Galactic neutrino background from cosmic ray interaction with the ISM content

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dc.creatorDe Donato, C.
dc.creatorMedina-Tanco, G. A.
dc.creatorD'Olivo, J. C.
dc.date2007-09-03
dc.date2007-10-18
dc.date.accessioned2026-07-07T08:36:45Z
dc.date.available2026-07-07T08:36:45Z
dc.descriptionWe use a diffusive model for the propagation of Galactic cosmic rays to estimate the charged pion production in interactions with protons of the interstellar medium. Cosmic ray nuclei from proton to iron are considered and the corresponding contribution to the neutrino secondary flux produced as a result of spallation is also estimated.
dc.description4 pages, 3 figures Proceeding of the 30th International Cosmic Ray Conference, Merida (2007), Yucatan, Mexico
dc.identifierhttps://arxiv.org/abs/0709.0278
dc.identifierhttp://arxiv.org/abs/0709.0278
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140173
dc.subjectAstrophysics
dc.titleGalactic neutrino background from cosmic ray interaction with the ISM content
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