γ-ray spectroscopy of neutron-deficient<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Te</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>110</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>. I. Low- and intermediate-spin structures
E. S. PaulOliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United KingdomA. J. BostonOliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United KingdomC. J. ChiaraDepartment of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USAM. DevlinDepartment of Chemistry, Washington University, St. Louis, Missouri 63130, USAD. B. FossanDepartment of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USAS. J. FreemanSchuster Laboratory, University of Manchester, Brunswick Street, Manchester M13 9PL, United KingdomD. R. LaFosseDepartment of Chemistry, Washington University, St. Louis, Missouri 63130, USAG. J. LaneDepartment of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USAM. J. LeddySchuster Laboratory, University of Manchester, Brunswick Street, Manchester M13 9PL, United KingdomI. Y. LeeNuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USAA. O. MacchiavelliNuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USAP. J. NolanOliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United KingdomD. G. SarantitesDepartment of Chemistry, Washington University, St. Louis, Missouri 63130, USAJ. M. SearsDepartment of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USAA. T. SempleOliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United KingdomJ. F. SmithStony Brook UniversityK. StarostaDepartment of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USA
ABI
Abstract
Excited states have been populated in ${}_{52}^{110}\text{Te}$ via the $^{58}\mathrm{Ni}$($^{58}\mathrm{Ni}$,$\ensuremath{\alpha}2p\ensuremath{\gamma}$) reaction at 250 MeV. The Gammasphere \ensuremath{\gamma}-ray spectrometer was augmented with ancillary detectors for charged-particle and neutron detection in order to provide clean channel selection. The known level scheme of $^{110}\mathrm{Te}$ has been greatly expanded with the addition of many new structures. Above spin ${8}^{+}$, negative-parity structures become yrast. The level scheme of $^{110}\mathrm{Te}$ below $30\ensuremath{\hbar}$ is discussed in this paper, including possible evidence for octupole correlations inferred from strong $B(E1)$ strengths.
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