Black p-Branes versus Black Holes in Non-asymptotically flat Einstein-Yang-Mills theory

Details Black p-Branes versus Black Holes in Non-asymptotically flat Einstein-Yang-Mills theory Black p-Branes versus Black Holes in Non-asymptotically flat Einstein-Yang-Mills theory

2010-12-02

arxiv.org/abs/1012.0389v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, 1 figure

Scientific paper

WWe present a class of non-asymptotically flat (NAF) charged black p-branes (BpB) with p-compact dimensions in higher dimensional Einstein-Yang-Mills (EYM) theory. Asymptotically the NAF structure manifests itself as an anti-de-sitter(AdS) spacetime. By comparing the entropies of BpB with those of black holes (BH) in same dimensions we derive transition criteria between the two types of black objects. An event horizon $(r_{+}) $ versus charge square $(Q^{2}) $ plot reveals such a transition provided both are characterized by the same $r_{+}$ and $Q$.

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