Dynamical formation of a hairy black hole in a cavity from the decay of unstable solitons

Recent numerical relativity simulations within the Einstein-Maxwell(charged-) Klein-Gordon (EMcKG) system have shown that the non-linear evolution of a superradiantly unstable Reissner-Nordstrm black hole (BH) enclosed in a cavity, leads to the formation of a BH with scalar hair. Perturbative eviden...

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Detalhes bibliográficos
Autor principal: Sanchis-Gual, N. (author)
Outros Autores: Degollado, J. C. (author), Font, J. A. (author), Herdeiro, C. (author), Radu, E. (author)
Formato: article
Idioma:eng
Publicado em: 1000
Assuntos:
Relativity and gravitation
Classical black holes
Numerical studies of black holes and black-hole binaries
Einstein–Maxwell spacetimes
Spacetimes with fluids
Radiation or classical fields
Texto completo:http://hdl.handle.net/10773/21136
País:Portugal
Oai:oai:ria.ua.pt:10773/21136

Texto Completo

http://hdl.handle.net/10773/21136

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