Classical Yang-Mills black hole hair in anti-de Sitter space

Details Classical Yang-Mills black hole hair in anti-de Sitter space Classical Yang-Mills black hole hair in anti-de Sitter space

2008-01-03

arxiv.org/abs/0801.0527v1

Lect.Notes Phys.769:49-87,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

41 pages, 14 figures. Based on the lecture given at the 4th Aegean Summer School

Scientific paper

10.1007/978-3-540-88460-6_2

The properties of hairy black holes in Einstein-Yang-Mills (EYM) theory are reviewed, focusing on spherically symmetric solutions. In particular, in asymptotically anti-de Sitter space (adS) stable black hole hair is known to exist for su(2) EYM. We review recent work in which it is shown that stable hair also exists in su(N) EYM for arbitrary N, so that there is no upper limit on how much stable hair a black hole in adS can possess.

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