Black holes and thermodynamics

By R. Adamson. 2003

582 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/281d3e543bbc785b7f1abce01ae6e86857135d23

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Citations in the corpus

The Holographic principle (2002, background): “It is all the more impressive that the GSL holds also in this case (Bekenstein, 1975; Hawking, 1976a).”
A new approach to static numerical relativity and its application to Kaluza–Klein black holes (2009, methodology): “In section 3, we then consider two types of algorithms for solving this elliptic system.”
Microscopic formulation of black holes in string theory (2002, background): “For the special case of the Reissner-Nördstrom black hole the first law reduces to dM = T H d A 4G N ¯ h + ΦdQ.”
Gravitational Condensate Stars: An Alternative to Black Holes (2001, unknown): “The application of thermodynamic arguments to BHs is itself put into doubt by the the inverse dependence of T H on M implying that a BH in thermal equilibrium with its own Hawking radiation has negative speciﬁc heat and, therefore, is unstable to thermodynamic ﬂuctuations [7].”
Gravity and the Thermodynamics of Horizons (2003, background): “A statistical mechanics derivation of entropy was originally attempted in [87]; the entropy has been interpreted as the logarithm of: (a) the number of ways in which black hole might have been formed [7,88]; (b) the number of internal black hole states consistent with a single black hole exterior[7,”
Holographic heat engines (2014, background): “Recently, the classic subject of black hole thermodynamics [1–4], which relates the mass M , surface gravity κ, and area A of a black hole to the energy U , temperature T , and entropy S, according to:”