English

Spin-asymmetry energy of nuclear matter

Nuclear Theory 2009-11-10 v1

Abstract

We calculate the density-dependent spin-asymmetry energy S(kf)S(k_f) of isospin-symmetric nuclear matter in the three-loop approximation of chiral perturbation theory. The interaction contributions to S(kf)S(k_f) originate from one-pion exchange, iterated one-pion exchange, and (irreducible) two-pion exchange with no, single, and double virtual Δ\Delta-isobar excitation. We find that the truncation to 1π1\pi-exchange and iterated 1π1\pi-exchange terms (which leads already to a good nuclear matter equation of state) is spin-unstable, since S(kf0)<0S(k_{f0})<0. The inclusion of the chiral πNΔ\pi N\Delta-dynamics guarantees the spin-stability of nuclear matter. The corresponding spin-asymmetry energy S(kf)S(k_f) stays positive within a wide range of an undetermined short-range parameter S5S_5 (which we also estimate from realistic NN-potentials). Our results reemphasize the important role played by two-pion exchange with virtual Δ\Delta-isobar excitation for the nuclear matter many-body problem. Its explicit inclusion is essential in order to obtain good bulk and single-particle properties.

Keywords

Cite

@article{arxiv.nucl-th/0410021,
  title  = {Spin-asymmetry energy of nuclear matter},
  author = {N. Kaiser},
  journal= {arXiv preprint arXiv:nucl-th/0410021},
  year   = {2009}
}

Comments

11 pages, 6 figuers, accepted for publication in Physical Review C