Impact of shell structure on the fusion of neutron-rich mid-mass nuclei with oxygen nuclei

ORAL

Abstract

The influence of shell effects on fusion of mid-mass nuclei is explored using isotopic chains of K and Ar ions on an oxygen target. Comparison of the reduced excitation functions reveals that the fusion cross section for the open neutron-shell projectile nuclei 41K and 45K is systematically larger than for the closed neutron-shell projectiles 39K and 47K. The São Paulo fusion model using matter densities from systematics fails to describe the measured excitation functions. Use of more realistic densities from a Dirac-Hartree-Bogoliubov (DHB) approach performs significantly better though it still overpredicts the closed-shell nuclei.

*This work was supported by the U.S. Department of Energy Office of Science under Grants No. DE-FG02-88ER-40404 (IndianaUniversity) and No. DE-FG02-93ER-407773 (Texas A&M University) and by the National Science Foundation underGrant No. PHY-1712832.

Publication: PHYSICAL REVIEW C 104, L041601 (2021)

Presenters

  • Romualdo T Desouza

    • Indiana University Bloomington

Authors

  • Romualdo T Desouza

    • Indiana University Bloomington
  • Varinderjit Singh

    • Indiana University
  • Sylvie Hudan

    • Indiana University Bloomington
  • D. Ackermann

    • GANIL
  • Abdelouahad Chbihi

    • GANIL
  • Austin Abbott

    • Texas A&M University–Kingsville
  • Andy Hannaman

    • Texas A&M University
  • Alan B McIntosh

    • Texas A&M University
  • Maxwell Q Sorensen

    • Texas A&M University
  • Zachary Tobin

    • Texas A&M University–Kingsville
  • Aditya Wakhle

    • Texas A&M
  • Sherry J Yennello

    • Texas A&M
  • Michael A Famiano

    • Western Michigan University
  • Kyle W Brown

    • Michigan State University
  • Clémentine Santamaria

    • NSCL/FRIB
  • Jesus Lubian

    • Universidade Federal Fluminense
  • Hugo Soler

    • Universidade Federal Fluminense
  • Brett V Carlson

    • Centro Tecnico Aerospacial