Solar neutrinos and the influence of radiative opacities on solar models.
Abstract
Use of new radiative opacities based on the hot Thomas-Fermi model of the atom yields a predicted solar neutrino flux which is still considerably larger than the flux observed in Davis's 37Cl experiment. Subject headings: interiors, solar - neutrinos
- Publication:
-
The Astrophysical Journal
- Pub Date:
- December 1974
- DOI:
- 10.1086/153296
- Bibcode:
- 1974ApJ...194..743C
- Keywords:
-
- Astronomical Models;
- Neutrinos;
- Opacity;
- Solar Corpuscular Radiation;
- Thomas-Fermi Model;
- Abundance;
- Radiative Transfer;
- Solar Flux Density;
- Solar Physics