A dense two-component plasma in a strong gravity field and thermal conductivity of neutron stars

Details A dense two-component plasma in a strong gravity field and thermal conductivity of neutron stars A dense two-component plasma in a strong gravity field and thermal conductivity of neutron stars

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...353.1129d&link_type=abstract

Astronomy and Astrophysics, v.353, p.1129-1133 (2000)

Astronomy and Astrophysics

Astrophysics

5

Dense Matter, Stars: Neutron

Scientific paper

Electron - impurity scattering in the crust of neutron stars may be a relevant mechanism in delaying the cooling and in enhancing the decay of the pulsar's magnetic field. Extending previous work, in the present note I investigate the physics of the interfaces between layers in the crust of an isolated neutron star. The calculations confirm the possible presence of high impurity concentrations and thus imply a decrease of the transport properties at low temperature.

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