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Formation of black hole and emission of gravitational waves

Numerical simulations were performed for the formation process of rotating black holes. It is suggested that Kerr black holes are formed for wide ranges of initial parameters. The nature of gravitational waves from a test particle falling into a Kerr black hole as well as the development of 3D numer...

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Detalles Bibliográficos
Autor principal: Nakamura, Takashi
Formato: Online Artículo Texto
Lenguaje:English
Publicado: The Japan Academy 2006
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4338837/
https://www.ncbi.nlm.nih.gov/pubmed/25792793