Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...405l...5m&link_type=abstract
Astronomy and Astrophysics, v.405, p.L5-L9 (2003)
Astronomy and Astrophysics
Astrophysics
13
Atomic Processes, Dense Matter, Equation Of State, Plasmas, Radiation Mechanisms: General, Planets And Satellites: General
Scientific paper
We show that Quantum Molecular Dynamics provides a powerful tool to extend and benchmark current opacities libraries into the complex regime of warm dense matter. In this regime, the medium can be constituted of electrons, protons, atoms and molecules, while plasma and many-body effects can not be treated as perturbations. Among the most notable features of this new approach for calculating Rosseland mean opacities is the ability to obtain a consistent set of material (equation-of-state), optical and electrical properties for various mixtures from the same simulation.
Collins Lee A.
Keady John Joseph
Kress Joel D.
Magee N. H.
Mazevet Stéphane
No associations
LandOfFree
Quantum Molecular Dynamics calculations of radiative opacities does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Quantum Molecular Dynamics calculations of radiative opacities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quantum Molecular Dynamics calculations of radiative opacities will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1462301