Gamma ray spectroscopy of $^{31}$Si

ORAL

Abstract

$^{31}$Si was produced through the $^{18}$O ($^{18}$O, $\alpha$n) reaction at the beam energy of 24 MeV, which preferentially populates the high spin states. The $\alpha$ particles were detected in Microball and the multiple $\gamma$-ray coincidences were detected by Gammashpere. There are 11 newly observed states and 22 new discovered $\gamma$ transitions. A strong competition is seen between negative-parity {}``intruder'' states and positive-parity pure s-d states. Shell model calculations agree relatively well with both groups of states.

*Supported in part by National Science Foundation and the Department of Energy

Authors

  • Pei-Luan Tai

    • Physics Department Florida State University
    • Florida State University
  • Leanne Hamilton

    • Physics Department Florida State University
  • Peter Bender

    • Physics Department Florida State University
  • Samuel Tabor

    • Physics Department Florida State University
    • Florida State University
  • Vandana Tripathi

    • Physics Department Florida State University
  • Calem Hoffman

    • Physics Department Florida State University
  • Roderick Clark

    • Lawrence Berkeley National Laboratory
  • Paul Fallon

    • Lawrence Berkeley National Laboratory
  • Augusto Macchiavelli

    • Lawrence Berkeley National Laboratory
  • S. Paschalis

    • Lawrence Berkeley National Laboratory
  • M. Petri

    • Lawrence Berkeley National Laboratory
  • Michael Carpenter

    • Argonne National Laboratory
  • Robert Janssens

    • Argonne National Laboratory
  • T. Lauritsen

    • Argonne National Laboratory
  • E.A. McCutchan

    • Argonne National Laboratory
  • D. Seweryniak

    • Argonne National Laboratory
  • S. Zhu

    • Argonne National Laboratory
  • C. Chiara

    • Argonne National Laboratory
  • X. Chen

    • Chemistry Department, Washington University
  • W. Reviol

    • Chemistry Department, Washington University
  • D. Sarantites

    • Chemistry Department, Washington University