2008
DOI: 10.1103/physrevc.78.024302
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Spectroscopy of neutron-richMn5963isotopes

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Cited by 51 publications
(35 citation statements)
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“…[23] may be evidence for β-delayed neutron decay of the 62 Cr ground state. It is worth noting that the in-beam γ -ray spectra for 61 Mn and 62 Mn obtained by Valiente-Dobón et al [22] include transitions of energies 157 and 155 keV, respectively, supporting the present assignment of the 157-keV γ -ray transition in Fig. 4 to the decay of 61 Cr.…”
Section: Resultssupporting
confidence: 89%
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“…[23] may be evidence for β-delayed neutron decay of the 62 Cr ground state. It is worth noting that the in-beam γ -ray spectra for 61 Mn and 62 Mn obtained by Valiente-Dobón et al [22] include transitions of energies 157 and 155 keV, respectively, supporting the present assignment of the 157-keV γ -ray transition in Fig. 4 to the decay of 61 Cr.…”
Section: Resultssupporting
confidence: 89%
“…It is likely that the 1142-keV state has low spin, either J π = 1/2 − or J π = 3/2 − . The level at 1142 keV is apparently weakly fed by β decay, was not identified in the yrast structure of 61 Mn [22], and does not depopulate to the 7/2 − level at 157 keV within the statistical certainty of this measurement. The 1497-keV level is tentatively assigned a J π of 3/2 − or 5/2 − because of the apparent allowed β-decay branch and the favorable competition between the two depopulating γ rays that suggests both transitions have M1 multipolarity.…”
Section: Resultsmentioning
confidence: 49%
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“…This latter model space is also good enough to account for the spectroscopy of moderately neutron-rich Mn [37] isotopes. However, when approaching N = 40 these fpg calculations fail to describe the structure of neutron-rich nuclei, in particular, [60][61][62] Cr [6,8,38] and 66 Fe [23].…”
Section: A Shell Model Valence Space and Effective Interactionmentioning
confidence: 99%