The Gamow–Teller (GT) strength transitions in nuclear structures and astrophysical processes proved to be very important to understand the mechanisms of formation of neutron stars and black holes, therefore the GT transitions in the 46Ti→46V, 47Ti→47V, 48Ti→48V, and 50Cr→50Mn charge-exchange reactions have been studied. The shell model calculations have been carried out in the fp-model space without any restrictions using the GXFP1A, KB3G, and FPD6 effective interactions. The calculation of the GT distribution is compared with recent available experimental data. The theoretical calculations are in reasonably good agreement with the experimental GT distributions and with the summed transition strengths B(GT). For the individual transformatio...
AbstractA comparative study of the nuclear Gamow–Teller response (GTR) within conceptually different...
The Gamow-Teller strength in the \u3b2+ direction to Sc46 was extracted via the Ti46(t,He3+\u3b3) re...
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...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
Given the importance of Gamow-Teller (GT) transitions in nuclear structure and astrophysical nuclear...
Due to the simplicity of the operator , a strength distribution of Gamow-Teller (GT) transitions d...
Weak interaction processes play an essential role in many astrophysical scenarios. In many cases the...
The Gamow-Teller (GT) transition is inarguably one of the most important nuclear weak transitions of...
We use the shell model Monte Carlo method to calculate complete 0f1p-shell response functions for Ga...
The Gamow-Teller (GT) transition is inarguably one of the most important nuclear weak transitions of...
Gamow-Teller (GT) transitions starting from unstable pf-shell nuclei are of interest not only in nuc...
In this work we have studied T-z = +2 -> +1, Gamow-Teller (GT) transitions in the Ti-48(He-3, t)V-48...
AbstractA comparative study of the nuclear Gamow–Teller response (GTR) within conceptually different...
The Gamow-Teller strength in the \u3b2+ direction to Sc46 was extracted via the Ti46(t,He3+\u3b3) re...
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...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
The Gamow-Teller transition strengths in pf-shell nuclei are important parameters in a presupernova ...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
Given the importance of Gamow-Teller (GT) transitions in nuclear structure and astrophysical nuclear...
Due to the simplicity of the operator , a strength distribution of Gamow-Teller (GT) transitions d...
Weak interaction processes play an essential role in many astrophysical scenarios. In many cases the...
The Gamow-Teller (GT) transition is inarguably one of the most important nuclear weak transitions of...
We use the shell model Monte Carlo method to calculate complete 0f1p-shell response functions for Ga...
The Gamow-Teller (GT) transition is inarguably one of the most important nuclear weak transitions of...
Gamow-Teller (GT) transitions starting from unstable pf-shell nuclei are of interest not only in nuc...
In this work we have studied T-z = +2 -> +1, Gamow-Teller (GT) transitions in the Ti-48(He-3, t)V-48...
AbstractA comparative study of the nuclear Gamow–Teller response (GTR) within conceptually different...
The Gamow-Teller strength in the \u3b2+ direction to Sc46 was extracted via the Ti46(t,He3+\u3b3) re...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440