Flipped neutrino emissivity of hot plasma in supernova core

Details Flipped neutrino emissivity of hot plasma in supernova core Flipped neutrino emissivity of hot plasma in supernova core

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..49.5593g&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 49, Issue 10, 15 May 1994, pp.5593-5596

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1

Elementary Particle Processes, Neutrino Interactions, Non-Standard-Model Neutrinos, Right-Handed Neutrinos, Etc., Neutron Stars

Scientific paper

We calculate the energy loss due to wrong-helicity sterile neutrinos
produced due to the decay of plasmons into flipped neutrino pairs at
relativistic temperatures and densities in the core of a nascent neutron
star and compare our results with other processes.

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