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Low-Scaling Self-Consistent Minimization of a Density Matrix Based Random Phase Approximation Method in the Atomic Orbital Space

机译:基于密度矩阵的随机相位近似方法在原子轨道空间中的低缩放自我一致性最小化

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摘要

An efficient minimization of the random phase approximation (RPA) energy with respect to the one-particle density matrix in the atomic orbital space is presented. The problem of imposing full self-consistency on functionals depending on the potential itself is bypassed by approximating the RPA Hamiltonian on the basis of the well-known Hartree-Fock Hamiltonian making our self-consistent RPA method completely parameter-free. It is shown that the new method not only outperforms post-Kohn-Sham RPA in describing noncovalent interactions but also gives accurate dipole moments demonstrating the high quality of the calculated densities. Furthermore, the main drawback of atomic orbital based methods, in increasing the prefactor as compared to their canonical counterparts, is overcome by introducing Cholesky decomposed projectors allowing the use of large basis sets. Exploiting the locality of atomic and/or Cholesky orbitals enables us to present a self-consistent RPA method which shows asymptotically quadratic scaling opening the door for calculations on large molecular systems.
机译:提出了相对于原子轨道空间中的单粒子密度矩阵的随机相位近似(RPA)能量的有效最小化。根据众所周知的Hartree-Fock Hamiltonian,通过近似RPA Hamiltonian,绕过潜在本身对潜在本身施加完全自我一致性的问题。结果表明,新方法不仅优于kohn-sham rpa后表明非共价相互作用,而且给出了准确的偶极矩,证明了高质量的计算密度。此外,通过引入巧克力分解的投影仪允许使用大量基础套件,克服了原子轨道基于方法的主要基于轨道的方法的主要缺点。利用原子和/或尖锐轨道的局部性使我们能够呈现一种自我一致的RPA方法,该方法显示出对大分子系统计算的渐近二次缩放的渐近缩放。

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