The DOI matches its Crossref record; 10 of the 10 references it cites were found in a registry or an index.
Black holes with unusual topology
Open accessAbstract
Einstein's equations with a negative cosmological constant admit solutions which are asymptotically anti--de Sitter space. Matter fields in anti--de Sitter space can be in stable equilibrium even if the potential energy is unbounded from below, violating the weak energy condition. Hence there is no fundamental reason that black hole horizons should have a spherical topology. In anti--de Sitter space Einstein's equations admit black hole solutions where the horizon can be a Riemann surface with genus $g.$ The case $g=0$ is the asymptotically anti--de Sitter black hole first studied by Hawking and Page, which has a spherical topology. The genus one black hole has a new free parameter entering the metric, the conformal class to which the torus belongs. The genus $g>1$ black hole has no other free parameters apart from the mass and the charge. All such black holes exhibit a natural temperature which is identified as the period of the Euclidean continuation and there is a mass formula connecting the mass with the surface gravity and the horizon area of the black hole. The Euclidean action and entropy are computed and used to argue that the mass spectrum of states is positive definite.
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Cites
The Large Scale Structure of Space-Time
Hawking, S. W., & Ellis, G. F. R. (1973) · doi:10.1017/cbo9780511524646 · Cited by 10,624
The four laws of black hole mechanics
Bardeen, J. M., Carter, B., & Hawking, S. W. (1973) · Communications in Mathematical Physics · doi:10.1007/bf01645742 · Cited by 3,932
Black hole in three-dimensional spacetime
Bañados, M., Teitelboim, C., & Zanelli, J. (1992) · Physical Review Letters · doi:10.1103/physrevlett.69.1849 · Cited by 3,831
Thermodynamics of black holes in anti-de Sitter space
Hawking, S. W., & Page, D. N. (1983) · Communications in Mathematical Physics · doi:10.1007/bf01208266 · Cited by 3,045
Quasilocal energy and conserved charges derived from the gravitational action
Brown, J. D., & York, J. W. (1993) · Physical Review D · doi:10.1103/physrevd.47.1407 · Cited by 1,793
Stability in gauged extended supergravity
Breitenlohner, P., & Freedman, D. Z. (1982) · Annals of Physics · doi:10.1016/0003-4916(82)90116-6 · Cited by 1,707
Black holes in general relativity
Hawking, S. W. (1972) · Communications in Mathematical Physics · doi:10.1007/bf01877517 · Cited by 1,561
Gravitational effects on and of vacuum decay
Coleman, S., & De Luccia, F. (1980) · Physical Review D · doi:10.1103/physrevd.21.3305 · Cited by 1,537
Black hole entropy in canonical quantum gravity and superstring theory
Susskind, L., & Uglum, J. (1994) · Physical Review D · doi:10.1103/physrevd.50.2700 · Cited by 754
The gravitational Hamiltonian, action, entropy and surface terms
Hawking, S. W., & Horowitz, G. T. (1996) · Classical and Quantum Gravity · doi:10.1088/0264-9381/13/6/017 · Cited by 704
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Quasinormal modes of black holes and black branes
Berti, E., Cardoso, V., & Starinets, A. O. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/16/163001 · Cited by 2,095
Towards a derivation of holographic entanglement entropy
Casini, H., Huerta, M., & Myers, R. C. (2011) · Journal of High Energy Physics · doi:10.1007/jhep05(2011)036 · Cited by 1,347
Charged AdS black holes and catastrophic holography
Chamblin, A., Emparan, R., Johnson, C. V., & Myers, R. C. (1999) · Physical Review D · doi:10.1103/physrevd.60.064018 · Cited by 1,016
Gauss-Bonnet black holes in AdS spaces
Cai, R.-G. (2002) · Physical Review D · doi:10.1103/physrevd.65.084014 · Cited by 948
Thermodynamics of Kerr-Newman-AdS black holes and conformal field theories
Caldarelli, M. M., Cognola, G., & Klemm, D. (2000) · Classical and Quantum Gravity · doi:10.1088/0264-9381/17/2/310 · Cited by 822
Metadata
- Authors
- Vanzo, L.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1997-11-15
- Volume
- 56
- Issue
- 10
- Pages
- 6475-6483
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2073416485
- Cited by
- 385
- References
- 10
- FWCI
- 13.58
- Type
- journal article
- Language
- en
- Open access
- green
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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