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Neutrinos in gravitational collapse: The Dirac formalism

dc.contributor.authorIyer, B R
dc.contributor.authorDhurandhar, S V
dc.contributor.authorVishveshwara, C V
dc.date.accessioned2006-05-16T09:00:14Z
dc.date.available2006-05-16T09:00:14Z
dc.date.issued1982-04-15
dc.description.abstractThe 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.extent1281970 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationPhysical Review D, 1982, Vol.25, 2053-2064en
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/2289/1238
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v25/p2053en
dc.rights(1982) by the American Physical Societyen
dc.titleNeutrinos in gravitational collapse: The Dirac formalismen
dc.typeArticleen

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