The Simplest Determination of the Thermodynamical Characteristics of Kerr-Newman Black Hole - General Relativity and Quantum CosmologyReport as inadecuate




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Abstract: In this work, generalizing our previous results, we determine in an originaland the simplest way three most important thermodynamical characteristicsBekenstein-Hawking entropy, Bekenstein quantization of the entropy or outerhorizon surface area and Hawking temperature of Kerr-Newman black hole. Westart physically by assumption that circumference of Kerr-Newman black holeouter horizon holds the natural integer number of corresponding reducedCompton-s wave length and use mathematically, practically, only simplealgebraic equations. It is conceptually similar to Bohr-s quantizationpostulate in Bohr-s atomic model interpreted by de Broglie relation.



Author: Vladan Pankovic, Simo Ciganovic, Rade Glavatovic

Source: https://arxiv.org/







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