Transport properties of the degenerate electron gas of neutron stars along the quantizing magnetic field

DOI10.1007/BF00651950zbMath0534.76127MaRDI QIDQ790693

D. G. Yakovlev

Publication date: 1984

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

cooling ratesthermopowerscattering mechanismsdegenerate relativistic electron gasdiffusion of magnetic fieldnuclear burningsurface layers of neutron starsthermal and electric conductivities

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar dynamics (85A05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (3)

The instability of gravity-capillary waves in the strong electric and magnetic fields on a neutron-star surface ⋮ Electrical conductivity of neutron star cores in the presence of a magnetic field. I: General solution for a multicomponent Fermi liquid ⋮ Electrical conductivity of neutron star cores in the presence of a magnetic field. II: A free-particle model of npe\({\sum}^ -\)-matter

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