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

D. G. Yakovlev·O. Y. Gnedin·A. Y. Potekhin
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Abstract

Matter 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).

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D. G. Yakovlev, O. Y. Gnedin, A. Y. Potekhin. 2000-12-20. Strongly coupled Coulomb and nuclear plasma in inner crusts of neutron stars. https://doi.org/10.1002/1521-3986(200103)41%3A2%2F3%3C227%3A%3Aaid-ctpp227%3E3.0.co%3B2-4

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