Study of the N = 32 and N = 34 Shell Gap for Ti and V by the First High-Precision Multireflection Time-of-Flight Mass Measurements at BigRIPS-SLOWRI
Study of the N = 32 and N = 34 Shell Gap for Ti and V by the First High-Precision Multireflection Time-of-Flight Mass Measurements at BigRIPS-SLOWRI
复制标题
通过 BigRIPS-SLOWRI 首次高精度多重反射飞行时间质量测量研究 Ti 和 V 的 N = 32 和 N = 34 壳间隙
DOI:
10.1103/physrevlett.130.012501
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发表时间:
2023
影响因子:
8.6
通讯作者:
Ni
中科院分区:
文献类型:
--
作者:
Iimura S.;Rosenbusch M.;Takamine A.;Tsunoda Y.;Wada M.;Chen S.;Hou D.S.;Xian W.;Ishiyama H.;Yan S.;Schury P.;Crawford H.;Doornenbal P.;Hirayama Y.;Ito Y.;Kimura S.;Koiwai T.;Kojima T.M.;Koura H.;Lee J.;Liu J.;Michimasa S.;Miyatake H.;Moon J.Y.;Naimi S.;Ni
The atomic masses of,, andhave been determined using the high-precision multireflection time-of-flight technique. The radioisotopes have been produced at RIKEN’s Radioactive Isotope Beam Factory (RIBF) and delivered to the novel designed gas cell and multireflection system, which has been recently commissioned downstream of the ZeroDegree spectrometer following the BigRIPS separator. Forand, the mass uncertainties have been reduced down to the order of 10 keV, shedding new light on theshell effect in Ti and V isotopes by the first high-precision mass measurements of the critical speciesand. With the new precision achieved, we reveal the nonexistence of theempirical two-neutron shell gaps for Ti and V, and the enhanced energy gap above the occupiedorbit is identified as a feature unique to Ca. We perform new Monte Carlo shell model calculations including theandorbits and compare the results with conventional shell model calculations, which exclude theand theorbits. The comparison indicates that the shell gap reduction in Ti is related to a partial occupation of the higher orbitals for the outer two valence neutrons at.