Linear perturbations of self-gravitating spherically symmetric configurations

TL;DR

This paper introduces a new covariant, gauge-invariant formalism for analyzing linear metric perturbations on spherically symmetric backgrounds in general relativity, applicable to both vacuum and matter-coupled cases, simplifying the study of gravitational waves and fluid perturbations.

Contribution

It develops a novel formalism that avoids harmonic decomposition and applies to dynamic, non-vacuum backgrounds, providing new master equations and a comprehensive treatment of matter coupling.

Findings

Derived covariant master equations for gravitational waves on Schwarzschild black holes.

Formulated a constrained wave system for metric and matter perturbations.

Applied the formalism to Einstein-Euler system, separating fluid perturbations into entropy, vorticity, and potential flow components.

Abstract

We present a new covariant, gauge-invariant formalism describing linear metric perturbation fields on any spherically symmetric background in general relativity. The advantage of this formalism relies in the fact that it does not require a decomposition of the perturbations into spherical tensor harmonics. Furthermore, it does not assume the background to be vacuum, nor does it require its staticity. In the particular case of vacuum perturbations, we derive two master equations describing the propagation of arbitrary linear gravitational waves on a Schwarzschild black hole. When decomposed into spherical harmonics, they reduce to covariant generalizations of the well-known Regge-Wheeler and Zerilli equations. Next, we discuss the general case where the metric perturbations are coupled to matter fields and derive a new constrained wave system describing the propagation of three gauge-invariant scalars from which the complete metric perturbations can be reconstructed. We apply our formalism to the Einstein-Euler system, dividing the fluid perturbations into two parts. The first part, which decouples from the metric perturbations, obeys simple advection equations along the background flow and describes the propagation of the entropy and the vorticity. The second part describes a perturbed potential flow, and together with the metric perturbations it forms a closed wave system.