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

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

2008-04-15

arxiv.org/abs/0804.2327v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, no figures

Scientific paper

In 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.)

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