Bulletin of the American Physical Society
66th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 7–11, 2024; Atlanta, Georgia
Session TO09: High Energy Density Science: Warm Dense Matter
9:30 AM–12:30 PM,
Thursday, October 10, 2024
Hyatt Regency
Room: Hanover DE
Chair: Ryan Rygg, Laboratory for Laser Energetics
Abstract: TO09.00013 : Improving the accuracy of warm-dense matter simulations with temperature-dependent meta-GGA exchange-correlation functional – fT(r2)SCAN*
11:54 AM–12:06 PM
Presenter:
Katerina P Hilleke
(Laboratory for Laser Energetics)
Authors:
Katerina P Hilleke
(Laboratory for Laser Energetics)
Valentin V Karasiev
(LLE, Univ. of Rochester)
Suxing Hu
(Laboratory for Laser Energetics, University of Rochester)
However, a growing body of work is devoted to DFT in the warm dense matter regime, where intense pressures and temperatures drive ground-state approximations beyond their limits. XC functionals with explicit temperature effects are needed to improve the accuracy of such DFT simulations.
Here, following the strategy adopted for fully-thermal LDA (KSDT) and GGA (KDT16) XC functionals, we present a meta-GGA XC free-energy functional with explicit temperature dependence, based on the SCAN functional: fTSCAN. fTSCAN has been benchmarked against high-temperature PIMC data and demonstrates proper low-temperature behavior for high transferability within a range of conditions from the ambient to the extreme.
We report progress as well towards an orbital-free extension of fTSCAN capable of improved scaling as well as the adaptation of fTSCAN to the regularized-restored (r2) SCAN formulation for improvements in numerical stability.
This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0004144 and US National Science Foundation PHY Grant No. 2205521.
*This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0004144 and US National Science Foundation PHY Grant No. 2205521.
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