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

V. V. Kiselev

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arXiv · gr-qc/0412110

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

V. V. Kiselev

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Abstract

We 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.

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V. V. Kiselev. 2005-01-04. Radial geodesics as a microscopic origin of black hole entropy. III: Exercise with the Kerr-Newman black hole. https://arxiv.org/abs/gr-qc/0412110

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