Ab-initio simulations and measurements of the free-free opacity in Aluminum
arXiv:1806.02726 · doi:10.1103/PhysRevE.100.043207
Abstract
The free-free opacity in dense systems is a property that both tests our fundamental understanding of correlated many-body systems, and is needed to understand the radiative properties of high energy-density plasmas. Despite its importance, predictive calculations of the free-free opacity remain challenging even in the condensed matter phase for simple metals. Here we show how the free-free opacity can be modelled at finite-temperatures via time-dependent density functional theory, and illustrate the importance of including local field corrections, core polarization and self-energy corrections. Our calculations for ground-state Al are shown to agree well with experimental opacity measurements performed on the Artemis laser facility across a wide range of x-ray to ultraviolet wavelengths. We extend our calculations across the melt to the warm-dense matter regime, and find good agreement with advanced plasma models based on inverse bremsstrahlung at temperatures above 10 eV.
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- Time-resolved XUV Opacity Measurements of Warm-Dense Aluminium
- Excited States in Warm and Hot Dense Matter
- Correlations Between Conduction Electrons in Dense Plasmas
- On collisional free-free photon absorption in warm dense matter
- Charge State Distributions in Dense Plasmas
- Electron Dynamics at High-Energy Densities in Nickel from Non-linear Resonant X-ray Absorption Spectra
- A Rate Model of Electron Populations for Non-linear High-Fluence X-ray Absorption Near-Edge Spectra
- Exploring relaxation dynamics in warm dense plasmas by tailoring non-thermal electron distributions with a free electron laser
- High-temperature self-energy corrections to x-ray absorption spectra