Applying the Liouville–Lanczos method of time-dependent density-functional theory to warm dense matter

Ab initio modeling of dynamic structure factors (DSF) and related density response properties in the warm dense matter (WDM) regime is a challenging computational task. The DSF, convolved with a probing X-ray beam and instrument function, is measured in X-ray Thomson scattering (XRTS) experiments, which allow the study of electronic structure properties at the microscopic level. Among the various ab initio methods, linear-response time-dependent density-functional theory (LR-TDDFT) is a key framework for simulating the DSF. The standard approach in LR-TDDFT for computing the DSF relies on the orbital representation. A significant drawback of this method is the unfavorable scaling of the number of required empty bands as the wavenumber increases, making LR-TDDFT impractical for modeling XRTS measurements over large energy scales, such as in backward scattering geometry. In this work, we consider and test an alternative approach to LR-TDDFT that employs the Liouville–Lanczos (LL) method for simulating the DSF of WDM. This approach does not require empty states and allows the DSF at large momentum transfer values and over a broad frequency range to be accessed. We compare the results obtained from the LL method with those from the solution of Dyson’s equation using the standard LR-TDDFT within the projector augmented-wave formalism for isochorically heated aluminum and warm dense hydrogen. Additionally, we utilize exact path integral Monte Carlo results for the imaginary-time density-density correlation function (ITCF) of warm dense hydrogen to rigorously benchmark the LL approach. We discuss the application of the LL method for calculating DSFs and ITCFs at different wavenumbers, the effects of pseudopotentials, and the role of Lorentzian smearing. The successful validation of the LL method under WDM conditions makes it a valuable addition to the ab initio simulation landscape, supporting experimental efforts and advancing WDM theory.

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Publication Details

Journal
Matter and Radiation at Extremes
Published
2025-05-05
DOI
https://doi.org/10.1063/5.0263947
Citations
5
Primary Topic
Advanced Chemical Physics Studies
Type
article
Field-Weighted Citation Impact
6.23

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article

Applying the Liouville–Lanczos method of time-dependent density-functional theory to warm dense matter

Sebastian Schwalbe, Jan Vorberger, Tobias Dornheim, Thomas R. Preston et al.
5 citations
Matter and Radiation at Extremes
Advanced Chemical Physics Studies
6.23
article

Applying the Liouville–Lanczos method of time-dependent density-functional theory to warm dense matter

Sebastian Schwalbe, Jan Vorberger, Tobias Dornheim, Thomas R. Preston, Zhandos A. Moldabekov, Thomas Gawne
article en
5 citations

Abstract

Ab initio modeling of dynamic structure factors (DSF) and related density response properties in the warm dense matter (WDM) regime is a challenging computational task. The DSF, convolved with a probing X-ray beam and instrument function, is measured in X-ray Thomson scattering (XRTS) experiments, which allow the study of electronic structure properties at the microscopic level. Among the various ab initio methods, linear-response time-dependent density-functional theory (LR-TDDFT) is a key framework for simulating the DSF. The standard approach in LR-TDDFT for computing the DSF relies on the orbital representation. A significant drawback of this method is the unfavorable scaling of the number of required empty bands as the wavenumber increases, making LR-TDDFT impractical for modeling XRTS measurements over large energy scales, such as in backward scattering geometry. In this work, we consider and test an alternative approach to LR-TDDFT that employs the Liouville–Lanczos (LL) method for simulating the DSF of WDM. This approach does not require empty states and allows the DSF at large momentum transfer values and over a broad frequency range to be accessed. We compare the results obtained from the LL method with those from the solution of Dyson’s equation using the standard LR-TDDFT within the projector augmented-wave formalism for isochorically heated aluminum and warm dense hydrogen. Additionally, we utilize exact path integral Monte Carlo results for the imaginary-time density-density correlation function (ITCF) of warm dense hydrogen to rigorously benchmark the LL approach. We discuss the application of the LL method for calculating DSFs and ITCFs at different wavenumbers, the effects of pseudopotentials, and the role of Lorentzian smearing. The successful validation of the LL method under WDM conditions makes it a valuable addition to the ab initio simulation landscape, supporting experimental efforts and advancing WDM theory.

Matter and Radiation at ExtremesVol. 10(4)
Helmholtz-Zentrum Dresden-Rossendorf (DE), Center for Advanced Systems Understanding (DE), European X-Ray Free-Electron Laser (DE)
Bundesministerium für Bildung und Forschung, Freistaat Sachsen, HORIZON EUROPE European Research Council
Openalex Percentile: Top 4%
Advanced Chemical Physics Studies
6.23
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