Gravitational collapse in spatially isotropic coordinates
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gr-qc
keywords
collapsestarcollapsescompletelyconfigurationcoordinatesdissipatingdissipation
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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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