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First order corrections to black hole thermodynamics: a simple approach enhanced

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arxiv 2312.07127 v3 pith:DGJBCRZX submitted 2023-12-12 gr-qc hep-th

First order corrections to black hole thermodynamics: a simple approach enhanced

classification gr-qc hep-th
keywords approachblackcorrectionsderivativehigherholetermsthermodynamics
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The inclusion of higher derivative terms in the gravitational action brings about corrections to the original forms of black hole solutions and thermodynamics. A simple and valuable approach has emerged over two decades ago, which states that the first order corrections to black hole thermodynamics, caused by higher derivative terms, can be achieved without explicitly solving the perturbed metric. However, a direct application of this approach may potentially yield incorrect answers as it comes to AdS black holes, which poses a challenge to the valuable approach. In this paper, we identify the subtlety associated with AdS black holes is that certain higher derivative terms may alter the asymptotic structure of the spacetime. By taking this subtlety into account, we successfully enhance the original approach and resolve the mentioned problem. Furthermore, we make an interesting observation that the extremalization analysis that underlies this approach also plays a fundamental role in the perturbation theories of quantum mechanics and other disciplines.

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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. Extremalization approach to black hole thermodynamics: perturbations around higher-derivative gravities

    gr-qc 2026-01 unverdicted novelty 5.0

    The extremalization approach to black hole thermodynamics extends to perturbations around known higher-derivative gravity backgrounds such as Einstein-Gauss-Bonnet, yielding first-order thermodynamic corrections in bo...

  2. Validity of the Background Subtraction Method for Black Hole Thermodynamics in Matter-Coupled Gravity Theories

    gr-qc 2025-11 unverdicted novelty 5.0

    Background subtraction for black hole thermodynamics is valid and equivalent to Iyer-Wald in matter-coupled gravity theories, with smooth performance in examples but subtleties for certain matter fields.

  3. Extremalization approach to black hole thermodynamics: perturbations around higher-derivative gravities

    gr-qc 2026-01 accept novelty 4.0

    The Reall–Santos extremalization method is extended to perturbations around Einstein–Gauss–Bonnet backgrounds, reproducing known quasi-topological black-hole thermodynamics without solving the perturbed metric.