Abstract
The electron capture of ${\mathrm{Lu}}^{173}$ (1.30 yr) to levels in ${\mathrm{Yb}}^{173}$ has been investigated using scintillation spectrometers and permanent magnet spectrographs. Levels in ${\mathrm{Yb}}^{173}$ were observed at 78.7 ($\frac{7}{2}\ensuremath{-}$), 179.5 ($\frac{9}{2}\ensuremath{-}$), 351.2 ($\frac{7}{2}+$), and 636.8 ($\frac{7}{2}\ensuremath{-}$) kev. The first two excited states may be interpreted as members of a rotational band based on theg round state [(512) $\frac{5}{2}\ensuremath{-}$]. The levels at 351 and 637 kev are probably the intrinsic levels [(633) $\frac{7}{2}+$] and [(514) $\frac{7}{2}\ensuremath{-}$], respectively, predicted by Nilsson. $L$ electron capture was observed to be the primary mode of population of the 637-kev level. Relative reduced transition probabilities were obtained for all transitions to the ground-state rotational band, and comparisons with theoretical branching ratios were made. $\mathrm{Log}(\mathrm{ft})$ values were estimated from the observed $K$-capture branching ratios.
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