(Anti-)de Sitter black hole thermodynamics and the generalized uncertainty principle
By B. Bolen, Marco Cavaglià. 2004
171 citations recorded by the source corpus.
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.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/f17fc0bf9d30ff07365878ba0a51bfba19b79601
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
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Citations in the corpus
- Minimal Length Scale Scenarios for Quantum Gravity (2012, background): “Corrections to the thermodynamical properties of a Schwarzschild black hole have been looked at in [22, 321, 100, 214, 217], the Reissner–Nordström black hole has been considered in [319], and black holes in anti-de Sitter space in [280, 281, 61].”