Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..98...37i&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 98, no. 1, Jan. 1984, p. 37-59.
Astronomy and Astrophysics
Astrophysics
15
Degenerate Matter, Electron Gas, Gas Transport, Neutron Stars, Stellar Magnetic Fields, Electrical Resistivity, Electron Phonon Interactions, Electron Scattering, Thermal Conductivity
Scientific paper
The expressions are derived for thermal and electric conductivities as well as thermopower of a degenerate relativistic electron gas, in the surface layers of neutron stars that lie along the magnetic field B = 4 x 10 to the 11th to 10 to the 14th G for two scattering mechanisms of electrons: Coulomb scattering on ions in the ion-liquid regime, and high temperature phonons in the solid regime. The results may be of use to study neutron star cooling rates, nuclear burning of the matter in the surface layers, diffusion of the magnetic field, etc.
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