Physics Letters B (Sep 2014)
Neutron spectroscopic factors of 55Ni hole-states from (p,d) transfer reactions
- A. Sanetullaev,
- M.B. Tsang,
- W.G. Lynch,
- Jenny Lee,
- D. Bazin,
- K.P. Chan,
- D. Coupland,
- V. Henzl,
- D. Henzlova,
- M. Kilburn,
- A.M. Rogers,
- Z.Y. Sun,
- M. Youngs,
- R.J. Charity,
- L.G. Sobotka,
- M. Famiano,
- S. Hudan,
- D. Shapira,
- W.A. Peters,
- C. Barbieri,
- M. Hjorth-Jensen,
- M. Horoi,
- T. Otsuka,
- T. Suzuki,
- Y. Utsuno
Affiliations
- 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
- K.P. Chan
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- D. Coupland
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- V. Henzl
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- D. Henzlova
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- M. Kilburn
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- A.M. Rogers
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- Z.Y. Sun
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- M. Youngs
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- R.J. Charity
- Department of Chemistry, Washington University, St. Louis, MO 63130, USA
- L.G. Sobotka
- Department of Chemistry, Washington University, St. Louis, MO 63130, USA
- M. Famiano
- Department of Physics, Western Michigan University, Kalamazoo, MI 49008, USA
- S. Hudan
- Department of Chemistry, Indiana University, Bloomington, IN 47405, USA
- D. Shapira
- Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
- W.A. Peters
- Rutgers University, Piscataway, NJ 08854, USA
- C. Barbieri
- Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom
- M. Hjorth-Jensen
- National Superconducting Cyclotron Laboratory & Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
- M. Horoi
- Department of Physics, Central Michigan University, Mount Pleasant, MI 48859, USA
- T. Otsuka
- Department of Physics, University of Tokyo, Tokyo, Japan
- T. Suzuki
- Department of Physics, Nihon University, Tokyo, Japan
- Y. Utsuno
- Advanced Science Research Center, Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195, Japan
- DOI
- https://doi.org/10.1016/j.physletb.2014.07.003
- Journal volume & issue
-
Vol. 736,
no. C
pp. 137 – 141
Abstract
Spectroscopic information has been extracted on the hole-states of 55Ni, the least known of the quartet of nuclei (55Ni, 57Ni, 55Co and 57Cu), one nucleon away from 56Ni, 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 55Ni. 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.
