Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...431..761k&link_type=abstract
The Astrophysical Journal, vol. 431, no. 2, pt. 1, p. 761-766
Astronomy and Astrophysics
Astrophysics
8
Degenerate Matter, Dense Plasmas, Energy Dissipation, Neutrinos, Particle Energy, Stellar Interiors, Cosmology, Plasma Density, Plasmons, Stellar Evolution, Vector Analysis
Scientific paper
The axial vector contribution to the plasma neutrino energy-loss rate for strongly degenerate electrons is calculated by using the accurate dispersion relation for the transverse plasmon which is valid for relativistically degenerate electrons. Comparison is made with previous calculations. It is found that the axial vector contribution to the plasma neutrino energy-loss rate is at most on the order of 10-4 of the vector contribution for strongly degenerate electrons, which is about 10-2 of the value recently reported by Braaten & Segel (1993).
Hayashi Hiroshi
Itoh Naoki
Kohyama Yasuharu
Obama Akihiko
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