Gamow-Teller strengths for selected nuclei in the iron region (A∼56) have been investigated via shell-model Monte Carlo calculations with realistic interactions in the complete fp basis. Results for all cases show significant quenching relative to single-particle estimates, in quantitative agreement with (n,p) data. The T=0 residual interaction and the f7/2-f5/2 spin-orbit splitting are shown to play major roles in the quenching mechanism. Calculated B(E2,21+→01+) values are in fair agreement with experiment using effective charges of ep=1.1e and en=0.1e
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
We have performed large-scale shell model calculations of the Gamow-Teller strength distributions in...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
Results of shell-model calculations of the Gamow-Teller strength distributions for the (n, p) or ele...
International audienceWe apply the charge-exchange subtracted second random-phase approximation (SSR...
Gamow-Teller transition properties for neutron-rich nitrogen, oxygen and fluorine isotopes are studi...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
A systematic shell model description of the experimental Gamow-Teller transition strength distributi...
We have performed large-scale shell model calculations of the Gamow-Teller strength distributions in...
We present Gamow-Teller strength distributions from shell model Monte Carlo studies of fp-shell nucl...
Isospin symmetry is expected for the T-z=+/- 1 -> 0 isobaric analogous transitions in isobars wit...
The Gamow-Teller strength distributions of 116Sb and 122Sb were measured with the 116,122Sn(3He,t)11...
The Gamow\u2013Teller strength distributions of 116Sb and 122Sb were measured with the 116,122Sn(3He...
We use the shell model Monte Carlo method to calculate complete 0f1p-shell response functions for Ga...
We performed self-consistent Hartree-Fock plus random-phase approximation (HF+RPA) calculations for ...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
We have performed large-scale shell model calculations of the Gamow-Teller strength distributions in...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
Results of shell-model calculations of the Gamow-Teller strength distributions for the (n, p) or ele...
International audienceWe apply the charge-exchange subtracted second random-phase approximation (SSR...
Gamow-Teller transition properties for neutron-rich nitrogen, oxygen and fluorine isotopes are studi...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
A systematic shell model description of the experimental Gamow-Teller transition strength distributi...
We have performed large-scale shell model calculations of the Gamow-Teller strength distributions in...
We present Gamow-Teller strength distributions from shell model Monte Carlo studies of fp-shell nucl...
Isospin symmetry is expected for the T-z=+/- 1 -> 0 isobaric analogous transitions in isobars wit...
The Gamow-Teller strength distributions of 116Sb and 122Sb were measured with the 116,122Sn(3He,t)11...
The Gamow\u2013Teller strength distributions of 116Sb and 122Sb were measured with the 116,122Sn(3He...
We use the shell model Monte Carlo method to calculate complete 0f1p-shell response functions for Ga...
We performed self-consistent Hartree-Fock plus random-phase approximation (HF+RPA) calculations for ...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
We have performed large-scale shell model calculations of the Gamow-Teller strength distributions in...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...