Actions for Production of high energy neutrinos in relativistic supernova shock waves [electronic resource].

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Production of high energy neutrinos in relativistic supernova shock waves [electronic resource].

Published
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy, 1979.
Physical Description
Pages: 12 : digital, PDF file
Additional Creators
United States. Department of Energy. Office of Scientific and Technical Information
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Summary
The possibility of producing high-energy neutrinos (> approx. 10 GeV) in relativistic supernova shock waves is considered. It is shown that, even if the dissipation in such shocks is due to hard hadron--hadron collisions, the resulting flux of neutrinos is too small to be observed by currently envisioned detectors. The associated burst of hard ..gamma..-rays, however, may be detectable. 3 tables.
Report Numbers
E 1.99:ucrl-82152
E 1.99: conf-7808107-1
conf-7808107-1
ucrl-82152
Subject(s)
Other Subject(s)
Note
Published through SciTech Connect.
01/01/1979.
"ucrl-82152"
" conf-7808107-1"
1978 DUMAD summer workshop, San Diego, CA, USA, 11 Aug 1978.
Weaver, T.A.
California Univ., Livermore (USA). Lawrence Livermore Lab.
Funding Information
W-7405-ENG-48
View MARC record | catkey: 13829391