Electron Conduction Opacity for Dense Stellar Plasmas

Details Electron Conduction Opacity for Dense Stellar Plasmas Electron Conduction Opacity for Dense Stellar Plasmas

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..23..231i&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 23, 231

Astronomy and Astrophysics

Astronomy

2

Scientific paper

RESUMEN: Se calcula la conductividad termica de Ia materia densa tanto para el estado de metal lfquido como para el estado cristalino. El calculo del estado de metal lfquido toma en cuenta el mejor conocimiento disponible sobre el factor de estructura i6nico en el lfmite clasico a alta temperatura y el apantallamiento didectrico producido por los electrones degenerados. El c6mputo del estado cristalino incluye la forma precisa del factor de Debyc-Waller. ABSRTACT: Thermal conductivity of the dense matter is calculated for the liquid metal state as well as for the crystalline lattice state. The calculation for the liquid metal state takes account of the best knowledge available on the structure factor of the ions in the high-temperature, classical limit and the dielectric screening due to degenerate electrons. The calculation for the crystalline lattice state takes account of the accurate form of the Debye-Waller factor. Key words: ATOMIC PROCESSES - DENSE MATTER

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