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Astron. Astrophys. 353, 1129-1133 (2000)

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

F.V. De Blasio

Department of Physics, University of Oslo, P.O. Boks 1048, Blindern, 0316 Oslo, Norway (f.v.d.blasio@fys.uio.no)

Received 3 March 1999 / Accepted 28 September 1999


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.

Key words: dense matter – stars: neutron

This article contains no SIMBAD objects.


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© European Southern Observatory (ESO) 2000

Online publication: January 18, 2000