arXiv · hep-th/9603078
Macroscopic and Microscopic Entropy of Near-Extremal Spinning Black Holes
Abstract
A seven parameter family of five-dimensional black hole solutions depending on mass, two angular momenta, three charges and the asymptotic value of a scalar field is constructed. The entropy is computed as a function of these parameters both from the Bekenstein-Hawking formula and from the degeneracies of the corresponding D-brane states in string theory. The expressions agree at and to leading order away from extremality.
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J. C. Breckenridge, D. A. Lowe, R. C. Myers, A. W. Peet, A. Strominger, C. Vafa. 1996-03-13. Macroscopic and Microscopic Entropy of Near-Extremal Spinning Black Holes. https://doi.org/10.1016/0370-2693(96)00553-9
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