The Simplest Determination of the Thermodynamical Characteristics of Kerr-Newman Black Hole

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dc.creatorPankovic, Vladan
dc.creatorCiganovic, Simo
dc.creatorGlavatovic, Rade
dc.date2008-04-15
dc.date.accessioned2026-07-07T09:32:40Z
dc.date.available2026-07-07T09:32:40Z
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 Kerr-Newman black hole. We start physically by assumption that circumference of Kerr-Newman black hole (outer) horizon holds the natural (integer) number of corresponding reduced Compton's wave length and use mathematically, practically, 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/0804.2327
dc.identifierhttp://arxiv.org/abs/0804.2327
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/158863
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Simplest Determination of the Thermodynamical Characteristics of Kerr-Newman Black Hole
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