Spherically-symmetric solutions in general relativity

TL;DR

This paper introduces a tetrad-based approach for solving spherically-symmetric Einstein equations, addressing gauge issues, and compares it with the Lemaître-Tolman-Bondi model, demonstrating advantages in physical interpretation and flexibility.

Contribution

The paper develops a tetrad-based method for spherically symmetric solutions in general relativity, offering improvements over the LTB model in handling gauge freedom and pressure.

Findings

Tetrad method avoids gauge ambiguities present in LTB.

Applicable to models with pressure and non-compensated regions.

Clarifies the behavior of horizons in cosmological models.

Abstract

We present a tetrad-based method for solving the Einstein field equations for spherically-symmetric systems and compare it with the widely-used Lema\^itre-Tolman-Bondi (LTB) model. In particular, we focus on the issues of gauge ambiguity and the use of comoving versus 'physical' coordinate systems. We also clarify the correspondences between the two approaches, and illustrate their differences by applying them to the classic examples of the Schwarzschild and Friedmann-Robertson-Walker spacetimes. We demonstrate that the tetrad-based method does not suffer from the gauge freedoms inherent to the LTB model, naturally accommodates non-zero pressure and has a more transparent physical interpretation. We further apply our tetrad-based method to a generalised form of 'Swiss cheese' model, which consists of an interior spherical region surrounded by a spherical shell of vacuum that is embedded in an exterior background universe. In general, we allow the fluid in the interior and exterior regions to support pressure, and do not demand that the interior region be compensated. We pay particular attention to the form of the solution in the intervening vacuum region and verify the validity of Birkhoff's theorem at both the metric and tetrad level. We then reconsider critically the original theoretical arguments underlying the so-called $R_h = ct$ cosmological model, which has recently received considerable attention. These considerations in turn illustrate the interesting behaviour of a number of 'horizons' in general cosmological models.