Radiating spherical collapse with heat flow

Details Radiating spherical collapse with heat flow Radiating spherical collapse with heat flow

2002-02-26

arxiv.org/abs/gr-qc/0202091v1

Int.J.Mod.Phys. D12 (2003) 667-676

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, including 3 figures, submitted to IJMP-D

Scientific paper

10.1142/S0218271803003086

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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