Elastic Stars in General Relativity: I. Foundations and Equilibrium Models

TL;DR

This paper develops a comprehensive relativistic theory of elastic matter sources, introduces new methods for describing elastic wave speeds, and applies the framework to static spherically symmetric models with elastic crusts or cores.

Contribution

It provides a modern, transparent formulation of elastic matter in general relativity and applies it to equilibrium models with elastic components.

Findings

Derived simple formulas for elastic wave speeds in relativistic matter.

Formulated the equations of motion using the Hadamard elasticity tensor.

Constructed static spherically symmetric models with elastic crusts or cores.

Abstract

The aim of this paper is twofold. First, we set up the theory of elastic matter sources within the framework of general relativity in a self-contained manner. The discussion is primarily based on the presentation of Carter and Quintana but also includes new methods and results as well as some modifications that in our opinion make the theory more modern and transparent. For instance, the equations of motion for the matter are shown to take a neat form when expressed in terms of the relativistic Hadamard elasticity tensor. Using this formulation we obtain simple formulae for the speeds of elastic wave propagation along eigendirections of the pressure tensor. Secondly, we apply the theory to static spherically symmetric configurations using a specific equation of state and consider models either having an elastic crust or core.