Central charges in extreme black hole/CFT correspondence
By G. Compère, Keiju Murata, T. Nishioka. 2009
142 citations recorded by the source corpus.
The Kerr/CFT correspondence has been recently broadened to the general extremal black holes under the assumption that the central charges from the non-gravitational fields vanish. To confirm this proposal, we derive the expression of the conserved charges in the Einstein-Maxwell-scalar theory with topological terms in four and five dimensions and check that the above assumption was correct. Combining the computed central charge with the expected form of the temperature, the Bekenstein-Hawking entropy of the general extremal black holes in four and five dimensions can be reproduced by using the Cardy formula.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/e7110c132e2a3e495d1e837c19721d8f8f30e61f
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Citations in the corpus
- Black hole superradiance from Kerr/CFT (2009, background): “The analysis was subsequently generalized to a large variety of extreme black holes with perfect agreement in every case [3–20].”
- New boundary conditions for AdS3 (2013, methodology): “The asymptotic charges and asymptotic symmetry algebra can be obtained using the formalism of [36, 37, 40, 41].”
- Advanced Lectures on General Relativity (2018, background): “Section 3 of [14] and Appendix A of [15].”
- Holographic entanglement entropy: an overview (2009, background): “Also the the appearance of the AdS2 spacetime plays an important role in the recent investigations of the attractor mechanism (see [156] and references therein), and more recently, in a new duality called the extremal black hole/CFT correspondence [157, 158].”