Exact analytical models of the streaming instability driven by intense neutrino beams

Details Exact analytical models of the streaming instability driven by intense neutrino beams Exact analytical models of the streaming instability driven by intense neutrino beams

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jcap...05..011s&link_type=abstract

Journal of Cosmology and Astroparticle Physics, Issue 05, pp. 011 (2006).

Physics

1

Scientific paper

Detailed properties of the neutrino streaming instability in a plasma are investigated for two particular choices of beamed neutrino distributions that permit exact analytical solutions to the dispersion relation. The dispersion relation is solved analytically, and it is shown that the maximum instability growth rate scales with powers κ of the Fermi constant GF lower than 2 (1 <= κ <= 4/3). For conditions present in type II supernovae, the neutrinos are sufficiently collimated for the neutrino streaming instability to operate.

Affiliated with

Also associated with

No associations

Rating

Exact analytical models of the streaming instability driven by intense neutrino beams 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 Exact analytical models of the streaming instability driven by intense neutrino beams, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Exact analytical models of the streaming instability driven by intense neutrino beams will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1008682