Dynamical Formation of Kerr Black Holes with Synchronized Hair: An Analytic Model
East and Pretorius have successfully evolved, using fully nonlinear numerical simulations, the superradiant instability of the Kerr black hole (BH) triggered by a massive, complex vector field. Evolutions terminate in stationary states of a vector field condensate synchronized with a rotating BH hor...
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| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2018
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| Texto completo: | http://hdl.handle.net/10773/21359 |
| País: | Portugal |
| Oai: | oai:ria.ua.pt:10773/21359 |