The Entropy for General Extremal Black Holes

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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Minor corrections, section 5 refined, references added.

Scientific paper

10.1007/JHEP04(2010)005

We use the Kerr/CFT correspondence to calculate the entropy for all known extremal stationary and axisymmetric black holes. This is done with the help of two ansatzs that are general enough to cover all such known solutions. Considering only the contribution from the Einstein-Hilbert action to the central charge(s), we find that the entropy obtained by using Cardy's formula exactly matches with the Bekenstein-Hawking entropy.

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