pith. sign in

arxiv: hep-th/9806078 · v1 · submitted 1998-06-10 · ✦ hep-th

Black Hole Entropy in Induced Gravity: Reduction to 2D Quantum Field Theory on the Horizon

V. Frolov , D. Fursaev This is my paper
classification ✦ hep-th
keywords gravityinducedblackentropyfieldholehorizonquantum
0
0 comments X
read the original abstract

It is argued that degrees of freedom responsible for the Bekenstein-Hawking entropy of a black hole in induced gravity are described by two dimensional quantum field theory defined on the bifurcation surface of the horizon. This result is proved for a class of induced gravity models with scalar, spinor and vector heavy constituents.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

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

  1. Symmetry-Resolved Entanglement Entropy from Heat Kernels

    hep-th 2025-11 unverdicted novelty 7.0

    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.