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Neutrino Astronomy. [Cyg X-1; SN 1987a]

Conference · · AIP Conference Proceedings (American Institute of Physics); (USA)
OSTI ID:6701304
 [1];  [2];  [3]
  1. Department of Physics, University of Wisconsin, Madison, WI 53706 (USA)
  2. Department of Physics and Astronomy, University of Hawaii, Honolulu, HI (USA)
  3. Bartol Research Institute, University of Delaware, Newark, DE (USA)
We review the arguments supporting the claim that the observation of PeV ({ital E}{approx gt}10{sup 15} eV) {gamma}-rays from cosmic sources at the flux-levels recently reported, guarantees the detection of neutrinos by detectors with an effective area of order 1 km{sup 2}. We emphasize the unique opportunities of neutrino astronomy as well as its multi-disciplinary facets touching astronomy, astrophysics, cosmology, and particle physcis. At present we do not know of any cost-effective method to commission neutrino telescopes with {ital O}(1km{sup 2}) effective area. We draw attention to the possibility of instrument Antarctic ice as a deep underground telescope detecting Cherenkov, radio of acoustic radiation from neutrino-induced electromagnetic showers.
DOE Contract Number:
AC02-76ER00881
OSTI ID:
6701304
Report Number(s):
CONF-8906234--
Conference Information:
Journal Name: AIP Conference Proceedings (American Institute of Physics); (USA) Journal Volume: 198:1
Country of Publication:
United States
Language:
English