Neutrinos in gravitational collapse: The Dirac formalism

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1238

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DC Field	Value	Language
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Dhurandhar, S.V.	-
dc.contributor.author	Vishveshwara, C.V.	-
dc.date.accessioned	2006-05-16T09:00:14Z	-
dc.date.available	2006-05-16T09:00:14Z	-
dc.date.issued	1982-04-15	-
dc.identifier.citation	Physical Review D, 1982, Vol.25, 2053-2064	en
dc.identifier.issn	1550-7998	-
dc.identifier.uri	http://hdl.handle.net/2289/1238	-
dc.description.abstract	The massless Dirac equations for the neutrino are studied in the background geometry relevant to a gravitational collapse, i.e., a Friedmann dust interior matched onto a Schwarzschild exterior. The interior normal modes are obtained and continued consistently across the collapsing surface into the exterior. This yields the expected spectral shifts quite naturally in addition to the phenomenon of backward emission. The complete exterior modes are obtained by matching solutions at the Schwarzschild barrier. The asymptotic transmission coefficient is computed, and this includes in addition to the effects of gravitational collapse the effects of the exterior potential barrier.	en
dc.format.extent	1281970 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRD/v25/p2053	en
dc.rights	(1982) by the American Physical Society	en
dc.title	Neutrinos in gravitational collapse: The Dirac formalism	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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