Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/1517
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Unnikrishnan, C. S | - |
dc.date.accessioned | 2007-05-07T05:26:59Z | - |
dc.date.available | 2007-05-07T05:26:59Z | - |
dc.date.issued | 1993 | - |
dc.identifier.citation | BASI, Vol. 21, pp. 413-416 | en |
dc.identifier.uri | http://hdl.handle.net/2248/1517 | - |
dc.description.abstract | We explore the physical nature of the singularity which forms in the gravitational collapse of spherically symmetric pressureless dust with inhomogeneous density distribution (Tolman-Bondi model). We show that in this model the singularity is weak when naked, and it is hidden by an event horizon when strong. Based on these results we arrive at a correct physical interpretation of the strong naked singularities demonstrated in similar collapse scenarios by many authors. We argue that in fact these naked singularities are unphysical and therefore pose no threat to the Cosmic Censorship Conjecture | en |
dc.format.extent | 316310 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.subject | Gravitational collapse | en |
dc.subject | Cosmic censorship | en |
dc.title | On naked singularities in spherically symmetric gravitational collapse | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Paper_8.pdf | 308.9 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.