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arXiv · 1312.2906

Gravitational collapse in spatially isotropic coordinates

Megan Govender·Robert Bogadi·Ranjan Sharma·Shyam Das
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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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Megan Govender, Robert Bogadi, Ranjan Sharma, Shyam Das. 2013-12-09. Gravitational collapse in spatially isotropic coordinates. https://arxiv.org/abs/1312.2906

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