The DOI matches its Crossref record; 37 of the 37 references it cites were found in a registry or an index.
Rotating attractors
Open accessAbstract
We prove that, in a general higher derivative theory of gravity coupled to abelian gauge fields and neutral scalar fields, the entropy and the near horizon background of a rotating extremal black hole is obtained by extremizing an entropy function which depends only on the parameters labeling the near horizon background and the electric and magnetic charges and angular momentum carried by the black hole. If the entropy function has a unique extremum then this extremum must be independent of the asymptotic values of the moduli scalar fields and the solution exhibits attractor behaviour. If the entropy function has flat directions then the near horizon background is not uniquely determined by the extremization equations and could depend on the asymptotic data on the moduli fields, but the value of the entropy is still independent of this asymptotic data. We illustrate these results in the context of two derivative theories of gravity in several examples. These include Kerr black hole, Kerr-Newman black hole, black holes in Kaluza-Klein theory, and black holes in toroidally compactified heterotic string theory.
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Cites
Black hole entropy is the Noether charge
Wald, R. M. (1993) · Physical Review D · doi:10.1103/physrevd.48.r3427 · Cited by 2,496
Some properties of the Noether charge and a proposal for dynamical black hole entropy
Iyer, V., & Wald, R. M. (1994) · Physical Review D · doi:10.1103/physrevd.50.846 · Cited by 1,736
Ferrara, S., Kallosh, R., & Strominger, A. (1995) · Physical Review D · doi:10.1103/physrevd.52.r5412 · Cited by 925
Ferrara, S., & Kallosh, R. (1996) · Physical Review D · doi:10.1103/physrevd.54.1514 · Cited by 722
Black hole entropy in M-Theory
MALDACENA, J. M., Strominger, A., & Witten, E. H. (1997) · Journal of High Energy Physics · doi:10.1088/1126-6708/1997/12/002 · Cited by 677
D-branes and spinning black holes
Breckenridge, J. C., Myers, R. C., Peet, A. W., & Vafa, C. (1997) · Physics Letters B · doi:10.1016/s0370-2693(96)01460-8 · Cited by 622
Macroscopic entropy of N = 2 extremal black holes
Strominger, A. (1996) · Physics Letters B · doi:10.1016/0370-2693(96)00711-3 · Cited by 549
Jacobson, T., Kang, G., & Myers, R. C. (1994) · Physical Review D · doi:10.1103/physrevd.49.6587 · Cited by 544
Black hole entropy function and the attractor mechanism in higher derivative gravity
Sen, A. (2005) · Journal of High Energy Physics · doi:10.1088/1126-6708/2005/09/038 · Cited by 515
Self-citationExtreme Kerr throat geometry: A vacuum analog ofAdS2×S2
Bardeen, J., & Horowitz, G. T. (1999) · Physical Review D · doi:10.1103/physrevd.60.104030 · Cited by 495
Cited by
New boundary conditions for AdS2
Godet, V., & Marteau, C. (2020) · Journal of High Energy Physics · doi:10.1007/jhep12(2020)020 · Cited by 61
Metadata
- Authors
- Astefanesei, D., Goldstein, K., Jena, R. P., Sen, A., & Trivedi, S. P.
- Venue
- Journal of High Energy Physics
- Published
- 2006-10-20
- Volume
- 2006
- Issue
- 10
- Pages
- 058-058
- ISSN
- 1029-8479 (ISSN-L)
- OpenAlex
- W3037079031
- Cited by
- 259
- References
- 37
- FWCI
- 19.75
- Type
- journal article
- Language
- en
- Open access
- bronze
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