Naked singularities and admissibility of initial conditions

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dc.creatorAntia, H. M.
dc.date1997-01-11
dc.date.accessioned2026-07-07T03:31:25Z
dc.date.available2026-07-07T03:31:25Z
dc.descriptionGravitational collapse of a spherically symmetric cloud has been extensively studied to investigate the nature of resulting singularity. However, there has been considerable debate about the admissibility of certain initial density distributions. Using the Newtonian limit of the equations governing collapse of a fluid with an equation of state $p=p(ρ)$ it is shown that the density distribution has to be even function of r in a spherically symmetric situation provided $dp/dρ\ne0$. Implications of this result on formation of strong naked singularities are examined.
dc.description3 pages, TeX
dc.identifierhttps://arxiv.org/abs/gr-qc/9701023
dc.identifierhttp://arxiv.org/abs/gr-qc/9701023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35857
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNaked singularities and admissibility of initial conditions
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