Role of Various Entropies in the Black Hole Information Loss Problem

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dc.creatorNieuwenhuizen, Th. M.
dc.creatorVolovich, I. V.
dc.date2005-07-27
dc.date.accessioned2026-07-07T04:18:29Z
dc.date.available2026-07-07T04:18:29Z
dc.descriptionIn a recent paper Hawking has argued that there is no information loss in black holes in asymptotically AdS spacetimes. We remind that there are several types of information (entropy) in statistical physics -- fine grained (microscopic) and coarse grained (macroscopic) ones which behave differently under unitary evolution. We suggest that the coarse grained information of the rest of the Universe is lost while fine grained information is preserved. A possibility to develop in quantum gravity an analogue of the Bogoliubov derivation of the irreversible Boltzmann and Navier - Stokes equations from the reversible mechanical equations is discussed.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0507272
dc.identifierhttp://arxiv.org/abs/hep-th/0507272
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53201
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectStatistical Mechanics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectQuantum Physics
dc.titleRole of Various Entropies in the Black Hole Information Loss Problem
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