High-Energy Neutrino Astronomy with the Super-Kamiokande Detector

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dc.creatorHabig, A.
dc.date2005-07-02
dc.date.accessioned2026-07-07T02:18:09Z
dc.date.available2026-07-07T02:18:09Z
dc.descriptionThe Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible point and bursting neutrino sources, as well as possible WIMP annihilation signatures. No significant evidence for such sources have been found, and the resulting flux limits have been calculated.
dc.description4 pages, 2 figures, submitted to proc. of 29th ICRC, Pune, India
dc.identifierhttps://arxiv.org/abs/astro-ph/0507051
dc.identifierhttp://arxiv.org/abs/astro-ph/0507051
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9381
dc.subjectAstrophysics
dc.titleHigh-Energy Neutrino Astronomy with the Super-Kamiokande Detector
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