Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 316, Issue 3, Pages 588-604Publisher
BLACKWELL SCIENCE LTD
DOI: 10.1046/j.1365-8711.2000.03547.x
Keywords
gravitation; relativity; supernovae : general
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A model is proposed of a collapsing radiating star consisting of an isotropic fluid with shear viscosity undergoing radial heat flow with outgoing radiation, The pressure of the star, at the beginning of the collapse, is isotropic but owing to the presence of the shear viscosity the pressure becomes more and more anisotropic. The behaviour of the density, pressure, mass, luminosity and the effective adiabatic index is analysed, Our work is compared to the case of a collapsing shearing fluid of a previous model, for a star with 6 M..
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