Neutron spectroscopic factors of 55 Ni hole-states from (p,d) transfer reactions

A. Sanetullaev (National Superconducting Cyclotron Laboratory, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, 48824, USA) ; M.B. Tsang (National Superconducting Cyclotron Laboratory, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, 48824, USA) ; W.G. Lynch (National Superconducting Cyclotron Laboratory, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, 48824, USA) ; Jenny Lee (National Superconducting Cyclotron Laboratory, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, 48824, USA) ; D. Bazin (National Superconducting Cyclotron Laboratory, Department of Physics and Astronomy, Michigan State University, East Lansing, MI, 48824, USA) ; et al. - Show all 25 authors

Spectroscopic information has been extracted on the hole-states of 55 Ni, the least known of the quartet of nuclei ( 55 Ni, 57 Ni, 55 Co and 57 Cu), one nucleon away from 56 Ni, the N=Z=28 double magic nucleus. Using the H1(Ni56,d)Ni55 transfer reaction in inverse kinematics, neutron spectroscopic factors, spins and parities have been extracted for the f7/2 , p3/2 and the s1/2 hole-states of 55 Ni. These new data provide a benchmark for large basis calculations that include nucleonic orbits in both the sd and pf shells. State of the art calculations have been performed to describe the excitation energies and spectroscopic factors of the s1/2 hole-state below Fermi energy.

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      "value": "Spectroscopic information has been extracted on the hole-states of 55 Ni, the least known of the quartet of nuclei ( 55 Ni, 57 Ni, 55 Co and 57 Cu), one nucleon away from 56 Ni, the N=Z=28 double magic nucleus. Using the H1(Ni56,d)Ni55 transfer reaction in inverse kinematics, neutron spectroscopic factors, spins and parities have been extracted for the f7/2 , p3/2 and the s1/2 hole-states of 55 Ni. These new data provide a benchmark for large basis calculations that include nucleonic orbits in both the sd and pf shells. State of the art calculations have been performed to describe the excitation energies and spectroscopic factors of the s1/2 hole-state below Fermi energy."
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Published on:
07 July 2014
Publisher:
Elsevier
Published in:
Physics Letters B (2014)

Pages 137-141
DOI:
https://doi.org/10.1016/j.physletb.2014.07.003
Copyrights:
The Authors
Licence:
CC-BY-3.0

Fulltext files: