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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
Abstract
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