Mimicking Black Holes in General Relativity

TL;DR

This thesis explores various models of black hole mimickers such as regular black holes and traversable wormholes within general relativity, analyzing their properties, stability, and astrophysical observables.

Contribution

It introduces new regular black hole and wormhole models, and applies the Darmois-Israel formalism for stability analysis, advancing understanding of black hole mimickers in classical GR.

Findings

Astrophysical observables calculated for a specific regular black hole model.

Constructed a wormhole from a regular black hole using cut-and-paste technique.

Performed stability analysis of the dynamic wormhole throat.

Abstract

The central theme of this thesis is the study and analysis of black hole mimickers. The concept of a black hole mimicker is introduced, and various mimicker spacetime models are examined within the framework of classical general relativity. The mimickers examined fall into the classes of regular black holes and traversable wormholes under spherical symmetry. The regular black holes examined can be further categorised as static spacetimes, however the traversable wormhole is allowed to have a dynamic (non-static) throat. Astrophysical observables are calculated for a recently proposed regular black hole model containing an exponential suppression of the Misner-Sharp quasi-local mass. This same regular black hole model is then used to construct a wormhole via the ''cut- and-paste'' technique. The resulting wormhole is then analysed within the Darmois-Israel thin-shell formalism, and a linearised stability analysis of the (dynamic) wormhole throat is undertaken. Yet another regular black hole model spacetime is proposed, extending a previous work which attempted to construct a regular black hole through a quantum ''deformation'' of the Schwarzschild spacetime. The resulting spacetime is again analysed within the framework of classical general relativity. In addition to the study of black hole mimickers, I start with a brief overview of the theory of special relativity where a new and novel result is presented for the combination of relativistic velocities in general directions using quaternions. This is succeed by an introduction to concepts in differential geometry needed for the successive introduction to the theory of general relativity. A thorough discussion of the concept of spacetime singularities is then provided, before analysing the specific black hole mimickers discussed above.