Radial geodesics as a microscopic origin of black hole entropy. III: Exercise with the Kerr-Newman black hole

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dc.creatorKiselev, V. V.
dc.date2004-12-22
dc.date2005-01-04
dc.date.accessioned2026-07-07T03:29:17Z
dc.date.available2026-07-07T03:29:17Z
dc.descriptionWe specify an angular motion on geodesics to reduce the problem to the case of radial motion elaborated in previous chapters. An appropriate value of entropy for a charged and rotating black hole is obtained by calculating the partition function on thermal geodesics confined under horizons. The quantum aggregation is classified in a similar way to the Reissner--Nordstrom black hole.
dc.description6 pages, 1 eps-figure, iopart class, acknowledgement extended
dc.identifierhttps://arxiv.org/abs/gr-qc/0412110
dc.identifierhttp://arxiv.org/abs/gr-qc/0412110
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35160
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleRadial geodesics as a microscopic origin of black hole entropy. III: Exercise with the Kerr-Newman black hole
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