Black Hole Thermodynamics in Semi-Classical and Superstring Theory
Sascha Vongehr

TL;DR
This paper reviews the development of black hole thermodynamics within semi-classical and superstring theory frameworks, focusing on entropy, Hawking radiation, and the information paradox, highlighting recent theoretical advances.
Contribution
It provides a comprehensive overview of how superstring theory addresses black hole entropy and related thermodynamic issues, integrating pre-string physics insights.
Findings
Superstring theory offers promising explanations for black hole entropy.
Recent models improve understanding of Hawking radiation.
Progress in resolving the black hole information paradox.
Abstract
This is a revised and shortened version of a MSc thesis submitted to the University of Sussex, UK. An introduction into the pre-string physics of black holes and related thermodynamics is given. Then, starting with an introduction of how superstring theory is approaching the problem of black hole entropy, work on that and closely related topics like Hawking radiation and the information paradox is reviewed.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
