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Spectroscopic factors in dripline nuclei

J. Wylie1,2, J. Okołowicz3, W. Nazarewicz1,2, M. Płoszajczak4, S. M. Wang (王思敏)1,5, X. Mao (毛兴泽)1,2, and N. Michel6,7

  • 1FRIB/NSCL Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
  • 2Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 3Institute of Nuclear Physics, Polish Academy of Sciences, Radzikowskiego 152, PL-31342 Kraków, Poland
  • 4Grand Accélérateur National d'Ions Lourds (GANIL), CEA/DSM - CNRS/IN2P3, BP 55027, F-14076 Caen Cedex, France
  • 5Institute of Modern Physics, Fudan University, Shanghai 200433, China
  • 6Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
  • 7School of Nuclear Science and Technology, University of Chinese Academy of Sciences, Beijing 100049, China

Phys. Rev. C 104, L061301 – Published 3 December, 2021

DOI: https://doi.org/10.1103/PhysRevC.104.L061301

Abstract

Single-nucleon knockout reaction studies of the proton-dripline nuclei C9 and O13 suggest an appreciable suppression of spectroscopic factors. In this work, we calculate the one-neutron and one-proton spectroscopic factors for the mirror pair C9−Li9 and O13 using two variants of the continuum shell model: the complex-energy Gamow shell model and the real-energy shell model embedded in the continuum. Our results indicate that the continuum effects strongly suppress the spectroscopic factors of well-bound orbits in the dripline systems but have less impact on the spectroscopic factors of weakly bound states.

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