Photo-coulomb neutrino process

Details Photo-coulomb neutrino process Photo-coulomb neutrino process

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aph....22..369b&link_type=abstract

Astroparticle Physics, Volume 22, Issue 5-6, p. 369-375.

Physics

3

:12.15.-Y, 12.15.-M, 13.15.+G, 13.85.Lg, 97.60.-S

Scientific paper

The photo-coulomb neutrino process (Z+γ→Z+ν+ν&OverBar) has been considered in the electro-weak theory and the influence of this process to the evolution of stars has been outlined. The scattering cross-section of this process is calculated in both low and high energy limit. The neutrino mass has been taken into account in this calculation. In the low-energy limit the neutrino luminosity is computed in the temperature range 108 109 K and is also compared to the previous result obtained according to the current-current coupling theory. The process may be significant for the evolution of stars in the later phases.

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