2016
DOI: 10.1103/physrevlett.116.122502
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Direct Lifetime Measurements of the Excited States inNi72

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Cited by 18 publications
(19 citation statements)
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References 29 publications
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“…This was claimed to indicate a possible weakening of the Z = 28 gap towards 78 Ni. In contrast to this result, recent measurements on 72,74 Ni [28,29] show a reduced B(E2)↑ value for these isotopes, which would corroborate the magic character of the N = 50 and Z = 28 shell gaps. For the N = 50 isotones between Z = 30 and Z = 40, previously reported Coulomb excitation measurements show no indication of a reduction in the N = 50 shell gap at Z = 30 [30,31].…”
Section: Introductioncontrasting
confidence: 52%
See 1 more Smart Citation
“…This was claimed to indicate a possible weakening of the Z = 28 gap towards 78 Ni. In contrast to this result, recent measurements on 72,74 Ni [28,29] show a reduced B(E2)↑ value for these isotopes, which would corroborate the magic character of the N = 50 and Z = 28 shell gaps. For the N = 50 isotones between Z = 30 and Z = 40, previously reported Coulomb excitation measurements show no indication of a reduction in the N = 50 shell gap at Z = 30 [30,31].…”
Section: Introductioncontrasting
confidence: 52%
“…Recent experimental studies have exploited the use of radioactive ion beams to gain a deeper understanding of the structure of nuclei under extreme isospin conditions. One of the most important results achieved is that the shell closures, which give rise to the magic numbers 2,8,20,28,50,82, and 126 near the line of β stability, change with varying number of protons and neutrons [1]. This so-called shell-evolution has been widely studied, in particular on the neutron-rich side of the nuclear chart.…”
Section: Introductionmentioning
confidence: 99%
“…The B(E2; 4 + 1 → 2 + 1 ) value for 72 Ni was measured to be 50(9) e 2 fm 4 in Ref. [23], which indicates that the 4 + 1 state may be mostly of seniority v = 4 (see, also, Fig. 4 in Ref.…”
mentioning
confidence: 91%
“…To fill at least aportion of this gap, we have been systematically studying the vibrational and electronic spectroscopy as wella sp hotochemistry of cyanoacetylene family members. [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17] These moleculesa re one of the most abundanti ns pace and have been detected in variousa stronomical objects includingd ark clouds at Heiles's Cloud 2g roup, particularly TCM-1 and -2, [18][19][20][21][22][23][24][25][26][27] the molecular envelopeo ft he star IRC + 10216, [28,29] the galactic core region of Sgr B2, [20,30] cometH ale-Bopp, [31] and Saturn's moon, Titan. [32][33][34] Several literature reportsa lso hint at their possible prebiotic importance.…”
Section: Introductionmentioning
confidence: 99%