, 88–118, (1931). 6.3.2, 252MathSciNetzbMATHGoogle Scholar
 [38]Cartan, é., Oeuvres Complètes, (GauthierVillars, Paris, 1950). 3 parts with 2 vols. each, 1950–1955. 24Google Scholar
 [39]Cartan, é., “La théorie unitaire d’EinsteinMayer”, in Oeuvres Complètes, Vol. III/2, pp. 1863–1875, (GauthierVillars, Paris, 1955). manuscrit datant de 1934 environ. 6.3.2Google Scholar
 [40]Cartan, é., and Schouten, J.A., “On Riemaniann geometries admitting an absolute parallelism”, Proc. K. Akad. Wetensch., 29, 933–946, (1926). 6.4.1zbMATHGoogle Scholar
 [41]Cartan, é., and Schouten, J.A., “On the Geometry of the Groupmanifold of Simple and Semisimple Groups”, Proc. K. Akad. Wetensch., 29, 803–815, (1926). 6.4.1zbMATHGoogle Scholar
 [42]Chandrasekhar, S., Eddington: The most distinguished astrophysicist of his time, (Cambridge University Press, Cambridge, 1983). [Google Books]. 10zbMATHCrossRefGoogle Scholar
 [43]Darrieus, M.G., “Sur une form remarquable des équations de MaxwellLorentz dans l’univers à cinq dimensions”, J. Phys. Radium, 8, 444–446, (1927). [DOI]. 6.3.1zbMATHCrossRefGoogle Scholar
 [44]Darwin, C.G., “The wave equations of the electron”, Proc. R. Soc. London, Ser. A, 118, 654–680, (1928). 7.1ADSzbMATHGoogle Scholar
 [45]Darwin, C.G., “La théorie ondulatoire de la matière”, Ann. Inst. Henri Poincare, 1, 25–51, (1930). 6.4.3MathSciNetGoogle Scholar
 [46]de Broglie, L., “L’univers à cinq dimensions et la mécanique ondulatoire”, J. Phys. Radium, 8, 65–73, (1927). [DOI]. 6.3.1zbMATHCrossRefGoogle Scholar
 [47]de Broglie, L., “Réponse à la note de M. O. Klein”, J. Phys. Radium, 8, 244, (1927). [DOI]. 6.3.1zbMATHCrossRefGoogle Scholar
 [48]de Donder, T.E., “Généralisation relativiste de la nouvelle théorie d’Einstein”, C. R. Acad. Sci., 187, 817–819, (1928). 6.4.3, 6.4.5zbMATHGoogle Scholar
 [49]De Sabbata, V., and Schmutzer, E., eds., Unified field theories in more than 4 dimensions, Proceedings of the International School of Cosmology and Gravitation, held at Erice, Italy, 20 May–1 June 1982, (World Scientific, Singapore, 1983). 102, 4.2Google Scholar
 [50]Debever, R., ed., élie Cartan — Albert Einstein: Lettres sur le parallélisme absolu 1929–1932, (Academie Royale de Belgique, Brussels, 1979). 6.4.1, 6.4.3, 6.4.3, 6.4.3, 6.4.4, 6.4.6Google Scholar
 [51]Dienes, P., “Sur la théorie électromagnétique relativiste”, C. R. Acad. Sci., 176, 238–241, (1923). 4.1.5zbMATHGoogle Scholar
 [52]Dirac, P.A.M., “The quantum theory of emission and absorption of radiation”, Proc. R. Soc. London, Ser. A, 114, 243–265, (1927). 1.2ADSzbMATHCrossRefGoogle Scholar
 [53]Dirac, P.A.M., “The quantum theory of the electron”, Proc. R. Soc. London, Ser. A, 117, 610–624, (1928). 2.1.5.2ADSzbMATHCrossRefGoogle Scholar
 [54]Dirac, P.A.M., “The quantum theory of the electron”, Proc. R. Soc. London, Ser. A, 118, 351–361, (1928). 2.1.5.2ADSzbMATHCrossRefGoogle Scholar
 [55]Dirac, P.A.M., “A Theory of Electrons and Protons”, Proc. R. Soc. London, Ser. A, 126, 360–365, (1930). 12, 309ADSzbMATHCrossRefGoogle Scholar
 [56]Dirac, P.A.M., “Quantised Singularities in the Electromagnetic Field”, Proc. R. Soc. London, Ser. A, 133, 60–72, (1931). 12ADSzbMATHCrossRefGoogle Scholar
 [57]Eddington, A.S., Space, Time, and Gravitation: An outline of the general relativity theory, (Cambiridge University Press, Cambridge, 1920). 4.1.4, 10Google Scholar
 [58]Eddington, A.S., “A generalisation of Weyl’s theory of the electromagnetic and gravitational fields”, Proc. R. Soc. London, Ser. A, 99, 104–122, (1921). 4.3.1, 4.3.1, 4.3.1, 5ADSzbMATHCrossRefGoogle Scholar
 [59]Eddington, A.S., The mathematical theory of relativity, (Cambridge University Press, Cambridge, 1924), 2nd edition. 1st edition 1923. 2.1.1, 4.1.4, 4.1.5zbMATHGoogle Scholar
 [60]Eddington, A.S., Relativitätstheorie in mathematischer Behandlung, (Springer, Berlin, 1925). 4.3.3, 5, 6.2, 10zbMATHGoogle Scholar
 [61]Eddington, A.S., “A symmetrical treatment of the wave equation”, Proc. R. Soc. London, Ser. A, 121, 524–542, (1928). 7.2.4, 7.2.4, 9ADSzbMATHCrossRefGoogle Scholar
 [62]Eddington, A.S., “Einstein’s FieldTheory”, Nature, 123(3095), 280–281, (1929). [DOI]. 6.4.4, 6.4.5ADSzbMATHCrossRefGoogle Scholar
