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Causality, Nonlocality, and Entanglement in Quantum Mechanics

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The Emerging Quantum

Abstract

This chapter takes us into the domains of quantum nonlocality. The journey starts with a brief introduction to Bohm’s causal theory of quantum mechanics, which serves to further discuss the nonlocality contained in the Schrödinger descriptionQuantum regime!and Schrödinger description. A critical discussion of this causal and deterministic approach illustrates the virtues and limitations associated with the BohmianCausality interpretationInterpretation of quantum mechanics. The tools developed in previous chapters are then applied to a more detailed analysis of quantum nonlocality, both for single-particle and bipartite systems. Some important results are derived, which throw light on the relationship between the quantum potentialQuantum potential and linearity, fluctuations, and nonlocalityQuantum potential!and nonlocality. The bipartite system is further analyzed and the connections between nonlocality, entanglementEntanglement and noncommutativity are disclosed for general continuous variables.

Why is the pilot-wave picture ignored in the text books? Should it not be taught, not as the only way, but as an antidote to the prevailing complacency? To show that vagueness, subjectivity, and indeterminism Indeterminism, are not forced on us by experimental facts, but by deliberate theoretical choice?

Bell (1987, page 160)

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Notes

  1. 1.

    It is much less known that almost simultaneously and independently, a similar result was published by Solomon (1933).

  2. 2.

    Take for example the spin projections along three different directions: \( \hat{A}=\hat{S}_{x},\) \(\hat{B}=\hat{S}_{y}\) and \(\hat{C}=(\hat{A}+\hat{B})/ \sqrt{2}=(\hat{S}_{x}+\hat{S}_{y})/\sqrt{2}\). If the system possesses spin \( 1/2\), the eigenvalues of each of these operators are the same and equal to \( \pm 1;\) clearly the eigenvalues of \(\hat{C}\) are not the linear combination \( (\pm 1\pm 1)/\sqrt{2}.\)

  3. 3.

    Since Hermann’s argument is little known, and is just the same discovered by Bell 30 years later, it seems of interest to transcribe it here: “Suppose we have an ensemble of physical systems, with \( \mathfrak {R}\) and \(\mathfrak {S}\) physical quantities that can be measured on this ensemble; the expectation value of \(\mathfrak {R}\) (Expt(\(\mathfrak {R}\))) is the average value of all measurementMeasurement outcomes that will be obtained when measuring \(\mathfrak {R}\) on all systems of the ensemble, and is also the value that is expected to be obtained when measuring \(\mathfrak {R}\) on an arbitrary element of this ensemble. Von Neumann requires that for this expectation value-function Expt(\(\mathfrak {R}\)), defined using an ensemble of physical systems and producing a number for every physical quantity, Expt(\(\mathfrak {R}+\mathfrak {S}\)) = Expt(\(\mathfrak {R}) + \text {Expt}(\mathfrak {S}\)). In words: The expectation value of a sum of physical quantities is equal to the sum of the expectation values of both quantities. With this assumption the proof of von Neumann either succeeds or fails.” “For classical physics this requirement is trivial and also for those quantum mechanical observables that \([\)commute\(]\)... Not trivial however is the relation for quantum mechanical quantities for which indeterminacy relations hold. In fact the sum of two such quantities is not even defined: Because a sharp measurement of one of them excludes sharp measurementMeasurement of the other one and thus because both quantities cannot have sharp values at the same time, the commonly used definition of the sum of two quantities breaks down.”

  4. 4.

    Feyerabend noticed that the postulates used in von Neumann’s derivation did not exclude dispersive hidden variables. Now if the hidden variablesHidden variables added to qm had an irreducible dispersion, the quantum variables themselves should continue to be dispersive and things remained essentially the same, except that the theorem needed some reformulation. Mugur-Schächter, on her part, argued that the demonstration was not as general as assumed, since it presupposes that the distribution of the hidden variables (once more, distributed variables) has properties similar to those of the quantum distribution.

  5. 5.

    Without pretending to undermine de Broglie’s credit for his seminal contribution, in most of this book we shall refer to Bohm’s theory, for short, as is customary in present-day literature. An alternative form of qm, similar to Bohm’s, had been proposed many years earlier by Madelung (1927).

  6. 6.

    The well-known book by Bell containing the collection of his articles on the foundations of qm (Bell 1987)was very influential in the revival of Bohm’s theoryBell!and Bohm’s theory. Bell appreciated the objective, deterministic and causal aspects of the pilot-wave theory. It was the search for an answer to the question: Is it that any hidden-variables theory is by necessity nonlocal? what prompted Bell’s work leading to his now famous inequalities.

