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Spin-asymmetry energy of nuclear matter

N. Kaiser

nucl-tharXiv:nucl-th/0410021

Abstract

We calculate the density-dependent spin-asymmetry energy S(kf) of isospin-symmetric nuclear matter in the three-loop approximation of chiral perturbation theory. The interaction contributions to S(kf) originate from one-pion exchange, iterated one-pion exchange, and (irreducible) two-pion exchange with no, single, and double virtual Δ-isobar excitation. We find that the truncation to 1π-exchange and iterated 1π-exchange terms (which leads already to a good nuclear matter equation of state) is spin-unstable, since S(kf0)<0. The inclusion of the chiral πNΔ-dynamics guarantees the spin-stability of nuclear matter. The corresponding spin-asymmetry energy S(kf) stays positive within a wide range of an undetermined short-range parameter S5 (which we also estimate from realistic NN-potentials). Our results reemphasize the important role played by two-pion exchange with virtual Δ-isobar excitation for the nuclear matter many-body problem. Its explicit inclusion is essential in order to obtain good bulk and single-particle properties.

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