Masses of neutron-rich Sc 52-54 and Ti 54,56 nuclides: The N=32 subshell closure in scandium
Masses of neutron-rich Sc 52-54 and Ti 54,56 nuclides: The N=32 subshell closure in scandium
复制标题
富中子 Sc 52-54 和 Ti 54,56 核素的质量:钪中的 N=32 亚壳闭合
DOI:
10.1103/physrevc.99.064303
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发表时间:
2019
影响因子:
3.1
通讯作者:
Sun B.H.
中科院分区:
文献类型:
--
作者:
Xu X.;Wang M.;Blaum K.;Holt J.D.;Litvinov Yu.A.;Schwenk A.;Simonis J.;Stroberg S.R.;Zhang Y.H.;Xu H.S.;Shuai P.;Tu X.L.;Zhou X.H.;Xu F.R.;Audi G.;Chen R.J.;Chen X.C.;Fu C.Y.;Ge Z.;Huang W.J.;Litvinov S.;Liu D.W.;Lam Y.H.;Ma X.W.;Mao R.S.;Ozawa A.;Sun B.H.
Isochronous mass spectrometry has been applied in the storage ring CSRe to measure the masses of the neutron-richandnuclei. The new mass excess valueskeV,keV, andkeV, deviate from the Atomic Mass Evaluation 2012 by, and, respectively. These large deviations significantly change the systematics of the two-neutron separation energies of scandium isotopes. The empirical shell gap extracted from our new experimental results shows a significant subshell closure atin scandium, with a similar magnitude as in calcium. Moreover, we presentab initiocalculations using the valence-space in-medium similarity renormalization group based on two- and three-nucleon interactions from chiral effective field theory. The theoretical results confirm the existence of a substantialshell gap in Sc and Ca with a decreasing trend towards lighter isotones, thus providing a consistent picture of the evolution of themagic number from theinto theshell.