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.
*This work is supported by the National Science Foundation under Grants PHY-0555893, PHY-0606007 and PHY 0216783.
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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