 [63]Eddington, A.S., The Expanding Universe, (Cambridge University Press, Cambridge, 1933). 4.3.1zbMATHCrossRefGoogle Scholar
 [64]Eddington, A.S., The Mathematical Theory of Relativity, (Cambridge University Press, Cambridge, 1960). Reprint of the 1st ed. 1923. 4.3.1, 4.3.3Google Scholar
 [65]Ehlers, J., “The nature and structure of spacetime”, in Mehra, J., ed., The Physicists Conception of Nature, Symposium held at ICTP, Miramare, Trieste, Italy, 18–25 September 1972, (Reidel, Dordrecht; Boston, 1973). 2.1.3.2Google Scholar
 [66]Ehlers, J., “über den Newtonschen Grenzwert der Einsteinschen Gravitationstheorie”, in Nitsch, J., Pfarr, J., and Stachow, E.W., eds., Grundlagenprobleme der modernen Physik: Festschrift für Peter Mittelstaedt zum 50. Geburtstag, (Bibliographisches Institut, Mannheim, 1981). 2.1.3.2Google Scholar
 [67]Ehlers, J., Pirani, F.A.E., and Schild, A., “The Geometry of Free Fall and Light Propagation”, in O’Raiffeartaigh, L., ed., Studies in Relativity: Papers in honour of J. L. Synge, pp. 63–84, (Clarendon Press, Oxford, 1972). 2.1.1, 2.1.3.2Google Scholar
 [68]Ehrenfest, P., “Einige die Quantenmechanik betreffende Erkundigungsfragen”, Z. Phys., 78, 555–559, (1932). [DOI]. 7.2.1ADSzbMATHCrossRefGoogle Scholar
 [69]Einstein, A., “Letter to De Haas, May 7, 1933”, personal communication. 7.3Google Scholar
 [70]Einstein, A., “Spielen Gravitationsfelder im Aufbau der materiellen Elementarteilchen eine wesentliche Rolle?”, Sitzungsber. Preuss. Akad. Wiss., 1919(XX), 349–356, (1919). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/69YV118A. 3.2, 69, 4, 6.1Google Scholar
 [71]Einstein, A., “Antwort auf vorstehende Betrachtung”, Die Naturwissenschaften, 8, 1010–1011, (1920). [DOI]. 3.1ADSCrossRefGoogle Scholar
 [72]Einstein, A., “Geometrie und Erfahrung”, Sitzungsber. Preuss. Akad. Wiss., 1921(V), 123–130, (1921). 3.2, 4zbMATHGoogle Scholar
 [73]Einstein, A., “über eine naheliegende Ergänzung des Fundamentes der allgemeinen Relativit ätstheorie”, Sitzungsber. Preuss. Akad. Wiss., 1921(XII) 261–264, (1921). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/QAB7NNDB. 4.1.5zbMATHGoogle Scholar
 [74]Einstein, A., “Bemerkungen zu meiner Arbeit ‘Zur allgemeinen Relativitätstheorie’”, Sitzungsber. Preuss. Akad. Wiss., 1923(XII), 76–77, (1923). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/EVSSPDP8. 4.3.2, 5, 9zbMATHGoogle Scholar
 [75]Einstein, A., “Bietet die Feldtheorie Möglichkeiten zur Lösung des Quantenproblems?”, Sitzungsber. Preuss. Akad. Wiss., 1923, 359–364, (1923). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/MXYDBZW5. 4.3.4zbMATHGoogle Scholar
 [76]Einstein, A., “Zur affinen Feldtheorie”, Sitzungsber. Preuss. Akad. Wiss., 1923(XVII), 137–140, (1923). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/GBEHMB2D. 4.3.2, 9Google Scholar
 [77]Einstein, A., “Zur allgemeinen Relativitätstheorie”, Sitzungsber. Preuss. Akad. Wiss., 1923(V), 32–38, (1923). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/B98WXTVX. 42, 4.3.2, 4.3.2, 5, 9zbMATHGoogle Scholar
 [78]Einstein, A., “Einheitliche Feldtheorie von Gravitation und Elektrizität”, Sitzungsber. Preuss. Akad. Wiss., 1925(XXII), 414–419, (1925). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/ZHDAXTXQ. 6.1zbMATHGoogle Scholar
 [79]Einstein, A., “Elektron und allgemeine Relativitätstheorie”, Physica, 5, 330–334, (1925). 6.1zbMATHGoogle Scholar
 [80]Einstein, A., “über die formale Beziehung des Riemannschen Krümmungstensors zu den Feldgleichungen der Gravitation”, Math. Ann., 97, 99–103, (1927). [DOI]. 6.1MathSciNetzbMATHCrossRefGoogle Scholar
 [81]Einstein, A., “Zu Kaluzas Theorie des Zusammenhangs von Gravitation und Elektrizität. Erste Mitteilung”, Sitzungsber. Preuss. Akad. Wiss., 1927(VI), 23–25, (1927). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/75ASGAHY. 6.3.1zbMATHGoogle Scholar
 [82]Einstein, A., “Zu Kaluzas Theorie des Zusammenhangs von Gravitation und Elektrizität. Zweite Mitteilung”, Sitzungsber. Preuss. Akad. Wiss., 1927(VI), 26–30, (1927). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/75ASGAHY. 6.3.1zbMATHGoogle Scholar
 [83]Einstein, A., “Neue Möglichkeit für eine einheitliche Feldtheorie von Gravitation und Elektrizit ät”, Sitzungsber. Preuss. Akad. Wiss., 1928(XVIII), 224–227, (1928). 6.4.1, 6.4.3, 6.4.4, 6.4.5, 6.4.5, 6.4.5zbMATHGoogle Scholar
