37Cl solar neutrino capture cross section

Details 37Cl solar neutrino capture cross section 37Cl solar neutrino capture cross section

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvc..36..879a&link_type=abstract

Physical Review C (Nuclear Physics), Volume 36, Issue 3, September 1987, pp.879-882

Physics

Nuclear Physics

11

Relation With Nuclear Matrix Elements And Nuclear Structure, 20<=A<=38

Scientific paper

We argue that the standard derivation of the Gamow-Teller contribution to the 37Cl solar neutrino capture cross section from the 37Ca delayed proton spectrum yields a B(GT) distribution that is too weak and shifted to lower excitation energies. Because the redistribution of Gamow-Teller strength occurs primarily above the analog state, where the neutrino reaction phase space is small, it has only a small effect (4%) on the solar neutrino cross section. However, our observations help resolve the discrepancy between the 37Ca β-decay and 37Cl(p,n) Gamow-Teller mappings.

Affiliated with

Also associated with

No associations

Rating

37Cl solar neutrino capture cross section does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with 37Cl solar neutrino capture cross section, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 37Cl solar neutrino capture cross section will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1677489