High-energy neutrino astronomy with the super-kamiokande detector

Research output: Contribution to conferencePaper

Abstract

The 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.

Original languageEnglish (US)
Pages267-270
Number of pages4
StatePublished - Jan 1 2005
Event29th International Cosmic Ray Conference, ICRC 2005 - Pune, India
Duration: Aug 3 2005Aug 10 2005

Other

Other29th International Cosmic Ray Conference, ICRC 2005
CountryIndia
CityPune
Period8/3/058/10/05

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  • Cite this

    Habig, A. T. (2005). High-energy neutrino astronomy with the super-kamiokande detector. 267-270. Paper presented at 29th International Cosmic Ray Conference, ICRC 2005, Pune, India.