Techniques for detection of cosmic diffuse neutrinos and anti-neutrinos

Details Techniques for detection of cosmic diffuse neutrinos and anti-neutrinos Techniques for detection of cosmic diffuse neutrinos and anti-neutrinos

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..512c&link_type=abstract

In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 19

Astronomy and Astrophysics

Astronomy

Antineutrinos, Cosmology, Diffuse Radiation, Neutrinos, Radiation Detectors, Relic Radiation, Spaceborne Astronomy, Telescopes

Scientific paper

We first indicate the energy regions where diffuse neutrinos or antineutrinos are expected. Techniques for the detection of these neutrinos are described. We focus on the prospects for detecting neutrinos or antineutrinos in the window between the atmospheric and solar neutrino flux, from 10-30 MeV. We also describe methods to detect neutrinos in the 100 MeV to GeV region using a lunar neutrino telescope. A brief comment is made concerning the detection of the 1.9-deg relic neutrinos.

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