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Coulomb plasmas in outer envelopes of neutron stars

A. Y. Potekhin·G. Chabrier·D. G. Yakovlev
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Abstract

Outer envelopes of neutron stars consist mostly of fully ionized, strongly coupled Coulomb plasmas characterized by typical densities about 10^4-10^{11} g/cc and temperatures about 10^4-10^9 K. Many neutron stars possess magnetic fields about 10^{11}-10^{14} G. Here we briefly review recent theoretical advances which allow one to calculate thermodynamic functions and electron transport coefficients for such plasmas with an accuracy required for theoretical interpretation of observations.

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A. Y. Potekhin, G. Chabrier, D. G. Yakovlev. 2000-12-14. Coulomb plasmas in outer envelopes of neutron stars. https://doi.org/10.1002/1521-3986(200103)41%3A2%2F3%3C231%3A%3Aaid-ctpp231%3E3.0.co%3B2-o

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