Abstract
Gamow-Teller transition strengths obtained in the reaction studied at 94, 159, and 197 MeV incident proton energies are presented, and used to evaluate the efficiency of as a solar neutrino detector. Excitation of the first excited state at in sensitive to solar neutrinos, is evaluated. The sum of Gamow-Teller strength up to particle emission threshold and up to 20 MeV excitation energy are also reported. This paper also provides a new measurement of the Coulomb displacement energy the excitation energy of the isobaric analog state, and the centroid of the Gamow-Teller resonance in
- Received 28 April 1998
DOI:https://doi.org/10.1103/PhysRevC.59.500
©1999 American Physical Society