Strongly coupled Coulomb and nuclear plasma in inner crusts of neutron stars

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dc.creatorYakovlev, D. G.
dc.creatorGnedin, O. Y.
dc.creatorPotekhin, A. Y.
dc.date2000-12-20
dc.date.accessioned2026-07-07T06:24:15Z
dc.date.available2026-07-07T06:24:15Z
dc.descriptionMatter of subnuclear density in the inner crusts of neutron stars consists of neutron-rich atomic nuclei immersed in strongly degenerate relativistic gas of electrons and strongly nonideal liquid of neutrons. We give a brief account of thermodynamic and kinetic properties of this matter which are greatly affected by Coulomb and nuclear interactions (a companion paper on the outer envelopes is astro-ph/0012316) and show how they can be studied from observations of thermal radiation of young (age < 100 yr) neutron stars (for a discussion of the latter possibility, see astro-ph/0012306).
dc.description4 pages, 1 figure, 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/0012424
dc.identifierhttp://arxiv.org/abs/astro-ph/0012424
dc.identifierContrib.Plasma Phys. 41 (2001) 227-230
dc.identifierdoi:10.1002/1521-3986(200103)41:2/3<227::AID-CTPP227>3.0.CO;2-4
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96478
dc.subjectAstrophysics
dc.subjectPlasma Physics
dc.titleStrongly coupled Coulomb and nuclear plasma in inner crusts of neutron stars
dc.typetext

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