1. Neutron-hole states in 131Sn and spin-orbit splitting in neutron-rich nuclei.
- Author
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Orlandi, R., Pain, S.D., Ahn, S., Jungclaus, A., Schmitt, K.T., Bardayan, D.W., Catford, W.N., Chapman, R., Chipps, K.A., Cizewski, J.A., Gross, C.G., Howard, M.E., Jones, K.L., Kozub, R.L., Manning, B., Matos, M., Nishio, K., O' Malley, P.D., Peters, W.A., and Pittman, S.T.
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ATOMIC nucleus , *PARTICLES (Nuclear physics) , *NEUTRONS , *COUPLINGS (Gearing) , *KINEMATICS - Abstract
Abstract In atomic nuclei, the spin-orbit interaction originates from the coupling of the orbital motion of a nucleon with its intrinsic spin. Recent experimental and theoretical works have suggested a weakening of the spin-orbit interaction in neutron-rich nuclei far from stability. To study this phenomenon, we have investigated the spin-orbit energy splittings of single-hole and single-particle valence neutron orbits of 132Sn. The spectroscopic strength of single-hole states in 131Sn was determined from the measured differential cross sections of the tritons from the neutron-removing 132Sn(d, t)131Sn reaction, which was studied in inverse kinematics at the Holifield Radioactive Ion Beam Facility at Oak Ridge National Laboratory. The spectroscopic factors of the lowest 3 / 2 + , 1 / 2 + and 5 / 2 + states were found to be consistent with their maximal values of (2 j + 1) , confirming the robust N = 82 shell closure at 132Sn. We compared the spin-orbit splitting of neutron single-hole states in 131Sn to those of single-particle states in 133Sn determined in a recent measurement of the 132Sn(d, p)133Sn reaction. We found a significant reduction of the energy splitting of the weakly bound 3 p orbits compared to the well-bound 2 d orbits, and that all the observed energy splittings can be reproduced remarkably well by calculations using a one-body spin-orbit interaction and a Woods–Saxon potential of standard radius and diffuseness. The observed reduction of spin-orbit splitting can be explained by the extended radial wavefunctions of the weakly bound orbits, without invoking a weakening of the spin-orbit strength. [ABSTRACT FROM AUTHOR]
- Published
- 2018
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