Experimental status of high energy neutrino astronomy

Details Experimental status of high energy neutrino astronomy Experimental status of high energy neutrino astronomy

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nuphs..14r..97s&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 14, Issue 1, p. 97-102.

Physics

Nuclear Physics

2

Scientific paper

Current status of high energy astronomy is reviewed from an experimental
point of view. Present data from the Baksan, Kamiokande, and IMB
detectors constrain neutrino flux enhancement factors (λ) to be
less than about 400, based on extrapolations from reported ultrahigh
energy (UHE) ``D.C.'' gamma ray observations.

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