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Quantum Studies Mathematics and Foundations

Could ordinary quantum mechanics be just fine for all practical purposes?

А. В. Никулов

Published Aug 29, 2015• 10 citations
Publisher
DOI
10.1007/s40509-015-0057-3

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In this paper we construct the commutators of the Fedosov * (a generalization of the Moyal star product) on the phase space of S2. It is shown that this product obeys the standard angular momentum commutation relations in ordinary nonrelativistic quantum mechanics. The purpose of this paper is three-fold. One is to find an exact, non-perturbative solution to the commutators of the Fedosov *. The other is to verify that these commutation relations correspond to angular momentum commutation relations as in ordinary nonrelativistic quantum mechanics. The last is to show a more general computation of the Fedosov *; essentially undeforming Fedosov's algorithm.
The paper takes up Bell's (1987) "Everett (?) theory" and develops it further. The resulting theory is about the system of all particles in the universe, each located in ordinary, 3-dimensional space. This many-particle system as a whole performs random jumps through 3N-dimensional configuration space - hence "Tychistic Bohmian Mechanics" (TBM). The distribution of its spontaneous localisations in configuration space is given by the Born Rule probability measure for the universal wavefunction. Contra Bell, the theory is argued to satisfy the minimal desiderata for a Bohmian theory within the Primitive Ontology framework (for which we offer a metaphysically more perspicuous formulation than is customary). TBM's formalism is that of ordinary Bohmian Mechanics (BM), without the postulate of continuous particle trajectories and their deterministic dynamics. This "rump formalism" receives, however, a different interpretation. We defend TBM as an empirically adequate and coherent quantum theory. Objections voiced by Bell and Maudlin are rebutted. The "for all practical purposes"-classical, Everettian worlds (i.e. quasi-classical histories) exist sequentially in TBM (rather than simultaneously, as in the Everett interpretation). In a temporally coarse-grained sense, they quasi-persist. By contrast, the individual particles themselves cease to persist.
In ordinary and relativistic quantum mechanics the energy spectra of most of the Hamiltonians cannot be obtained exactly. Approximate methods have to be used among which the variational one is particuarly popular. The purpose of this paper is to show that when the matrices appearing in a Dirac equation with interaction, are replaced by a direct product of matrices associated with ordinary and what we call sign spins, then a standard complete set of non-relativistic wavefunctions can be used to carry out the variational calculations. To illustrate the power of our method we analyse first the variational energies of ordinary and Dirac relativistic oscillator Hamiltonians, and then indicate the procedure for the general one-particle case. The extensions to higher spins, or to a larger number of particles, are briefly mentioned in the conclusion.