Neutrinos in gravitational collapse: analysis of the flux profile.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1076

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DC Field	Value	Language
dc.contributor.author	Dhurandhar, S.V.	-
dc.contributor.author	Vishveshwara, C.V.	-
dc.date.accessioned	2006-01-04T05:39:53Z	-
dc.date.available	2006-01-04T05:39:53Z	-
dc.date.issued	1984-04	-
dc.identifier.citation	Pramana, 1984, Vol. 22, p159-171.	en
dc.identifier.issn	0304-4289	-
dc.identifier.uri	http://hdl.handle.net/2289/1076	-
dc.description.abstract	The flux profile of the neutrinos emitted from a collapsing spherical object, as seen by a remote observer is studied. The model of the collapsing star consists of the Friedmann dust interior matched onto the Schwmhild exterior. It is assumed that the neutrino emission occurs from an interior shell in a very short time interval. It is found that the nature of the flux profile falls onto four distinct categories depending on the progress of collapse. Interesting features such as bursts, discontinuities, decay, etc arc observed when the collapse has sufficiently progressed.	en
dc.format.extent	539433 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	Dense matter	en
dc.subject	Neutrines	en
dc.subject	Collapsing stars	en
dc.subject	Flux profile	en
dc.title	Neutrinos in gravitational collapse: analysis of the flux profile.	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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