 [84]Einstein, A., “RiemannGeometrie mit Aufrechterhaltung des Begriffes des Fernparallelismus”, Sitzungsber. Preuss. Akad. Wiss., 1928(XVII), 217–221, (1928). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/B8AG2G5E. 6.4.1, 6.4.3, 6.4.4, 6.4.5, 6.4.5, 6.4.5, 7.2.3zbMATHGoogle Scholar
 [85]Einstein, A., “Einheitliche Feldtheorie und Hamiltonsches Prinzip”, Sitzungsber. Preuss. Akad. Wiss., 1929(X), 156–159, (1929). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/EVNERTBY. 6.4.3, 6.4.5zbMATHGoogle Scholar
 [86]Einstein, A., “The New Field Theory I, II”, Observatory, 51, 82–87, (1929). 6.4.2, 11ADSGoogle Scholar
 [87]Einstein, A., “über den gegenwärtigen Stand der Feldtheorie”, in Honegger, E., ed., Festschrift, Prof. Dr. A. Stodola zum 70. Geburtstag, überreicht von seinen Freunden und Schülern, (Orell Füssli, Zurich, 1929). 6.4.3, 11Google Scholar
 [88]Einstein, A., “Zur einheitlichen Feldtheorie”, Sitzungsber. Preuss. Akad. Wiss., 1929(I), 2–7, (1929). 6.4.2, 6.4.3, 199, 201, 6.4.3, 6.4.3, 6.4.4, 6.4.5, 6.4.5, 7.2.3zbMATHGoogle Scholar
 [89]Einstein, A., “Auf die RiemannMetrik und den Fernparallelismus gegründete einheitliche Feldtheorie”, Math. Ann., 102, 685–697, (1930). [DOI]. 6.4.1, 6.4.3, 6.4.3, 6.4.4, 231, 6.4.5MathSciNetzbMATHCrossRefGoogle Scholar
 [90]Einstein, A., “Die Kompatibilität der Feldgleichungen in der einheitlichen Feldtheorie”, Sitzungsber. Preuss. Akad. Wiss., 1930(I), 18–23, (1930). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/NMS7SWKE. 6.4.3, 6.4.3, 6.4.6zbMATHGoogle Scholar
 [91]Einstein, A., “Professor Einstein’s adress at the University of Nottingham”, Science, 71, 608–611, (1930). 1.2, 6.4.3CrossRefGoogle Scholar
 [92]Einstein, A., “Théorie unitaire du champs physique”, Ann. Inst. Henri Poincare, 1, 1–24, (1930). 6.4.3, 11Google Scholar
 [93]Einstein, A., “Zur Theorie der Räume mit RiemannMetrik und Fernparallelismus”, Sitzungsber. Preuss. Akad. Wiss., 1930(VI), 401–402, (1930). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/K17BZ9SW. 6.4.3, 6.4.3, 6.4.5zbMATHGoogle Scholar
 [94]Einstein, A., “Gravitational and electromagnetic fields”, Science, 74, 438–439, (1931). 6.3.2, 10Google Scholar
 [95]Einstein, A., “Maxwell’s influence on the development of the conception of physical reality”, in James Clerk Maxwell: A Commemoration Volume 1831–1931, (Cambridge University Press, Cambridge, 1931). 1.2Google Scholar
 [96]Einstein, A., “Der gegenwärtige Stand der Relativitätstheorie”, Die Quelle, 82, 440–442, (1932). 1.2, 6.3.2Google Scholar
 [97]Einstein, A., “A Generalization of the Relativistic Theory of Gravitation”, Ann. Math., 46, 578–584, (1945). [DOI]. 2.1.3.2, 2.3MathSciNetzbMATHCrossRefGoogle Scholar
 [98]Einstein, A., Briefe an Maurice Solovine, (GauthierVillars, Paris, 1956). 6.4.3zbMATHGoogle Scholar
 [99]Einstein, A., Correspondance avec Michele Besso: 1903–1955, (Hermann, Paris, 1972). ed. Speziali, P. 4.1.3, 4.1.4, 4.3.3, 4.3.4, 6.1, 6.1, 6.3.2, 7.3, 11Google Scholar
 [100]Einstein, A., “Zur Methodik der Theoretischen Physik”, in Albert Einstein: Mein Weltbild, (Ullstein, Frankfurt am Main, 1984). 1st ed. 1934 Amsterdam. 7.3Google Scholar
 [101]Einstein, A., “Letter to David Hilbert”, in Schulman, R., Kox, A.J., Janssen, M., and Illy, J., eds., Einstein Collected Papers, Vol. 8A, Doc 144, p. 199, (Princeton University Press, Princeton, NJ, 1997). 3.1Google Scholar
 [102]Einstein, A., and Bergmann, P., “On a generalization of Kaluza’s theory of electricity”, Ann. Math., 39, 683–701, (1938). [DOI]. 6.3.1MathSciNetzbMATHCrossRefGoogle Scholar
 [103]Einstein, A., Born, H., and Born, M., Albert Einstein, Hedwig und Max Born, Briefwechsel: 1916–1955/kommentiert von Max Born; Geleitwort von Bertrand Russell; Vorwort von Werner Heisenberg, (Edition Erbrich, Frankfurt am Main, 1982). 4.1.4, 4.3.4, 234, 7.2.3, 313Google Scholar
 [104]Einstein, A., and Fokker, A.D., “Nordströmsche Gravitationstheorie vom Standpunkt des absoluten Differentialkalküls”, Ann. Phys. (Leipzig), 44, 321–328, (1914). [DOI]. 4.2ADSzbMATHCrossRefGoogle Scholar
