Entropy of extreme three-dimensional charged black holes
arXiv:hep-th/9911005 · doi:10.1016/S0370-2693(99)01240-X
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.
latex file, 8 pages. To be published in Physics Letters B
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