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A menagerie of hairy black holes

Elizabeth Winstanley

Oct 6, 2015

8 pages

Part of 2nd Karl Schwarzschild Meeting on Gravitational Physics, 39-46

Published in:

Springer Proc.Phys. 208 (2018) 39-46

Contribution to:

- KSM 2015
, 39-46

Published: 2018

e-Print:

1510.01669 [gr-qc]

DOI:

10.1007/978-3-319-94256-8_3

View in:

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Abstract: (Springer)

According to the no-hair conjecture, equilibrium black holes are simple objects, completely determined by global charges which can be measured at infinity. This is the case in Einstein-Maxwell theory due to beautiful uniqueness theorems. However, the no-hair conjecture is not true in general, and there is now a plethora of matter models possessing hairy black hole solutions. In this note we focus on one such matter model: Einstein-Yang-Mills (EYM) theory, and restrict our attention to four-dimensional, static, non-rotating black holes for simplicity. We outline some of the menagerie of EYM solutions in both asymptotically flat and asymptotically anti-de Sitter space. We attempt to make sense of this black hole zoo in terms of Bizon’s modified no-hair conjecture.

Note:

8 pages, submitted to the Proceedings of the Second Karl Schwarzschild Meeting, Frankfurt, 20-24 July 2015

References(31)

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