Constant curvature black holes

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 57, Issue 2, 1998, Pages 1068-1072

  Bañados, Máximo ^a  

^a CENTRO DE ESTUDIOS CIENTÍFICOS CECS   (Chile)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0039886647     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.1068     Document Type: Article

References (18)

1. M. Bañados, C. Teitelboim, and J. Zanelli, “New Black Hole Topology and Signature in Higher Dimensions,” 1993 (unpublished).
2. This problem has also been analyzed in S. Aminneborg, I. Bengtsson, S. Holst, and P. Peldan, Class. Quantum Grav. 13, 2707 (1996). The global properties of our solutions are different to the ones reported in that paper. To see that, it is enough to look at the Penrose diagrams exhibit in that reference which clearly differ from our three-dimensional diagrams.
3. See also, in this context, R. B. Mann, gr-qc/9705007.
4. W. L. Smith and R. B. Mann, Phys. Rev. D 56, 4942 (1997).
5. For a systematic study of all possible identifications in four dimensions see, S. Holst and P. Peldan, gr-qc/9705067.
6. The thermodynamics of the solutions found in 2 has been studied in D. Brill, J. Louko, and P. Peldan, Phys. Rev. D 56, 3600 (1994).
7. L. Vanzo, Phys. Rev. D 56, 6475 (1997).
8. M. Bañados, M. Henneaux, C. Teitelboim, and J. Zanelli, Phys. Rev. D 48, 1506 (1993).
9. We thank M. Henneaux for pointing this out to us.
10. A. H. Chamseddine, Nucl. Phys. B346, 213 (1990).
11. A. Achúcarro and P. K. Townsend, Phys. Lett. B 180, 89 (1986).
12. M. Bañados, L. J. Garay, and M. Henneaux, Nucl. Phys. B476, 611 (1996).
13. M. BañadosL. J. GarayM. HenneauxPhys. Rev. D 53, R593 (1996).
14. E. Witten, Nucl. Phys. B311, 46 (1988).
15. We thank C. Teitelboim for discussions on this point.
16. S. Carlip, J. Gegenberg, and R. B. Mann, Phys. Rev. D 51, 6854 (1995).
17. R. M. Wald, Phys. Rev. D 48, 3427 (1993).
18. T. Jacobson and R. C. Myers, Phys. Rev. Lett. 70, 3684 (1993).