Non-thermal evolution of dense plasmas driven by intense x-ray fields

Author:

Ren Shenyuan,Shi Yuanfeng,van den Berg Quincy Y.ORCID,Kasim Muhammad F.,Chung Hyun-Kyung,Fernandez-Tello Elisa V.,Velarde PedroORCID,Wark Justin S.ORCID,Vinko Sam M.ORCID

Abstract

AbstractThe advent of x-ray free-electron lasers has enabled a range of new experimental investigations into the properties of matter driven to extreme conditions via intense x-ray-matter interactions. The femtosecond timescales of these interactions lead to the creation of transient high-energy-density plasmas, where both the electrons and the ions may be far from local thermodynamic equilibrium. Predictive modelling of such systems remains challenging because of the different timescales at which electrons and ions thermalize, and because of the vast number of atomic configurations required to describe highly-ionized plasmas. Here we present CCFLY, a code designed to model the time-dependent evolution of both electron distributions and ion states interacting with intense x-ray fields on ultra-short timescales, far from local thermodynamic equilibrium. We explore how the plasma relaxes to local thermodynamic equilibrium on femtosecond timescales in terms of the charge state distribution, electron density, and temperature.

Funder

RCUK | Engineering and Physical Sciences Research Council

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

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