Demonstration of X-ray Thomson scattering as diagnostics for miscibility in warm dense matter

The gas and ice giants in our solar system can be seen as a natural laboratory for the physics of highly compressed matter at temperatures up to thousands of kelvins. In turn, our understanding of their structure and evolution depends critically on our ability to model such matter. One key aspect is...

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Publicat a:Nat Commun
Autors principals: Frydrych, S., Vorberger, J., Hartley, N. J., Schuster, A. K., Ramakrishna, K., Saunders, A. M., van Driel, T., Falcone, R. W., Fletcher, L. B., Galtier, E., Gamboa, E. J., Glenzer, S. H., Granados, E., MacDonald, M. J., MacKinnon, A. J., McBride, E. E., Nam, I., Neumayer, P., Pak, A., Voigt, K., Roth, M., Sun, P., Gericke, D. O., Döppner, T., Kraus, D.
Format: Artigo
Idioma:Inglês
Publicat: Nature Publishing Group UK 2020
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Article
Accés en línia:https://ncbi.nlm.nih.gov/pmc/articles/PMC7251136/
https://ncbi.nlm.nih.gov/pubmed/32457297
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41467-020-16426-y
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