Spherical Gravitational Collapse with Heat Flux and Cosmic Censorship

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dc.creatorWagh, S. M.
dc.creatorSaraykar, R. V.
dc.creatorMuktibodh, P. S.
dc.creatorGovinder, K. S.
dc.date2001-12-16
dc.date.accessioned2026-07-07T03:26:31Z
dc.date.available2026-07-07T03:26:31Z
dc.descriptionIn 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.
dc.descriptionSubmitted to General Relativity and Gravitation
dc.identifierhttps://arxiv.org/abs/gr-qc/0112034
dc.identifierhttp://arxiv.org/abs/gr-qc/0112034
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34074
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSpherical Gravitational Collapse with Heat Flux and Cosmic Censorship
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