Relative Entropy from Coherent States in Black Hole Thermodynamics and Cosmology

TL;DR

This paper explores how relative entropy of coherent states relates to the thermodynamics of black holes and cosmological horizons, providing a unified framework for static and dynamical cases, including Vaidya spacetime.

Contribution

It extends the application of relative entropy to dynamical horizons and cosmological scenarios, deriving a natural notion of entropy for evolving black holes.

Findings

Relative entropy variation links to horizon growth via stress-energy conservation.

A natural entropy proportional to horizon area emerges for dynamical black holes.

Additional work term appears in the entropy variation for dynamical horizons.

Abstract

The aim of this work is to study the role of relative entropy in the thermodynamics of black holes and cosmological horizons. We adapt some recent results on the relative entropy of coherent excitations of the vacuum, to find the variation of generalised entropy of static and dynamical black holes and for cosmological horizons. We review the argument for static black holes by Hollands and Ishibashi (2019) with simple modifications. We link the variation of relative entropy to the growth of the horizon using a conservation law for the stress-energy tensor, and we recover the known results. We then study the application of the same framework to the case of dynamical horizons. We study in detail the case of Vaidya spacetime, and we find that a notion of black hole entropy naturally emerges, equals to one-fourth of the area of the dynamical horizon. In the case of dynamical black holes we find an additional term, which is not present in the static case, and that represents the work done on the black hole. We finally show in a simple case that it is possible to follow the same scheme to assign an entropy to the horizons emerging in cosmological scenarios.