Nuclear shape and structure in neutron-rich Tc110,111

Y. X. Luo, J. H. Hamilton, J. O. Rasmussen, A. V. Ramayya, I. Stefanescu, J. K. Hwang, X. L. Che, S. J. Zhu, P. M. Gore, E. F. Jones, D. Fong, S. C. Wu, I. Y. Lee, T. N. Ginter, W. C. Ma, G. M. Ter-Akopian, A. V. Daniel, M. A. Stoyer, R. Donangelo, and A. Gelberg
Phys. Rev. C 74, 024308 – Published 18 August 2006

Abstract

The high-spin nuclear structure of Tc isotopes is extended to more neutron-rich regions based on the measurements of prompt γ rays from the spontaneous fission of Cf252 at the Gammasphere. The high-spin level scheme of N=67 neutron-rich Tc110 (Z=43) is established for the first time, and that of Tc111 is extended and expanded. The ground band of Tc111 reaches the band-crossing region, and the new observation of the weakly populated α=1/2 member of the band provides important information on signature splitting. The systematics of band crossings in the isotopic and isotonic chains and a CSM calculation suggest that the band crossing of the ground band of Tc111 is due to alignment of a pair of h11/2 neutrons. The best fit to signature splitting, branching ratios, and excitations of the ground band of Tc111 by the rigid triaxial rotor plus particle model calculations result in a shape of ɛ2=0.32 and γ=26° for this nucleus. Its triaxiality is larger than that of Tc107,109, which indicates increasing triaxiality in Tc isotopes with increasing neutron number. The identification of the weakly populated K+2 satellite band provides strong evidence for the large triaxiality of Tc111. In Tc110, the four lowest-lying levels observed are very similar to those in Tc108. At an excitation of 478.9 keV above the lowest state observed, ten states of a ΔI=1 band are observed. This band of Tc110 is very analogous to the ΔI=1 bands in Tc106,108, but it has greater and reversal signature splitting at higher spins.

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  • Received 27 February 2006

DOI:https://doi.org/10.1103/PhysRevC.74.024308

©2006 American Physical Society

Authors & Affiliations

Y. X. Luo1,2, J. H. Hamilton1, J. O. Rasmussen2, A. V. Ramayya1, I. Stefanescu3, J. K. Hwang1, X. L. Che4, S. J. Zhu1,4,5, P. M. Gore1, E. F. Jones1, D. Fong1, S. C. Wu6, I. Y. Lee2, T. N. Ginter2,7, W. C. Ma8, G. M. Ter-Akopian9, A. V. Daniel9, M. A. Stoyer10, R. Donangelo11, and A. Gelberg12

  • 1Physics Department, Vanderbilt University, Nashville, Tennessee 37235, USA
  • 2Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 3KU Leuven, Instituut voor Kern- en Stralingsfysica, Celestijnenlaan 200D, B-3001 Leuven, Belgium
  • 4Physics Department, Tsinghua University, Beijing 100084, China
  • 5Joint Institute for Heavy Ion Research, Oak Ridge, Tennessee 37831, USA
  • 6Department of Physics, National Tsing Hua University, Hsinchu, Taiwan
  • 7National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
  • 8Mississippi State University, Drawer 5167, Mississippi State, Mississippi 39762, USA
  • 9Flerov Laboratory for Nuclear Reactions, JINR, Dubna, Russia
  • 10Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 11Universidade Federal do Rio de Janeiro, CP 68528, RG Brazil
  • 12Institut für Kernphysik, Universität zu Köln, D-50937, Köln, Germany

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Vol. 74, Iss. 2 — August 2006

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