Hairy Black Holes, Horizon Mass and Solitons

Details Hairy Black Holes, Horizon Mass and Solitons Hairy Black Holes, Horizon Mass and Solitons

2000-11-22

arxiv.org/abs/gr-qc/0011081v3

Class.Quant.Grav. 18 (2001) 919-940

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

25 pages, 5 (new) figures. Revtex file. Final version to appear in CQG

Scientific paper

10.1088/0264-9381/18/5/310

Properties of the horizon mass of hairy black holes are discussed with emphasis on certain subtle and initially unexpected features. A key property suggests that hairy black holes may be regarded as `bound states' of ordinary black holes without hair and colored solitons. This model is then used to predict the qualitative behavior of the horizon properties of hairy black holes, to provide a physical `explanation' of their instability and to put qualitative constraints on the end point configurations that result from this instability. The available numerical calculations support these predictions. Furthermore, the physical arguments are robust and should be applicable also in more complicated situations where detailed numerical work is yet to be carried out.

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