Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9851371 | Nuclear Physics A | 2005 | 35 Pages |
Abstract
We extend a recent three-loop calculation of nuclear matter by including the effects from two-pion exchange with single and double virtual Î(1232)-isobar excitation. Regularization dependent short-range contributions from pion-loops are encoded in a few NN-contact coupling constants. The empirical saturation point of isospin-symmetric nuclear matter, E¯0=â16 MeV, Ï0=0.16 fmâ3, can be well reproduced by adjusting the strength of a two-body term linear in density (and tuning an emerging three-body term quadratic in density). The nuclear matter compressibility comes out as K=304 MeV. The real single-particle potential U(p,kf0) is substantially improved by the inclusion of the chiral ÏNÎ-dynamics: it grows now monotonically with the nucleon momentum p. The effective nucleon mass at the Fermi surface takes on a realistic value of Mâ(kf0)=0.88M. As a consequence of these features, the critical temperature of the liquid-gas phase transition gets lowered to the value Tcâ15 MeV. In this work we continue the complex-valued single-particle potential U(p,kf)+iW(p,kf) into the region above the Fermi surface p>kf. The effects of 2Ï-exchange with virtual Î-excitation on the nuclear energy density functional are also investigated. The effective nucleon mass associated with the kinetic energy density is MËâ(Ï0)=0.64M. Furthermore, we find that the isospin properties of nuclear matter get significantly improved by including the chiral ÏNÎ-dynamics. Instead of bending downward above Ï0 as in previous calculations, the energy per particle of pure neutron matter E¯n(kn) and the asymmetry energy A(kf) now grow monotonically with density. In the density regime Ï=2Ïn<0.2 fmâ3 relevant for conventional nuclear physics our results agree well with sophisticated many-body calculations and (semi)-empirical values.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
S. Fritsch, N. Kaiser, W. Weise,