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Gravitational collapse for a radiating anisotropic fluid

Veneroni, L. S. M ; da Silva, M. F. A

International journal of modern physics. D, Gravitation, astrophysics, cosmology, 2019-01, Vol.28 (2), p.1950034 [Periódico revisado por pares]

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Título:
Gravitational collapse for a radiating anisotropic fluid
Autor: Veneroni, L. S. M ; da Silva, M. F. A
Assuntos: Anisotropic fluids ; Anisotropy ; Black holes ; Event horizon ; Gravitational collapse ; Heat flux ; Luminosity ; Stellar evolution
É parte de: International journal of modern physics. D, Gravitation, astrophysics, cosmology, 2019-01, Vol.28 (2), p.1950034
Descrição: Interested in the collapse of a radiating star, we study the temporal evolution of a fluid with heat flux and bulk viscosity, including anisotropic pressure. As a starting point, we adopt an initial configuration that satisfies the regularities conditions as well as the energy conditions to a certain range of the mass–radius ratio for the star, defining acceptable models. For this set of models, we verify that the energy conditions remain satisfied until the black hole formation. Astrophysically relevant quantities, such as the luminosity perceived by an observer at infinity, the time of event horizon formation and the loss of mass during the collapse, are presented.
Editor: Singapore: World Scientific Publishing Company
Idioma: Inglês

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