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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Detalles Bibliográficos
Autores principales: Mabey, P., Richardson, S., White, T. G., Fletcher, L. B., Glenzer, S. H., Hartley, N. J., Vorberger, J., Gericke, D. O., Gregori, G.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2017
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5290263/
https://www.ncbi.nlm.nih.gov/pubmed/28134338
http://dx.doi.org/10.1038/ncomms14125

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5290263/
https://www.ncbi.nlm.nih.gov/pubmed/28134338
http://dx.doi.org/10.1038/ncomms14125

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