Collapse of a radiating anisotropic star

Details Collapse of a radiating anisotropic star Collapse of a radiating anisotropic star

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.206..219c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 206, no. 2, p. 219-234

Astronomy and Astrophysics

Astronomy

7

Anisotropic Fluids, Heat Flux, Stellar Evolution, Stellar Models, Stellar Physics, Stellar Radiation, Adiabatic Conditions, Black Holes (Astronomy), Stellar Luminosity, Stellar Mass

Scientific paper

Futher results are obtained concerning the model of a collapsing anisotropic body by Kolassis and Santos (1989). It is assumed an anisotropic equation of state for the static configuration, and a relation between the radiation density and heat flux. The total luminosity received by an observer at infinity is independent of the anisotropy of the fluid and of the radiation produced in the body. Numerical calculations are preformed for a body having a mass of 5 Solar Mass in order to obtain the effective adiabatic index.

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