Gamow-Teller strength distributions in-shell nuclei
- 1 December 1997
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review C
- Vol. 56 (6) , 3079-3086
- https://doi.org/10.1103/physrevc.56.3079
Abstract
We use the shell model Monte Carlo method to calculate complete -shell response functions for Gamow-Teller (GT) operators and obtain the corresponding strength distributions using a maximum entropy technique. The approach is validated against direct diagonalization for Ti. Calculated GT strength distributions agree well with data from and reactions for nuclei with –64. We also calculate the temperature evolution of the GT distributions for representative nuclei and find that the GT distributions broaden and the centroids shift to lower energies with increasing temperature.
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This publication has 41 references indexed in Scilit:
- Gamow-Teller strength in(n,p) reactions at 198 MeVPhysical Review C, 1995
- Spin-isospin strength distributions forfpshell nuclei: Results for the(n,p),(n,p), and(n,p) reactions at 198 MeVPhysical Review C, 1994
- Search for important weak interaction nuclei in presupernova evolutionThe Astrophysical Journal Supplement Series, 1994
- The 54,56Fe(n, p)54,56Mn reactions at En = 97 MeVNuclear Physics A, 1993
- Nuclear spin and isospin excitationsReviews of Modern Physics, 1992
- Gamow-Teller strength observed in the 48Ti(n, p)48Sc reaction: Implications for the double beta decay of 48CaNuclear Physics A, 1990
- Gamow-Teller strength deduced from charge exchange reactions onat 300 MeVPhysical Review C, 1989
- Status of the Nuclear Shell ModelAnnual Review of Nuclear and Particle Science, 1988
- Stellar weak-interaction rates for sd-shell nuclei. I - Nuclear matrix element systematics with application to Al-26 and selected nuclei of importance to the supernova problemThe Astrophysical Journal Supplement Series, 1980
- Effective interactions for the 1p shellNuclear Physics, 1965