Charge exchange reactions and the efficiency of solar neutrino detectors

Details Charge exchange reactions and the efficiency of solar neutrino detectors Charge exchange reactions and the efficiency of solar neutrino detectors

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvl..73...30a&link_type=abstract

Physical Review Letters, Volume 73, Issue 1, July 4, 1994, pp.30-33

Other

24

Charge-Exchange Reactions, Elementary Particle Processes

Scientific paper

The efficiencies of solar neutrino detectors are often based in part on weak interaction strengths determined by (p,n) and other charge exchange reactions. Although the (p,n) determinations are surprisingly good, it is shown that they may be inaccurate for important Gamow-Teller transitions whose strengths are a small fraction of the sum rule limit. This emphasizes the importance of direct calibration with ν sources for detectors such as 127I and 115In where direct β-decay information cannot be obtained. It may also bear on recent attempts to compare charge exchange and beta decay in the mass-37 system.

Affiliated with

Also associated with

No associations

Rating

Charge exchange reactions and the efficiency of solar neutrino detectors 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 Charge exchange reactions and the efficiency of solar neutrino detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Charge exchange reactions and the efficiency of solar neutrino detectors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-823731