The Simplest Determination of the Thermodynamical Characteristics of Schwarzschild, Kerr Andreissner-Nordstrom Black Hole

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dc.creatorPankovic, Vladan
dc.creatorIvanovic, Jovan
dc.creatorPredojevic, Milan
dc.creatorIvanovic, Aleksandar-Meda
dc.date2008-03-05
dc.date.accessioned2026-07-07T09:24:53Z
dc.date.available2026-07-07T09:24:53Z
dc.descriptionIn this work, generalizing our previous results, we determine in an original and the simplest way three most important thermodynamical characteristics (Bekenstein-Hawking entropy, Bekenstein quantization of the entropy or (outer) horizon surface area and Hawking temperature) of Schwarzschild, Kerr and Reissner-Nordstrom black hole. We start physically by assumption that circumference of black hole (outer) horizon holds the natural (integer) number of corresponding reduced Compton's wave length and use mathematically only simple algebraic equations. (It is conceptually similar to Bohr's quantization postulate in Bohr's atomic model interpreted by de Broglie relation.)
dc.description5 pages, no figures
dc.identifierhttps://arxiv.org/abs/0803.0620
dc.identifierhttp://arxiv.org/abs/0803.0620
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/156227
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Simplest Determination of the Thermodynamical Characteristics of Schwarzschild, Kerr Andreissner-Nordstrom Black Hole
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