Radiative heat transfer in surface layers of neutron stars with a magnetic field |
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Authors: | N A Silant'ev D G Yakovlev |
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Institution: | (1) A. F. Ioffe Institute of Physics and Technology of the U.S.S.R. Academy of Sciences, Leningrad, U.S.S.R. |
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Abstract: | Thermal conductivity due to Thomson scattering and free-free absorption of photons is numerically evaluated for a non-relativistic non-degenerate plasma in a magnetic field for a number of values ofb =![hstrok](/content/p8584225746q5g37/xxlarge295.gif) B/kT 1000. In the case of pure scattering, simple fitting formulae are derived. Atb 6, the magnetic field is shown to decrease (by about one order) the characteristic densities above which heat transfer is mainly determined by free-free transitions. |
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