High-energy neutrinos from CYG X-3

Details High-energy neutrinos from CYG X-3 High-energy neutrinos from CYG X-3

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986izssr..50.2245w&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Tbilisi, Georgian SSR, Apr. 1986) Akademiia Nauk SSSR, Izvestiia, Seriia Fiz

Astronomy and Astrophysics

Astronomy

Energetic Particles, Gamma Ray Astronomy, Neutrinos, X Ray Sources, Energy Spectra, Muons, Pulsars, Radiation Detectors, Underground Structures

Scientific paper

The neutrino flux averaged over the orbital period of Cyg X-3 is calculated to be approximately 10 to the -7th/sq m s for a threshold energy of approximately 100 GeV. This value is within the detection capability limits of underground detectors and can be detected by large-area detectors planned for the future. It is concluded that detection of the neutrino flux from Cyg X-3 and its phase dependence can yield important information about the emission model of gamma quanta and neutrinos.

Affiliated with

Also associated with

No associations

Rating

High-energy neutrinos from CYG X-3 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 High-energy neutrinos from CYG X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-energy neutrinos from CYG X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1150493