Electronic Density Response of Warm Dense Hydrogen: Ab initio Path Integral Monte Carlo Simulations
arXiv:2203.01797 · doi:10.1103/PhysRevLett.129.066402
Abstract
The properties of hydrogen under extreme conditions are important for many applications, including inertial confinement fusion and astrophysical models. A key quantity is given by the electronic density response to an external perturbation, which is probed in X-ray Thomson scattering (XRTS) experiments -- the state of the art diagnostics from which system parameters like the free electron density , the electronic temperature , and the charge state can be inferred. In this work, we present highly accurate path integral Monte Carlo (PIMC) results for the electronic density response of hydrogen. We obtain the exchange-correlation (XC) kernel , which is of central relevance for many applications, such as time-dependent density functional theory (TD-DFT). This gives us a first unbiased look into the electronic density response of hydrogen in the warm-dense matter regime, thereby opening up a gamut of avenues for future research.
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Cited by in corpus (21)
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- First principles simulations of dense hydrogen
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- X-ray Thomson scattering spectra from DFT-MD simulations based on a modified Chihara formula
- Effective electronic forces and potentials from ab initio path integral Monte Carlo simulations
- Linear-response time-dependent density functional theory approach to warm dense matter with adiabatic exchange--correlation kernels
- Non-empirical mixing coefficient for hybrid XC functionals from analysis of the XC kernel
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- Generalized density functional theory framework for the non-linear density response of quantum many-body systems
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