Spin-orbit interaction in relativistic nuclear structure models
arXiv:1607.06567 · doi:10.1103/PhysRevC.94.024304
Abstract
Relativistic self-consistent mean-field (SCMF) models naturally account for the coupling of the nucleon spin to its orbital motion, whereas non-relativistic SCMF methods necessitate a phenomenological ansatz for the effective spin-orbit potential. Recent experimental studies aim to explore the isospin properties of the effective spin-orbit interaction in nuclei. SCMF models are very useful in the interpretation of the corresponding data, however standard relativistic mean-field and non-relativistic Hartree-Fock models use effective spin-orbit potentials with different isovector properties, mainly because exchange contributions are not treated explicitly in the former. The impact of exchange terms on the effective spin-orbit potential in relativistic mean-field models is analysed, and it is shown that it leads to an isovector structure similar to the one used in standard non-relativistic Hartree-Fock. Data on the isospin dependence of spin-orbit splittings in spherical nuclei could be used to constrain the isovector-scalar channel of relativistic mean-field models. The reproduction of the empirical kink in the isotope shifts of even Pb nuclei by relativistic effective interactions points to the occurrence of pseudospin symmetry in the single-neutron spectra in these nuclei.
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- Contribution of the rho meson and quark sub-structure to the nuclear spin-orbit potential
- Symmetry breaking of Gamow-Teller and magnetic-dipole transitions and its restoration in calcium isotopes
- Localisation and alpha radioactivity
- Impact of finite-range spin-orbit and tensor terms in Gogny EDF
- Effects of isovector spin-orbit interaction on the charge-weak form factor difference in Ca, Pb, Zr and Ni
- Implication of odd-even staggering in the charge radii of calcium isotopes
- Nuclear Matter and Finite Nuclei: Relativistic Thomas-Fermi Approximation Versus Relativistic Mean-Field Approach