The DOI matches its Crossref record; 56 of the 56 references it cites were found in a registry or an index.
Microscopic black hole entropy in theories with higher derivatives
Open accessAbstract
We discuss higher derivative corrections to black hole entropy in theories that allow a near horizon AdS3 × X geometry. In arbitrary theories with diffeomorphism in- variance we show how to obtain the spacetime central charge in a simple way. Black hole entropy then follows from the euclidean partition function, and we show that this gives agreement with Wald's formula. In string theory there are certain diffeomorphism anoma- lies that we exploit. We thereby reproduce some recent computations of corrected entropy formulas, and extend them to the nonextremal, nonsupersymmetric context. Examples include black holes in M-theory on K3 × T 2 , whose entropy reproduces that of the per- turbative heterotic string with both right and left movers excited and angular momentum included. Our anomaly based approach also sheds light on why exact results have been obtained in four dimensions while ignoring R 4 type corrections.
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Cites
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Some properties of the Noether charge and a proposal for dynamical black hole entropy
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A Stress Tensor for Anti-de Sitter Gravity
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Self-citationHenningson, M., & Skenderis, K. (1998) · Journal of High Energy Physics · doi:10.1088/1126-6708/1998/07/023 · Cited by 1,373
Black hole entropy from near-horizon microstates
Strominger, A. (1998) · Journal of High Energy Physics · doi:10.1088/1126-6708/1998/02/009 · Cited by 1,135
The fuzzball proposal for black holes: an elementary review
Mathur, S. D. (2005) · Fortschritte der Physik · doi:10.1002/prop.200410203 · Cited by 937
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AdS3 black holes and a stringy exclusion principle
Maldacena, J., & Strominger, A. (1998) · Journal of High Energy Physics · doi:10.1088/1126-6708/1998/12/005 · Cited by 822 · cited 1×
“llows directly from the central charges. Hence, so too does the black hole entropy. 3 Other choices lead to the so-called “SL(2,Z)” family of black holes. 6 Let us illustrate this in more detail; see [12]. An asymptotically AdS3 solution carries an energy H and angular momentum J. In the CFT on the boundary J is the m…”
Background
Cited by
de Rham, C. (2014) · Living Reviews in Relativity · doi:10.12942/lrr-2014-7 · Cited by 1,120
Chiral gravity in three dimensions
Li, W., Song, W., & Strominger, A. (2008) · Journal of High Energy Physics · doi:10.1088/1126-6708/2008/04/082 · Cited by 451
Holographic gravitational anomalies
Kraus, P., & Larsen, F. (2006) · Journal of High Energy Physics · doi:10.1088/1126-6708/2006/01/022 · Cited by 261
Self-citationAstefanesei, D., Goldstein, K., Jena, R. P., Sen, A., & Trivedi, S. P. (2006) · Journal of High Energy Physics · doi:10.1088/1126-6708/2006/10/058 · Cited by 259
Sailing from warped AdS3 to warped dS3 in topologically massive gravity
Anninos, D. (2010) · Journal of High Energy Physics · doi:10.1007/jhep02(2010)046 · Cited by 36
Metadata
- Authors
- Kraus, P., & Larsen, F.
- Venue
- Journal of High Energy Physics
- Published
- 2005-09-13
- Volume
- 2005
- Issue
- 09
- Pages
- 034-034
- ISSN
- 1029-8479 (ISSN-L)
- OpenAlex
- W2124265343
- Cited by
- 264
- References
- 56
- FWCI
- 19.06
- Type
- journal article
- Language
- en
- Open access
- bronze
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