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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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| Publicado no: | Nat Commun |
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| Main Authors: | , , , , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Nature Publishing Group
2017
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| Assuntos: | |
| Acesso em linha: | 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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