Coulomb plasmas in outer envelopes of neutron stars

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dc.creatorPotekhin, A. Y.
dc.creatorChabrier, G.
dc.creatorYakovlev, D. G.
dc.date2000-12-14
dc.date.accessioned2026-07-07T06:24:14Z
dc.date.available2026-07-07T06:24:14Z
dc.descriptionOuter 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.
dc.description4 pages, 2 figures, latex2e using cpp2e.cls (included). Proc. PNP-10 Workshop, Greifswald, Germany, 4-9 Sept. 2000. Accepted for publication in Contrib. Plasma Phys. 41 (2001) no. 2-3
dc.identifierhttps://arxiv.org/abs/astro-ph/0012316
dc.identifierhttp://arxiv.org/abs/astro-ph/0012316
dc.identifierContrib.Plasma Phys. 41 (2001) 231-234
dc.identifierdoi:10.1002/1521-3986(200103)41:2/3<231::AID-CTPP231>3.0.CO;2-O
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96477
dc.subjectAstrophysics
dc.subjectPlasma Physics
dc.titleCoulomb plasmas in outer envelopes of neutron stars
dc.typetext

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