Abstract
We present a new family of asymptotically AdS four-dimensional black hole solutions with scalar hair of a gravitating system consisting of a scalar field minimally coupled to gravity with a self-interacting potential. For a certain profile of the scalar field we solve the Einstein equations and we determine the scalar potential. Thermodynamically we show that there is a critical temperature below which there is a phase transition of a black hole with hyperbolic horizon to the new hairy black hole configuration.
Original language | English |
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Article number | 21 |
Journal | Journal of High Energy Physics |
Volume | 2013 |
Issue number | 12 |
DOIs | |
State | Published - Dec 2013 |
Keywords
- Black holes
- Classical theories of gravity
- Spacetime singularities