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- W2331083485 abstract "The rest mass of ${mathrm{O}}^{17}$ is calculated from the known rest masses of ${mathrm{N}}^{14}$, ${mathrm{He}}^{4}$, and ${mathrm{H}}^{1}$ and the masses due to the kinetic energies of ${mathrm{He}}^{4}$, ${mathrm{H}}^{1}$, and ${mathrm{O}}^{17}$ as determined by Blackett and Harkins in the transmutation reaction ${mathrm{N}}^{14}$+${mathrm{He}}^{4}$ensuremath{rightarrow}${mathrm{O}}^{17}$+${mathrm{H}}^{1}$. The only assumptions involved are that the conservation of momentum and of mass-energy holds in these reactions. The masses secured in this way from seven sets of data do not agree within the probable limits of error for the experimental data. It is suggested that this is due either to the formation of ${mathrm{O}}^{17}$ atoms of different masses and energies in this reaction or to the emission of gamma-rays during the collision. The former of these predicts discontinuous energy levels while the latter would probably cause the rest mass of ${mathrm{O}}^{17}$ as calculated here to vary continuously. The relation of this calculation to the experiments of Bothe and Pose on the ranges of H particles from boron and aluminum is discussed." @default.
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- W2331083485 date "1931-04-15" @default.
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- W2331083485 title "The Masses ofO17" @default.
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- W2331083485 doi "https://doi.org/10.1103/physrev.37.923" @default.
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