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Identification of a new isomeric state in <sup>76</sup>Zn following the β decay of <sup>76</sup>Cu

ORAL

Abstract

Shell evolution far from stability can be explored by measuring the properties of isomeric states, which provide a sensitive probe of the microscopic structure of the nucleus. Beta decay is an attractive method for isomer identification because daughter nuclei can be populated in an excited state which subsequently decays to the ground state through one or more isomeric transitions. A β-decay experiment was recently performed at the National Superconducting Cyclotron Laboratory (NSCL) to identify and study isomeric states in the vicinity of the doubly magic nucleus 78Ni. Radioactive ions produced by beam fragmentation at the NSCL's Coupled Cyclotron Facility were implanted into a CeBr3 scintillator detector coupled to a position-sensitive photomultiplier tube (PSPMT). Ancillary arrays of HPGe clover and LaBr3 detectors were positioned around the implantation detector to measure β-delayed γ rays. The entire suite of detectors was instrumented with the NSCL Digital Data Acquisition System (DDAS). Dynode traces recorded by DDAS were analyzed to selectively identify isomeric transitions. The previously observed 2634-keV level in 76Zn, populated following the β decay of 76Cu, was identified as isomeric with a half-life of 25.4(4) ns. A combination of timing and γ-ray spectroscopy was used to confirm this assignment. Shell-model calculations were performed which indicate that this state may be a high-spin negative-parity state formed by the occupation of the neutron 0g9/2 orbital. The experimental results and theoretical interpretation will be presented.

Presenters

  • Aaron Chester

    Michigan State University, National Superconducting Cyclotron Laboratory

Authors

  • Aaron Chester

    Michigan State University, National Superconducting Cyclotron Laboratory

  • Alex Brown

    Michigan State University, Michigan State Universtiy, National Superconducting Cyclotron Laboratory; Department of Physics and Astronomy, Michigan State University

  • Michael P Carpenter

    Argonne National Laboratory, ANL

  • James J Carroll

    DEVCOM/Army Research Laboratory

  • C.J. J Chiara

    DEVCOM/Army Research Laboratory, ANL

  • Patrick Copp

    Argonne National Laboratory, Argonne national Laboratory

  • Benjamin P Crider

    Mississippi State Univ, Mississippi State University, Department of Physics and Astronomy, Mississippi State University

  • Jason T Harke

    Lawrence Livermore National Laboratory, Lawrence Livermore Natl Lab

  • Daniel E Hoff

    University of Massachusetts Lowell, Lawrence Livermore National Laboratory

  • Kay Kolos

    Lawrence Livermore Natl Lab, LLNL, Lawrence Livermore National Laboratory

  • Sean N Liddick

    National Superconducting Cyclotron Laboratory, Michigan State University, NSCL/FRIB, NSCL, National Superconducting Cyclotron Laboratory; Department of Chemistry, Michigan State University, Michigan State University, National Superconducting Cyclotron Laboratory; Michigan State University, FRIB

  • Brenden Longfellow

    Lawrence Livermore National Laboratory, Lawrence Livermore Natl Lab

  • Mejdi J Mogannam

    National Superconducting Cyclotron Laboratory; Department of Chemistry, Michigan State University

  • Timilehin H Ogunbeku

    Mississippi State University, Department of Physics and Astronomy, Mississippi State University

  • Andrea L Richard

    Lawrence Livermore Natl Lab, National Superconducting Cyclotron Labor, Lawrence Livermore National Laboratory

  • Olalekan A Shehu

    Department of Physics and Astronomy, Mississippi State University, University of Rhode Island

  • Ronald Unz

    Department of Physics and Astronomy, Mississippi State University

  • Yongchi Xiao

    Department of Chemistry, University of Kentucky, Michigan State University, University of Kentucky