Quantum corrections to the entropy of charged rotating black holes

2010/02/18 by M. Akbar, K. Saifullah · 1 citation
Physics and Astronomy · Mathematics · #gr-qc #hep-th #math-ph #math.MP

paper · pdf · doi:10.1140/epjc/s10052-010-1279-5

published as Eur. Phys. J. C Vol 67 (2010) 205

arxiv created 2010/02/18 · arxiv updated 2015/05/18

Abstract

Hawking radiation from a black hole can be viewed as quantum tunneling of particles through the event horizon. Using this approach we provide a general framework for studying corrections to the entropy of black holes beyond semiclassical approximations. Applying the properties of exact differentials for three variables to the first law thermodynamics, we study charged rotating black holes and explicitly work out the corrections to entropy and horizon area for the Kerr-Newman and charged rotating BTZ black holes. It is shown that the results for other geometries like the Schwarzschild, Reissner-Nordström and anti-de Sitter Schwarzschild spacetimes follow easily.

Cited by

• Regularization of Kerr-NUT spacetimes and their thermodynamical quantities

Related

• Quantum Entropy of Charged Rotating Black Holes
• Black hole quantum tunnelling and black hole entropy correction
• Corrected entropy of high dimensional black holes
• The effect of quantum correction on Hawking radiation for Schwarzschild black holes
• Area spectrum and black hole thermodynamics