A strong diffusive ion mode in dense ionized matter predicted by Langevin dynamics

The state and evolution of planets, brown dwarfs and neutron star crusts is determined by the properties of dense and compressed matter. Due to the inherent difficulties in modelling strongly coupled plasmas, however, current predictions of transport coefficients differ by orders of magnitude. Colle...

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Vydáno v:Nat Commun
Hlavní autoři: Mabey, P., Richardson, S., White, T. G., Fletcher, L. B., Glenzer, S. H., Hartley, N. J., Vorberger, J., Gericke, D. O., Gregori, G.
Médium: Artigo
Jazyk:Inglês
Vydáno: Nature Publishing Group 2017
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On-line přístup:https://ncbi.nlm.nih.gov/pmc/articles/PMC5290263/
https://ncbi.nlm.nih.gov/pubmed/28134338
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms14125
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