Abstract
The difficult issues related to the interpretation of quantum mechanics and, in particular, the “measurement problem” are revisited using as motivation the process of generation of structure from quantum fluctuations in inflationary cosmology. The unessential mathematical complexity of the particular problem is bypassed, facilitating the discussion of the conceptual issues, by considering, within the paradigm set up by the cosmological problem, another problem where symmetry serves as a focal point: a simplified version of Mott’s problem.
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Notes
We are ignoring the fact that certain interpretations are problematic.The point however is that to the extent that they are applied in a particular manner in concrete situations they do not offer predictions that differ from the text book version of Quantum Theory.
The favored version of the theory actually deals with a composite variable representing the quantum aspects of the inflaton field and a certain component of the space-time metric [6].
We refer here to the stage corresponding to several e-folds after the start of inflation, when the background corresponds to an inflating, flat, Robertson Walker space-time, and the “quantum fluctuations” are described by the Bunch-Davies vacuum, or some similarly highly symmetric state. This characterization is thought to be accurate up to exponentially small corrections in the number of e-folds, a detail that we will ignore as is customary in all inflationary analyses.
There are, apparently, some people who disagree with this view, but we will not consider their thinking any further here.
It even seems possible to construct wave packets with high n in an hydrogen atom that resemble to some degree the situation above.
There are apparently philosophical views inspired in Kantian ontology where this statement could be questioned.
In fact in order to do that one would need not only to define the privileged basis but also to add a postulate about actualization.
Except, of course the zero modo of the inflaton.
This point is sometimes characterized as the “transition from the quantum regime to the classical regime”, but we find this a bit misleading: most people would agree that there are no classical or quantum regimes. The fundamental description ought to be always a quantum description. However, there exist regimes in which certain quantities can be described to a sufficient accuracy by their classical counterparts represented by the corresponding expectation values. All this depends, of course, on the physical state, the underlying dynamics, the quantity of interest, and the context which one is considering.
On the other hand, it is worth noting that the Hamiltonian of interaction between particle and detector has a explicitly local form in the first basis but not in the second. This might be used but it would have to be explicitly formulated as part of the theory. Spontaneous localization theories, and de-Broglie Bohm approaches, for instance focus on position as playing a preferential role.
Let \(\hat{S}\) be a symmetry operator and \(|\Psi (0)\rangle \) an initial symmetric state, i.e. \(\hat{S} |\Psi (0)\rangle =|\Psi (0)\rangle \). Let \(\hat{H}(t)\) be the system’s hamiltonian, taken to be invariant under the symmetry i.e. \([\hat{H} (t),\hat{S}]=0\). Then \(\hat{S}|\Psi (t)\rangle =\hat{S}e^{i\int _{0} ^{t}H(t^{\prime })dt^{\prime }}|\Psi (0)\rangle =e^{i\int _{0}^{t}H(t^{\prime })dt^{\prime }}\hat{S}|\Psi (0)\rangle =e^{i\int _{0}^{t}H(t^{\prime })dt^{\prime } }|\Psi (0)\rangle =|\Psi (t)\rangle \) i.e. the evolved state is also symmetric.
According to [92] the posture is that one should believe both, and use the appropriate one in connection with the questions one is asking. This posture is not shared by other authors, for instance [87]. Moreover it seems the implicit views regarding the nature of science are very problematic in general (see for instance [93, 96,97,98,99]).
There exists many variants of the major themes we have considered here, and they have not been described in detail because the differences have no bearing on the issue at hand. Namely these variants fail to address the issue we face, for exactly the same reasons as the major ones they are closely connected with. However, we acknowledge that there might exist some other proposal we are unaware of, and which fare better in dealing with the problem we have been considering in this work.
With the possible exception of the d’ Broglie- Bohm approach, where the source of the primordial asymmetries is found in the initial conditions.
We are ignoring here the issue of how this decay became actualized into that particular direction, as the point here is to exemplify a specific technical issue.
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Acknowledgements
This work was supported, in part, by CONACYT (México) Project 101712, a PAPPIT-UNAM (México) project IN107412 and sabbatical fellowships from CONACYT and DGAPA-UNAM (México). D.S. wants to thank the IAFE at the university of Buenos Aires for the hospitality during the sabbatical stay. This work was partially supported by Grants: of the Research Council of Argentina (CONICET), by the Endowment for Science and by Technology of Argentina (FONCYT), and by the University of Buenos Aires. We acknowledge very useful discussions with B. Kay and Elias Okon.
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Appendix
Appendix
In this appendix, we discuss some specific issues that arise in the attempt to use decoherence related arguments in the context of the problem at hand.
The first issue is that connected to the implication of symmetry regarding the choice of a preferential basis or so called pointer states.
The simplest example exhibiting this problem is provided by a standard EPR-R setup: Consider the decay of a spin 0 particle into two spin 1/2 particles. Take the direction of the decay as being the x axis (the particles momenta are \(\vec P= \pm P \hat{x}\) with \(\hat{x}\) the unit vector in the \(\vec x \) direction)Footnote 15. Now, we characterize the two particle states, that emerges after the decay in terms of the \(\vec {z}\) polarization states of the two Hilbert spaces of individual particles. As it is known, the conservation of the angular momentum of the system indicates that the state must be:
The state is clearly invariant under rotations around the x axis (simply because it is an eigen-state with zero angular momentum along that axis). The density matrix for the system is thus \(\rho = |\chi \rangle \langle \chi |\). Now assume we decide we are not interested in one of the particles (call it 1), and thus we regard it as an environment for the system of interest (particle 2). The reduced density matrix is then:
Now suppose we want to say that as the reduced density matrix is diagonal, we have found the pointer basis and that somehow the particle must be considered as having its spin along the z axis defined to be either \(+1/2 \) or \(-1/2\).
