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Masses of neutron-rich Sc52–54 and Ti54,56 nuclides: The N=32 subshell closure in scandium

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Isochronous mass spectrometry has been applied in the storage ring CSRe to measure the masses of the neutron-rich Sc52–54 and Ti54,56 nuclei. The new mass excess values ME(Sc52)=−40525(65) keV, ME(Sc53)=−38910(80)… Click to show full abstract

Isochronous mass spectrometry has been applied in the storage ring CSRe to measure the masses of the neutron-rich Sc52–54 and Ti54,56 nuclei. The new mass excess values ME(Sc52)=−40525(65) keV, ME(Sc53)=−38910(80) keV, and ME(Sc54)=−34485(360) keV, deviate from the Atomic Mass Evaluation 2012 by 2.3σ, 2.8σ, and 1.7σ, 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 at N=32 in scandium, with a similar magnitude as in calcium. Moreover, we present ab initio calculations 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 substantial N=32 shell gap in Sc and Ca with a decreasing trend towards lighter isotones, thus providing a consistent picture of the evolution of the N=32 magic number from the pf into the sd shell.

Keywords: sc52 ti54; masses neutron; rich sc52; neutron rich; subshell closure; closure scandium

Journal Title: Physical Review C
Year Published: 2019

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