Linear-ScalingLocal Natural Orbital-Based Full TriplesTreatment in Coupled-Cluster Theory

We present an efficient, asymptotically linear-scaling implementation of the canonically O(N8) coupled-cluster method with singles, doubles, and full triples excitations (CCSDT) method. We apply the domain-based local pair natural orbital (DLPNO) approach for computing CCSDT amplitudes. Our method, called DLPNO–CCSDT, uses the converged coupled-cluster amplitudes from a preceding DLPNO–CCSD­(T) computation as a starting point for the solution of the CCSDT equations in the local natural orbital basis. To simplify the working equations, we <i>t</i><sub>1</sub>-dress our two-electron integrals and Fock matrices, allowing our equations to take on the form of CCDT. With appropriate parameters, our method can recover more than 99.99% of the total canonical CCSDT correlation energy. In addition, we demonstrate that our method consistently yields sub-kJ mol<sup>–1</sup> errors in relative energies when compared to canonical CCSDT, and, likewise, when computing the difference between CCSDT and CCSD­(T). Finally, to highlight the low scaling of our algorithm, we present timings on linear alkanes (up to 30 carbons and 730 basis functions) and water clusters (up to 131 water molecules and 3144 basis functions).

Publication Details

Journal
Figshare
Published
2025-02-21
DOI
https://doi.org/10.1021/acs.jctc.4c01716.s001
Primary Topic
Advanced Chemical Physics Studies
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article
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article

Linear-ScalingLocal Natural Orbital-Based Full TriplesTreatment in Coupled-Cluster Theory

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Advanced Chemical Physics Studies
article

Linear-ScalingLocal Natural Orbital-Based Full TriplesTreatment in Coupled-Cluster Theory

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Abstract

We present an efficient, asymptotically linear-scaling implementation of the canonically O(N8) coupled-cluster method with singles, doubles, and full triples excitations (CCSDT) method. We apply the domain-based local pair natural orbital (DLPNO) approach for computing CCSDT amplitudes. Our method, called DLPNO–CCSDT, uses the converged coupled-cluster amplitudes from a preceding DLPNO–CCSD­(T) computation as a starting point for the solution of the CCSDT equations in the local natural orbital basis. To simplify the working equations, we <i>t</i><sub>1</sub>-dress our two-electron integrals and Fock matrices, allowing our equations to take on the form of CCDT. With appropriate parameters, our method can recover more than 99.99% of the total canonical CCSDT correlation energy. In addition, we demonstrate that our method consistently yields sub-kJ mol<sup>–1</sup> errors in relative energies when compared to canonical CCSDT, and, likewise, when computing the difference between CCSDT and CCSD­(T). Finally, to highlight the low scaling of our algorithm, we present timings on linear alkanes (up to 30 carbons and 730 basis functions) and water clusters (up to 131 water molecules and 3144 basis functions).

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