Pairing properties in relativistic mean field models obtained from effective field theory

We apply recently developed effective field theory nuclear models in mean field approximation (parameter sets G1 and G2) to describe ground-state properties of nuclei from the valley of β stability up to the drip lines. For faster calculations of open-shell nuclei we employ a modified BCS approach which takes into account quasibound levels owing to their centrifugal barrier, with a constant pairing strength. We test this simple prescription by comparing with available Hartree-plus-Bogoliubov results. Using the new effective parameter sets we then compute separation energies, density distributions, and spin-orbit potentials in isotopic (isotonic) chains of nuclei with magic neutron (proton) numbers. The new forces describe the experimental systematics similarly to conventional nonlinear σ-ω relativistic force parameters like NL3.