BTZ black holes from the five-dimensional general relativity with a negative cosmological constant

Details BTZ black holes from the five-dimensional general relativity with a negative cosmological constant BTZ black holes from the five-dimensional general relativity with a negative cosmological constant

1998-10-25

arxiv.org/abs/hep-th/9810205v2

Phys.Lett. B450 (1999) 41-47

Physics

High Energy Physics

High Energy Physics - Theory

14 pages, RevTeX, version to appear in Phys. Lett. B, arguments clarified

Scientific paper

10.1016/S0370-2693(99)00120-3

We show that the five-dimensional general relativity with a negative cosmological constant allows the solutions of the form M_3 \times M_g where M_3 is the three-dimensional BTZ black hole and M_g is a higher genus (g>1) Riemann surface with a fixed size. It is shown that this type of spontaneous compactification on a Riemann surface is possible only for the genus larger than one. From type IIB string theory point of view, certain near horizon geometry of D three-branes wrapped on the compact Riemann surface (g>1) is the BTZ (or AdS_3) space-time tensored with the Riemann surface and a constant size five-sphere. The relevance of our analysis to the positive energy conjecture of Horowitz and Myers is discussed.

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