The Decoherence of Phase Space Histories

dc.creatorBrun, Todd A.
dc.date1994-04-12
dc.date1994-04-13
dc.date.accessioned2026-07-07T08:59:23Z
dc.date.available2026-07-07T08:59:23Z
dc.descriptionIn choosing a family of histories for a system, it is often convenient to choose a succession of locations in phase space, rather than configuration space, for comparison to classical histories. Although there are no good projections onto phase space, several approximate projections have been used in the past; three of these are examined in this paper. Expressions are derived for the probabilities of histories containing arbitrary numbers of projections onto phase space, and the conditions for the decoherence of these histories are studied.
dc.description20 pages (RevTex 3.0 macros)
dc.identifierhttps://arxiv.org/abs/gr-qc/9404021
dc.identifierhttp://arxiv.org/abs/gr-qc/9404021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147692
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleThe Decoherence of Phase Space Histories
dc.typetext

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