Spin structure of light nuclei related to nucleon-nucleus elastic scattering

ORAL

Abstract

We discuss recent work related to the calculation of \textit{ab initio} microscopic effective interactions for elastic nucleon-nucleus scattering. In the framework of the spectator expansion of the multiple scattering series, we can construct a leading-order consistent effective interaction that includes information about the spin of the struck nucleon. Using one-body densities from the no-core shell model, we are able to examine the spin structure of the target $0^+$ nucleus and investigate the effects of the underlying shell structure on the resulting effective interaction as well as physical observables. With a focus on differences along isotopic chains, we present results for light nuclei and discuss the relevant physics.

*This work was supported in part by the U.S. DoE (DE-FG02-93ER40756 and DE-SC0018223) and by the U.S. NSF (OIA-1738287 and PHY-1913728). Computational resources provided by Blue Waters (supported by U.S. NSF OCI-0725070 and ACI-1238993, and the state of Illinois), LSU HPC (www.hpc.lsu.edu), and the National Energy Research Scientific Computing Center (NERSC), a U.S. DoE Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.

Authors

  • Robert Baker

    • Ohio University
  • Matthew Burrows

    • Ohio University
  • Charlotte Elster

    • Ohio University
  • Gabriela Popa

    • Ohio University
  • Kristina Launey

    • Louisiana State University
    • Louisiana State University, Baton Rouge, LA 70803
    • Louisiana State University, Baton Rouge
  • Pieter Maris

    • Iowa State University
  • Stephen Weppner

    • Eckerd College