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Predicting Complete Basis Set Limit Quasiparticle Energies from Triple-ζ Calculations.

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We developed a linear model to predict basis set incompleteness errors in GW quasi-particle (QP) energies using only orbital kinetic energy. This method accurately extrapolates QP energies to the complete basis set limit, improving computational chemistry accuracy.

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Area of Science:

  • Computational Chemistry
  • Quantum Chemistry
  • Materials Science

Background:

  • Basis set incompleteness errors (BSIEs) are significant in GW calculations.
  • Accurate prediction of quasi-particle (QP) energies is crucial for electronic structure.
  • Existing extrapolation methods can be computationally expensive or inaccurate.

Purpose of the Study:

  • To develop a simple linear model for estimating BSIEs in GW QP energies.
  • To enable accurate extrapolation of QP energies to the complete basis set (CBS) limit.
  • To provide a computationally efficient alternative to traditional extrapolation techniques.

Main Methods:

  • A linear model was developed using orbital kinetic energy to predict BSIEs.
  • The model was parametrized for G0W0, qsGW, and vertex-corrected GW methods.
  • Reference CBS limit values were obtained using extensive correlation-consistent basis sets (TZ/6Z) for molecules with 10 elements.

Main Results:

  • The developed model achieves BSIE extrapolation to the CBS limit with 20-30 meV accuracy for Gaussian- and Slater-type orbital basis sets.
  • The model allows extrapolation from triple-zeta (TZ) basis sets.
  • The commonly used inverse linear extrapolation method was found to produce larger errors unless a quadruple-zeta calculation is included.

Conclusions:

  • A simple linear model effectively estimates BSIEs for GW QP energies.
  • The model provides accurate CBS extrapolation, particularly useful for Gaussian- and Slater-type orbital basis sets.
  • This approach offers a more accurate and efficient way to obtain reliable QP energies compared to standard extrapolation methods.