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The black hole information problem and JT gravity / NEIL TALWAR

Swansea University Author: NEIL TALWAR

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DOI (Published version): 10.23889/SUThesis.69255

Abstract

General relativity tells us that, quite generically, compact objects, such as heavy stars, can and will undergo gravitational collapse to form black holes [1]. Black holes are characterised by an event horizon, a surface which divides spacetime into two parts: the exterior of the black hole and the...

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Published: Swansea University, Wales, UK 2024
Institution: Swansea University
Degree level: Doctoral
Degree name: Ph.D
Supervisor: Hollowood, T
URI: https://cronfa.swan.ac.uk/Record/cronfa69255
Abstract: General relativity tells us that, quite generically, compact objects, such as heavy stars, can and will undergo gravitational collapse to form black holes [1]. Black holes are characterised by an event horizon, a surface which divides spacetime into two parts: the exterior of the black hole and the interior of the black hole, a region from which nothing, not even light, can escape. As a consequence, for an observer in the exterior region, there is apparently no way to get a signal from and learn anything about the interior.
Keywords: Black holes, holography, quantum information, JT gravity
College: Faculty of Science and Engineering
Funders: STFC