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An atomic orbital represents the three-dimensional regions in an atom where an electron has the highest probability to reside. The radial distribution function indicates the total probability of finding an electron within the thin shell at a distance r from the nucleus. The atomic orbitals have distinct shapes which are determined by l, the angular momentum quantum number. The orbitals are often drawn with a boundary surface, enclosing densest regions of the cloud.
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The mathematical expression known as the wave function, ψ, contains information about each orbital and the wavelike properties of electrons in an isolated atom. When atoms are bound together in a molecule, the wave functions combine to produce new mathematical descriptions that have different shapes. This process of combining the wave functions for atomic orbitals is called hybridization and is mathematically accomplished by the linear combination of atomic orbitals. The new orbitals that...
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Orbitals are the areas outside of the atomic nucleus where electrons are most likely to reside. They are characterized by different energy levels, shapes, and three-dimensional orientations. The location of electrons is described most generally by a shell or principal energy level, then by a subshell within each shell, and finally, by individual orbitals found within the subshells.
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Low-Scaling Self-Consistent Minimization of a Density Matrix Based Random Phase Approximation Method in the Atomic

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A new self-consistent random phase approximation (RPA) method offers parameter-free calculations, accurately describing noncovalent interactions and dipole moments for large molecular systems.

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Area of Science:

  • Computational Chemistry
  • Quantum Chemistry
  • Theoretical Physics

Background:

  • Accurate calculation of molecular properties is crucial in chemistry and physics.
  • Random Phase Approximation (RPA) methods are valuable for describing electron correlation, but can be computationally demanding.
  • Existing methods often struggle with self-consistency or computational scaling for large systems.

Purpose of the Study:

  • To develop an efficient and self-consistent Random Phase Approximation (RPA) method in atomic orbital (AO) space.
  • To overcome limitations of existing RPA methods, including computational cost and accuracy for specific interactions.
  • To enable accurate calculations for larger molecular systems.

Main Methods:

  • Minimization of RPA energy with respect to the one-particle density matrix in AO space.
  • Approximation of the RPA Hamiltonian using the Hartree-Fock Hamiltonian for parameter-free, self-consistent calculations.
  • Introduction of Cholesky decomposed projectors to manage computational prefactors in AO-based methods.
  • Exploitation of orbital locality for asymptotically quadratic scaling.

Main Results:

  • The developed self-consistent RPA method is parameter-free.
  • The method outperforms post-Kohn-Sham RPA for noncovalent interactions.
  • Accurate dipole moments were obtained, indicating high-quality electron densities.
  • The method achieves asymptotically quadratic scaling, overcoming the prefactor drawback of AO-based methods.

Conclusions:

  • The new self-consistent RPA method provides an efficient and accurate approach for electronic structure calculations.
  • The method's scalability opens possibilities for studying large molecular systems.
  • This work advances the application of RPA in computational chemistry and materials science.