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• W2520153966 abstract "We develop a multicomponent hydrodynamic model based on moments of the Born–Bogolyubov–Green–Kirkwood–Yvon hierarchy equations for physical conditions relevant to astrophysical plasmas. These equations incorporate strong correlations through a density functional theory closure, while transport enters through a relaxation approximation. This approach enables the introduction of Coulomb coupling correction terms into the standard Burgers equations. The diffusive currents for these strongly coupled plasmas is self-consistently derived. The settling of impurities and its impact on cooling can be greatly affected by strong Coulomb coupling, which we show can be quantified using the direct correlation function." @default.
• W2520153966 created "2016-09-23" @default.
• W2520153966 creator A5044155444 @default.
• W2520153966 creator A5087113189 @default.
• W2520153966 date "2016-09-15" @default.
• W2520153966 modified "2023-10-14" @default.
• W2520153966 title "A DYNAMIC DENSITY FUNCTIONAL THEORY APPROACH TO DIFFUSION IN WHITE DWARFS AND NEUTRON STAR ENVELOPES" @default.
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• W2520153966 doi "https://doi.org/10.3847/0004-637x/829/1/16" @default.
• W2520153966 hasPublicationYear "2016" @default.
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