The flavor distribution of Cosmic Neutrinos

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, one figure. Initial results remain valid, but an extended improvement has been made compared to the first version, i

Scientific paper

Simple approximate expressions for the relative flavor fluxes of energetic cosmic neutrinos detected on Earth, are presented in terms of their initial fluxes at the surface of the producing cosmic sites, assuming the neutrino mixing angles to lie in the experimentally favored region. These expressions highlight the main sensitivities to the initial production fluxes as well as to small variations of the mixing angles within the experimentally preferred region, thus providing simple methods to disentangle these physical quantities from cosmic neutrino data. This is more so, due to some striking mathematical properties of the relative neutrino flavors at $(s_{23}=1/\sqrt{2}, \~s_{13}=0)$, which somehow characterize the whole experimentally preferred region. We also assess the quality of our approximate expressions through a numerical comparison with the exact results.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The flavor distribution of Cosmic Neutrinos 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 The flavor distribution of Cosmic Neutrinos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The flavor distribution of Cosmic Neutrinos will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-558631

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.