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- W2010599688 abstract "The energy levels of 90Nb populated by the decay of 5.7 h 90Mo have been studied with the use of high-resolution germanium γ-ray spectrometers. The γ-ray spectrum revealed a number of low-intensity transitions in addition to the intense 122 and 257 keV lines. The multipolarities of most of these transitions were determined by means of K-shell conversion coefficients, which were calculated from the photon intensities measured in this work together with previously reported conversion electron intensities. In addition, coincidence relationships among the more intense transitions were studied with γγ coincidence systems using Ge(Li)Ge(Li) and Ge(Li)NaI(Tl) detectors. These and previously reported data have been used to construct a decay scheme in which all of the transitions of greater than 1 % intensity are placed. The low-energy transition depopulating the 24 sec isomeric state has not been observed directly, but from lifetime considerations its multipolarity is interpreted as M2, and from energy differences its energy is inferred as 2.38 ± 0.36 keV." @default.
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- W2010599688 date "1968-03-01" @default.
- W2010599688 modified "2023-09-30" @default.
- W2010599688 title "Energy levels of 90Nb populated by the decay of 90Mo" @default.
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- W2010599688 doi "https://doi.org/10.1016/0375-9474(68)90031-6" @default.
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