Journal
PHYSICAL REVIEW C
Volume 67, Issue 3, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.67.037301
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The equation of state of spin and isospin polarized nuclear matter is determined in the framework of the Brueckner theory including three-body forces. The Landau parameters in the spin and spin-isospin sectors are derived as a function of the baryonic density. The results are compared with the Gamow-Teller collective modes. The relevance of G(0) and G(0)' for neutron stars is shortly discussed, including the magnetic susceptibility and the neutron star cooling.
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