Solar Neutrinos
Abstract
The predicted capture rate in the Cl37 experiment for detecting solar neutrinos is calculated using the results of recent nuclear experiments and solar-model investigations. It is shown that additional experiments (e.g., with H2, Li7, B11, or ν-e scattering) are necessary to establish the relative contributions of the proton-proton chain and the CNO cycle to solar energy generation.
- Publication:
-
Physical Review Letters
- Pub Date:
- August 1966
- DOI:
- 10.1103/PhysRevLett.17.398
- Bibcode:
- 1966PhRvL..17..398B