4.6 Article

Fully self-consistent finite-temperature GW in Gaussian Bloch orbitals for solids

Journal

PHYSICAL REVIEW B
Volume 106, Issue 23, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevB.106.235104

Keywords

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Funding

  1. Office of Science of the U.S. Department of Energy [DE-AC05-00OR22725]
  2. Department of Energy [DE-SC0022198]
  3. U.S. Department of Energy, Office of Science, Office of Advanced Scientific Computing Research and Office of Basic Energy Sciences, Scientific Discovery through Advanced Computing (SciDAC) program [DE-SC0022198]
  4. Simons Foundation via the Simons Collaboration on the Many-Electron problem
  5. U.S. Department of Energy (DOE) [DE-SC0022198] Funding Source: U.S. Department of Energy (DOE)

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In this paper, we present the algorithmic and implementation details for the fully self-consistent finite-temperature GW method in Gaussian Bloch orbitals for solids. The method is tested by evaluating the band gaps of selected semiconductors and insulators, and it shows agreement with other implementations. By migrating computationally intensive calculations to graphics processing units, optimal performance is achieved on large supercomputers. This work demonstrates the applicability of Gaussian orbital based scGW for correlated material simulations.
We present algorithmic and implementation details for the fully self-consistent finite-temperature GW method in Gaussian Bloch orbitals for solids. Our implementation is based on the finite-temperature Green's function formalism in which all equations are solved on the imaginary axis, without resorting to analytical continuation during the self-consistency. No quasiparticle approximation is employed and all matrix elements of the selfenergy are explicitly evaluated. The method is tested by evaluating the band gaps of selected semiconductors and insulators. We show agreement with other, differently formulated, finite-temperature scGW implementations when finite-size corrections and basis-set errors are taken into account. By migrating computationally intensive calculations to graphics processing units, we obtain scalable results on large supercomputers with nearly optimal performance. Our work demonstrates the applicability of Gaussian orbital based scGW for ab initio correlated material simulations and provides a sound starting point for embedding methods built on top of GW.

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