Nuclear level density and γ-decay strength of Sr93

A. Sweet, D. L. Bleuel, N. D. Scielzo, L. A. Bernstein, A. C. Dombos, B. L. Goldblum, C. M. Harris, T. A. Laplace, A. C. Larsen, R. Lewis, S. N. Liddick, S. M. Lyons, F. Naqvi, A. Palmisano-Kyle, A. L. Richard, M. K. Smith, A. Spyrou, J. Vujic, and M. Wiedeking
Phys. Rev. C 109, 054305 – Published 6 May 2024

Abstract

This work presents the first experimentally determined nuclear level density and γ-ray strength function of the short-lived fission product Sr93, accomplished using the β-Oslo method. Direct measurement of the Sr92(n,γ)Sr93 cross section is not currently possible, as the half-life of 2.66 hours is too short; instead, Sr93 was formed through β decay of Rb93 to excitation energies around the neutron separation energy. The γ-ray spectra were measured using a total absorption spectrometer at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University (MSU). The statistical properties of the Sr93 nucleus were experimentally determined, including the γ-ray strength function and nuclear level density. At low energies, the γ-ray strength function exhibits a constant γ-decay strength, rather than a slightly increasing strength with decreasing γ-ray energy as had been previously observed for several nuclei in this mid-mass region. These statistical properties were then implemented in the reaction code talys1.95 to calculate the Sr92(n,γ)Sr93 cross section.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
4 More
  • Received 25 August 2022
  • Revised 22 November 2023
  • Accepted 23 February 2024

DOI:https://doi.org/10.1103/PhysRevC.109.054305

©2024 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

A. Sweet1,*, D. L. Bleuel1, N. D. Scielzo1, L. A. Bernstein2,3, A. C. Dombos4,5,6, B. L. Goldblum2,3, C. M. Harris4,5,6, T. A. Laplace2, A. C. Larsen7, R. Lewis4,8, S. N. Liddick4,8, S. M. Lyons4, F. Naqvi4, A. Palmisano-Kyle4,5,6, A. L. Richard1,†, M. K. Smith4, A. Spyrou4,5,6, J. Vujic2, and M. Wiedeking9,10,‡

  • 1Lawrence Livermore National Laboratory (LLNL), Livermore, California 94551, USA
  • 2Department of Nuclear Engineering, University of California, Berkeley (UCB), California 94720, USA
  • 3Lawrence Berkeley National Laboratory (LBNL), Berkeley, California 94720, USA
  • 4Facility for Rare Isotope Beams (FRIB)/National Superconducting Cyclotron Laboratory (NSCL), Michigan State University (MSU), East Lansing, Michigan 48824, USA
  • 5Department of Physics and Astronomy, Michigan State University (MSU), East Lansing, Michigan 48824, USA
  • 6Joint Institute for Nuclear Astrophysics (JINA), Michigan State University (MSU), East Lansing, Michigan 48824, USA
  • 7Department of Physics, University of Oslo (UiO), N-0316 Oslo, Norway
  • 8Department of Chemistry, Michigan State University (MSU), East Lansing, Michigan 48824, USA
  • 9Department of Subatomic Physics, iThemba LABS, Somerset West 7129, South Africa
  • 10School of Physics, University of the Witwatersrand, Johannesburg 2050, South Africa

  • *Formerly at the University of California, Berkeley, California, USA.
  • Formerly at the Facility for Rare Isotope Beams, National Superconducting Cyclotron Laboratory, Michigan State University, Michigan, USA. Currently at Ohio University, Ohio, USA.
  • Currently at Lawrence Berkeley National Laboratory (LBNL), California, USA.

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 109, Iss. 5 — May 2024

Reuse & Permissions
Access Options
CHORUS

Article part of CHORUS

Accepted manuscript will be available starting 6 May 2025.
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×