The Spin Orbit term in the Nuclear Shell Model
arXiv:2009.11214 · doi:10.1103/PhysRevC.103.024306
Abstract
Quasi-nuclear systems, representing nuclei with variable size, are studied to investigate the occurrence of the spin-orbit term in the nuclear mean field in the transition from infinite nuclear matter to finite nuclei. Relativistic as well as non-relativistic mean field calculations based on models for the nucleon-nucleon () interaction, which fit the scattering data, are considered. A very strong correlation between the strength of the spin-orbit term and radius of the nuclear system is observed. The origin of the spin-orbit term is analyzed by inspecting the contributions of the different partial waves and various mesons in a One-Boson-Exchange model of the interaction. The influence of correlation effects and the enhancement of the small component of Dirac spinors for nucleons in the nuclear medium is discussed.
13 pages, 7 figures
References in corpus (9)
- Chiral effective field theory and nuclear forces
- Evolution of nuclear shells with the Skyrme density dependent interaction
- Low-momentum interactions with smooth cutoffs
- Chiral three-nucleon interaction and the carbon-14 dating beta decay
- Effects of three-nucleon spin-orbit interaction on isotope shifts of Pb nuclei
- Relativistic Effects and Three-Nucleon Forces in Nuclear Matter and Nuclei
- Weakly bound nuclei and realistic NN interactions
- Nuclear Saturation with Low Momentum Interactions
- Pairing in Nuclear Matter and Finite Nuclei