(Anti-)de Sitter Black Hole Thermodynamics and the Generalized Uncertainty Principle

Gen.Rel.Grav. 37 (2005) 1255-1262 We extend the derivation of the Hawking temperature of a Schwarzschild black hole via the Heisenberg uncertainty principle to the de Sitter and anti-de Sitter spacetimes. The thermodynamics of the Schwarzschild-(anti-)de Sitter black holes is obtained from the gener...

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Bibliographic Details
Main Authors Bolen, Brett, Cavaglia, Marco
Format Journal Article
LanguageEnglish
Published 17.11.2004
Subjects
Physics - General Relativity and Quantum Cosmology
Physics - High Energy Physics - Theory
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Summary:Gen.Rel.Grav. 37 (2005) 1255-1262 We extend the derivation of the Hawking temperature of a Schwarzschild black hole via the Heisenberg uncertainty principle to the de Sitter and anti-de Sitter spacetimes. The thermodynamics of the Schwarzschild-(anti-)de Sitter black holes is obtained from the generalized uncertainty principle of string theory and non-commutative geometry. This may explain why the thermodynamics of (anti-)de Sitter-like black holes admits a holographic description in terms of a dual quantum conformal field theory, whereas the thermodynamics of Schwarzschild-like black holes does not.
DOI:10.48550/arxiv.gr-qc/0411086