×

String theory formulation of the three-dimensional black hole. (English) Zbl 0972.83564

Summary: A black hole solution to three-dimensional general relativity with a negative cosmological constant has recently been found. We show that a slight modification of this solution yields an exact solution to string theory. This black hole is equivalent (under duality) to the previously discussed three-dimensional black string solution. Since the black string is asymptotically flat and the black hole is asymptotically anti-de Sitter, this suggests that strings are not affected by a negative cosmological constant in three dimensions.

MSC:

83C57 Black holes
83E30 String and superstring theories in gravitational theory

References:

[1] M. Banados, Phys. Rev. Lett. 69 pp 1849– (1992) · Zbl 0968.83514 · doi:10.1103/PhysRevLett.69.1849
[2] J. Balog, Nucl. Phys. B325 pp 225– (1989) · doi:10.1016/0550-3213(89)90380-5
[3] P. Petropoulos, Phys. Lett. B 236 pp 151– (1990) · doi:10.1016/0370-2693(90)90819-R
[4] I. Bars, Nucl. Phys. B348 pp 89– (1991) · doi:10.1016/0550-3213(91)90223-K
[5] S. Hwang, Nucl. Phys. B354 pp 100– (1991) · doi:10.1016/0550-3213(91)90177-Y
[6] L. Dixon, Nucl. Phys. B261 pp 678– (1985) · doi:10.1016/0550-3213(85)90593-0
[7] L. Dixon, Nucl. Phys. B274 pp 285– (1986) · doi:10.1016/0550-3213(86)90287-7
[8] E. Witten, Phys. Rev. D 44 pp 314– (1991) · Zbl 0900.53037 · doi:10.1103/PhysRevD.44.314
[9] J. Horne, Nucl. Phys. B368 pp 444– (1992) · Zbl 0942.83516 · doi:10.1016/0550-3213(92)90536-K
[10] S. Deser, Ann. Phys. (N.Y.) 152 pp 220– (1984) · doi:10.1016/0003-4916(84)90085-X
[11] S. Hawking, Proc. R. Soc. London A 314 pp 529– (1970) · Zbl 0954.83012 · doi:10.1098/rspa.1970.0021
[12] M. Roček, Nucl. Phys. B373 pp 630– (1992) · doi:10.1016/0550-3213(92)90269-H
[13] A. Giveon, Nucl. Phys. B380 pp 128– (1992) · doi:10.1016/0550-3213(92)90518-G
[14] T. Buscher, Phys. Lett. B 201 pp 466– (1988) · doi:10.1016/0370-2693(88)90602-8
[15] T. Buscher, Phys. Lett. B 194 pp 59– (1987) · doi:10.1016/0370-2693(87)90769-6
[16] J. Horne, Phys. Rev. Lett. 68 pp 568– (1992) · Zbl 0969.81620 · doi:10.1103/PhysRevLett.68.568
[17] D. Garfinkle, Phys. Rev. D 46 pp 4286– (1992) · doi:10.1103/PhysRevD.46.4286
[18] R. Dijkgraaf, Nucl. Phys. B371 pp 269– (1992) · doi:10.1016/0550-3213(92)90237-6
[19] I. Bars, Phys. Rev. D 46 pp 4510– (1992) · doi:10.1103/PhysRevD.46.4510
[20] M. Perry, Phys. Rev. Lett. 70 pp 2669– (1993) · Zbl 1051.83526 · doi:10.1103/PhysRevLett.70.2669
[21] G. Horowitz, Nucl. Phys. B360 pp 197– (1991) · doi:10.1016/0550-3213(91)90440-9
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.