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Statistical Origin of Black Hole Entropy in Induced Gravity

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arxiv hep-th/9607104 v1 pith:GL2KGYQE submitted 1996-07-12 hep-th gr-qc

V. P. Frolov , D. V. Fursaev , A. I. Zelnikov This is my paper · ORCID
classification hep-thgr-qc
keywords entropyinducedgravityactionblackfieldsholeorigin
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abstract

The statistical-mechanical origin of the Bekenstein-Hawking entropy $S^{BH}$ in the induced gravity is discussed. In the framework of the induced gravity models the Einstein action arises as the low energy limit of the effective action of quantum fields. The induced gravitational constant is determined by the masses of the heavy constituents. We established the explicit relation between statistical entropy of constituent fields and black hole entropy $S^{BH}$.

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Cited by 2 Pith papers

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

  1. Symmetry-Resolved Entanglement Entropy from Heat Kernels

    hep-th 2025-11 unverdicted novelty 7.0 of 10

    An improved heat kernel framework with phase-factor reconstruction computes symmetry-resolved entanglement entropy for charged systems and derives a cMERA flow equation that agrees with CFT and holographic calculations.

  2. Schwinger instability, modular flow, and holographic entropy for near-extremal charged BTZ black hole

    hep-th 2025-05 reject novelty 3.0 of 10

    A semiclassical study of charged pair creation and horizon entropy in near-extremal charged BTZ, whose central alignment claim is not actually established by the calculations.

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