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Heat and charge transport in envelopes of weakly and strongly magnetized neutron stars

Published online by Cambridge University Press:  12 April 2016

Alexander Potekhin
Alexander Potekhin*
Affiliation:
Ioffe Physical-Technical Institute, 194021 St.-Petersburg, Russia

Abstract

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Thermal and electrical electron conductivities are calculated for a broad range of physical parameters typical for envelopes of neutron stars. An appropriate effective electron-ion scattering potential is used, based on calculations involving modified ion structure factors suggested recently for the treatment of the transport problems in dense Coulomb plasmas. These results are applied to calculation of the thermal structure of neutron-star envelopes.

Type
Part 9. Population and Neutron Star Properties
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 621 - 622
Copyright
Copyright © Astronomical Society of the Pacific 2000

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