Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6737
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dc.contributor.authorGupta, Nayantara-
dc.date.accessioned2017-09-22T07:27:06Z-
dc.date.available2017-09-22T07:27:06Z-
dc.date.issued2016-02-
dc.identifier.citationAstroparticle Physics, 2016, Vol.74, p1-5en_US
dc.identifier.issn0927-6505-
dc.identifier.urihttp://hdl.handle.net/2289/6737-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractThe photo-disintegration of cosmic ray nuclei by starlight leads to the production of secondary antineutrinos. We have assumed that the flux of the ultrahigh energy cosmic ray nuclei near the Galactic plane region is the same as that observed near the earth and calculated the antineutrino flux produced from their photo-disintegration. The IceCube detector has measured the neutrino/antineutrino flux in the TeV–PeV energy range. Our calculated secondary antineutrino flux in the energy range of 10–100 TeV is found to be much less compared to the flux detected by the IceCube collaboration. The upper limit on the intensity of the radiation field in the extragalactic medium is much lower than that near the Galactic center. If we extend our formalism to the extragalactic medium the contribution from the photo-disintegration of ultrahigh energy cosmic ray heavy nuclei remains insignificant due to their very low flux.en_US
dc.language.isoenen_US
dc.publisherElsevier B.V.en_US
dc.relation.urihttp://adsabs.harvard.edu/abs/2016APh....74....1Gen_US
dc.relation.urihttps://arxiv.org/abs/1503.04328en_US
dc.relation.urihttp://dx.doi.org/10.1016/j.astropartphys.2015.08.003en_US
dc.rights2016 Elsevier B.V.en_US
dc.subjectHigh energy neutrionsen_US
dc.titleVery high energy antineutrinos from photo-disintegration of cosmic ray nucleien_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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