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Black hole motion in Euclidean space as a diffusion process. II

K. Ropotenko*

  • State Service for Special Communication and Information Protection of Ukraine, 13 Solomianska Street, Kyiv 03680, Ukraine

  • *ropotenko@ukr.net

Phys. Rev. D 87, 044037 – Published 19 February, 2013

DOI: https://doi.org/10.1103/PhysRevD.87.044037

Abstract

A diffusion equation approach to black hole thermodynamics in Euclidean sector is proposed. A diffusion equation for a generic Kerr-Newman black hole in Euclidean sector is derived from the Bloch equation. Black hole thermodynamics is also derived and it is found, in particular, that the entropy of a Kerr-Newman black hole is the same, apart from the logarithmic corrections, as the Bekenstein-Hawking entropy of the black hole.

See Also

Black hole motion in Euclidean space as a diffusion process

K. Ropotenko
Phys. Rev. D 85, 104032 (2012)

Article Text

References (3)

  1. K. Ropotenko, Phys. Rev. D 85, 104032 (2012).
  2. R. P. Feynman, Statistical Mechanics (Benjamin, New York, 1972).
  3. M.Toda, R. Kubo, and N. Saito, Statistical Physics I: Equilibrium Statistical Mechanics (Springer, Berlin, 1983).

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