Neutrino Driven Streaming Instabilities in a Dense Plasma

Details Neutrino Driven Streaming Instabilities in a Dense Plasma Neutrino Driven Streaming Instabilities in a Dense Plasma

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phrvl..83.2703s&link_type=abstract

Physical Review Letters, Volume 83, Issue 14, October 4, 1999, pp.2703-2706

Astronomy and Astrophysics

Astrophysics

52

Scientific paper

The nonlinear self-consistent propagation of neutrinos in a dense plasma is described using the relativistic kinetic equations for neutrinos and electrons. The general nonlinear dispersion relation for a neutrino fluid coupled with a plasma is derived. For scenarios close to realistic astrophysical conditions, neutrino driven streaming instabilities can develop, with growth rates which scale with the Fermi constant GF, thus leading to significant energy transfer from the neutrinos to the plasma.

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