Quantum evolution of the Universe from $τ=0$

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dc.creatorCherkas, S. L.
dc.date2003-12-30
dc.date.accessioned2026-07-07T03:28:22Z
dc.date.available2026-07-07T03:28:22Z
dc.descriptionWe have shown that DeWitt constraint H=0 on the physical states of the Universe does not prevent Heisenberg operators and its mean values to evolve with time. Mean value from observable, which is singular in classical theory, is also singular in a quantum case.
dc.description5 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0312120
dc.identifierhttp://arxiv.org/abs/gr-qc/0312120
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34802
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuantum evolution of the Universe from $τ=0$
dc.typetext

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