On the possibility of detecting high energy neutrinos from the galactic disc

Details On the possibility of detecting high energy neutrinos from the galactic disc On the possibility of detecting high energy neutrinos from the galactic disc

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nuphs..14..163c&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 14, Issue 2, p. 163-165.

Physics

Nuclear Physics

Scientific paper

We discuss the possibility of detecting H.E. neutrinos from the galactic disc by recording the upgoing muons produced by νμ in the rock and crossing a large area detector. We use as normalization point the galactic gamma-ray flux observed by satellites at Eo  100 MeV and different values of the power law index of energy spectrum γ, compatible with experimental data and the models of cosmic ray propagation. With a detector area Aeff = 105 m2 a signal could be detected in case of values of γ  1.5.

Affiliated with

Also associated with

No associations

Rating

On the possibility of detecting high energy neutrinos from the galactic disc 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 On the possibility of detecting high energy neutrinos from the galactic disc, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the possibility of detecting high energy neutrinos from the galactic disc will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1382700