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- W3136131229 abstract "${mathrm{Sc}}^{46}$ and ${mathrm{Ti}}^{51}$ have been prepared in the Clinton pile. The characteristic radiations of these isotopes have been investigated by absorption and coincidence methods.${mathrm{Sc}}^{46}$ was found to emit beta-rays having a range of 0.076 ${mathrm{g}mathrm{r}mathrm{a}mathrm{m}/mathrm{c}mathrm{m}}^{2}$ in aluminum and gamma-rays having a maximum energy of 1.0 Mev as determined by coincidence absorption. No hard beta-rays having an end point in the vicinity of 1.5 Mev were observed to be emitted by ${mathrm{Sc}}^{46}$. The beta-gamma-coincidence rate was found to be ${1.4ifmmodetimeselsetexttimesfi{}10}^{ensuremath{-}3}$ coincidence per beta-particle and independent of the beta-ray energy, while the gamma-gamma-coincidence rate was ${(0.62ifmmodepmelsetextpmfi{}0.06)ifmmodetimeselsetexttimesfi{}10}^{ensuremath{-}3}$ coincidence per gamma-ray. These coincidence rates suggest that each beta-ray is followed by two gamma-rays.The 72-day isomer of ${mathrm{Ti}}^{51}$ emitted beta-rays having a range of 0.09 ${mathrm{g}mathrm{r}mathrm{a}mathrm{m}/mathrm{c}mathrm{m}}^{2}$ in aluminum and gamma-rays having a maximum energy of 1.0 Mev by coincidence absorption. The beta-gamma-coincidence rate was ${0.9ifmmodetimeselsetexttimesfi{}10}^{ensuremath{-}3}$ coincidence per beta-ray and was independent of the beta-ray energy. The gamma-gamma-coincidence rate was ${(0.35ifmmodepmelsetextpmfi{}0.03)ifmmodetimeselsetexttimesfi{}10}^{ensuremath{-}3}$ coincidence per gamma-ray. These coincidence rates indicate that the beta-transition leads to an excited state of the ${mathrm{V}}^{51}$ residual nucleus and that some or all of the residual nuclei de-excite with the emission of two or more gamma-rays in cascade." @default.
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- W3136131229 date "1948-01-15" @default.
- W3136131229 modified "2023-10-17" @default.
- W3136131229 title "Radiations fromScandium46andTitanium51" @default.
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- W3136131229 doi "https://doi.org/10.1103/physrev.73.141" @default.
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