Neutrinos from Auger Sources

dc.creatorHalzen, Francis
dc.creatorO'Murchadha, Aongus
dc.date2008-02-06
dc.date2008-02-28
dc.date.accessioned2026-07-07T09:23:29Z
dc.date.available2026-07-07T09:23:29Z
dc.descriptionThe Pierre Auger observatory has presented evidence that the arrival directions of cosmic rays with energies in excess of 6x10^7 TeV may be correlated with nearby active galactic nuclei (AGN). In this context we revisit a suggestion based on gamma ray observations that nearby Fanaroff-Riley I galaxies such as Cen A and M87 are the sources of the local cosmic rays. We compute the accompanying neutrino flux and find a flux within reach of second-generation kilometer-scale neutrino telescopes.
dc.description4 pages, LaTeX file using RevTEX4, 1 B/W .eps figure, typos corrected
dc.identifierhttps://arxiv.org/abs/0802.0887
dc.identifierhttp://arxiv.org/abs/0802.0887
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/155751
dc.subjectAstrophysics
dc.titleNeutrinos from Auger Sources
dc.typetext

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