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J. Chem. Phys. 130, 114108 (2009); doi:10.1063/1.3086717 (18 pages)

Efficient and accurate local approximations to coupled-electron pair approaches: An attempt to revive the pair natural orbital method

Frank Neese1,2, Frank Wennmohs1, and Andreas Hansen1

1Lehrstuhl für Theoretische Chemie, Institut für Physikalische und Theoretische Chemie, Universität Bonn, Wegelerstr. 12, D-53115 Bonn, Germany
2Max-Planck Institut für Bioanorganische Chemie, Stiftstr. 12-14, D-45470 Mülheim an der Ruhr, Germany

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(Received 26 November 2008; accepted 2 February 2009; published online 20 March 2009)

Coupled-electron pair approximations (CEPAs) and coupled-pair functionals (CPFs) have been popular in the 1970s and 1980s and have yielded excellent results for small molecules. Recently, interest in CEPA and CPF methods has been renewed. It has been shown that these methods lead to competitive thermochemical, kinetic, and structural predictions. They greatly surpass second order Møller–Plesset and popular density functional theory based approaches in accuracy and are intermediate in quality between CCSD and CCSD(T) in extended benchmark studies. In this work an efficient production level implementation of the closed shell CEPA and CPF methods is reported that can be applied to medium sized molecules in the range of 50–100 atoms and up to about 2000 basis functions. The internal space is spanned by localized internal orbitals. The external space is greatly compressed through the method of pair natural orbitals (PNOs) that was also introduced by the pioneers of the CEPA approaches. Our implementation also makes extended use of density fitting (or resolution of the identity) techniques in order to speed up the laborious integral transformations. The method is called local pair natural orbital CEPA (LPNO-CEPA) (LPNO-CPF). The implementation is centered around the concepts of electron pairs and matrix operations. Altogether three cutoff parameters are introduced that control the size of the significant pair list, the average number of PNOs per electron pair, and the number of contributing basis functions per PNO. With the conservatively chosen default values of these thresholds, the method recovers about 99.8% of the canonical correlation energy. This translates to absolute deviations from the canonical result of only a few kcal mol−1. Extended numerical test calculations demonstrate that LPNO-CEPA (LPNO-CPF) has essentially the same accuracy as parent CEPA (CPF) methods for thermochemistry, kinetics, weak interactions, and potential energy surfaces but is up to 500 times faster. The method performs best in conjunction with large and flexible basis sets. These results open the way for large-scale chemical applications.

© 2009 American Institute of Physics

Article Outline

  1. INTRODUCTION
  2. THEORY
    1. The closed-shell CISD and CEPA equations
    2. PNOs
    3. Improved PNOs
    4. PNO form of the residual
    5. Approximations
    6. Perturbative correction
    7. Implementation
  3. NUMERICAL RESULTS
    1. Computational details
    2. Accuracy
      1. Dependence of the results on the thresholds
      2. PNO distributions
      3. Dependence of the results on the localization method
      4. Dependence of the results on the PNO construction method
      5. Study of the numerical error
      6. Reaction energies
      7. Weak interactions
    3. Efficiency
      1. Scaling
      2. Analysis of timings
    4. Smoothness of potential energy surfaces
      1. Bond dissociation: Ketene
      2. Rotational barriers
  4. SUMMARY AND DISCUSSION

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KEYWORDS and PACS

PACS

  • 31.15.E-

    Density-functional theory

  • 31.15.bw

    Coupled-cluster theory

  • 82.60.-s

    Chemical thermodynamics

  • 31.50.-x

    Potential energy surfaces

  • 33.15.Bh

    General molecular conformation and symmetry; stereochemistry

PUBLICATION DATA

ISSN:

0021-9606 (print)  
1089-7690 (online)

For access to fully linked references, you need to log in.
    M. Schütz, G. Hetzer, and H. J. Werner, J. Chem. Phys. 111, 5691 (1999)JCPSA6000111000013005691000001.

    M. Heckert, M. Kallay, D. P. Tew, W. Klopper, and J. Gauss, J. Chem. Phys. 125, 044108 (2006)JCPSA6000125000004044108000001
    Y. J. Bomble, J. Vazquez, M. Kallay, C. Michauk, P. G. Szalay, A. G. Csaszar, J. Gauss, and J. F. Stanton, ibid. 125, 064108 (2006)JCPSA6000125000006064108000001
    A. Tajti, P. G. Szalay, A. G. Csaszar, M. Kallay, J. Gauss, E. F. Valeev, B. A. Flowers, J. Vazquez, and J. F. Stanton, ibid. 121, 11599 (2004)JCPSA6000121000023011599000001.