 [105]Einstein, A., and Grommer, J., “Beweis der Nichtexistenz eines überall regulären zentrisch symmetrischen Feldes nach der Feldtheorie von Kaluza”, in Einstein, A., ed., Mathematica et physica, Scripta Hierosolymitana, vol. 1, pp. 1–4, (Hebrew University, Jerusalem, 1923). 4.2zbMATHGoogle Scholar
 [106]Einstein, A., and Mayer, W., “Zwei strenge statische Lösungen der Feldgleichungen der einheitlichen Feldtheorie”, Sitzungsber. Preuss. Akad. Wiss., 1930(VI), 110–120, (1930). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/GEYDB1K1. 6.4.3, 244zbMATHGoogle Scholar
 [107]Einstein, A., and Mayer, W., “Einheitliche Theorie von Gravitation und Elektrizität”, Sitzungsber. Preuss. Akad. Wiss., 1931(XXV), 541–557, (1931). 6.2, 6.3.2, 6.3.2, 10zbMATHGoogle Scholar
 [108]Einstein, A., and Mayer, W., “Systematische Untersuchung über kompatible Feldgleichungen, welche in einem Riemannschen Raume mit Fernparallelismus gesetzt werden können”, Sitzungsber. Preuss. Akad. Wiss., 1931(XIII), 257–265, (1931). 6.4.3zbMATHGoogle Scholar
 [109]Einstein, A., and Mayer, W., “Einheitliche Theorie von Gravitation und Elektrizität. (Zweite Abhandlung.)”, Sitzungsber. Preuss. Akad. Wiss., 1932(XII), 130–137, (1932). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/TSH25SM0. 6.3.2zbMATHGoogle Scholar
 [110]Einstein, A., and Mayer, W., “SemiVektoren und Spinoren”, Sitzungsber. Preuss. Akad. Wiss., 1932(XXXII), 522–550, (1932). Related online version (cited on 30 October 2009): http://einsteinannalen.mpiwgberlin.mpg.de/related_texts/sitzungsberichte/VA2YYBC8. 7.3zbMATHGoogle Scholar
 [111]Einstein, A., and Mayer, W., “Die Diracgleichungen für Semivektoren”, Proc. K. Akad. Wetensch., 36, 497–516, (1933). 7.3zbMATHGoogle Scholar
 [112]Einstein, A., and Mayer, W., “Spaltung der natürlichen Feldgleichungen für SemiVektoren in SpinorGleichungen vom Diracschen Typus”, Proc. K. Akad. Wetensch., 36(2), 615–619, (1933). 7.3zbMATHGoogle Scholar
 [113]Einstein, A., and Mayer, W., “Darstellung der SemiVektoren als gewöhnliche Vektoren von besonderem Differentiationscharakter”, Ann. Math., 35, 104–110, (1934). [DOI]. 7.3MathSciNetzbMATHCrossRefGoogle Scholar
 [114]Eisenhart, L.P., “Fields of parallel vectors in the geometry of paths”, Proc. Natl. Acad. Sci. USA, 8, 207–212, (1922). [DOI]. 2ADSzbMATHCrossRefGoogle Scholar
 [115]Eisenhart, L.P., “Spaces with corresponding paths”, Proc. Natl. Acad. Sci. USA, 8, 233–238, (1922). [DOI]. 2ADSzbMATHCrossRefGoogle Scholar
 [116]Eisenhart, L.P., “Another interpretation of the fundamental gauge vector of Weyl’s theory of relativity”, Proc. Natl. Acad. Sci. USA, 9, 175–178, (1923). [DOI]. 4.1.5ADSCrossRefGoogle Scholar
 [117]Eisenhart, L.P., “The geometry of paths and general relativity”, Ann. Math., 24, 367–392, (1923). [DOI]. 5MathSciNetzbMATHCrossRefGoogle Scholar
 [118]Eisenhart, L.P., “Linear connections of a space which are determined by simply transitive continuous groups”, Proc. Natl. Acad. Sci. USA, 11, 246–249, (1925). [DOI]. 6.4.1, 6.4.3ADSzbMATHCrossRefGoogle Scholar
 [119]Eisenhart, L.P., Riemannian Geometry, (Princeton University Press, Princeton, NJ, 1925). 34, 6.4, 7.2.2zbMATHGoogle Scholar
 [120]Eisenhart, L.P., “Einstein’s recent theory of gravitation and electricity”, Proc. Natl. Acad. Sci. USA, 12, 125–129, (1926). [DOI]. 6.1ADSzbMATHCrossRefGoogle Scholar
 [121]Eisenhart, L.P., NonRiemannian Geometry, AMS Colloquium Publications, vol. VIII, (American Mathematical Society, Providence, RI, 1927). 2.1.2, 5, 6.4Google Scholar
 [122]Eisenhart, L.P., and Veblen, O., “The Riemann Geometry and its generalizations”, Proc. Natl. Acad. Sci. USA, 8, 19–23, (1922). [DOI]. 2, 5ADSzbMATHCrossRefGoogle Scholar
 [123]Eyraud, H., “La Théorie affine asymétrique du champs électromagnétique et gravifique et le rayonnement atomique”, C. R. Acad. Sci., 180, 1245–1248, (1925). 5zbMATHGoogle Scholar
 [124]Eyraud, H., “Sur le charactère riemannien projectif du champ gravifique électromagnétique”, C. R. Acad. Sci., 180, 127–129, (1925). 5zbMATHGoogle Scholar
 [125]Fabre, L., Les Théories d’Einstein, (Payot, Paris, 1921). Nouvelle éd. 10Google Scholar
 [126]Finsler, P., über Kurven und Flächen in allgemeinen Räumen, Lehrbücher und Monographien aus dem Gebiete der exakten Wissenschaften: Mathematische Reihe, vol. 11, (Birkhäuser, Basel, 1951). Unveränderter Nachdruck der Dissertation von 1918. 2.1.1, 3.1Google Scholar
