Charge radii of neutron-deficient 55, 56Ni
ORAL
Abstract
The 56Ni nucleus is doubly magic with the neutron number N = 28, which occurs due to a shell gap driven by the spin-orbit force, but is considered to be a soft core. The mean-square charge radii <r2> were determined for 55, 56Ni using collinear laser spectroscopy technique at BECOLA at NSCL/MSU to investigate how the softness manifests itself in <r2> at and below N = 28, and to benchmark nuclear theories. Details of the experiment and preliminary results will be presented.
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Presenters
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K. Minamisono
NSCL/Dep. Phys. Astron., MSU, Michigan State University, NSCL
Authors
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K. Minamisono
NSCL/Dep. Phys. Astron., MSU, Michigan State University, NSCL
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D. M. Rossi
Institute für Kernphysik, Technische Universität Darmstadt, Inst. Kernphysik, TU Darmstadt
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N. Everett
NSCL/Dep. Phys. Astron., MSU
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D. Garand
NSCL, MSU
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R. P. de Groote
Dep. Phys. Univ. Jyväskylä
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P. Imgram
Inst. Kernphysik, TU Darmstadt
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C. Kalman
NSCL/Dep. Chem., MSU
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A. Klose
Department of Chemistry, Augustana University, Dep. Chem., Augustana Univ.
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J. D. D Lantis
NSCL/Dep. Chem., MSU, Michigan State University, NSCL
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Y. Liu
Phys. Divi., ORLN
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P. F. Mantica
FRIB, FRIB/Dep. Chem., MSU
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A. J. Miller
Michigan State University, NSCL, NSCL/Dep. Phys. Astron., MSU
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Witold Nazarewicz
FRIB, FRIB/Dep. Phys. Astron., MSU, Michigan State Univ, Michigan State University
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W. Nörtershäuser
Inst. Kernphysik, TU Darmstadt
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R. C. Powel
NSCL/Dep. Phys. Astron., MSU, NSCL
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P. -G. Reinhard
Institute für Theoretische Physik, Universität Erlangen, Ins. Theo. Phys., Univ. Erlangen-Numberg
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E. Romeo-Romero
Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37966, USA, UT Knoxville/ORLN
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F. Sommer
Inst. Kernphysik, TU Darmstadt
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C. S. Sumithrarachchi
Michigan State Univ, NSCL, NSCL, MSU, National Superconducting Cyclotron Laboratory
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A. Teigelhöfer
TRIUMF