1972
DOI: 10.1016/0375-9474(72)90501-5
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High-spin levels in 95Mo and 97Mo from (α, xn) reactions

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Cited by 36 publications
(12 citation statements)
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“…It is also observed to be directly populated in our (d,p) study. A 253-keV γ-ray with intensity of 32(32)% has been reported to originate from this 1073-keV level [39], but this transition could not be observed in our measurement.…”
Section: Level: 1073 Kevcontrasting
confidence: 85%
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“…It is also observed to be directly populated in our (d,p) study. A 253-keV γ-ray with intensity of 32(32)% has been reported to originate from this 1073-keV level [39], but this transition could not be observed in our measurement.…”
Section: Level: 1073 Kevcontrasting
confidence: 85%
“…However, based on our observation, which is also corroborated by Ref. [39], the 1888.5-keV level has been either misplaced or mislabelled. The correct level energy is 1880 keV.…”
Section: Level: 1676 Kevsupporting
confidence: 83%
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“…Most of the γ rays reported in the literature [4][5][6][7]9] have been observed in this experiment. The γ -ray coincidence relationships and their ADO ratios have been analyzed with care, leading to the establishment of the revised level schemes for 94,94 Mo that significantly differ from the previous work.…”
Section: Resultsmentioning
confidence: 52%
“…The high-spin states of 94,95 Mo were investigated a long time ago by Lederer et al [5,6] and Mesko et al [7] via (α, xnγ ) reactions. The level schemes have been extended up to I ∼19 at 12 MeV excitation energy by Kharraja and coworkers [4] using heavy-ion-induced fusion-evaporation reactions and the early implementation phase of the Gammasphere array.…”
Section: Introductionmentioning
confidence: 99%