No-hair theorems for black holes in the Abelian Higgs model
arXiv:0906.2353 · doi:10.1088/1126-6708/2009/11/054
Abstract
Motivated by the study of holographic superconductors, we generalize no-hair theorems for minimally coupled scalar fields charged under an Abelian gauge field, in arbitrary dimensions and with arbitrary horizon topology. We first present a straightforward generalization of no-hair theorems for neutral scalar hair. We then consider the existence of extremal black holes with scalar hair, and in the case of horizons with zero or positive curvature, provide a bound on the mass and charge of the scalar field that are necessary for the scalar hair to develop.
12 pages. v2: expanded abstract, added references
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Cited by in corpus (12)
- Hairy black holes and solitons in global AdS 5
- Small Hairy Black Holes in
- A scalar field condensation instability of rotating anti-de Sitter black holes
- Phase Transition to a Hairy Black Hole in Asymptotically Flat Spacetime
- Ultraspinning instability: the missing link
- Rotating Hairy Black Holes in AdSS
- Inhomogeneous charged black hole solutions in asymptotically anti-de Sitter spacetime
- Extremal Hairy Black Holes
- Hairy charged Gauss-Bonnet solitons and black holes
- The Rich Structure of Gauss-Bonnet Holographic Superconductors
- A scalar field instability of rotating and charged black holes in (4+1)-dimensional Anti-de Sitter space-time
- Formation of scalar hair on Gauss-Bonnet solitons and black holes