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Understanding XANES spectra of two-temperature warm dense copper using ab initio simulations
- Source :
- Physical Review B, Physical Review B, American Physical Society, 2020, 101 (12), ⟨10.1103/PhysRevB.101.125127⟩, Physical Review B, 2020, 101 (12), ⟨10.1103/PhysRevB.101.125127⟩
- Publication Year :
- 2020
- Publisher :
- American Physical Society, 2020.
-
Abstract
- Using ab initio molecular-dynamics simulations combined with linear-response theory, we studied the x-ray absorption near-edge spectra (XANES) of a two-temperature dense copper plasma. As the temperature increases, XANES spectra exhibit a pre-edge structure balanced by a reduction of the absorption just behind the edge. By performing systematic simulations for various thermodynamic conditions, we establish a formulation to deduce the electronic temperature Te directly from the spectral integral of the pre-edge that can be used for various thermodynamic conditions encountered in a femtosecond heating experiment where thermal non equilibrium and expanded states have to be considered.<br />Comment: 9 pages, 10 figures submitted to Physical Review B
- Subjects :
- [PHYS]Physics [physics]
Condensed Matter - Materials Science
Materials science
Ab initio
chemistry.chemical_element
Materials Science (cond-mat.mtrl-sci)
FOS: Physical sciences
02 engineering and technology
Plasma
Edge (geometry)
021001 nanoscience & nanotechnology
7. Clean energy
01 natural sciences
Copper
Molecular physics
Physics - Plasma Physics
XANES
Spectral line
Plasma Physics (physics.plasm-ph)
chemistry
0103 physical sciences
Femtosecond
010306 general physics
0210 nano-technology
Absorption (electromagnetic radiation)
Subjects
Details
- Language :
- English
- ISSN :
- 24699950 and 24699969
- Database :
- OpenAIRE
- Journal :
- Physical Review B, Physical Review B, American Physical Society, 2020, 101 (12), ⟨10.1103/PhysRevB.101.125127⟩, Physical Review B, 2020, 101 (12), ⟨10.1103/PhysRevB.101.125127⟩
- Accession number :
- edsair.doi.dedup.....453875dddf4a038514ccd89eceed892b
- Full Text :
- https://doi.org/10.1103/PhysRevB.101.125127⟩