1997
DOI: 10.1016/s0370-2693(97)00077-4
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Collectivity in 44S

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Cited by 247 publications
(202 citation statements)
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“…The efficiencies of the ␤ and ␥ detectors were measured using 45,46 Ar, [23][24][25][26] Ne, 90 Kr sources collected on line, corresponding to a broad energy range of emitted ␥ rays. The detection efficiency for ␤ particles was measured by comparing singles and ␤-gated Ge spectra and was found to be 35(4)%.…”
Section: A Experimentsmentioning
confidence: 99%
“…The efficiencies of the ␤ and ␥ detectors were measured using 45,46 Ar, [23][24][25][26] Ne, 90 Kr sources collected on line, corresponding to a broad energy range of emitted ␥ rays. The detection efficiency for ␤ particles was measured by comparing singles and ␤-gated Ge spectra and was found to be 35(4)%.…”
Section: A Experimentsmentioning
confidence: 99%
“…Evidence for a breakdown of the traditional N = 28 magic number resulted from the pioneering observation of low-lying quadrupole collectivity in 44 S [1,2] and fueled the field of rare-isotope science in the quest to unravel the origin of shell and shape evolution in exotic nuclei with experimental programs worldwide.…”
Section: Introductionmentioning
confidence: 99%
“…The N = 28 shell closure in neutron-rich Si and S isotopes has received considerable experimental [4][5][6][7][8][9][10][11][12][13] and theoretical attention [14][15][16][17][18][19][20][21][22][23]. Experimental data [5,6,[8][9][10][11] indicate gradual quenching of the N = 28 shell gap toward neutron-rich isotones and the onset of deformation in N ≈ 28 S and Si isotopes. Unlike the case of smaller magic numbers, the neutron single-particle levels f 7/2 and p 3/2 that compose the N = 28 shell gap belong to the same major shell in the absence of spin-orbit splitting, and their angular momentum differs by 2.…”
mentioning
confidence: 99%