Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole

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dc.creatorKiselev, V. V.
dc.date2004-12-21
dc.date2005-01-04
dc.date.accessioned2026-07-07T03:29:17Z
dc.date.available2026-07-07T03:29:17Z
dc.descriptionThe entropy of charged black hole is calculated by using the partition function evaluated at radial geodesics confined under horizons. We establish two quantum phase states inside the black hole and a transition between them.
dc.description10 pages, 6 eps-figures, iopart class, acknowledgement extended
dc.identifierhttps://arxiv.org/abs/gr-qc/0412097
dc.identifierhttp://arxiv.org/abs/gr-qc/0412097
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35157
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleRadial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole
dc.typetext

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