Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4465
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dc.contributor.authorGupta, Nayantara-
dc.contributor.authorMani, H.S.-
dc.date.accessioned2012-05-08T04:45:11Z-
dc.date.available2012-05-08T04:45:11Z-
dc.date.issued2005-07-
dc.identifier.citationJournal of Physics G, 2005, Vol.31, p599en
dc.identifier.issn0954-3899-
dc.identifier.issn1361-6471 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4465-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractWe consider the non-radiative two-body decay of a neutrino to a daughter neutrino with degraded energy and a very light particle (Majoron). Ultrahigh-energy neutrinos from an astrophysical source like a gamma ray burst undergoing this decay process are found to produce different number of events in the detector depending on whether they are Majorana or Dirac particles. The next generation large-scale experiments like Multi-OWL is expected to provide us an accurate determination of the flux of neutrinos from astrophysical sources and this may enable us to distinguish between the Dirac and Majorana nature of neutrino.en
dc.language.isoenen
dc.publisherIOP Publishing Ltden
dc.relation.urihttp://adsabs.harvard.edu/abs/2005JPhG...31..599Gen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0404218en
dc.relation.urihttp://dx.doi.org/10.1088/0954-3899/31/7/006en
dc.rights2005 IOP Publishing Ltden
dc.titleProspect of determining the Dirac/Majorana state of the neutrino by a Multi-OWL experimenten
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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