Ultra High Energy Neutrino-Relic Neutrino Interactions In Dark Halos to Solve Infrared-Tev And GZK Cut-Off

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dc.creatorFargion, D.
dc.creatorGrossi, M.
dc.creatorLucentini, P. G. De Sanctis
dc.date2001-07-11
dc.date.accessioned2026-07-07T01:59:16Z
dc.date.available2026-07-07T01:59:16Z
dc.descriptionUltra High Energy Neutrino scattering on Relic Light Neutrinos in Dark Galactic or Local Group lead to Z and WW,ZZ showering: the nucleon component of the shower may overcome the GZK cut-off while the electro-magnetic tail at TeVs up to EeVs energy may solve the Infrared-TeV cut-off in a natural way. Different Gamma TeV puzzles may find a solution within this scenario: new predictions on UHECR spectra in future data are derived.
dc.description4 pages, 3 figures, 2 tables ICRC 2001 HE 3.6 Dark Matter - Germany
dc.identifierhttps://arxiv.org/abs/astro-ph/0107203
dc.identifierhttp://arxiv.org/abs/astro-ph/0107203
dc.identifier27th ICRC 2001, HE 3.6, Vol. 4, p.1578-1581, Germany, 2001.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3043
dc.subjectAstrophysics
dc.titleUltra High Energy Neutrino-Relic Neutrino Interactions In Dark Halos to Solve Infrared-Tev And GZK Cut-Off
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