 [127]Fisher, J.W., “The Wave Equation in Five Dimensions”, Proc. R. Soc. London, Ser. A, 123, 489–493, (1929). 7.1, 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [128]Fisher, J.W., and Flint, H.T., “The Equations of the Quantum Theory”, Proc. R. Soc. London, Ser. A, 126, 644–653, (1930). 7.1ADSzbMATHCrossRefGoogle Scholar
 [129]Flint, H.T., “The First and Second Order Equations of the Quantum Theory”, Proc. R. Soc. London, Ser. A, 124, 143–150, (1929). 7.1ADSzbMATHCrossRefGoogle Scholar
 [130]Fock, V.A., “über die invariante Form der Wellen und der Bewegungsgleichung für einen geladenen Massenpunkt”, Z. Phys., 39, 226–232, (1926). [DOI]. 6.3.1, 7.2.2, 270ADSzbMATHCrossRefGoogle Scholar
 [131]Fock, V.A., “Geometrisierung der Diracschen Theorie des Elektrons”, Z. Phys., 57, 261–277, (1929). [DOI]. 7.2.1, 7.2.2, 7.2.2, 7.2.2, 7.2.3ADSzbMATHCrossRefGoogle Scholar
 [132]Fock, V.A., “L’équation d’onde de Dirac et la Géometrie de Riemann”, J. Phys. Radium, 10, 392–405, (1929). [DOI]. 7.2.2, 7.2.2, 7.2.3zbMATHCrossRefGoogle Scholar
 [133]Fock, V.A., “Sur les équations de Dirac dans la théorie de relativité générale”, C. R. Acad. Sci., 189, 25–27, (1929). 7.2.1, 7.2.2, 7.2.3zbMATHGoogle Scholar
 [134]Fock, V.A., and Ivanenko, D.D., “Géometrie quantique linéaire et déplacement parallèle”, C. R. Acad. Sci., 188, 1470–1472, (1929). 7.2.2, 7.2.3zbMATHGoogle Scholar
 [135]Fock, V.A., and Ivanenko, D.D., “über eine mögliche geometrische Deutung der relativistischen Quantentheorie”, Z. Phys., 54, 798–802, (1929). [DOI]. 6.4.5, 7.2.2, 274ADSzbMATHCrossRefGoogle Scholar
 [136]Fölsing, A., Albert Einstein: Eine Biographie, (Suhrkamp, Frankfurt am Main, 1993). 1.1Google Scholar
 [137]Förster, R., Beiträge zur spezielleren Theorie der Riemannschen PFunktion, (Teubner, Leipzig, 1908). PhD Thesis, University of Leipzig. 322Google Scholar
 [138]Fréedericksz, V., and Isakson, A., “Einige Bemerkungen über die Feldgeometrie”, Phys. Z., 30, 645, (1929). 5zbMATHGoogle Scholar
 [139]French, A.P., ed., Einstein: A Centenary Volume, (Heinemann, London, 1979). 4.3.2zbMATHGoogle Scholar
 [140]Frenkel, J., “Die Wellenmechanik des rotierenden Elektrons und die Grundgleichnungen des elektromagnetischen Feldes”, Z. Phys., 52, 356–363, (1928). 7.1, 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [141]Frenkel, J., “Zur Wellenmechanik des rotierenden Elektrons”, Z. Phys., 47, 786–803, (1928). [DOI]. 7.2.4ADSCrossRefGoogle Scholar
 [142]Friedmann, A., and Schouten, J.A., “über die Geometrie der halbsymmetrischen übertragungen”, Math. Z., 21, 211–223, (1924). [DOI]. 5, 6.2MathSciNetzbMATHCrossRefGoogle Scholar
 [143]Goenner, H., “Unified field theories from Eddington and Einstein up to now”, in de Sabbata, V., and Karade, T. M., eds., Relativistic Astrophysics and Cosmology, Vol. 1, Proceedings of the Sir Arthur Eddington Centenary Symposium, Nagpur, India, (World Scientific, Singapore, 1984). 2.2Google Scholar
 [144]Goenner, H., and Havas, P., “SphericallySymmetric SpaceTimes with vanishing Curvature Scalar”, J. Math. Phys., 21, 1159–1167, (1980). [DOI]. 66ADSzbMATHCrossRefGoogle Scholar
 [145]Goenner, H., and Wünsch, D., What did Kaluza and Klein contribute to KaluzaKleintheory?, 235, (Max Planck Institute for the History of Science, Berlin, 2003). 101, 6.3.1Google Scholar
 [146]Goldstein, C., and Ritter, J., The Varieties of Unity: Sounding Unified Theories 1920–1930, 149, (Max Planck Institute for the History of Science, Berlin, 2000). 1.1Google Scholar
 [147]Gonseth, F., and Juvet, G., “Les équations de l’électromagnétisme et l’équation de M. Schrödinger”, C. R. Acad. Sci., 185, 535–538, (1927). eratum p. 732. 7.2.4zbMATHGoogle Scholar
 [148]Gonseth, F., and Juvet, G., “Sur la métrique de l’espace à cinq dimensions de l’électromagnétisme at de la gravitation”, C. R. Acad. Sci., 185, 412–413, (1927). 7.2.4zbMATHGoogle Scholar
 [149]Gonseth, F., and Juvet, G., “Sur l’équation de M. Schrödinger”, C. R. Acad. Sci., 185, 448–450, (1927). eratum p. 624. 7.2.4zbMATHGoogle Scholar
 [150]Gonseth, F., and Juvet, G., “Sur les équations de l’électromagnétisme”, C. R. Acad. Sci., 185, 341–343, (1927). eratum p. 483. 7.2.4zbMATHGoogle Scholar
