Mechanism of Generation of Black Hole Entropy in Sakharov's Induced Gravity
V.P. Frolov, D.V. Fursaev

TL;DR
This paper proposes a mechanism in Sakharov's induced gravity explaining black hole entropy through finite 'physical' modes, linking entropy, Noether charge, and quantum fluctuations, and clarifying the nature of degrees of freedom responsible for black hole thermodynamics.
Contribution
It introduces a finite subset of modes accounting for black hole entropy in induced gravity and relates entropy to Noether charge and quantum fluctuations.
Findings
Physical modes' entropy matches Bekenstein-Hawking entropy.
Difference between Rindler and physical modes is a surface integral Q.
Probability distribution of physical modes peaks at zero energy, matching black hole entropy.
Abstract
The mechanism of generation of the Bekenstein-Hawking entropy of a black hole in the Sakharov's induced gravity is proposed. It is suggested that the "physical" degrees of freedom, which explain the entropy , form only a finite subset of the standard Rindler-like modes defined outside the black hole horizon. The entropy of the Rindler modes, or entanglement entropy, is always ultraviolet divergent, while the entropy of the "physical" modes is finite and it coincides in the induced gravity with . The two entropies and differ by a surface integral Q interpreted as a Noether charge of non-minimally coupled scalar constituents of the model. We demonstrate that energy E and Hamiltonian H of the fields localized in a part of space-time, restricted by the Killing horizon , differ by the quantity , where is the temperature of a…
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