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Area law corrections from state counting and supergravity

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arxiv hep-th/9910179 v1 pith:TTNFH6SY submitted 1999-10-22 hep-th

Gabriel Lopes Cardoso , Bernard de Wit , Thomas Mohaupt This is my paper · ORCID
classification hep-th
keywords blackcountingholesstateareaentropyagreementbekenstein-hawking
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Modifications of the Bekenstein-Hawking area law for black holes are crucial in order to find agreement between the microscopic entropy based on state counting and the macroscopic entropy based on an effective field theory computation. We discuss this and related issues for the case of four-dimensional N=2 supersymmetric black holes. We also briefly comment on the state counting for N=4 and N=8 black holes.

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Cited by 3 Pith papers

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

  1. Black Hole Entropy, Quantum Corrections and EFT Transitions

    hep-th 2025-02 conditional novelty 7.0 of 10

    Quantum corrections to BPS black hole entropy in 4d N=2 string compactifications can be resummed into a finite formula that interpolates between four- and five-dimensional EFT descriptions and matches exact 5d microst...

  2. The Double EFT Expansion in Quantum Gravity

    hep-th 2025-01 conditional novelty 7.0 of 10

    Quantum gravity EFT actions organize higher-curvature corrections into a field-theoretic expansion suppressed by the lightest new mass and a quantum-gravitational expansion suppressed by the species scale.

  3. Pure D-brane Black Holes: BPS Counting and non-BPS Vacua

    hep-th 2026-01 conditional novelty 5.0 of 10

    The (1,1,1,5) and (1,1,1,6) D2-D2-D2-D6 BPS systems yield 2032 and 5616 vacua, matching U-duality, while the analogous non-BPS system has no zero-energy vacua and six doubly-degenerate low-energy minima.

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