 [151]Gordon, W., “Der Strom der Diracschen Elektronentheorie”, Z. Phys., 50, 630–632, (1928). [DOI]. 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [152]Gorelik, G., “Hermann Weyl and Large Numbers in Relativistic Cosmology”, in Balashov, Y., and Vizgin, V., eds., Einstein Studies in Russia, Einstein Studies, vol. 10, pp. 91–106, (Birkhäuser, Boston; Basel, 2002). [Google Books]. 4.1.2ADSzbMATHCrossRefGoogle Scholar
 [153]Grommer, J., “Eine kleine Bemerkung zur neuen Einsteinschen Feldtheorie”, Phys. Z., 30, 645, (1929). 6.4.5zbMATHGoogle Scholar
 [154]Grüning, M., Ein Haus für Albert Einstein: Erinnerungen, Briefe, Dokumente, (Verlag der Nation, Berlin, 1990). 6.4.4Google Scholar
 [155]Hattori, K., “ über eine formale Erweiterung der Relativitätstheorie und ihren Zusammenhang mit der Theorie der Elektrizität”, Phys. Z., 29, 538–549, (1928). 6.2zbMATHGoogle Scholar
 [156]Havas, P., “Einstein, Relativity and Gravitation Research in Vienna before 1938”, in Goenner, H., Renn, J., Ritter, J., and Sauer, T., eds., The Expanding Worlds of General Relativity, Einstein Studies, vol. 7, pp. 161–206, (Birkhäuser, Boston; Basel, 1999). [Google Books]. 81ADSMathSciNetzbMATHCrossRefGoogle Scholar
 [157]Hehl, F.W., von der Heyde, P., Kerlick, G.D., and Nester, J.M., “General relativity with spin and torsion: Foundation and prospects”, Rev. Mod. Phys., 48, 393–416, (1976). 45ADSCrossRefGoogle Scholar
 [158]Heisenberg, W., and Pauli, W., “Zur Quantendynamik der Wellenfelder”, Z. Phys., 56, 1–61, (1929). [DOI]. 7.1ADSzbMATHCrossRefGoogle Scholar
 [159]Hermann, A., Einstein: Der Weltweise und sein Jahrhundert. Eine Biographie, (Piper, Munich, 1994). 1.1Google Scholar
 [160]Hessenberg, G., “Vektorielle Begründung der Differentialgeometrie”, Math. Ann., 78, 187–217, (1917). 3.1, 128MathSciNetzbMATHCrossRefGoogle Scholar
 [161]Hilbert, D., “Die Grundlagen der Physik (Erste Mitteilung.)”, Nachr. Koenigl. Gesellsch. Wiss. Goettingen, Math.Phys. Kl., 1915, 395–407, (1915). Related online version (cited on 30 October 2009): http://echo.mpiwgberlin.mpg.de/content/modernphysics/hilbert/hilbert_grundlagen_1915. 4.3.2zbMATHGoogle Scholar
 [162]Hilbert, D., “Letter from David Hilbert”, in Schulman, R., Kox, A.J., Janssen, M., and Illy, J., eds., Einstein Collected Papers, Vol. 8A, Doc 140, p. 195, (Princeton University Press, Princeton, NJ, 1997). 3.1Google Scholar
 [163]Hoffmann, B., “Projective Relativity and the Quantum Field”, Phys. Rev., 37, 88–89, (1930). 6.3.2ADSzbMATHCrossRefGoogle Scholar
 [164]Hosokawa, T., “Connections in the manifold admitting generalized transformations”, Proc. Imp. Acad. Japan, 8, 348–351, (1932). [DOI]. 154MathSciNetzbMATHCrossRefGoogle Scholar
 [165]Infeld, L., “Bemerkungen zu der Arbeit von Herrn K. Hattori”, Phys. Z., 29, 810–811, (1928). 6.2zbMATHGoogle Scholar
 [166]Infeld, L., “Zur Feldtheorie von Elektrizität und Gravitation”, Phys. Z., 29, 145–147, (1928). [DOI]. 6.2zbMATHGoogle Scholar
 [167]Infeld, L., and van der Waerden, B.L., “Die Wellengleichung des Elektrons in der allgemeinen Relativitätstheorie”, Sitzungsber. Preuss. Akad. Wiss., 1933(IX), 380–401, (1933). 7.2.1, 7.3zbMATHGoogle Scholar
 [168]Infeld, L., and van der Waerden, B.L., “Die Wellengleichung des Elektrons in der allgemeinen Relativitätstheorie”, Sitzungsber. Preuss. Akad. Wiss., 1933(IX), 380–401, (1933). 7.2.2zbMATHGoogle Scholar
 [169]Ivanenkov, D.D., and Fock, V.A., “Vorträge und Diskussionen der TheoretischPhysikalischen Konferenz in Charkow (19.–25. Mai 1929)”, Phys. Z., 30, 645–655, (1929). 7.2.2Google Scholar
 [170]Jauch, J.M., and Rohrlich, F., The Theory of Photons and Electrons: The relativistic quantum field theory of charged particles with spin onehalf, Texts and Monographs in Physics, (Springer, New York, 1980), 2nd edition. 139Google Scholar
 [171]Jehle, H., “Zur allgemeinen relativistischen Quantenmechanik”, Z. Phys., 87, 370–374, (1933). 7ADSzbMATHCrossRefGoogle Scholar
 [172]Jehle, H., “Zur allgemeinrelativistischen Quantenmechanik II. Kosmologische Quantenerscheinungen”, Z. Phys., 94, 692–706, (1935). [DOI]. 7ADSzbMATHCrossRefGoogle Scholar
