Radiating spherical collapse with heat flow
arXiv:gr-qc/0202091 · doi:10.1142/S0218271803003086
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.
13 pages, including 3 figures, submitted to IJMP-D