Abstract
Cs129(T1/2=32 h) and Cs130(T1/2=30 min) were produced by J127(α,2n)Cs129and J127(α,n)Cs130reactions, respectively. The γ-ray-spectra from the decays of Cs129 and Cs130 have been investigated using Li-drifted Ge-counters and scintillation spectrometers. In the decay of Cs12915 γ-rays have been observed having the following energies and relative intensities: 95 keV (1.6), 177 keV (1.1), 267 keV (1.7), 278 keV (4.8), 317 keV (7.6), 371 keV (100), 410 keV (69), 511 keV (≦ 0.1), 548 keV (10.5), 587 keV (1.7), 623 keV (0.12), 660 keV (0.07), 864 keV (0.09), 907 keV (0.67) and 948 keV (0.2). The electron capture branching ratios to the ground state and excited states of Xe129were determined; logft values for the various decay branches were derived from these ratios. In the decay of Cs130twoγ-transitions with the following energies and intensities relative to the β+ emission have been found: 535 keV (11) and 585 keV (1.3). A new level at 1122 keV in Xe130is proposed.
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Dem Niedersächsischen Kultusministerium und dem Bundesministerium für wissenschaftliche Forschung gebührt Dank für zusätzliche Mittel.
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Gföller, D., Flammersfeld, A. Der Zerfall der Cäsiumisotope Cs129 und Cs130 . Z. Physik 194, 239–247 (1966). https://doi.org/10.1007/BF01571248
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DOI: https://doi.org/10.1007/BF01571248