Phys.Lett. B 853, 138678 (2024)

J.Chen, B.P.Kay, C.R.Hoffman, T.L.Tang, I.A.Tolstukhin, D.Bazin, R.S.Lubna, Y.Ayyad, S.Beceiro-Novo, B.J.Coombes, S.J.Freeman, L.P.Gaffney, R.Garg, H.Jayatissa, A.N.Kuchera, P.MacGregor, A.J.Mitchell, W.Mittig, B.Monteagudo, A.Munoz-Ramos, C.Muller-Gatermann, F.Recchia, N.Rijal, C.Santamaria, M.Z.Serikow, D.K.Sharp, J.Smith, J.K.Stecenko, G.L.Wilson, A.H.Wuosmaa, C.X.Yuan, J.C.Zamora, Y.N.Zhang

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

NUCLEAR REACTIONS ²H(³²Si, p), E=8.3 MeV/nucleon; measured reaction products, Ep, Ip. ³³Si; deduced excitation-energy spectrum, σ(θ), spectroscopic factors of the low-lying states, spin-orbit splitting between neutron 1p orbitals. Comparison with the prediction of proton density depletion based on relativistic mean-field theory. SOLARIS spectrometer, the ReA6 reaccelerator-beam facility of the National Superconducting Cyclotron Laboratory (NSCL).

doi: 10.1016/j.physletb.2024.138678