Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole

V. V. Kiselev

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Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole

V. V. Kiselev

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Abstract

The entropy of charged black hole is calculated by using the partition function evaluated at radial geodesics confined under horizons. We establish two quantum phase states inside the black hole and a transition between them.

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V. V. Kiselev. 2005-01-04. Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole. https://arxiv.org/abs/gr-qc/0412097

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