6533b821fe1ef96bd127bf96

RESEARCH PRODUCT

Measurement of lifetimes in Fe-62,Fe-64, Co-61,Co-63, and Mn-59

M. KlintefjordJ. LjungvallA. GörgenS. M. LenziF. L. Bello GarroteA. BlazhevE. ClémentG. De FranceJ.-p. DelarocheP. DésesquellesA. DewaldD. T. DohertyC. FransenA. GengelbachG. GeorgievM. GirodEnrique Sanchis PerisA. GottardoAndrés Gadea RagaVicente González MillánJ. J. Valiente DobónD. MengoniT. KonstantinopoulosA. KorichiA. LemassonJ. LibertA. Lopez-martensC. MichelagnoliA. NavinJ. NybergR. M. Pérez-vidalS. RocciaE. SahinI. StefanA. E. StuchberyR. MenegazzoF. RecchiaD. BarrientosB. BirkenbachA. Boston

subject

Electromagnetisme MesuramentsFísica nuclear

description

Lifetimes of the 4(1)(+) states in Fe-62,Fe-64 and the 11/2(1)(-) states in Co-61,Co-63 and Mn-59 were measured at the Grand Accelerateur National d'Ions Lourds (GANIL) facility by using the Advanced Gamma Tracking Array (AGATA) and the large-acceptance variable mode spectrometer (VAMOS++). The states were populated through multinucleon transfer reactions with a U-238 beam impinging on a Ni-64 target, and lifetimes in the picosecond range were measured by using the recoil distance Doppler shift method. The data show an increase of collectivity in the iron isotopes approaching N = 40. The reduction of the subshell gap between the nu 2p(1/2) and nu 1g(9/2) orbitals leads to an increased population of the quasi-SU(3) pair (nu 1g(9/2), nu 2d(5/2)), which causes an increase in quadrupole collectivity. This is not observed for the cobalt isotopes withN < 40 for which the neutron subshell gap is larger due to the repulsive monopole component of the tensor nucleon-nucleon interaction. The extracted experimental B(E2) values are compared with large-scale shell-model calculations and with beyond-mean-field calculations with the Gogny D1S interaction. A good agreement between calculations and experimental values is found, and the results demonstrate in particular the spectroscopic quality of the Lenzi, Nowacki, Poves, and Sieja (LNPS) shell-model interaction.

10.1103/physrevc.95.024312http://hdl.handle.net/10550/65850