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Born-Infeld black holes in (A)dS spaces

Rong-Gen CaiCASPER, Department of Physics, Baylor University, Waco, TX76798-7316, USADa-Wei PangInstitute of Theoretical Physics, Chinese Academy of Sciences, P.O. Box 2735, Beijing 100080, China and Graduate School of the Chinese Academy of Sciences, Beijing, 100039, ChinaAnzhong WangCASPER, Department of Physics, Baylor University, Waco, TX76798-7316, USA
2004en
ABI

Аннотация

We study some exact solutions in a $D(\ensuremath{\ge}4)$-dimensional Einstein-Born-Infeld theory with a cosmological constant. These solutions are asymptotically de Sitter or anti-de Sitter, depending on the sign of the cosmological constant. Black hole horizon and cosmological horizon in these spacetimes can be a positive, zero or negative constant curvature hypersurface. We discuss the thermodynamics associated with black hole horizon and cosmological horizon. In particular we find that for the Born-Infeld black holes with Ricci flat or hyperbolic horizon in AdS space, they are always thermodynamically stable, and that for the case with a positive constant curvature, there is a critical value for the Born-Infeld parameter, above which the black hole is also always thermodynamically stable, and below which a unstable black hole phase appears. In addition, we show that although the Born-Infeld electrodynamics is nonlinear, both black hole horizon entropy and cosmological horizon entropy can be expressed in terms of the Cardy-Verlinde formula. We also find a factorized solution in the Einstein-Born-Infeld theory, which is a direct product of two constant curvature spaces: one is a two-dimensional de Sitter or anti-de Sitter space, the other is a ($D\ensuremath{-}2$)-dimensional positive, zero or negative constant curvature space.

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