2013/09/30 by P. A. Gonzalez, Eleftherios Papantonopoulos, Joel Saavedra +1 · 2 citations
Physics and Astronomy · #gr-qc #hep-th
paper · pdf · doi:10.1007/jhep12(2013)021
Version accepted for publication in JHEP
arxiv created 2013/11/26 · arxiv updated 2015/06/17
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.