Gamow-Teller strength inand
- 1 October 1995
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review C
- Vol. 52 (4) , R1736-R1740
- https://doi.org/10.1103/physrevc.52.r1736
Abstract
Through a sequence of large scale shell model calculations, Gamow-Teller strengths ( and ) in and are obtained. They reproduce the experimental values by quenching the operator through the standard factor of 0.77. Comparisons are made with recent shell model Monte Carlo calculations. Results are shown to depend critically on the interaction. It is argued that the experimental data contain enough strength in the region above the resonance to make them consistent with the sum rule.
Keywords
All Related Versions
This publication has 23 references indexed in Scilit:
- Spin-isospin strength distributions forfpshell nuclei: Results for the(n,p),(n,p), and(n,p) reactions at 198 MeVPhysical Review C, 1994
- Shell-model calculations of Gamow-Teller strength inV51,Fe54, andCo59Physical Review C, 1993
- The 54,56Fe(n, p)54,56Mn reactions at En = 97 MeVNuclear Physics A, 1993
- Gamow-Teller strength in theFe54(p,n)54Co reaction at 135 MeVPhysical Review C, 1990
- Gamow-Teller strength deduced from charge exchange reactions onat 300 MeVPhysical Review C, 1989
- Gamow-Teller electron capture strength distributions in stars: Unblocked iron and nickel isotopesNuclear Physics A, 1985
- Excitation of giant spin-isospin multipole vibrations in 54, 56Fe and 58, 60NiNuclear Physics A, 1983
- Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60The Astrophysical Journal, 1982
- Shell-model calculations for the zinc isotopesNuclear Physics A, 1976
- Finite-NucleusMatrix in the Microscopic Description of Inelastic Proton ScatteringPhysical Review Letters, 1969