1. Time-Resolved XUV Opacity Measurements of Warm Dense Aluminum
- Author
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D. S. Rackstraw, Johan Bielecki, S. Roling, Jaromir Chalupsky, Michael P. Desjarlais, H. Fleckenstein, Věra Hájková, T. R. Preston, Janos Hajdu, Justin Wark, Muhammad Kasim, Saša Bajt, Kerstin Muehlig, Libor Juha, Sven Toleikis, V. Vozda, Tomáš Burian, P. Hollebon, Jakob Andreasson, O. Ciricosta, Sam Vinko, Helmut Zacharias, and Emma McBride
- Subjects
Materials science ,Opacity ,Atom and Molecular Physics and Optics ,General Physics and Astronomy ,FOS: Physical sciences ,01 natural sciences ,Fusion, plasma och rymdfysik ,Physics::Plasma Physics ,0103 physical sciences ,ddc:530 ,010306 general physics ,Inertial confinement fusion ,Astrophysics::Galaxy Astrophysics ,Plasma ,Warm dense matter ,Computational Physics (physics.comp-ph) ,Fusion, Plasma and Space Physics ,Physics - Plasma Physics ,Computational physics ,Plasma Physics (physics.plasm-ph) ,Physics - Data Analysis, Statistics and Probability ,Extreme ultraviolet ,Attenuation coefficient ,Femtosecond ,Atom- och molekylfysik och optik ,Astrophysics::Earth and Planetary Astrophysics ,Physics - Computational Physics ,Ultrashort pulse ,Data Analysis, Statistics and Probability (physics.data-an) - Abstract
The free-free opacity in plasmas is fundamental to our understanding of energy transport in stellar interiors and for inertial confinement fusion research. However, theoretical predictions in the challenging dense plasma regime are conflicting and there is a dearth of accurate experimental data to allow for direct model validation. Here we present time-resolved transmission measurements in solid-density Al heated by an XUV free-electron laser. We use a novel functional optimization approach to extract the temperature-dependent absorption coefficient directly from an oversampled pool of single-shot measurements, and find a pronounced enhancement of the opacity as the plasma is heated to temperatures of order of the Fermi energy. Plasma heating and opacity enhancement are observed on ultrafast timescales, within the duration of the femtosecond XUV pulse. We attribute further rises in the opacity on ps timescales to melt and the formation of warm dense matter.
- Published
- 2020
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