Neutrino astronomy

Details Neutrino astronomy Neutrino astronomy

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..198...39h&link_type=abstract

IN: Astrophysics in Antarctica (A92-22401 07-89). New York, American Institute of Physics, 1989, p. 39-51. Research supported by

Mathematics

Logic

4

Gamma Ray Astronomy, Neutrinos, Particle Flux Density, Particle Telescopes, Antarctic Regions, Atmospheric Attenuation, Electromagnetic Fields, Hadrons, Technological Forecasting

Scientific paper

The present evaluation of arguments for the claim that observations of PeV gamma-rays from cosmic sources at, recently reported flux-levels, ensure the detection of neutrinos by detectors with an effective area of about 1 sq km, gives attention to the interdisciplinary involvement of astronomy, astrophysics, cosmology, and particle physics. It is noted that no effective method exists for the creation of neutrino telescopes of the requisite effective area. The possibility of instrumenting Antarctic ice in such a way as to serve as a deep underground telescope for detecting Cherenkov, radio, or acoustic radiation from neutrino-induced EM showers is discussed.

Affiliated with

Also associated with

No associations

Rating

Neutrino astronomy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Neutrino astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1559846