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Title: Evolution of the nuclear spin-orbit splitting explored via the 32Si(d,p)33Si reaction using SOLARIS

Journal Article · · Physics Letters. B
ORCiD logo [1];  [2];  [2];  [2];  [2];  [3];  [3];  [4];  [3];  [5];  [6];  [7];  [3];  [2];  [8];  [9];  [5];  [3];  [10];  [4] more »;  [2];  [11];  [3];  [3];  [3];  [9];  [12];  [12];  [13];  [12];  [14];  [3];  [14] « less
  1. Southern University of Science and Technology (SUSTech), Shenzhen (China); Argonne National Laboratory (ANL), Argonne, IL (United States)
  2. Argonne National Laboratory (ANL), Argonne, IL (United States)
  3. Michigan State University, East Lansing, MI (United States)
  4. Universidade de Santiago de Compostela (Spain)
  5. Australian National University, Canberra (Australia)
  6. University of Manchester (United Kingdom); European Organization for Nuclear Research (CERN), Geneva (Switzerland)
  7. University of Liverpool (United Kingdom)
  8. Davidson College, NC (United States)
  9. University of Manchester (United Kingdom)
  10. Michigan State University, East Lansing, MI (United States); Hope College, Holland, MI (United States)
  11. National Institute of Nuclear Physics (INFN), Legnaro (Italy). National Laboratory of Legnaro (INFN-LNL); Universitá di Padova (Italy)
  12. University of Connecticut, Storrs, CT (United States)
  13. Louisiana State University, Baton Rouge, LA (United States)
  14. Sun Yat-Sen University, Guangzhou (China)

The spin-orbit splitting between neutron 1p orbitals at 33Si has been deduced using the single-neutron-adding (d,p) reaction in inverse kinematics with a beam of 32Si, a long-lived radioisotope. Reaction products were analyzed by the newly implemented SOLARIS spectrometer at the reaccelerated-beam facility at the National Superconducting Cyclotron Laboratory. The measurements show reasonable agreement with shell-model calculations that incorporate modern cross-shell interactions, but they contradict the prediction of proton density depletion based on relativistic mean-field theory. The evolution of the neutron 1p-shell orbitals is systematically studied using the present and existing data in the isotonic chains of N = 17, 19, and 21. In each case, a smooth decrease in the separation of the 1p3/2 - 1p1/2 orbitals is seen as the respective p-orbitals approach zero binding, suggesting that the finite nuclear potential strongly influences the evolution of nuclear structure in this region.

Research Organization:
Argonne National Laboratory (ANL), Argonne, IL (United States)
Sponsoring Organization:
Australian Research Council (ARC); International Technology Center Pacific (ITC-PAC); National Science Foundation (NSF); Science and Technology Facilities Council (STFC); Spanish Ministerio de Economia y Competitividad (MINECO); USDOE Office of Science (SC), Nuclear Physics (NP)
Grant/Contract Number:
AC02-06CH11357; SC0000661; SC0009883; SC0014552; SC0020451
OSTI ID:
2526252
Journal Information:
Physics Letters. B, Journal Name: Physics Letters. B Vol. 853; ISSN 0370-2693
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English

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