 [173]Jordan, P., “über die Polarisation der Lichtquanten”, Z. Phys., 44, 292–300, (1927). 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [174]Jordan, P., “über Wellen und Korpuskeln in der Quantenmechanik”, Z. Phys., 45, 766–775, (1927). [DOI]. 1.2ADSzbMATHCrossRefGoogle Scholar
 [175]Jordan, P., “Zur Quantenmechanik der Gasentartung”, Z. Phys., 44, 473–480, (1927). 1.2ADSzbMATHCrossRefGoogle Scholar
 [176]Jordan, P., Schwerkraft und Weltall, (Vieweg, Braunschweig, 1955), 2nd edition. 1.1zbMATHGoogle Scholar
 [177]Jordan, P., Albert Einstein: Sein Lebenswerk und die Zukunft der Physik, Wirkung und Gestalt, vol. 6, (Huber, Frauenfeld; Stuttgart, 1969). 1.1Google Scholar
 [178]Jordan, P., and Klein, O., “Zum Mehrkörperproblem der Quantentheorie”, Z. Phys., 45, 751–765, (1927). [DOI]. 1.2ADSzbMATHCrossRefGoogle Scholar
 [179]Jordan, P., and Wigner, E., “über das Paulische ‘Aquivalenzverbot’”, Z. Phys., 47, 631–651, (1928). [DOI]. 1.2ADSzbMATHCrossRefGoogle Scholar
 [180]Juvet, G., “Les formules de Frenet pour un espace de M. Weyl”, C. R. Acad. Sci., 172, 1647–1650, (1921). 4.1.5, 9zbMATHGoogle Scholar
 [181]Kaluza, T., “Zum Unitätsproblem in der Physik”, Sitzungsber. Preuss. Akad. Wiss., 1921, 966–972, (1921). Zum Unitätsproblem in der Physik. 2.4, 4.2, 7.2.4zbMATHGoogle Scholar
 [182]Kawaguchi, A., “Die Differentialgeometrie in der verallgemeinerten Mannigfaltigkeit”, Rend. Circ. Mat. Palermo, 56, 245–276, (1932). [DOI]. 154zbMATHCrossRefGoogle Scholar
 [183]Kirsten, C., and Treder, H.J., Albert Einstein in Berlin 19131933, Teil I: Darstellungen und Dokumente, (AkademieVerlag, Berlin, 1979). 1.1, 6.4.2, 192, 205, 7.2.3zbMATHGoogle Scholar
 [184]Klein, O., “The Atomicity of Electricity as a Quantum Law”, Nature, 118, 516, (1926). [DOI]. 6.3.1, 7.2.4ADSCrossRefGoogle Scholar
 [185]Klein, O., “Quantentheorie und fünfdimensionale Relativitätstheorie”, Z. Phys., 37, 895–906, (1926). [DOI]. 4.2, 6.3.1, 6.3.2, 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [186]Klein, O., “Elektrodynamik und Wellenmechanik vom Standpunkt des Korrespondenzprinzips”, Z. Phys., 41, 407–442, (1927). [DOI]. 6.3.1ADSzbMATHCrossRefGoogle Scholar
 [187]Klein, O., “Elektrodynamik und Wellenmechanik vom Standpunkt des Korrespondenzprinzips”, Z. Phys., 41, 407–442, (1927). [DOI]. 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [188]Klein, O., “Sur l’article de M. L. de Broglie: ‘L’univers à cinq dimensions et la méchanique ondulatoire’”, J. Phys. Radium, 8, 242–243, (1927). [DOI]. 6.3.1zbMATHCrossRefGoogle Scholar
 [189]Klein, O., “Zur fünfdimensionalen Darstellung der Relativitätstheorie”, Z. Phys., 46, 188–208, (1928). [DOI]. 6.3.1, 7.2.4ADSzbMATHCrossRefGoogle Scholar
 [190]Kojevnikov, A., “Dirac’s Quantum Electrodynamics”, in Balashov, Y., and Vizgin, V., eds., Einstein Studies in Russia, Einstein Studies, vol. 10, pp. 229–259, (Birkhäuser, Boston; Basel, 2002). [Google Books]. 1.2ADSzbMATHCrossRefGoogle Scholar
 [191]König, M., Herleitung und Untersuchung der Feld und Bewegungsgleichungen von an das Gravitationsfeld gekoppelten TensorfeldTheorien, Masters Thesis, (Universität Göttingen, Göttingen, 2000). 64Google Scholar
 [192]König, R., “Beiträge zu einer allgemeinen linearen Mannigfaltigkeitslehre”, Jahresber. Deutsch. Math.Verein., 28, 213–228, (1919). 3zbMATHGoogle Scholar
 [193]König, R., “über affine Geometrie XXIV. Ein Beitrag zu ihrer Grundlegung”, Ber. Saechs. Gesellsch. Wiss., 71, 1–19, (1919). 3.1zbMATHGoogle Scholar
 [194]Kopff, A., in Kopf, A., ed., MüllerPouillets Lehrbuch der Physik, Vol. 5/2: Physik des Kosmos, (Vieweg, Braunschweig, 1928). 10Google Scholar
 [195]Kosambi, D., “Affingeometrische Grundlagen der einheitlichen Feldtheorie”, Sitzungsber. Preuss. Akad. Wiss., 1932, 342–345, (1932). 6.2zbMATHGoogle Scholar
 [196]Kretschmann, E., “über den physikalischen Sinn der Relativitätspostulate; A. Einsteins neue und seine ursprüngliche Relativitätstheorie”, Ann. Phys. (Leipzig), 53, 592–614, (1917). 2.1.3.2, 9zbMATHGoogle Scholar
 [197]Kunii, S., “On a unified field theory of gravitational and electromagnetic fields”, Mem. Coll. Sci. Kyoto Univ., Ser. A, 14, 195–212, (1931). 154zbMATHGoogle Scholar