  7. 7.

    This is achieved by simply inverting the reasoning in the derivations. Two crucial postulates are needed: one is of course the guidance equation; the second demand serves to introduce the quantum potential \(V_{Q}\) into Eq. (8.9) on the basis of an appropriately contrived argument. The simplest procedure is to consider the quantum potentialQuantum potential as an empirical—and thus phenomenological—expression, and to proceed from there on. There exist all sorts of interpretations and ‘derivations’ of the quantum potential, as commented in footnote 4.14.

  8. 8.

    The kinetic origin of the quantum potentialQuantum potential is discussed in de la Peña et al. (2011).De la Peña, L. To the varied proposals to derive the quantum potential cited in footnote 4.14, one should add those of Dürr et al. (1992)Van@Ván, P. Goldstein, S., and Ván and Fülöp (2003)Fülöp, T., as well as.the thermodynamic approach of Grössing (2008, 2009)Grössing, G.. A somewhat bolder one is that of Floyd (2002)Floyd, E. R., who proposes a trajectory description based on a peculiar quantum potential containing derivatives of third order. An interesting point of this theory is that it contains extra parameters that allow for a distribution of the velocity \(\varvec{v},\) resulting in a more realisticDescription!realist description. Salesi (1996) and Recami and Salesi (1998) propose that the quantum potential can be derived by considering the energy associated with the internal zitterbewegung (considered as the antecedent of the spin). A similar proposal is made by Esposito (1999)Esposito, S., who associates the quantum potential with the (internal) kinetic energy due to a generalized spin; see also Yang (2006)Yang, C. D.. For these authors, the notions of spin, zitterbewegungZitterbewegung and quantum potential are intimately related. Garbaczewski (1992)Garbaczewski, P. offers a nice derivation of the quantum potential as due to the fluctuationsSpin!and fluctuations of the momentumFluctuations!momentum. In Carroll, R. Carroll (2007, 2010), additional arguments are introduced about the origin of the quantum potentialQuantum potential!origin, related to Fisher information.

  9. 9.

    The field \(\psi \) differs in essence from those known to classical physics. In contrast to the gravitational or the electromagnetic field, for example, it does not have a generating source. Moreover, it affects the particle (by guiding it) but is not affected by it. This lack of reciprocity in the field-particle influence led de Broglie (1956)De Broglie, L. (and afterwards Bohm himself) to regard the pilot-wave theory as just a step towards a necessarily more developed theory. [See item 15 in Bell (1987)].

  10. 10.

    This assertion requires some qualification. It is not too difficult to find (both in orthodox textbooks and in research papers, and of course also in popular works), arguments that bear implicitly or explicitly on the notion of trajectory. For example, in discussions on van der WaalsBoyer!and van der Waals forces or molecular forces a drawing is sometimes made of atoms with well-localized orbiting (point) electrons, and the Hamiltonian is written accordingly. True, at some moment an average is taken, but nevertheless the discussion refers, or at least seems to refer, to orbiting point particles. Another example is an atom or a particle in a Stern-Gerlach experiment, which in every analysis is considered to follow a definite trajectory.

  11. 11.

    It is this statistical treatment what engenders ‘indistinguishability’, and this occurrs regardless of whether the system is classical or quantum. This, for instance, explains the use of the notion of indistinguishabilityIndistinguishability to solve the Gibbs paradoxGibbs paradox in classical statistical physics (see e.g. Mandl 1988).

  12. 12.

    Also Nelson’s theoryNelson theory!and nonlocality Nelson theory and more generally the stochastic description of qm have been successfully used to investigate quantum trajectories, as shown by the examples in Chap. 2.

  13. 13.

    Further examples can be seen in Holland (1993), Lopreore and Wyatt (1999, 2000)Wyatt, R. E.—who have generated what they call the ‘quantum trajectory method’—; Suñé and Oriols (2000)Suñé, J., Matzkin and Nurock (2008),Nurock, V. Matzkin, A. Sanz et al. (2002)Sanz, A. S. Miret-Artés, S., Philippidis et al. (1982), and Kumar Chattaraj (2010).

  14. 14.

    In a variant of Bohm’s theory the idea of a fluid à la Madelung is entertained. By considering this fluid to be subject to fluctuations, a random element is then added; see Bohm and Vigier (1954)Vigier, J.-P.. See also Wang (2006)Wang, X.-S. for related work.

