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| HAL : in2p3-00372092, version 1 |
| DOI : 10.1016/j.nuclphysbps.2009.02.069 |
| Fiche détaillée |  Récupérer au format |
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| Neutrino Oscillation Workshop - NOW 2008, Conca Specchiulla, Oranto : Italie (2009) |
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| Cosmogenic neutrino production from the propagation of ultra-high energy cosmic-ray nuclei |
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| D. Allard1 |
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| (2009) |
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| In this proceeding, we study the production of cosmogenic neutrinos from the propagation of ultra-high energy cosmic-ray (UHECR) nuclei. After discussing the main production channels for cosmic-ray nuclei, we investigate the dependence of the expected fluxes on astrophysical parameter such as the composition, the cosmological distribution of the sources, or the maximum energy of the accelerated cosmic-rays. We finally discuss the detectability of these cosmogenic neutrinos between 10^12 and 10^20 eV. |
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| 1 : | APC - AstroParticule et Cosmologie |
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| APC - AHE |
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| Thème(s) | : | Physique/Astrophysique/Phénomènes cosmiques de haute energie Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie |
| in2p3-00372092, version 1 | |
| http://hal.in2p3.fr/in2p3-00372092 | |
| oai:hal.in2p3.fr:in2p3-00372092 | |
| Contributeur : Simone Lantz | |
| Soumis le : Mardi 31 Mars 2009, 11:54:11 | |
| Dernière modification le : Lundi 25 Juin 2012, 17:15:59 | |
