By using Yb of high purity (99.8%) irradiated in the maximum flux of the Argonne pile and studied by scintillation and magnetic photographic spectrometers, a reevaluation of the energies of the radiations has been made. Several previously unreported gamma rays are found and nuclear level schemes for Tm¹⁶⁹, Lu¹⁷⁵, and Lu¹⁷⁷ are proposed. Several of the levels appear to be rotational states in the unified nuclear model. Yb¹⁶⁹ decays with a half-life of 30.6 days by K capture, followed by eleven gamma rays in Tm¹⁶⁹. Rotational levels lie at 8.4, 118.3, and 139.1 kev. The gamma energies are 8.4, 20.6, 63.2, 93.6, 109.9, 118.3, 130.7, 177.7, 198.6, 261.0, and 308.3 kev. Yb¹⁷⁵ decays with a half-life of 4.2 days by β emission (471 kev max) followed by five gamma rays in Lu¹⁷⁵. Rotational levels exist at 114.1, and 251.9 kev. The gamma energies are 114.1, 137.8, 145.0, 282.9, and 397.0 kev. Yb¹⁷⁷ decays with a half-life of 1.88 hour by β emission followed by gamma transitions in Lu¹⁷⁷. In addition to any lower energy gamma rays, two high-energy transitions are found at 1.080 and 1.228 Mev. The latter is a cross over for the 1.080- and 0.148-Mev gammas which are in coincidence. The expected well-known daughter product Lu¹⁷⁷, if present at all, is too weak to be observed by the magnetic spectrometers.
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Cork et al. (1956) studied this question.
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