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• W3100293961 startingPage "1950034" @default.
• W3100293961 abstract "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." @default.
• W3100293961 created "2020-11-23" @default.
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• W3100293961 creator A5062776347 @default.
• W3100293961 date "2019-01-01" @default.
• W3100293961 modified "2023-10-18" @default.
• W3100293961 title "Gravitational collapse for a radiating anisotropic fluid" @default.
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• W3100293961 doi "https://doi.org/10.1142/s0218271819500342" @default.
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