Black hole formation, holographic thermalization and the AdS/CFT correspondence

TL;DR

This paper explores black hole formation and thermalization in the context of the AdS/CFT correspondence, using numerical and analytical methods to understand strongly coupled quantum field theories and gravity duals.

Contribution

It introduces new solutions for black hole formation in three-dimensional gravity, including non-spherical cases, and develops methods to construct higher spin black holes.

Findings

Black hole formation can be studied via gravitational collapse in AdS.

Confinement affects thermalization, leading to quasiperiodic behavior.

New solutions for non-spherical black holes and higher spin black holes were discovered.

Abstract

The AdS/CFT correspondence is one of the most important discoveries in theoretical physics in recent years. It states that certain quantum mechanical theories can actually be described by classical gravity in one higher dimension, in a spacetime called anti-de Sitter (AdS) space. What makes this duality so useful is that it relates theories with weak coupling to theories with strong coupling and thus provides a new tool for tackling strongly coupled quantum field theories, which are notoriously difficult to handle using conventional methods. During the course of my PhD I have mostly studied time dependent processes, in particular thermalization processes, in quantum field theories using the AdS/CFT correspondence. On the gravity side, this is dual to dynamical formation of black holes from the collapse of matter fields. By studying the gravitational collapse process in detail, we can then draw conclusions about the dynamical formation of a thermal state in the dual quantum field theory. Using mostly numerical methods, I have studied how confinement affects thermalization in quantum field theories, where the system may never thermalize and field theory observables undergo interesting quasiperiodic behaviour. I have also studied formation of black holes in three dimensions which due to the simplified nature of three-dimensional gravity can be done using analytical methods. This has led to the discovery of new solutions of three-dimensional gravity corresponding to the formation of black holes without spherical symmetry, which can provide a deeper understanding of thermalization in two-dimensional quantum field theories. In a third line of research, I have studied higher spin gravity in three dimensions, an exotic extension of three-dimensional gravity which includes fields with spin higher than two, and we outline a new method to construct black hole solutions carrying higher spin charge.