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Radiating spherical collapse with heat flow

M. Govender
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Abstract

We present here a simple model of radiative gravitational collapse with radial heat flux which describes qualitatively the stages close to the formation of a superdense cold star. Starting with a static general solution for a cold star, the model can generate solutions for the earlier evolutionary stages. The temporal evolution of the model is specified by solving the junction conditions appropriate for radiating gravitational collapse.

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M. Govender. 2002-02-26. Radiating spherical collapse with heat flow. https://doi.org/10.1142/s0218271803003086

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