Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4936
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dc.contributor.authorSethi, S.K.-
dc.date.accessioned2012-07-14T10:30:44Z-
dc.date.available2012-07-14T10:30:44Z-
dc.date.issued1996-
dc.identifier.citationPhysical Review D, 1996, Vol.54, p1301en
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368(Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4936-
dc.descriptionRestricted Accessen
dc.description.abstractWe calculate constraints on radiatively decaying neutrinos from the recent detection of singly ionized helium in the diffuse intergalactic medium (IGM) at z~=3.3. We consider a model in which neutrinos predominantly decay into invisible relativistic particles with a rate τ-1, and with a small branching ratio into the radiative mode. To satisfy the observation, which puts a lower bound on the number density of singly ionized helium atoms in the IGM, we show that, for τ>~1018 sec (1 eV/m2ν), transition moment of neutrinos, μ12, is constrained to be <=4-8×10-17 μB for 110 eV<~mν<~10 keV. Implications of this bound for particle physics and cosmology are briefly discussed.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996PhRvD..54.1301Sen
dc.relation.urihttp://arxiv.org/abs/astro-ph/9507116en
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.54.1301en
dc.rights1996 American Physical Societyen
dc.subjectDecays of heavy neutrinosen
dc.subjectElectromagnetic decaysen
dc.subjectIntergalactic matteren
dc.subjectquasar absorption and emission-line systemsen
dc.subjectLyman foresten
dc.titleNew astrophysical constraint on radiatively decaying neutrinosen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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