Non-thermal evolution of dense plasmas driven by intense x-ray fields
<p>The 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-de...
Main Authors: | , , , , , |
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Format: | Journal article |
Language: | English |
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Springer Nature
2023
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_version_ | 1826310566167183360 |
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author | Ren, S Shi, Y van den Berg, QY Kasim, MF Wark, JS Vinko, SM |
author_facet | Ren, S Shi, Y van den Berg, QY Kasim, MF Wark, JS Vinko, SM |
author_sort | Ren, S |
collection | OXFORD |
description | <p>The 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.</p> |
first_indexed | 2024-03-07T07:53:50Z |
format | Journal article |
id | oxford-uuid:fc056a04-34c2-4877-b999-d8b467627327 |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T07:53:50Z |
publishDate | 2023 |
publisher | Springer Nature |
record_format | dspace |
spelling | oxford-uuid:fc056a04-34c2-4877-b999-d8b4676273272023-08-03T11:15:58ZNon-thermal evolution of dense plasmas driven by intense x-ray fieldsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:fc056a04-34c2-4877-b999-d8b467627327EnglishSymplectic ElementsSpringer Nature2023Ren, SShi, Yvan den Berg, QYKasim, MFWark, JSVinko, SM<p>The 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.</p> |
spellingShingle | Ren, S Shi, Y van den Berg, QY Kasim, MF Wark, JS Vinko, SM Non-thermal evolution of dense plasmas driven by intense x-ray fields |
title | Non-thermal evolution of dense plasmas driven by intense x-ray fields |
title_full | Non-thermal evolution of dense plasmas driven by intense x-ray fields |
title_fullStr | Non-thermal evolution of dense plasmas driven by intense x-ray fields |
title_full_unstemmed | Non-thermal evolution of dense plasmas driven by intense x-ray fields |
title_short | Non-thermal evolution of dense plasmas driven by intense x-ray fields |
title_sort | non thermal evolution of dense plasmas driven by intense x ray fields |
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