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2013

Phase Transition to a Hairy Black Hole in Asymptotically Flat Spacetime

Kolyvaris, Theodoros, Koutsoumbas, George, Papantonopoulos, Eleftherios et al.

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We discuss a phase transition of a Reissner-Nordstr\"om black hole to a hairy black hole in asymptotically flat spacetime.

The hair is due to a massive charged scalar field.
The no-hair theorem is evaded thanks to a derivative coupling of the scalar field to the Einstein tensor.
The resulting hairy configuration is spherically symmetric.

Phase Transition to a Hairy Black Hole in Asymptotically Flat Spacetime · Around

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