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Spherical Gravitational Collapse with Heat Flux and Cosmic Censorship

S. M. Wagh·R. V. Saraykar·P. S. Muktibodh·K. S. Govinder
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Abstract

In this paper, we investigate the nature of the singularity in the spherically symmetrical, shear-free, gravitational collapse of a star with heat flux using a separable metric [cqg1]. For any non-singular, regular, radial density profile for a star described by this metric, eq. (2.1), the singularity of the gravitational collapse is not naked locally. Our results here unequivocally support the Strong Cosmic Censorship Hypothesis.

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S. M. Wagh, R. V. Saraykar, P. S. Muktibodh, K. S. Govinder. 2001-12-16. Spherical Gravitational Collapse with Heat Flux and Cosmic Censorship. https://arxiv.org/abs/gr-qc/0112034

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