  15. 15.

    Here it is in place to recall the argument against the Copenhagen interpretationInterpretation raised by Einstein (1953), considering the stationary states of an infinite one-dimensional square well potential. The spatial part of the wave function can be written in the form \(\varphi =N\sin kx.\) From Eq. (8.11) it follows that \(v=0,\) hence there is no flow velocity. However, by writing the wave function in the form \(\psi =(N/2i)(e^{ikx}-e^{-ikx}),\) it can be interpreted as referring to two similar subensembles of particles, traveling to the right and to the left, with velocities \(\pm \hbar k/m.\) Thus, it is the net (mean) velocity that is null. Einstein used this example to argue that the statistical reading is the single one that can be made in the limit of high energies. Since passing to this limit does not change the nature of the problem, Einstein concluded that one should consider the wave function as describing an ensemble, not an individual particle.

  16. 16.

    In the usual quantum theory of measurement, the process of extracting from (8.21) the observed result \(\Phi _{n}\) (the reductionReduction|see collapse or collapse of the after-measurement state) is referred to as the problem of objectificationObjectification. See e.g. Mittelstaedt (2009).

  17. 17.

    The possibility that the result of a measurement depends on both the system under observation and the measuring apparatus is also present at the classical level. A common example of the class of nondisturbing classical procedures is a photocell detector that checks the presence or absence of somebody before closing the door of an elevator. An example of the second class could be a ‘tail or head’ detector for tossed coins which operates by inserting a card to stop and receive the coins. Of course this second mechanism can be replaced with more elaborate optical procedures that do not disturb the observed coins. This is a matter of the measurer’s skills and of the existing technical possibilities.

  18. 18.

    A first peculiarity of \(V_{Q}\) is that it is independent of the field’s strength, or rather of the intensity (\(\sim \!\rho \)) of the wave\(.\) This follows from the fact that \(V_{Q}(\rho )=V_{Q}(A\rho )\) for any constant \(A,\) and indicates that the effects due to the particles do not depend on the number of particles present; but on their distribution. That there are forces within the classical realm, particularly in the hydrodynamical analogy, with similar peculiarities does not suffice to surmount the problem, since in the hydrodynamical case there is a medium that supports and transmits the presure and the stresses. By contrast, in the quantum single-particle problem we are not dealing with a collective system; the ‘collection’ may be a conceptual ensemble, devoid of physical existence.

  19. 19.

    Bell inequalities is a collective name referring to a number of inequalities (such as the chsh-type inequalities) that involve correlations between variables of the constituents of a composite system and are violated by qm, reputedly due to the nonlocal properties of the quantum description.

  20. 20.

    The transmitted particles are among those that gain enough energy to travel not through the barrier, but over it (see e.g. Lopreore and Wyatt 1999).

  21. 21.

    This feature is not exclusive of the present example, but rather the general rule: \(V_{Q}\) does not decay as \(x\rightarrow \pm \infty ,\) i.e., at far distances from the particles.

  22. 22.

    The effective interaction potential introduced via \(V_{Q}(\varvec{x}_{1}, \varvec{x}_{2})\), which remains ‘hidden’ in the depths of the Schrödinger equation, formally transforms the original noninteracting system into an interacting one [see Eq. (8.52)]. By contrast, the possible nonfactorizability of \(\exp (iS)\) does not manifest itself as a formal interaction potential in Eq. (8.52). The nonlocal effect of this kind of entanglement is manifested when a description in terms of forces is made, as we have seen.

  23. 23.

    We use here the term covariance to refer to a two-point momentum \(\langle \hat{F}_{1}\hat{G}_{2}\rangle \), even if the product \(\langle \hat{F}_{1}\rangle \langle \hat{G}_{2}\rangle \) differs from zero. In the literature the term ‘correlation’Correlation is frequently used for \(\langle \hat{F}_{1} \hat{G}_{2}\rangle \), so we use it here when convenient.

  24. 24.

    From this perspective, the conclusions reached regarding the dispersive and nonlocal features of the quantum potential (a quantity that depends on \(u\) only) become evident.

  25. 25.

