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arXiv · 1311.4278

Transport coefficients of nuclear matter in neutron star cores

P. S. Shternin·M. Baldo·P. Haensel
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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.

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P. S. Shternin, M. Baldo, P. Haensel. 2013-11-18. Transport coefficients of nuclear matter in neutron star cores. https://doi.org/10.1103/physrevc.88.065803

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