Neutrino, Cosmos, and New Physics

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dc.creatorDolgov, A. D.
dc.date2005-04-26
dc.date.accessioned2026-07-07T03:54:40Z
dc.date.available2026-07-07T03:54:40Z
dc.descriptionObservational manifestations of possible breaking of spin-statistics relation for neutrinos are considered. It is argued that bosonic neutrinos may form cosmological cold dark matter, improve agreement of BBN predictions with observations, make operative Z-burst model of ultra-high energy cosmic rays, etc. Restrictions for an admixture of bosonic component to neutrino which follow from double beta decay are discussed.
dc.description17 pages, 2 figures; talks at Neutrino Telescopes, Venice, 22/02-25/02, 2005 and Rencontre LaThuile-05, 27/02-05/03, 2005
dc.identifierhttps://arxiv.org/abs/hep-ph/0504238
dc.identifierhttp://arxiv.org/abs/hep-ph/0504238
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44335
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrino, Cosmos, and New Physics
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