1304.4752 (M. V. Glushikhina et al.)

Calculation of thermal conductivity coefficients for magnetized neutron star    [PDF]

M. V. Glushikhina, G. S. Bisnovatyi-Kogan

The coefficients that determine the electron heat transfer and diffusion in the crust of neutron stars are calculated on the basis of a solution of the Boltzmann equation with allowance for degeneracy.

View original: http://arxiv.org/abs/1304.4752