The KKW Generalized Analysis for a Magnetic Stringy Black Hole
General Relativity and Quantum Cosmology
2016-08-31 v2
Abstract
We apply the Keski-Vakkuri, Kraus and Wilczek (KKW) generalized analysis to a magnetic stringy black hole solution to compute its temperature and entropy. The solution that we choose in the Einstein-dilaton-Maxwell theory is the dual solution known as the magnetic black hole solution. Our results show that the expressions of the temperature and entropy of this non-Schwarzschild-type black hole are not the Hawking temperature and the Bekenstein-Hawking entropy, respectively. In addition, the extremal magnetic stringy black hole is not frozen because it has a constant non-zero temperature.
Cite
@article{arxiv.gr-qc/0412111,
title = {The KKW Generalized Analysis for a Magnetic Stringy Black Hole},
author = {I. Radinschi},
journal= {arXiv preprint arXiv:gr-qc/0412111},
year = {2016}
}
Comments
8 pages, LaTex