Equilibration dynamics and conductivity of warm dense hydrogen

We investigate subpicosecond dynamics of warm dense hydrogen at the XUV free-electron laser facility (FLASH) at DESY (Hamburg). Ultrafast impulsive electron heating is initiated by a ≤ 300-fs short x-ray burst of 92-eV photon energy. A second pulse probes the sample via x-ray scattering at jitter-fr...

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Veröffentlicht in:Physical review. E, Statistical, nonlinear, and soft matter physics Statistical, nonlinear, and soft matter physics, 2014-07, Vol.90 (1), p.013104-013104, Article 013104
Hauptverfasser: Zastrau, U, Sperling, P, Becker, A, Bornath, T, Bredow, R, Döppner, T, Dziarzhytski, S, Fennel, T, Fletcher, L B, Förster, E, Fortmann, C, Glenzer, S H, Göde, S, Gregori, G, Harmand, M, Hilbert, V, Holst, B, Laarmann, T, Lee, H J, Ma, T, Mithen, J P, Mitzner, R, Murphy, C D, Nakatsutsumi, M, Neumayer, P, Przystawik, A, Roling, S, Schulz, M, Siemer, B, Skruszewicz, S, Tiggesbäumker, J, Toleikis, S, Tschentscher, T, White, T, Wöstmann, M, Zacharias, H, Redmer, R
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Sprache:eng
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Zusammenfassung:We investigate subpicosecond dynamics of warm dense hydrogen at the XUV free-electron laser facility (FLASH) at DESY (Hamburg). Ultrafast impulsive electron heating is initiated by a ≤ 300-fs short x-ray burst of 92-eV photon energy. A second pulse probes the sample via x-ray scattering at jitter-free variable time delay. We show that the initial molecular structure dissociates within (0.9 ± 0.2) ps, allowing us to infer the energy transfer rate between electrons and ions. We evaluate Saha and Thomas-Fermi ionization models in radiation hydrodynamics simulations, predicting plasma parameters that are subsequently used to calculate the static structure factor. A conductivity model for partially ionized plasma is validated by two-temperature density-functional theory coupled to molecular dynamic simulations and agrees with the experimental data. Our results provide important insights and the needed experimental data on transport properties of dense plasmas.
ISSN:1539-3755
1550-2376
DOI:10.1103/PhysRevE.90.013104