Decay of Ta177 and Lu177 to Levels in Hf177

H. I. West, Jr., L. G. Mann, and R. J. Nagle
Phys. Rev. 124, 527 – Published 15 October 1961
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Abstract

The decays of Ta177 and Lu177 to levels in Hf177 have been investigated with beta-ray spectrometers, NaI(Tl) gamma-ray spectrometers, and fast coincidence and angular correlation techniques. Energy levels in Hf177 have been characterized according to their energy (kev), the Nilsson asymptotic quantum numbers (NnzΛ), the total angular momentum and its component along the symmetry axis (I, K), and the parity (π) as follows: 0[514 72, 72]; 112.97[514 92, 72]; 249.7[514 112, 72]; 321.34[624 92, 92+]; 447.9[624 112, 92+]; 420.95[642 32, 32+]; 488.8[642 52, 32+]; 585.8[642 72, 32+]; 509.0[512 52, 52]; 605.5[512 72, 52]; 746.04[633 72, 72+]; 848.2[633 92, 72+]; and 1058.38[503 72, 72]. The levels at 447.9, 488.8, and 585.8 kev are tentative. The spins and parities have been uniquely determined by angular correlation and internal conversion data for the levels at 746.0 and 848.2 kev, if we assume the spins and parities of the levels at 0, 113.0, 249.7, and 321.3 kev are correct as determined from earlier work. For the level at 1058.4 kev the ft value is needed in addition to angular correlation and conversion data in order to determine the spin and parity uniquely. The spins of Lu177 and Hf177 have previously been measured directly as 72, and the Ta177 spin is expected to be 72 on the basis of other tantalum isotopes. The following half-lives were measured: 56.56 hr for Ta177, 0.32 nsec for the level at 113.0 kev, and 0.52 nsec for the level at 321.3 kev. The KL electron capture ratio to the 1058.4-kev level and the β+K-capture ratio to the ground state determine the total decay energy to be 1166±6 kev.

  • Received 24 March 1961

DOI:https://doi.org/10.1103/PhysRev.124.527

©1961 American Physical Society

Authors & Affiliations

H. I. West, Jr., L. G. Mann, and R. J. Nagle

  • Lawrence Radiation Laboratory, University of California, Livermore, California

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Issue

Vol. 124, Iss. 2 — October 1961

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