pith. sign in

arxiv: 1410.7645 · v1 · pith:PUOIBFJ7new · submitted 2014-10-28 · 🌌 astro-ph.SR · physics.plasm-ph

Diffusion coefficients in white dwarfs

classification 🌌 astro-ph.SR physics.plasm-ph
keywords diffusioncoefficientsdwarfsmethodwhiteaccountsadvancedapproach
0
0 comments X
read the original abstract

Models of diffusion in white dwarfs universally rely on the coefficients calculated by Paquette et al. (1986). We present new calculations of diffusion coefficients based on an advanced microscopic theory of dense plasmas and a numerical simulation approach that intrinsically accounts for multiple collisions. Our method is validated against a state-of-the-art method and we present results for the diffusion of carbon ions in a helium plasma.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.