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Kerr/CFT correspondence and fivedimensional BMPV black holes, 0812.4440v1
 22 M. Cvetic and D. Youm, General Rotating Five Dimensional Black Holes of Toroidally Compactified Heterotic String, Nucl. Phys. B476
, 1996
"... We apply a recently proposed Kerr/CFT correspondence to extremal supersymmetric fivedimensional charged spinning black holes, constructed by Breckenridge, Myers, Peet and Vafa. By computing the central charge of the dual CFT and FrolovThorne temperature, Cardy’s formula succeeds in reproducing Bek ..."
Deviations from the Area Law for Supersymmetric Black Holes
, 1999
"... We review modifications of the BekensteinHawking area law for black hole entropy in the presence of higherderivative interactions. In fourdimensional N = 2 compactifications of string theory or Mtheory these modifications are crucial for finding agreement between the macroscopic entropy obtained ..."
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We review modifications of the BekensteinHawking area law for black hole entropy in the presence of higherderivative interactions. In fourdimensional N = 2 compactifications of string theory or Mtheory these modifications are crucial for finding agreement between the macroscopic entropy
Hawking Radiation due to Photon and Gravitino
, 901
"... Applying the Hamilton–Jacobi method we investigate the tunneling of photon and gravitino through an event horizon beyond semiclassical approximation. Quantum corrections of the single particle action for both cases are found to be proportional to the semiclassical contribution. We show the importanc ..."
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the importance of gauge condition for analysing photon tunneling. Modifications of the Hawking temperature and the Bekenstein–Hawking area law is obtained and the first order correction is shown to be related with the trace anomaly. 1
Entropy in the NUTKerrNewman Black Holes Due to an Arbitrary Spin Field
, 2008
"... Abstract: Membrane method is used to compute the entropy of the NUTKerrNewman black holes. It is found that even though the Euler characteristic is greater than two, the BekensteinHawking area law is still satisfied. The formula S = χA/8 relating the entropy and the Euler characteristic becomes i ..."
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Abstract: Membrane method is used to compute the entropy of the NUTKerrNewman black holes. It is found that even though the Euler characteristic is greater than two, the BekensteinHawking area law is still satisfied. The formula S = χA/8 relating the entropy and the Euler characteristic becomes
physics pp. 511–527 Quantum aspects of black hole entropy
, 2000
"... Abstract. This survey intends to cover recent approaches to black hole entropy which attempt to go beyond the standard semiclassical perspective. Quantum corrections to the semiclassical Bekenstein– Hawking area law for black hole entropy, obtained within the quantum geometry framework, are treated ..."
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Abstract. This survey intends to cover recent approaches to black hole entropy which attempt to go beyond the standard semiclassical perspective. Quantum corrections to the semiclassical Bekenstein– Hawking area law for black hole entropy, obtained within the quantum geometry framework, are treated
Quantum Tunneling Beyond Semiclassical Approximation
 JHEP
, 2008
"... Hawking radiation as tunneling by HamiltonJacobi method beyond semiclassical approximation is analysed. We compute all quantum corrections in the single particle action revealing that these are proportional to the usual semiclassical contribution. We show that a simple choice of the proportionality ..."
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Cited by 17 (1 self)
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of the proportionality constants reproduces the one loop back reaction effect in the spacetime, found by conformal field theory methods, which modifies the Hawking temperature of the black hole. Using the law of black hole mechanics we give the corrections to the BekensteinHawking area law following from the modified
Near horizon geometry and black holes in four dimensions
 Nucl. Phys. B528
, 1998
"... A large class of extremal and nearextremal four dimensional black holes in Mtheory feature near horizon geometries that contain three dimensional asymptotically antide Sitter spaces. Globally, these geometries are derived from AdS3 by discrete identifications. The microstates of such black holes ..."
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Cited by 33 (7 self)
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can be counted by exploiting the conformal symmetry induced on the antide Sitter boundary, and the result agrees with the BekensteinHawking area law. This approach, pioneered by Strominger, clarifies the physical nature of the black hole microstates. It also suggests that recent analyses
Thermodynamics of (2+1)dimensional Rotating de Sitter Space
, 2002
"... Brief comments on a plausible holographic relationship between the opposite rotational dragging effect of a (2+1)dimensional rotating de Sitter space and the nonunitarity of a boundary conformal field theory are given. In addition to the comments, we study how the opposite rotational dragging effe ..."
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and the entropy of dS space satisfies the BekensteinHawking area law given by
ADM reduction of Einstein action and black hole entropy,” arXiv:1304.0014 [hepth
"... We reduce the 4D EinsteinHilbert action to a constantradius hypersurface of foliation. The resulting theory is a scalar theory defined on a 3D hypersurface of the original black hole background, and has an exponential potential. Once the the hypersurface is located at the Schwarzschild radius, th ..."
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Cited by 6 (6 self)
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, the 3D theory is effectively reduced to a 2D Liouville type theory. We compute the entropy associated with the hypersurface intrinsic degrees of freedom, and show that its leading order reproduces the BekensteinHawking area law. The subleading terms come in logarithm/inverse powers of the area. ar X iv
Macroscopic Entropy Formulae and NonHolomorphic Corrections for Supersymmetric Black Holes
, 1999
"... In fourdimensional N = 2 compactifications of string theory or Mtheory, modifications of the BekensteinHawking area law for black hole entropy in the presence of higherderivative interactions are crucial for finding agreement between the macroscopic entropy obtained from supergravity and sublead ..."
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Cited by 99 (8 self)
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In fourdimensional N = 2 compactifications of string theory or Mtheory, modifications of the BekensteinHawking area law for black hole entropy in the presence of higherderivative interactions are crucial for finding agreement between the macroscopic entropy obtained from supergravity
Results 1  10
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