The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presupernova models. A high-energy-resolution (He-3,t) experiment was performed on the T-z=1 nucleus Ti-46 at 0(degrees) and at an intermediate incident energy of 140 MeV/nucleon for the study of precise GT transition strengths to the final T-z=0 nucleus V-46. With an energy resolution of 33 keV, individual GT transitions were observed and GT strengths were derived for them up to the excitation energy of 4.5 MeV. The GT strengths were compared with shell-model calculations using various effective interactions. In this low-lying region, most GT states have isospin T=0. A few GT states with isospin T=1 were identified from the existence of the correspond...
Owing to its simplicity and also its nature of spin-isospin (sigma tau) excitation, Gamow-Teller (GT...
Using the high-resolution O-18(He-3, t)F-18 reaction at 0 degrees and at 140 MeV/nucleon, Gamow-Tell...
Under the assumption that isospin is a good quantum number, symmetry is expected for the transitions...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
The Gamow-Teller (GT) transition strengths in fp -shell nuclei are important parameters in presupern...
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 ...
In this work we have studied T-z = +2 -> +1, Gamow-Teller (GT) transitions in the Ti-48(He-3, t)V-48...
Given the importance of Gamow-Teller (GT) transitions in nuclear structure and astrophysical nuclear...
In this work we have studied T-z = +2 -> +1, Gamow-Teller (GT) transitions in the Ti-48(He-3, t)V-48...
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 ...
Gamow-Teller (GT) transitions starting from the T-z = +2 nucleus Zn-64 to the T-z = +1 nucleus Ga-64...
Owing to its simplicity and also its nature of spin-isospin (sigma tau) excitation, Gamow-Teller (GT...
Using the high-resolution O-18(He-3, t)F-18 reaction at 0 degrees and at 140 MeV/nucleon, Gamow-Tell...
Under the assumption that isospin is a good quantum number, symmetry is expected for the transitions...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
The Gamow-Teller (GT) transition strengths in fp-shell nuclei are important parameters in presuperno...
The Gamow-Teller (GT) transition strengths in fp -shell nuclei are important parameters in presupern...
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 ...
In this work we have studied T-z = +2 -> +1, Gamow-Teller (GT) transitions in the Ti-48(He-3, t)V-48...
Given the importance of Gamow-Teller (GT) transitions in nuclear structure and astrophysical nuclear...
In this work we have studied T-z = +2 -> +1, Gamow-Teller (GT) transitions in the Ti-48(He-3, t)V-48...
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 ...
Gamow-Teller (GT) transitions starting from the T-z = +2 nucleus Zn-64 to the T-z = +1 nucleus Ga-64...
Owing to its simplicity and also its nature of spin-isospin (sigma tau) excitation, Gamow-Teller (GT...
Using the high-resolution O-18(He-3, t)F-18 reaction at 0 degrees and at 140 MeV/nucleon, Gamow-Tell...
Under the assumption that isospin is a good quantum number, symmetry is expected for the transitions...