Nuclear spin-orbit interaction from chiral pion-nucleon dynamics
arXiv:nucl-th/0206056 · doi:10.1016/S0375-9474(02)01044-8
Abstract
Using the two-loop approximation of chiral perturbation theory, we calculate the momentum and density dependent nuclear spin-orbit strength . This quantity is derived from the spin-dependent part of the interaction energy of a nucleon scattering off weakly inhomogeneous isospin symmetric nuclear matter. We find that iterated -exchange generates at saturation density, MeV, a spin-orbit strength at of MeVfm in perfect agreement with the empirical value used in the shell model. This novel spin-orbit strength is neither of relativistic nor of short range origin. The potential underlying the empirical spin-orbit strength becomes a rather weak one, MeV, after the identification as suggested by the present calculation. We observe however a strong -dependence of leading even to a sign change above MeV. This and other features of the emerging spin-orbit Hamiltonian which go beyond the usual shell model parametrization leave questions about the ultimate relevance of the spin-orbit interaction generated by -exchange for a finite nucleus. We also calculate the complex-valued isovector single-particle potential in isospin asymmetric nuclear matter proportional to . For the real part we find reasonable agreement with empirical values and the imaginary part vanishes at the Fermi-surface .
20 pages, 10 Figures, Accepted for publication in Nuclear Physics A
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- The baryon-decuplet in the chiral dynamics of Lambda-hyperons in nuclear matter
- Isovector nuclear spin-orbit interaction from chiral pion-nucleon dynamics