The problem is that the symmetry of the state \(|\chi \rangle \) regarding rotations around the x axis is reflected in the fact that we could have written this density matrix also as
leading, this time, to the conclusion that the particle must be considered as having its spin along the y axis defined to be either \(+1/2 \) or \(-1/2\).
In fact, as the density matrix is proportional to the identity ( i.e. \(\rho ^{(2)} = \frac{1}{ 2} I\)) it would have the same form in any orthogonal basis.
One might be inclined to consider that this problem occurs only in very simple situations, such as the one of the above example, and that, in general, we will not encounter such difficulty. However that consideration is mistaken as can be seen from the general result encapsulated in the following:
1.1 Theorem
Consider a quantum system made of a subsystem S and an environment E, with corresponding Hilbert spaces \(H_{S}\) and \(H_{E}\) so that the complete system is described by states in the product Hilbert space \(H_{S}\otimes H_{E}\). Let G be a symmetry group acting on the Hilbert space of the full system in a way that does not mix the system and environment. That is, the unitary representation O of G on \(H_{S}\otimes H_{E}\) is such that \(\forall g \in G\), \(\hat{O}(g) = \hat{O}^{S}(g)\otimes \hat{O}^{E}(g)\), where \(\hat{O}^{S}(g)\) and \(\hat{O}^{E}(g)\) act on \(H_{S}\) and \(H_{E}\) respectively.
Let the system be characterized by a density matrix \(\hat{\rho }\) which is invariant under G. Then the reduced density matrix of the subsystem is a multiple of the identity in each invariant subspace of \(H_{S}\).
1.2 Proof
The reduced density matrix \(\hat{\rho }_{S}= Tr_{E} ( \hat{\rho })\).The trace over the environment of any operator \(\hat{A}\) in \(H_{S}\otimes H_{E}\) is obtained by taking any orthonormal basis \(\lbrace |e_{j}\rangle \rbrace \) of \(H_{E}\) and evaluating \(\Sigma _{j} \langle e_{j}| \hat{A} |e_{j}\rangle \).
Now, by assumption, we have \(\hat{\rho }= {\hat{O}(g)}^{\dagger }\hat{\rho }\hat{O}(g)\), \(\forall g \in G\). Then, for all \(g \in G\), we have \(\hat{\rho }_{S} = \Sigma _{j} \langle e_{j}| \hat{\rho }|e_{j}\rangle = \Sigma _{j} \langle e_{j}| {\hat{O}^{S}(g)}^{\dagger }\otimes { \hat{O}^{E}(g)}^{\dagger }\hat{\rho }\hat{O}^{S}(g)\otimes \hat{O}^{E}(g) |e_{j}\rangle = \Sigma _{j} {{\hat{O}}^{S} (g)}^{\dagger }\langle e^{\prime }_{j}| \hat{\rho }|e^{\prime }_{j}\rangle {\hat{O}}^{S}(g)\), where \(|e^{\prime }_{j}\rangle \equiv O^{E}(g) |e_{j}\rangle \). However, the fact that the operator \({\hat{O}}^{E}(g)\) is unitary implies that the transformed states \(\lbrace |e^{\prime }_{j}\rangle \rbrace \) form also an orthonormal basis of \(H_{E}\).
Thus we have \(\hat{\rho }_{S} = {{\hat{O}}^{S}(g)}^{\dagger }( \Sigma _{j} \langle e^{\prime }_{j}| \hat{\rho }|e^{\prime }_{j}\rangle ) {\hat{O}}^{S}(g ) = {{\hat{O}}^{S}(g)}^{\dagger }\hat{\rho }_{S} {\hat{O}}^{S}(g )\) or equivalently \(\hat{\rho }_{S} {{\hat{O}}^{S}(g)} = {\hat{O}}^{S}(g ) \hat{\rho }_{S}\). So we have found that \([ \hat{\rho }_{S} , {\hat{O}}^{S}(g )]=0\), \(\forall g \in G\), and thus by Schur’s lemma it follows that \(\hat{\rho }_{S}\) must be a multiple of the identity in each invariant subspace of \(H_{S}\), QED.
In particular, this result indicates that, if we start with a pure state invariant under the symmetry group, the reduced density matrix must be a multiple of the identity in each invariant subspace of \(H_{S}\). This is exemplified by the well known case of a standard EPR setting, where a spinless particle decays into two photons, and where one considers the photons’ spin degrees of freedom. The reduced density matrix describing one of the photons is a multiple of the identity, and thus the decoherence that results from tracing over the first photon’s spin does not determine a preferential basis for the characterization of the spin of the second photon. Decoherence then fails under these conditions to provide a well defined preferential context for the interpretation of the reduced density matrix, as representing the various alternatives for the state of the subsystem after decoherence.
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Castagnino, M., Fortin, S., Laura, R. et al. Interpretations of Quantum Theory in the Light of Modern Cosmology. Found Phys 47, 1387–1422 (2017). https://doi.org/10.1007/s10701-017-0100-9
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DOI: https://doi.org/10.1007/s10701-017-0100-9
Keywords
- Interpretation of quantum mechanics
- Measurement problem
- Foundations of quantum mechanics