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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Detalles Bibliográficos
Autores principales: 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.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2020
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7251136/
https://www.ncbi.nlm.nih.gov/pubmed/32457297
http://dx.doi.org/10.1038/s41467-020-16426-y

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7251136/
https://www.ncbi.nlm.nih.gov/pubmed/32457297
http://dx.doi.org/10.1038/s41467-020-16426-y

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