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Level Densities and Gamma-Ray Strengths Inferred from Ground and Isomeric States in <sup>70</sup>Cu

ORAL

Abstract

One of the fundamental assumptions involved in calculations of astrophysical rates and neutron-capture cross sections is the generalized Brink-Axel hypothesis. This states that the gamma-ray strength function (γSF) is independent of how the initial compound nucleus is formed with respect to the initial excitation energy, spin, or parity. Here we test this hypothesis on the basis of the spin-independence of the γSF using 70Cu, which has three β-decaying isomeric states with spins of 6-, 3-, and 1+ for the ground state, 101 keV-state, and 242-keV state, respectively. 70Cu ions were produced at the National Superconducting Cyclotron Laboratory and thermalized in the gas stopper before being transmitted to the Low-Energy Beam Ion Trap Facility (LEBIT), where the isomers were separated based on mass through the LEBIT ion trap. Specific isomers were then delivered from the trap into the Summing NaI (SuN) total absorption spectrometer, where the γSF and nuclear level density (NLD) can be obtained using the β-Oslo method, an indirect technique for constraining neutron-capture cross sections. Preliminary results on the experimental isomer ratios, γSF, and NLD will be presented.

Presenters

  • Andrea L Richard

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

Authors

  • Andrea L Richard

    Lawrence Livermore Natl Lab, National Superconducting Cyclotron Labor, 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

  • Artemis Spyrou

    Michigan State University, Michigan State University, NSCL/FRIB, FRIB

  • Isaac T Yandow

    Michigan State University

  • Ryan J Ringle

    National Superconducting Cyclotron Laboratory, MSU, Michigan State University, National Superconducting Cyclotron Laboratory, Facility for Rare Isotopes Beams

  • Aaron Chester

    Michigan State University, National Superconducting Cyclotron Laboratory

  • Katherine L Childers

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

  • Paul A Deyoung

    Hope College

  • Jordan Owens-Fryar

    Michigan State University

  • Alec S Hamaker

    Michigan State University

  • Caley Harris

    Michigan State University, NSCL/FRIB, Michigan State University, FRIB

  • Rebecca Lewis

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

  • Kasey R Lund

    National Superconducting Cyclotron Laboratory, MSU

  • Stephanie Lyons

    Pacific Northwest National Laboratory, Michigan State University, National Superconducting Cyclotron Laboratory; Michigan State University, FRIB

  • Alicia Palmisano

    Michigan State University, NSCL/FRIB, Michigan State University, UTK, FRIB, University of Tennessee

  • Daniel J Puentes

    Michigan State University

  • Rachel Sandler

    Central Michigan Univ

  • Chandana S Sumithrarachchi

    Michigan State University, National Superconducting Cyclotron Laboratory, MSU, National Superconducting Cyclotron Laboratory

  • Mathis Wiedeking

    iThemba LABS, University of the Witwatersrand, iThemba LABS

  • Yongchi Xiao

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