Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4437
Full metadata record
DC FieldValueLanguage
dc.contributor.authorNath, Biman B.-
dc.date.accessioned2012-05-07T08:35:16Z-
dc.date.available2012-05-07T08:35:16Z-
dc.date.issued1992-09-
dc.identifier.citationPhysical Review D, 1992, Vol.46, p2341en
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368-
dc.identifier.urihttp://hdl.handle.net/2289/4437-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractIt is shown that, for a nontrivial radiative decay channel of the 17-keV neutrino, the photons would distort the microwave background radiation through ionization of the Universe. The constraint on the branching ratio of such decays from Cosmic Background Explorer measurements is found to be more stringent than that from SN 1987A. The limit on the branching ratio in terms of the Compton y parameter is Bγ<=1.5×10-7[τν/(1011 sec)]0.45 (y/10-3)1.11h-1 for an Ω=1, ΩB=0.1 universe.en
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992PhRvD..46.2341Nen
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.46.2341en
dc.relation.urihttp://arxiv.org/abs/astro-ph/9208004en
dc.rights(1992) by the American Physical Societyen
dc.subjectBackground radiationsen
dc.subjectParticle-theory and field-theory models of the early Universeen
dc.titleConstraints on radiative decay of the 17-keV neutrino from COBE measurementsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1992_PhysRevD_V46_p2341.pdf
  Restricted Access
Restricted Access198.82 kBAdobe PDFView/Open Request a copy


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.