Black Hole Thermodynamics and Statistical Mechanics

dc.creatorCarlip, Steven
dc.date2008-07-28
dc.date.accessioned2026-07-07T12:34:43Z
dc.date.available2026-07-07T12:34:43Z
dc.descriptionWe have known for more than thirty years that black holes behave as thermodynamic systems, radiating as black bodies with characteristic temperatures and entropies. This behavior is not only interesting in its own right; it could also, through a statistical mechanical description, cast light on some of the deep problems of quantizing gravity. In these lectures, I review what we currently know about black hole thermodynamics and statistical mechanics, suggest a rather speculative "universal" characterization of the underlying states, and describe some key open questions.
dc.description35 pages, Springer macros; for the Proceedings of the 4th Aegean Summer School on Black Holes
dc.identifierhttps://arxiv.org/abs/0807.4520
dc.identifierhttp://arxiv.org/abs/0807.4520
dc.identifierLect.Notes Phys.769:89-123,2009
dc.identifierdoi:10.1007/978-3-540-88460-6_3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217533
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Hole Thermodynamics and Statistical Mechanics
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