Gravitational collapse in spatially isotropic coordinates
General Relativity and Quantum Cosmology
2017-11-20 v1
Abstract
We investigate the dynamical nature of the collapse process of a spherically symmetric star in quasi-static hydrodynamical equilibrium. The star collapses from an initial static configuration by dissipating energy in the form of a radial heat flux. The dissipation ensures that the singularity is never formed and the stellar mass completely evaporates over a finite time.
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Cite
@article{arxiv.1312.2906,
title = {Gravitational collapse in spatially isotropic coordinates},
author = {Megan Govender and Robert Bogadi and Ranjan Sharma and Shyam Das},
journal= {arXiv preprint arXiv:1312.2906},
year = {2017}
}
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Submitted for publication