Entropy of extreme three-dimensional charged black holes
High Energy Physics - Theory
2009-10-31 v1
Abstract
It is shown that three-dimensional charged black holes can approach the extreme state at nonzero temperature. Unlike even dimensional cases, the entropy for the extreme three-dimensional charged black hole is uniquely described by the Bekenstein-Hawking formula, regardless of different treatments of preparing the extreme black hole, namely, Hawking's treatment and Zaslavskii's treatment.
Keywords
Cite
@article{arxiv.hep-th/9911005,
title = {Entropy of extreme three-dimensional charged black holes},
author = {Bin Wang and Elcio Abdalla},
journal= {arXiv preprint arXiv:hep-th/9911005},
year = {2009}
}
Comments
latex file, 8 pages. To be published in Physics Letters B