Shape transitions in neutron-rich Ru isotopes: spectroscopy of 109,110,111,112Ru

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The spectroscopy of neutron-rich {sup 109,110,111,112}Ru nuclei was studied by measuring the prompt {gamma} rays originated from fission fragments, produced by the {sup 238}U({alpha},f) fusion-fission reaction, in coincidence with the detection of both fragments. For {sup 109,111}Ru, both the negative-parity (h{sub 11/2} orbitals) and positive-parity (g{sub 7/2} and/or d{sub 5/2} orbitals) bands were extended to substantially higher spin and excitation energy than known previously. The ground-state and {gamma}-vibrational bands of {sup 110,112}Ru also were extended to higher spin, allowing observation of the second band crossing at the rotational frequency of {approx}450 keV in {sup 112}Ru, which is {approx}50 keV above ... continued below

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Hua, H; Cline, D; Hayes, A B; Teng, R; Riley, D; Clark, R M et al. June 29, 2005.

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The spectroscopy of neutron-rich {sup 109,110,111,112}Ru nuclei was studied by measuring the prompt {gamma} rays originated from fission fragments, produced by the {sup 238}U({alpha},f) fusion-fission reaction, in coincidence with the detection of both fragments. For {sup 109,111}Ru, both the negative-parity (h{sub 11/2} orbitals) and positive-parity (g{sub 7/2} and/or d{sub 5/2} orbitals) bands were extended to substantially higher spin and excitation energy than known previously. The ground-state and {gamma}-vibrational bands of {sup 110,112}Ru also were extended to higher spin, allowing observation of the second band crossing at the rotational frequency of {approx}450 keV in {sup 112}Ru, which is {approx}50 keV above the first band crossing. At a similar rotational frequency, the first band crossing for the h{sub 11/2} band in {sup 111}Ru was observed, which is absent in {sup 109}Ru. These band crossings most likely are caused by the alignment of the g{sub 9/2} proton pair. This early onset of the band crossing for the aligned {pi}g{sub 9/2} orbitals may be evidence of a triaxial shape transition from prolate to oblate occurring in {sup 111}Ru. The data together with a comparison of cranked shell model predictions are presented.

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  • Journal Name: Physical Review, C (Nuclear Physics); Journal Volume: 73

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  • Report No.: UCRL-JRNL-213850
  • Grant Number: W-7405-ENG-48
  • Office of Scientific & Technical Information Report Number: 884779
  • Archival Resource Key: ark:/67531/metadc892633

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  • June 29, 2005

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  • Sept. 23, 2016, 2:42 p.m.

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  • Dec. 8, 2016, 10:55 p.m.

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Hua, H; Cline, D; Hayes, A B; Teng, R; Riley, D; Clark, R M et al. Shape transitions in neutron-rich Ru isotopes: spectroscopy of 109,110,111,112Ru, article, June 29, 2005; Livermore, California. (digital.library.unt.edu/ark:/67531/metadc892633/: accessed June 20, 2018), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.