2015
DOI: 10.1103/physrevlett.114.252501
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Low-Lying Structure ofAr50and theN=32Subshell Closure

Abstract: The low-lying structure of the neutron-rich nucleus (50)Ar has been investigated at the Radioactive Isotope Beam Factory using in-beam γ-ray spectroscopy with (9)Be((54)Ca,(50)Ar+γ)X, (9)Be((55)Sc,(50)Ar+γ)X, and (9)Be((56)Ti,(50)Ar+γ)X multinucleon removal reactions at ∼220  MeV/u. A γ-ray peak at 1178(18) keV is reported and assigned as the transition from the first 2(+) state to the 0(+) ground state. A weaker, tentative line at 1582(38) keV is suggested as the 4(1)(+)→2(1)(+) transition. The experimental r… Show more

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Cited by 55 publications
(47 citation statements)
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“…[20], may influence their excitation energies and strengths. It has been found recently that the N = 32 subshell closure remains intact below the Ca isotopes [54,55] and theory prognoses a steep increase of 2 + 1 energies in Ne and Mg from N = 28 to N = 32 [20]. Owing to the developments in radioactive isotope beam science, measuring the onset of the expected drop in excitation strength may soon become feasible for magnesium isotopes.…”
Section: Discussionmentioning
confidence: 99%
“…[20], may influence their excitation energies and strengths. It has been found recently that the N = 32 subshell closure remains intact below the Ca isotopes [54,55] and theory prognoses a steep increase of 2 + 1 energies in Ne and Mg from N = 28 to N = 32 [20]. Owing to the developments in radioactive isotope beam science, measuring the onset of the expected drop in excitation strength may soon become feasible for magnesium isotopes.…”
Section: Discussionmentioning
confidence: 99%
“…Indeed, recent developments in accelerator technology and isotope separators have made it possible to explore unreached regions of the Segrè chart, yielding many new, exotic phenomena that cannot be explained in the framework of the standard shell model. Several highlights include the weakening of the traditional magic numbers N = 8 [3][4][5], 20 [6], and 28 [7][8][9], while new magic numbers at N = 16 [10,11], 32 [12][13][14][15][16][17][18][19][20], and 34 [21] have been reported. The next conventional neutron magic number, N = 50, has also attracted much attention recently, and investigations into the robustness of this magic number in neutron-rich systems have been encouraged.…”
Section: Introductionmentioning
confidence: 99%
“…Along the proton drip line, 31 Ar was found to exhibit the exotic β3p decay mode [29]. For the neutron-rich even-even isotopes, large-scale shell-model calculations reproduced the measured B(E2) in 48 Ar [30] and 50 Ar [31]-indicating an N = 32 subshell closure analogous to those observed in neighboring Ca and Ti isotopes-while overestimating the collectivity in 46 Ar. This is puzzling, as both B(E2) data from Coulomb excitation [32][33][34] and mass measurements [35] point to a robust N = 28 shell closure for Z = 18.…”
Section: Introductionmentioning
confidence: 58%