Astrophysical imaging of Kerr black holes with scalar hair

We address the astrophysical imaging of a family of deformed Kerr black holes (BHs). These are stationary, asymptotically flat BH spacetimes that are solutions of general relativity minimally coupled to a massive, complex scalar field: Kerr BHs with scalar hair (KBHsSH). Such BHs bifurcate from the...

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Detalhes bibliográficos
Autor principal: Vincent, F. H. (author)
Outros Autores: Gourgoulhon, E. (author), Herdeiro, C. (author), Radu, E. (author)
Formato: article
Idioma:eng
Publicado em: 2017
Texto completo:http://hdl.handle.net/10773/16930
País:Portugal
Oai:oai:ria.ua.pt:10773/16930