    A. D. Boese, M. Oren, O. Atasoylu, J. M. L. Martin, M. Kallay, and J. Gauss, J. Chem. Phys. 120, 4129 (2004)JCPSA6000120000009004129000001
    A. Karton, E. Rabinovich, J. M. L. Martin, and B. Ruscic, ibid. 125, 144108 (2006)JCPSA6000125000014144108000001.

    C. Hampel and H. J. Werner, J. Chem. Phys. 104, 6286 (1996)JCPSA6000104000016006286000001
    M. Schütz and H. -J. Werner, ibid. 114, 661 (2001)JCPSA6000114000002000661000001.

    T. Korona and H. J. Werner, J. Chem. Phys. 118, 3006 (2003)JCPSA6000118000007003006000001.

    H. -J. Werner, F. R. Manby, and P. J. Knowles, J. Chem. Phys. 118, 8149 (2003)JCPSA6000118000018008149000001.

    R. A. Mata and H. J. Werner, J. Chem. Phys. 125, 184110 (2006)JCPSA6000125000018184110000001.

    A. A. Auer and M. Nooijen, J. Chem. Phys. 125, 024104 (2006)JCPSA6000125000002024104000001.

    M. Schütz, J. Chem. Phys. 116, 8772 (2002)JCPSA6000116000020008772000001.

    D. Kats, T. Korona, and M. Schütz, J. Chem. Phys. 125, 104106 (2006)JCPSA6000125000010104106000001
    D. Kats, T. Korona, and M. Schütz, ibid. 127, 064107 (2007)JCPSA6000127000006064107000001.

    N. J. Russ and T. D. Crawford, J. Chem. Phys. 121, 691 (2004)JCPSA6000121000002000691000001.

    J. E. Subotnik, A. Sodt, and M. Head-Gordon, J. Chem. Phys. 128, 034103 (2008)JCPSA6000128000003034103000001.

    W. Meyer, J. Chem. Phys. 58, 1017 (1973)JCPSA6000058000003001017000001.

    R. Ahlrichs, P. Scharf, and C. Erhardt, J. Chem. Phys. 82, 890 (1985)JCPSA6000082000002000890000001.

    P. R. Taylor, J. Chem. Phys. 74, 1256 (1981)JCPSA6000074000002001256000001.

    P. Fulde and H. Stoll, J. Chem. Phys. 97, 4185 (1992)JCPSA6000097000006004185000001.

    J. P. Malrieu, J. P. Daudey, and R. Caballol, J. Chem. Phys. 101, 8908 (1994)JCPSA6000101000010008908000001
    J. P. Daudey, J. L. Heully, and J. P. Malrieu, ibid. 99, 1240 (1993)JCPSA6000099000002001240000001.

    C. Edmiston and M. Krauss, J. Chem. Phys. 42, 1119 (1965)JCPSA6000042000003001119000001
    C. Edmiston, ibid. 45, 1833 (1966)JCPSA6000045000005001833000001.

    P. Pulay, S. Saebø, and W. Meyer, J. Chem. Phys. 81, 1901 (1984)JCPSA6000081000004001901000001.

    P. O. Löwdin, Phys. Rev. 97, 1474 (1955).

    P. Pulay, S. Saebø, and W. Meyer, J. Chem. Phys. 81, 1901 (1984)JCPSA6000081000004001901000001.

    A. Schäfer, H. Horn, and R. Ahlrichs, J. Chem. Phys. 97, 2571 (1992)JCPSA6000097000004002571000001.

    A. Schäfer, C. Huber, and R. Ahlrichs, J. Chem. Phys. 100, 5829 (1994)JCPSA6000100000008005829000001.

    F. Weigend, F. Furche, and R. Ahlrichs, J. Chem. Phys. 119, 12753 (2003)JCPSA6000119000024012753000001.

    J. E. Subotnik, A. Sodt, and M. Head-Gordon, J. Chem. Phys. 128, 034103 (2008)JCPSA6000128000003034103000001.


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