γ rays from neutron-rich Ti nuclei in the vicinity of N = 32 have been studied at Gammasphere using deep-inelastic reactions induced by 48 Ca beams on thick 208 Pb and 238 U targets. The 53 Ti yrast cascade was identified for the first time, and the location in energy of states with spin up to I = 21/2 was determined. The excitations of 53 Ti provide new tests of effective interactions for full- pf -shell calculations. Comparisons between theory and experiment for the highest spin states in 53 Ti favor the recently proposed GXPF1A interaction, which accounts for the appearance of a neutron subshell closure at N = 32 in Ti isotopes as well as for the lack of a similar subshell closure at N = 34, as predicted by earlier cal...
Gamma rays from 52 Ti have been studied with Gammasphere and the Fragment Mass Analyzer using reacti...
Recent experimental characterization of the subshell closure at N 32 in the Ca, Ti, and Cr isotones...
γ rays in the πν-1 nucleus 208Bi have been studied at the Gammasphere using deep-inelastic reactions...
γ rays from neutron-rich Ti nuclei in the vicinity of N = 32 have been studied at Gamma...
\u3b3 rays from neutron-rich Ti nuclei in the vicinity of N=32 have been studied at Gammasphere usin...
Gamma rays from neutron-rich Ti nuclei in the vicinity of N = 32 have been studied at Gammasphere us...
Gamma rays from neutron-rich nuclei in the vicinity of Z = 20, N = 28 have been studied at Gammasphe...
Gamma rays from 52 Ti have been studied with Gammasphere and the Fragment Mass Analyzer using reacti...
The level structures of 55 Vand 55 Ti, the two nuclei with a single nucleon outside the semi-magic 5...
The level structure of Ti-54(22)32 has been explored for the first time by combining P-decay measure...
The even 52 – 56 Ti isotopes have been studied with intermediate-energy Coulomb excitation ...
My project clarifies previous measurements made for the high excitation states of titanium isotopes,...
The low-lying yrast states in the 51 Ca and 52 Sc nuclei were investigated to obtain information on ...
The isomeric and β-decay properties of neutron-rich Sc53-57 and Ca53,54 nuclei near neutron number N...
The even 52 – 56 Ti isotopes have been studied with intermediate-energy Coulomb excitation ...
Gamma rays from 52 Ti have been studied with Gammasphere and the Fragment Mass Analyzer using reacti...
Recent experimental characterization of the subshell closure at N 32 in the Ca, Ti, and Cr isotones...
γ rays in the πν-1 nucleus 208Bi have been studied at the Gammasphere using deep-inelastic reactions...
γ rays from neutron-rich Ti nuclei in the vicinity of N = 32 have been studied at Gamma...
\u3b3 rays from neutron-rich Ti nuclei in the vicinity of N=32 have been studied at Gammasphere usin...
Gamma rays from neutron-rich Ti nuclei in the vicinity of N = 32 have been studied at Gammasphere us...
Gamma rays from neutron-rich nuclei in the vicinity of Z = 20, N = 28 have been studied at Gammasphe...
Gamma rays from 52 Ti have been studied with Gammasphere and the Fragment Mass Analyzer using reacti...
The level structures of 55 Vand 55 Ti, the two nuclei with a single nucleon outside the semi-magic 5...
The level structure of Ti-54(22)32 has been explored for the first time by combining P-decay measure...
The even 52 – 56 Ti isotopes have been studied with intermediate-energy Coulomb excitation ...
My project clarifies previous measurements made for the high excitation states of titanium isotopes,...
The low-lying yrast states in the 51 Ca and 52 Sc nuclei were investigated to obtain information on ...
The isomeric and β-decay properties of neutron-rich Sc53-57 and Ca53,54 nuclei near neutron number N...
The even 52 – 56 Ti isotopes have been studied with intermediate-energy Coulomb excitation ...
Gamma rays from 52 Ti have been studied with Gammasphere and the Fragment Mass Analyzer using reacti...
Recent experimental characterization of the subshell closure at N 32 in the Ca, Ti, and Cr isotones...
γ rays in the πν-1 nucleus 208Bi have been studied at the Gammasphere using deep-inelastic reactions...