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Article overview
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Nuclear energy density functional from chiral pion-nucleon dynamics | N. Kaiser
; S. Fritsch
; W. Weise
; | Date: |
11 Dec 2002 | Journal: | Nucl.Phys. A724 (2003) 47-68 | Subject: | nucl-th | Abstract: | We calculate the nuclear energy density functional relevant for N=Z even-even nuclei in the systematic framework of chiral perturbation theory. The calculation includes the one-pion exchange Fock diagram and the iterated one-pion exchange Hartree and Fock diagrams. From these few leading order contributions in the small momentum expansion one obtains already a very good equation of state of isospin symmetric nuclear matter. We find that in the region below nuclear matter saturation density the effective nucleon mass $widetilde M^*(
ho)$ deviates by at most 15% from its free space value $M$, with $0.89MM$ for higher densities. The parameterfree strength of the $(vec
abla
ho)^2$-term, $F_
abla(k_f)$, is at saturation density comparable to that of phenomenological Skyrme forces. The magnitude of $F_J(k_f)$ accompanying the squared spin-orbit density $vec J ^2$ comes out somewhat larger. The strength of the nuclear spin-orbit interaction, $F_{so}(k_f)$, as given by iterated one-pion exchange is about half as large as the corresponding empirical value, however, with the wrong negative sign. The novel density dependencies of $widetilde M^*(
ho)$ and $F_{
abla,so,J}(k_f)$ as predicted by our parameterfree calculation should be examined in nuclear structure calculations (after introducing an additional short range spin-orbit contribution constant in density). | Source: | arXiv, nucl-th/0212049 | Services: | Forum | Review | PDF | Favorites |
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