 [198]Lanczos, C., “Die Erhaltungssätze in der feldmässigen Darstellung der Diracschen Theorie”, Z. Phys., 57, 484–493, (1929). [DOI]. 1.2, 7.1ADSzbMATHCrossRefGoogle Scholar
 [199]Lanczos, C., “Die tensoranalytischen Beziehungen der Diracschen Gleichung”, Z. Phys., 57, 447–473, (1929. [DOI]. 7.1ADSzbMATHCrossRefGoogle Scholar
 [200]Lanczos, C., “Zur kovarianten Formulierung der Diracschen Gleichung”, Z. Phys., 57, 474–483, (1929). [DOI]. 7.1ADSzbMATHCrossRefGoogle Scholar
 [201]Lanczos, C., “Die neue Feldtheorie Einsteins”, Ergeb. Exakten Naturwiss., 10, 97–132, (1931). [DOI]. 6.4.4, 8ADSzbMATHCrossRefGoogle Scholar
 [202]Lanczos, C., “Elektromagnetismus als natürliche Eigenschaft der Riemannschen Geometrie”, Z. Phys., 73, 147–168, (1931). [DOI]. 6.4.4, 8ADSzbMATHCrossRefGoogle Scholar
 [203]Laporte, O., and Uhlenbeck, G.E., “Application of Spinor Analysis to the Maxwell and Dirac Equations”, Phys. Rev., 37, 1380–1397, (1931). [DOI]. 7.3ADSzbMATHCrossRefGoogle Scholar
 [204]LeviCivita, T., “Nozione di parallelismo in una varietà qualunque e conseguente specificazione geometrica della curvatura Riemanniana”, Rend. Circ. Mat. Palermo, 42, 173–205, (1917). 2.1.3.2, 3.1zbMATHCrossRefGoogle Scholar
 [205]LeviCivita, T., Lezioni di calcolo differenziale assoluto, (Stock, Roma, 1925). 6.4.5, 10zbMATHGoogle Scholar
 [206]LeviCivita, T., “A proposed modification of Einstein’s field theory”, Nature, 123, 678–679, (1929). [DOI]. 6.4.5ADSzbMATHCrossRefGoogle Scholar
 [207]LeviCivita, T., “Vereinfachte Herstellung der Einsteinschen einheitlichen Feldgleichungen”, Sitzungsber. Preuss. Akad. Wiss., 1929(IX), 137–153, (1929). 6.4.5, 7.2.2zbMATHGoogle Scholar
 [208]LeviCivita, T., “Diracsche und Schrödingersche Gleichungen”, Sitzungsber. Preuss. Akad. Wiss., 1933(V), 240–250, (1933). 7.2.2zbMATHGoogle Scholar
 [209]Lichnerowicz, A., Théories de la Gravitation et de L’électromagnétisme, (Masson, Paris, 1955). 1.1zbMATHGoogle Scholar
 [210]Lopes Gagean, D., and Costa Leite, M., “A theoria de KaluzaKlein”, Analise (Lisboa), 5, 151–198, (1986). 6.3.1Google Scholar
 [211]Lorentz, H.A., “The determination of the potentials in the general theory of relativity with some remarks about the measurement of lengths and intervals of time and about the theories of Weyl and Eddington”, in Collected Papers, vol. 5, pp. 363–382, (Nijhoff, The Hague, 1937). Original paper in Proc. Acad. Amsterdam, 29 (1923) 383. 4.1.2, 4.3.1CrossRefGoogle Scholar
 [212]Ludwig, G., Fortschritte der projektiven Relativitätstheorie, (Vieweg, Braunschweig, 1951). 1.1zbMATHCrossRefGoogle Scholar
 [213]Madelung, E., “Eine übertragung der Diracschen Theorie des Elektrons in gewohnte Formen”, Z. Phys., 54, 303–306, (1929). [DOI]. 7ADSzbMATHCrossRefGoogle Scholar
 [214]Maeterlick, M., Geheimnisse des Weltalls, (Deutsche Verlagsanstalt, Stuttgart, 1930). 6.4.2Google Scholar
 [215]Majer, U., and Sauer, T., “Hilbert’s ‘World Equations’ and His Vision of a Unified Science”, in Kox, A.J., and Eisenstaedt, J., eds., The Universe of General Relativity, Einstein Studies, vol. 11, pp. 259–266, (Birkhäuser, Boston; Basel, 2005). [physics/0405110], [Google Books]. 4.3.2ADSMathSciNetzbMATHCrossRefGoogle Scholar
 [216]Mandel, H., “Zur Herleitung der Feldgleichungen in der allgemeinen Relativitätstheorie. (Erste Mitteilung.)”, Z. Phys., 39, 136–145, (1926). [DOI]. 6.3.1, 6.3.2ADSzbMATHCrossRefGoogle Scholar
 [217]Mandel, H., “Zur Herleitung der Feldgleichungen in der allgemeinen Relativitätstheorie. (Zweite Mitteilung.)”, Z. Phys., 45, 285–306, (1927). [DOI]. 6.3.2ADSCrossRefGoogle Scholar
 [218]Mandel, H., “über den Zusammenhang zwischen der Einsteinschen Theorie des Fernparallelismus und der fünfdimensionalen Feldtheorie”, Z. Phys., 56, 838–844, (1929). [DOI]. 6.3.2, 6.4.5ADSzbMATHCrossRefGoogle Scholar
 [219]Mandel, H., “über den Zusammenhang zwischen der Einsteinschen Theorie des Fernparallelismus und der fünfdimensionalen Feldtheorie”, Z. Phys., 56, 838–844, (1929). [DOI]. 6.3.2ADSzbMATHCrossRefGoogle Scholar
 [220]Mandel, H., “Zur Axiomatik der fünfdimensionalen Relativitätstheorie”, Z. Phys., 54, 564–566, (1929). [DOI]. 6.3.1ADSzbMATHCrossRefGoogle Scholar
 [221]Mandel, H., “Zur tensoriellen Form der wellenmechanischen Gleichung des Elektrons”, Z. Phys., 54, 567–570, (1929). [DOI]. 7.2.4