    When the operator \(\hat{A}\) does not correspond to a single particle, this statement ceases to be true. For example, for \(\hat{A}=A_{1}( \hat{x}_{1})A_{2}(\hat{x}_{2}),\) the entanglement is revealed in the covariance Covariance \(\left\langle A_{1}A_{2}\right\rangle \) even though none of the variables is momentum-dependent. In fact, the point here is to show that the present approach allows to reach conclusions about entanglement by focusing on single-particle variables, rather than on correlations between variables of the two subsystems, as is customarily done [see discussion following Eq. (8.96)].

  26. 26.

    The \(p\)-local mean value of a dynamic variable \(g\) is defined, in analogy with Eq. (4.50), as its partial average over the configuration space, using the distribution \(Q\),

    $$\begin{aligned} \left\langle g\right\rangle (p_{1},p_{2})=\left\langle g\right\rangle _{p}= \frac{1}{\rho _{p}}\int gQ(x_{1},x_{2},p_{1},p_{2})dx_{1}dx_{2}. \end{aligned}$$
  27. 27.

    The fact that the kind of variables that may exhibit nonlocality is representation-dependent does not mean that the very existence of nonlocality is representation-dependent. Indeed, for any entangled state \( \left| \psi \right\rangle \) there will always be some variable exhibiting nonlocal features; which one depends on the representation used to project \(\left| \psi \right\rangle \).

  28. 28.

    Equation (8.87) is just Eq. (8.92) with \(\hat{A}_{i}=f(\hat{x} _{i})\), yet Eq. (8.86) differs from the structure of (8.92). To see this consider in particular Eq. (8.84) with \(n=1;\) then \( P_{i}(\pi _{i},\partial _{i}^{k}\pi _{i})=m_{i}v_{i}(x_{i})\ne \left\langle x_{i}\right| \hat{p}_{i}\left| x_{i}\right\rangle \), so indeed (8.86) is not Eq. (8.92) for \(\hat{A}=\hat{g}_{i}\) and \(\alpha =x_{i}\).

  29. 29.

    Notice that the use of a fixed representation for both elements of the composite system, i.e. \(\{ \left| \alpha \right\rangle _{1}\} ,\) \(\{ \left| \beta \right\rangle _{2}\} \), is a matter of necessity when discussing entanglement. The same applies when considering measurements on a system. In fact, given an \((\alpha ,\beta )\)-representation, the distribution function \(\rho \left( \alpha ,\beta \right) \) is defined as the joint probabilityProbability!joint density that determines the probability of obtaining the values \(\alpha \) and \(\beta \) when performing the projective measurements corresponding to the proyectors \(\Pi _{A_{1}}^{\alpha }=\left| \alpha \right\rangle \left\langle \alpha \right| \) \(\in \mathcal {H}_{1}\) and \(\Pi _{B_{2}}^{\beta }=\left| \beta \right\rangle \left\langle \beta \right| \) \(\in \mathcal {H}_{2},\) respectively. Thus the representation used is linked with the variables that are measured in a certain experiment.

  30. 30.

    This conclusion is in line with the results obtained in Sect. 7.2.5. Specifically, the discussion following Eq. (7.63) tells us that for entanglement to become manifest through a correlation, both dynamical variables involved (i.e., \(F,G\), the equivalent of \(A_{1},B_{2}\) in the present case) must have nondiagonal elements in a given representation (the energy representation, in that case).

  31. 31.

    Note that, as already remarked in connection with von Neumann’s theorem [see Eq. (8.2)], the equality

    $$\begin{aligned} \langle \hat{C}\rangle =\langle \hat{a}\hat{b}\rangle +\langle \hat{a}\hat{B} \rangle +\langle \hat{A}\hat{b}\rangle -\langle \hat{A}\hat{B}\rangle \end{aligned}$$

    does not hold in general if the operators in the terms of the sum do not commute. This important restriction needs to be borne in mind when attempting to apply (8.94) [or (8.96)] to draw conclusions aboutAccardi L. Fargue, D. correlations. See e.g. Accardi (1984).

  32. 32.

    With an eye put on note (31), making sure that the average is taken over the same distribution in each term.

  33. 33.

    The extra correlations that lead to the violation of a Bell inequality exist also in the case of photons, due to the correlations between the excitations of the field and the corresponding modes of the zpf; see e.g. Casado, A. Casado et al. (1998).

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Correspondence to Ana María Cetto .

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de la Peña, L., Cetto, A.M., Valdés Hernández, A. (2015). Causality, Nonlocality, and Entanglement in Quantum Mechanics. In: The Emerging Quantum. Springer, Cham. https://doi.org/10.1007/978-3-319-07893-9_8

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