Production and detection of high-energy neutrinos from Cygnus X-3

Details Production and detection of high-energy neutrinos from Cygnus X-3 Production and detection of high-energy neutrinos from Cygnus X-3

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..32.1145k&link_type=abstract

Physical Review D (Particles and Fields), Volume 32, Issue 5, 1 September 1985, pp.1145-1151

Physics

36

X-Ray Binaries

Scientific paper

Cygnus X-3 is a potent source of high-energy γ rays, with energies up to 104 TeV. In the context of a model where these γ rays are produced by the collision of a high-energy proton beam with matter we calculate the flux, spectrum, and ``light curve'' of the neutrinos produced. Neutrinos with energies of 3-100 TeV may be detectable in large, underground detectors by the muons they produce in the surrounding rock.

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