Transport coefficients of nuclear matter in neutron star cores
arXiv:1311.4278 · doi:10.1103/PhysRevC.88.065803
Abstract
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.
38 pages, 17 figures, accepted in PRC
References in corpus (4)
Cited by in corpus (23)
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