States in Sb126 populated in the β decay of 105-yr Sn126

H. A. Smith, Jr.,, M. E. Bunker, J. W. Starner, C. J. Orth, and K. E. G. Löbner
Phys. Rev. C 13, 387 – Published 1 January 1976
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Abstract

The low-energy level structure of the odd-odd nucleus Sb126 has been investigated by studying the radioactive decay of 105-yr Sn126, using Ge(Li) and Si(Li) detectors. Based on conversion-electron and γ-ray singles data, γγ and γe prompt and delayed coincidence measurements, and complementary γ-ray energy and intensity balance arguments, a decay scheme for Sn126 has been deduced which accommodates all of the observed γ-ray transitions. The energies (keV), spins, and parities of the levels established in Sb126 are as follows: 0.0 [8], 17.7 [5+], 40.4 [3], 83.1 [4, (3)], 104.7 [3+], and 128.0 [2+]. The respective half-lives of these six states are: 12.4 day, 19.0 min, ≅11 s, 5.1 ns, 553 ns, and 78.0 ns, the latter four values having been determined in the present investigation. The level assignments are discussed within the framework of the single-particle shell model and in relation to the proposed assignments of low-lying energy levels of neighboring odd-odd antimony isotopes.

RADIOACTIVITY Sn126 [from U235(n,f)]; measured Eγ, Iγ, Ice, γγ, βγ, and eγ coin, level T12's; deduced ICC, γ multipolarities, Sb126 levels, J, π; calculated γ-hindrance factors. Ge(Li), Si(Li) detectors; mass-separated source.

  • Received 8 September 1975

DOI:https://doi.org/10.1103/PhysRevC.13.387

©1976 American Physical Society

Authors & Affiliations

H. A. Smith, Jr.,*, M. E. Bunker, J. W. Starner, and C. J. Orth

  • University of California, Los Alamos Scientific Laboratory, Los Alamos, New Mexico 87544

K. E. G. Löbner

  • Technical University, Munich, Germany
  • University of California, Los Alamos Scientific Laboratory, Los Alamos, New Mexico 87544

  • *Present address: Department of Physics, Indiana University, Bloomington, Indiana 47401.

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Vol. 13, Iss. 1 — January 1976

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