Possible detection of relic neutrinos and their mass

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dc.creatorRingwald, A.
dc.date2001-11-09
dc.date.accessioned2026-07-07T03:45:47Z
dc.date.available2026-07-07T03:45:47Z
dc.descriptionRecently the possibility was widely discussed that a large fraction of the highest energy cosmic rays may be decay products of Z bosons which were produced in the resonant annihilation of ultrahigh energy cosmic neutrinos on cosmological relic neutrinos. If one takes this so-called Z-burst scenario seriously, one may infer the mass of the heaviest relic neutrino as well as the necessary ultrahigh energy cosmic neutrino flux from a comparison of the predicted Z-burst spectrum with the observed cosmic ray spectrum.
dc.description8 pages, 11 figures, needs icrc.cls (included). Invited so-called "Highlight Talk", to appear in the Proceedings of the 27th International Cosmic Ray Conference (ICRC 2001), Hamburg, Germany, August 2001
dc.identifierhttps://arxiv.org/abs/hep-ph/0111112
dc.identifierhttp://arxiv.org/abs/hep-ph/0111112
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41051
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titlePossible detection of relic neutrinos and their mass
dc.typetext

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