Survey of Neutron Spectroscopic Factors for \emph{Z}=8 to 28 nuclei

ORAL

Abstract

Spectroscopic factor (SF) is a fundamental quantity in nuclear physics. SFs are extensively used from nuclear structure to astrophysical network calculations. They provide an important probe to test how well shell models describe the structure of nuclei. In this talk, we will compare neutron spectroscopic factors obtained for the sd shell nuclei, Ca, Ti, Cr and Ni isotopes to shell models. Of particular interests are the comparisons of data with different shell model interactions in these regions including the evolution of single particle states around \emph{Z}=20, \emph{N}=27 and \emph{N}=29 regions.

–

Authors

  • J. Lee*

    NSCL, JINA, and Dept of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA

  • P. Dai

    Physics Department, Chinese University of Hong Kong, Shatin, Hong Kong, China

  • Mihai Horoi

    Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA, Department of Physics, Central Michigan University, Mount Pleasant, MI 48859

  • W.G. Lynch

    JINA, NSCL, and Dept. of Physics and Astronomy, MSU, East Lansing, MI 48824, USA, NSCL and Dept. of Physics and Astronomy, MSU, East Lansing, MI, NSCL, JINA, and Dept of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA, NSCL MSU

  • S.C. Su

    Physics Department, Chinese University of Hong Kong, Shatin, Hong Kong, China

  • B. Tsang*

    JINA, NSCL, and Dept. of Physics and Astronomy, MSU, East Lansing, MI 48824, USA, NSCL and Dept. of Physics and Astronomy, MSU, East Lansing, MI, NSCL, JINA, and Dept of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA

  • S. Warren

    NSCL, JINA, and Dept of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 48824, USA