Spin-asymmetry energy of nuclear matter
arXiv:nucl-th/0410021 · doi:10.1103/PhysRevC.70.054001
Abstract
We calculate the density-dependent spin-asymmetry energy of isospin-symmetric nuclear matter in the three-loop approximation of chiral perturbation theory. The interaction contributions to originate from one-pion exchange, iterated one-pion exchange, and (irreducible) two-pion exchange with no, single, and double virtual -isobar excitation. We find that the truncation to -exchange and iterated -exchange terms (which leads already to a good nuclear matter equation of state) is spin-unstable, since . The inclusion of the chiral -dynamics guarantees the spin-stability of nuclear matter. The corresponding spin-asymmetry energy stays positive within a wide range of an undetermined short-range parameter (which we also estimate from realistic NN-potentials). Our results reemphasize the important role played by two-pion exchange with virtual -isobar excitation for the nuclear matter many-body problem. Its explicit inclusion is essential in order to obtain good bulk and single-particle properties.
11 pages, 6 figuers, accepted for publication in Physical Review C
References in corpus (3)
- A microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models
- Chiral approach to nuclear matter: Role of two-pion exchange with virtual delta-isobar excitation
- Single-particle potential in a chiral approach to nuclear matter including short range NN-terms
Cited by in corpus (10)
- Chiral approach to nuclear matter: Role of two-pion exchange with virtual delta-isobar excitation
- In-medium chiral condensate beyond linear density approximation
- Spin polarized neutron matter within the Dirac-Brueckner-Hartree-Fock approach
- Spin- and isospin-polarized states of nuclear matter in the Dirac-Brueckner-Hartree-Fock model
- Spin-polarized neutron matter at different orders of chiral effective field theory
- Quasi-particle interaction in nuclear matter from chiral pion-nucleon dynamics
- Nuclear matter symmetry energy from generalized polarizabilities: dependences on momentum, isospin, density and temperature
- The splitting of the one-body potential in spin-polarized isospin-symmetric nuclear matter
- Isospin-Asymmetry Dependence of the Thermodynamic Nuclear Equation of State in Many-Body Perturbation Theory
- Spin-isospin stability of nuclear matter