Metric fluctuations of an evaporating black hole from back reaction of stress tensor fluctuations

TL;DR

This study investigates quantum-induced spacetime fluctuations around evaporating black holes, revealing that fluctuations grow over time and challenge classical horizon localization, suggesting a finite effective horizon width.

Contribution

It provides the first systematic quantitative analysis of metric fluctuations due to stress tensor fluctuations in evaporating black holes within the stochastic gravity framework.

Findings

Fluctuations grow significantly over the black hole's evaporation time.

Simple horizon flux correlations are invalid, affecting fluctuation predictions.

Quantum fluctuations imply a finite effective width for the black hole horizon.

Abstract

This paper delineates the first steps in a systematic quantitative study of the spacetime fluctuations induced by quantum fields in an evaporating black hole under the stochastic gravity program. The central object of interest is the noise kernel, which is the symmetrized two-point quantum correlation function of the stress tensor operator. As a concrete example we apply it to the study of the spherically-symmetric sector of metric perturbations around an evaporating black hole background geometry. For macroscopic black holes we find that those fluctuations grow and eventually become important when considering sufficiently long periods of time (of the order of the evaporation time), but well before the Planckian regime is reached. In addition, the assumption of a simple correlation between the fluctuations of the energy flux crossing the horizon and far from it, which was made in earlier work on spherically-symmetric induced fluctuations, is carefully scrutinized and found to be invalid. Our analysis suggests the existence of an infinite amplitude for the fluctuations when trying to localize the horizon as a three-dimensional hypersurface, as in the classical case, and, as a consequence, a more accurate picture of the horizon as possessing a finite effective width due to quantum fluctuations. This is supported by a systematic analysis of the noise kernel in curved spacetime smeared with different functions under different conditions, the details are collected in the appendices. This case study shows a pathway for probing quantum metric fluctuations near the horizon and understanding their physical meaning.