Decay of Ce144 and Pr144
R. L. Hickok, William A. McKinley, S. C. Fultz
Abstract
R. L. Hickok, William A. McKinley, S. C. Fultz
Abstract
The beta and gamma spectra from the decay of ${\mathrm{Ce}}^{144}$ and ${\mathrm{Pr}}^{144}$ have been investigated by means of a magnetic-lens beta spectrometer and single-channel scintillation spectrometers. Three partial beta spectra with end-point energies and relative intensities of 184 kev (30%), 245 kev (5%), and 320 kev (65%) were observed for ${\mathrm{Ce}}^{144}$. Gamma rays and internal conversion lines corresponding to 54, 80, and 134-kev transitions were also detected. Internal conversion coefficients indicate an $M1$ multipolarity for the 80- and 134-kev transitions. ${\mathrm{Pr}}^{144}$ yields three partial beta spectra with end-point energies and relative intensities of 0.90 Mev (2%), 2.45 Mev (3%), and 3.15 Mev (95%). Corresponding gamma rays were also detected. Beta-gamma and gamma-gamma coincidence measurements substantiate the proposed decay scheme.
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The beta and gamma spectra from the decay of ${\mathrm{Ce}}^{144}$ and ${\mathrm{Pr}}^{144}$ have been investigated by means of a magnetic-lens beta spectrometer and single-channel scintillation spectrometers. Three partial beta spectra with end-point energies and relative intensities of 184 kev (30%), 245 kev (5%), and 320 kev (65%) were observed for ${\mathrm{Ce}}^{144}$. Gamma rays and internal conversion lines corresponding to 54, 80, and 134-kev transitions were also detected. Internal conversion coefficients indicate an $M1$ multipolarity for the 80- and 134-kev transitions. ${\mathrm{Pr}}^{144}$ yields three partial beta spectra with end-point energies and relative intensities of 0.90 Mev (2%), 2.45 Mev (3%), and 3.15 Mev (95%). Corresponding gamma rays were also detected. Beta-gamma and gamma-gamma coincidence measurements substantiate the proposed decay scheme.
Key concepts: Physics, Spectral line, Atomic physics, Analytical Chemistry (journal), Chemistry, Astronomy, Chromatography