Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2006-01-31
Phys.Rev. C72 (2005) 014007
Physics
Nuclear Physics
Nuclear Theory
10 pages, 6 figures, published in: Phys. Rev. C72, 014007 (2005)
Scientific paper
10.1103/PhysRevC.72.014007
We calculate the density-dependent spin-isospin asymmetry energy $J(k_f)$ of nuclear matter in the three-loop approximation of chiral perturbation theory. The interaction contributions to $J(k_f)$ originate from one-pion exchange, iterated one-pion exchange, and irreducible two-pion exchange with no, single, and double virtual $\Delta$-isobar excitation. We find that the approximation to $1\pi$-exchange and iterated $1\pi$-exchange terms (which leads already to a good nuclear matter equation of state by adjusting an emerging contact-term) is spin-isospin stable, since $J(k_{f0})\simeq 24 {\rm MeV}>0$. The inclusion of the chiral $\pi N\Delta$-dynamics, necessary in order to guarantee the spin-stability of nuclear matter, keeps this property intact. The corresponding spin-isospin asymmetry energy $J(k_f)$ stays positive even for extreme values of an undetermined short-distance parameter $J_5$ (whose possible range we estimate from realistic NN-potentials). The largest positive contribution to $J(k_f)$ (a term linear in density) comes from a two-body contact-term with its strength fitted to the empirical nuclear matter saturation point.
No associations
LandOfFree
Spin-isospin stability of nuclear matter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spin-isospin stability of nuclear matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spin-isospin stability of nuclear matter will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-353988