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

Abstract

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 frak su(2) EYM. We review recent work in which it is shown that stable hair also exists in frak 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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Authors/Creators:	Winstanley, E. (E.Winstanley@sheffield.ac.uk)
Copyright, Publisher and Additional Information:	© 2009 Springer-Verlag Berlin Heidelberg. This is an author produced version of a paper published in 'Lecture Notes in Physics'. Uploaded in accordance with the publisher's self-archiving policy.
Dates:	Published: 2009
Institution:	The University of Sheffield
Academic Units:	The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Depositing User:	Mrs Megan Hobbs
Date Deposited:	01 Apr 2010 11:33
Last Modified:	17 Nov 2015 21:37
Published Version:	http://dx.doi.org/10.1007/978-3-540-88460-6_2
Status:	Published
Publisher:	Springer
Series Name:	Lecture Notes in Physics
Identification Number:	https://doi.org/10.1007/978-3-540-88460-6_2
Related URLs:	arXiv URL

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

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0801.0527v1

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