Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2011-12-29
Physics
High Energy Physics
High Energy Physics - Theory
16 pages including 8 figures, v2: discussion on soliton solutions extended; v3: matches version accepted for publication in JH
Scientific paper
We study the stability of static as well as of rotating and charged black holes in (4+1)-dimensional Anti-de Sitter space-time which possess spherical horizon topology. We observe a non-linear instability related to the condensation of a charged, tachyonic scalar field and construct "hairy" black hole solutions of the full system of coupled Einstein, Maxwell and scalar field equations. We observe that the limiting solution for small horizon radius is either a hairy soliton solution or a singular solution that is not a regular extremal solution. Within the context of the gauge/gravity duality the condensation of the scalar field describes a holographic conductor/superconductor phase transition on the surface of a sphere.
Brihaye Yves
Hartmann Betti
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