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- W2265924852 abstract "The disintegration of ${mathrm{Ho}}^{166}$ (27.3 hr) has been studied by scintillation counter coincidence techniques. Gamma rays of 1.53 Mev and 1.61 Mev are present in low intensity, in addition to the previously identified 80-kev and 1.36-Mev transitions. Both the 1.36-Mev and the 1.53-Mev gamma rays are in coincidence with the 80-kev transition. For the 80-kev $E2$ transition the $K$-conversion coefficient has been measured as 1.9ifmmodepmelsetextpmfi{}0.2 and the total conversion coefficient as 7.6ifmmodepmelsetextpmfi{}1.5. The $ensuremath{beta}$ branching has been determined from $ensuremath{beta}ensuremath{-}ensuremath{gamma}$ and $ensuremath{gamma}ensuremath{-}ensuremath{gamma}$ coincidence measurements and by a comparison of the $ensuremath{beta}ensuremath{-}ensuremath{gamma}$ coincidences with ${mathrm{Tm}}^{170}$. The results indicate a ground state branch of ensuremath{sim}25 percent, a branch of ensuremath{sim}74 percent to the 80-kev state, a branch of ensuremath{sim}1 percent to a state at 1.44 Mev and a branch of ensuremath{sim}0.3 percent to a state at 1.61 Mev in ${mathrm{Er}}^{166}$. The spin of ${mathrm{Ho}}^{166}$ is probably 2-." @default.
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- W2265924852 date "1954-03-15" @default.
- W2265924852 modified "2023-09-27" @default.
- W2265924852 title "The Decay ofHo166" @default.
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- W2265924852 doi "https://doi.org/10.1103/physrev.93.1345" @default.
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