Black hole motion in Euclidean space as a diffusion process

K. Ropotenko
Phys. Rev. D 85, 104032 – Published 21 May 2012

Abstract

A diffusion equation for a black hole is derived from the Bunster-Carlip equations. Its solution has the standard form of a Gaussian distribution. The second moment of the distribution determines the quantum of black hole area. The entropy of diffusion process is the same, apart from the logarithmic corrections, as the Bekenstein-Hawking entropy.

  • Received 29 February 2012

DOI:https://doi.org/10.1103/PhysRevD.85.104032

© 2012 American Physical Society

Authors & Affiliations

K. Ropotenko*

  • State Service for Special Communication and Information Protection of Ukraine, 5/7 Patorzhynskoho str., Kyiv, 01034, Ukraine

  • *ro@stc.gov.ua

See Also

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

K. Ropotenko
Phys. Rev. D 87, 044037 (2013)

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Issue

Vol. 85, Iss. 10 — 15 May 2012

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