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Superselection from canonical constraints

Michael J W Hall

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The evolution of both quantum and classical ensembles may be described via the probability density P on configuration space, its canonical conjugate S, and an ensemble Hamiltonian \skew3\tilde{H}[P,S] . For quantum ensembles this evolution is, of course, equivalent to the Schrödinger equation for the wavefunction, which is linear. However, quite simple constraints on the canonical fields P and S correspond to nonlinear constraints on the wavefunction. Such constraints act to prevent certain superpositions of wavefunctions from being realized, leading to superselection-type rules. Examples leading to superselection for energy, spin direction and 'classicality' are given. The canonical formulation of the equations of motion, in terms of a probability density and its conjugate, provides a universal language for describing classical and quantum ensembles on both continuous and discrete configuration spaces, and is briefly reviewed in an appendix.


PACS

03.65.Ge Solutions of wave equations: bound states

03.65.Ta Foundations of quantum mechanics; measurement theory

02.50.Cw Probability theory

MSC

81Q05 Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other quantum-mechanical equations

60K99 None of the above, but in this section

Subjects

Computational physics

Quantum information and quantum mechanics

Dates

Issue 31 (6 August 2004)

Received 21 April 2004, in final form 1 June 2004

Published 21 July 2004



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