Reconciling Ionization Energies and Band Gaps of Warm Dense Matter Derived with Ab Initio Simulations and Average Atom Models
ORAL
Abstract
Average atom (AA) models allow one to efficiently compute electronic and optical properties of materials over a wide range of conditions and are often employed to interpret experimental data. However, at high pressure, predictions from AA models have been shown to disagree with results from ab initio computer simulations. We represent a new AA model, AvIon, that computes the electronic eigenstates with novel boundary conditions within the ion sphere. Bound and free states are derived consistently. We drop the common AA assumption that the free-particle spectrum starts at the potential threshold, which we found to be incompatible with ab initio calculations. We perform ab initio simulations of crystalline and liquid states for several elements over a wide range of densities and show that the computed band structures are in excellent agreement with predictions from AvIon.
*GM acknowledges support from the Programme National de Physique Stellaire (PNPS) of CNRS/INSU, MB from the Center of Advanced Systems Understanding, FS from the European Union through a Marie Sklodowska-Curie action (grant 750901) and BM from the National Science Foundation-Department of Energy (DOE) partnership for plasma science
and engineering (grant DE-SC0016248) and by the DOE-NNSA (grant DE-NA0003842).
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Presenters
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Maximilian Boehme
- CASUS, Helmholtz Zentrum Dresden-Rossendorf
- Matter Under Extreme Conditions, Center for Advanced Systems Understanding