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Thermodynamic relation of accelerating black holes in anti-de Sitter spacetime

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arxiv 2407.21329 v3 pith:5LOQEZD5 submitted 2024-07-31 gr-qc hep-th

classification gr-qchep-th
keywords blackholesacceleratingextremalityrelationanti-deparameterperturbative
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We consider accelerating black holes in four-dimensional anti-de Sitter spacetime and investigate the extremality relations by examining perturbative corrections to both the entropy of black holes and their extremality bounds. It is shown that the so-called Goon and Penco (univeral) relation is also valid for accelerating black holes. Furthermore, it is found that an appropriate matching condition is necessary between the perturbation parameter of the relation with the perturbative correction to such black holes, and the parameter with information about the conical deficits on the north and south poles with the cosmic string tensions in order to satisfy the extremality relations. This result indicates that the extremality (univeral) relation of a class of accelerating black holes holds exhibit behavior similar to the Weak Gravity Conjecture.

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Cited by 1 Pith paper

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

  1. Thermodynamic relation on rotating charged black strings with arbitrary cosmological constant

    hep-th 2025-07 conditional novelty 2.0 of 10

    For rotating charged black strings, the Goon-Penco relation follows directly from the extended first law, making the claimed universality a thermodynamic identity.

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