Physics – Plasma Physics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..119i&link_type=abstract
In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 119-122 (SEE N94-22624 05-75)
Physics
Plasma Physics
Dense Plasmas, High Temperature Plasmas, Neutrinos, Stellar Evolution, Energy Dissipation, High Energy Interactions, Nuclear Reactions, Particle Production, Plasma Waves
Scientific paper
The neutrino emission processes in dense high temperature plasmas are reviewed. The neutrino emission processes are key factors which decide the evolution of stars. Stellar evolution proceeds through the balance between the energy generation due to thermonuclear reactions and the energy loss due to neutrino emission processes. Recent developments in the study of the four major neutrino emission processes are reviewed. The energy loss rates due to pair, photon, plasma and bremstrahlung neutrino processes are calculated using Weinberg-Salam theory. The screening effects, the ionic correlation effects, and the plasma effects are taken into account.
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