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Macroscopic and Microscopic Entropy of Near-Extremal Spinning Black Holes

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arxiv hep-th/9603078 v1 pith:E2ADEFMN submitted 1996-03-13 hep-th

Macroscopic and Microscopic Entropy of Near-Extremal Spinning Black Holes

classification hep-th
keywords blackentropyagreeangularasymptoticawaybekenstein-hawkingcharges
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Classical Unattainability of Extremality in non-BPS D-brane Systems

    hep-th 2026-01 conditional novelty 6.0

    For a non-BPS four-charge D-brane system in N=8 string theory, the worldline potential has no classical zero-energy minimum, so extremality is unattainable; entropy is proposed as the logarithm of the number of isolat...

  2. An extremal black hole with a unique ground state

    hep-th 2024-11 unverdicted novelty 6.0

    Microscopic D-brane description of non-supersymmetric extremal black holes yields a unique ground state with non-zero energy, confirming absence of degeneracy.

  3. Gravitational index of the D1-D5-P black string

    hep-th 2026-07 conditional novelty 4.0

    Complex, supersymmetric, non-extremal Euclidean saddles for the D1-D5-P black string realize the gravitational index and match the Cardy formula of the dual elliptic genus.