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

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

2000-12-20

arxiv.org/abs/astro-ph/0012424v1

Contrib.Plasma Phys. 41 (2001) 227-230

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure, LaTeX2e using cpp2e.cls (included). Proc. PNP-10 Workshop, Greifswald, Germany, 4-9 Sept. 2000. Accepted fo

Scientific paper

10.1002/1521-3986(200103)41:2/3<

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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