Calculation of thermal conductivity coefficients for magnetized neutron star
High Energy Astrophysical Phenomena
2013-04-24 v2
Abstract
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.
Keywords
Cite
@article{arxiv.1304.4752,
title = {Calculation of thermal conductivity coefficients for magnetized neutron star},
author = {M. V. Glushikhina and G. S. Bisnovatyi-Kogan},
journal= {arXiv preprint arXiv:1304.4752},
year = {2013}
}