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arXiv · hep-th/9607107

Near-extremal black hole entropy and fluctuating 3-branes

I. R. Klebanov·A. A. Tseytlin
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Abstract

We discuss the known microscopic interpretations of the Bekenstein-Hawking entropy for configurations of intersecting M-branes. In some cases the entropy scales as that of a massless field theory on the intersection. A different situation, found for configurations which reduce to 1-charge D=5 black holes or 2-charge D=4 black holes, is explained by a gas of non-critical strings at their Hagedorn temperature. We further suggest that the entropy of configurations reducing to 1-charge D=4 black holes is due to 3-branes moving within 5-branes.

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I. R. Klebanov, A. A. Tseytlin. 1996-07-20. Near-extremal black hole entropy and fluctuating 3-branes. https://doi.org/10.1016/0550-3213(96)00459-2

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