  We calculate thermal conductivity and shear viscosity of nucleons in dense
nuclear matter of neutron star cores in the non-relativistic
Brueckner-Hartree-Fock framework. Nucleon-nucleon interaction is described by
the Argonne v18 potential with addition of the Urbana IX effective three-body
forces. We find that this three body force leads to decrease of the kinetic
coefficients with respect to the two-body case. The results of calculations are
compared with electron and muon transport coefficients as well as with the
results of other authors.
