Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...395..622i&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 395, no. 2, Aug. 20, 1992, p. 622-631.
Astronomy and Astrophysics
Astrophysics
74
Degenerate Matter, Electron Plasma, Energy Dissipation, Neutrinos, Plasmons, Stellar Interiors, Elementary Particles, Relativistic Particles, Stellar Evolution
Scientific paper
The neutrino energy-loss rates due to plasma neutrino process are calculated for strongly degenerate electrons by using the accurate relativistic dispersion relations for the longitudinal and transverse plasmons. The calculated plasma neutrino energy loss rates are generally valid for relativistically degenerate electrons as well as for nonrelativistically degenerate electrons. The ratio of the result of the present calculation to that of the previous calculations ranges between 0.39 and 3.22 depending upon densities and temperatures. The results of the calculation are expressed by an analytical fitting formula.
Hikita Atsushi
Itoh Naoki
Kohyama Yasuharu
Mutoh Haruhiko
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