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A full coupled-cluster singles and doubles model: The inclusion of disconnected triples

George D. Purvis; Rodney J. Bartlett · The Journal of Chemical Physics · 1982

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The coupled-cluster singles and doubles model (CCSD) is derived algebraically, presenting the full set of equations for a general reference function explicitly in spin–orbital form. The computational implementation of the CCSD model, which involves cubic and quartic terms, is discussed and results are reported and compared with full CI calculations for H2O and BeH2. We demonstrate that the CCSD exponential ansatz sums higher-order correlation effects efficiently even for BeH2, near its transition state geometry where quasidegeneracy efforts are quite large, recovering 98% of the full CI correlation energy. For H2O, CCSD plus the fourth-order triple excitation correction agrees with the full CI energy to 0.5 kcal/mol. Comparisons with low-order models provide estimates of the effect of the higher-order terms T1T2, T21T2, T31, and T41 on the correlation energy.

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APA 7

Purvis, G. D. & Bartlett, R. J. (1982). A full coupled-cluster singles and doubles model: The inclusion of disconnected triples. https://doi.org/10.1063/1.443164

MLA

Purvis, George D, and Rodney J. Bartlett. "A full coupled-cluster singles and doubles model: The inclusion of disconnected triples." 1982. https://doi.org/10.1063/1.443164.

Chicago

Purvis, George D. and Rodney J. Bartlett. 1982. "A full coupled-cluster singles and doubles model: The inclusion of disconnected triples.". https://doi.org/10.1063/1.443164.

Harvard

Purvis, G. D. and Bartlett, R. J. 1982, A full coupled-cluster singles and doubles model: The inclusion of disconnected triples, The Journal of Chemical Physics, available at: https://doi.org/10.1063/1.443164 [Accessed 8 Aug. 2026].

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Title
A full coupled-cluster singles and doubles model: The inclusion of disconnected triples
Author / contributors
George D. Purvis; Rodney J. Bartlett
Publisher
The Journal of Chemical Physics
Publication year
1982
Language
English

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