Spin-isospin excitations of the medium-mass nucleus Co-58 were studied using the (n, p)-type (d,He-2) charge-exchange reaction at an incident energy E-d = 170 MeV and small scattering angles. The achieved energy resolution of 130 keV, full width at half maximum, allowed the extraction of Gamow-Teller strength to 13 peaks at excitation energies lower than 4.1 MeV in the residual nucleus Co-58 and is consistent with the results of a multipole-decomposition analysis. The identification of Gamow-Teller transitions is possible by comparison of the measured cross sections with DWBA calculations. The results are used to discuss the relevance of the Gamow-Teller strength distribution at low excitation energy with regard to electron-capture rates us...
The Ni-64(d,He-2)Co-64 reaction was studied at the AGOR cyclotron of KVI, Groningen, with the Big-Bi...
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 ...
Spin-isospin excitations of the medium-mass nucleus Co-58 were studied using the (n, p)-type (d,He-2...
Spin-isospin excitations of the medium-mass nucleus Co-58 were studied using the (n, p)-type (d,He-2...
AbstractSpin–isospin excitations of the medium-mass nucleus 58Co were studied using the (n,p)-type (...
Electron capture and beta decay play important roles in the evolution of presupernovae stars and the...
Electron capture and beta decay play important roles in the evolution of presupernovae stars and the...
Electron capture and beta decay play important roles in the evolution of presupernovae stars and the...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Gamow-Teller (GT) transition is the most popular nuclear weak process with the nature of spin-isospi...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Electron capture and beta decay play important roles in the evolution of pre-supernovae stars and th...
The Ni-64(d,He-2)Co-64 reaction was studied at the AGOR cyclotron of KVI, Groningen, with the Big-Bi...
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 ...
Spin-isospin excitations of the medium-mass nucleus Co-58 were studied using the (n, p)-type (d,He-2...
Spin-isospin excitations of the medium-mass nucleus Co-58 were studied using the (n, p)-type (d,He-2...
AbstractSpin–isospin excitations of the medium-mass nucleus 58Co were studied using the (n,p)-type (...
Electron capture and beta decay play important roles in the evolution of presupernovae stars and the...
Electron capture and beta decay play important roles in the evolution of presupernovae stars and the...
Electron capture and beta decay play important roles in the evolution of presupernovae stars and the...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Gamow-Teller (GT) transition is the most popular nuclear weak process with the nature of spin-isospi...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Gamow-Teller transitions in fp-shell nuclei have been studied using the Ni-58(d, He-2) charge exchan...
Electron capture and beta decay play important roles in the evolution of pre-supernovae stars and th...
The Ni-64(d,He-2)Co-64 reaction was studied at the AGOR cyclotron of KVI, Groningen, with the Big-Bi...
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 ...