Nuclear energy density functional from chiral pion-nucleon dynamics revisited
arXiv:0912.3207 · doi:10.1016/j.nuclphysa.2010.02.004
Abstract
We use a recently improved density-matrix expansion to calculate the nuclear energy density functional in the framework of in-medium chiral perturbation theory. Our calculation treats systematically the effects from -exchange, iterated -exchange, and irreducible -exchange with intermediate -isobar excitations, including Pauli-blocking corrections up to three-loop order. We find that the effective nucleon mass entering the energy density functional is identical to the one of Fermi-liquid theory when employing the improved density-matrix expansion. The strength of the surface-term as provided by the pion-exchange dynamics is in good agreement with that of phenomenological Skyrme forces in the density region . The spin-orbit coupling strength receives contributions from iterated -exchange (of the ``wrong sign'') and from three-nucleon interactions mediated by -exchange with virtual -excitation (of the ``correct sign''). In the region around fm where the spin-orbit interaction in nuclei gains most of its weight these two components tend to cancel, thus leaving all room for the short-range spin-orbit interaction. The strength function multiplying the square of the spin-orbit density comes out much larger than in phenomenological Skyrme forces and it has a pronounced density dependence.
18 pages, 7 figures, submitted to Nuclear Physics A
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