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- •Table of Contents
- •Preface
- •Contributors
- •1. INTRODUCTION
- •2. HIERARCHIES OF AB INITIO THEORY
- •2.3. Computational Cost
- •3.2. The CCSD(T) Model
- •4.1. Electronic and Nuclear Contributions
- •4.2. Dependence on the AO Basis Set
- •5.2. Extrapolations from Principal Expansions
- •6. CALIBRATION OF THE EXTRAPOLATION TECHNIQUE
- •6.2. Total Electronic Energy
- •6.3. Core Contributions to AEs
- •7. MOLECULAR VIBRATIONAL CORRECTIONS
- •8. RELATIVISTIC CONTRIBUTIONS
- •9. CALCULATION OF ATOMIZATION ENERGIES
- •10. CONCLUSIONS AND PERSPECTIVES
- •2. STEPS IN THE W1 AND W2 THEORIES, AND THEIR JUSTIFICATION
- •2.1. Reference Geometry
- •2.2. The SCF Component of TAE
- •2.3. The CCSD Valence Correlation Component of TAE
- •2.4. Connected Triple Excitations: the (T) Valence Correlation Component of TAE
- •2.6. Scalar Relativistic Correction
- •3. PERFORMANCE OF W1 AND W2 THEORIES
- •3.2. Electron Affinities (the G2/97 Set)
- •3.4. Heats of Formation (the G2/97 Set)
- •3.5. Proton Affinities
- •4. VARIANTS AND SIMPLIFICATIONS
- •4.2. W1h and W2h Theories
- •4.5. W1c Theory
- •4.6. Detecting Problems
- •5. EXAMPLE APPLICATIONS
- •5.1. Heats of Vaporization of Boron and Silicon
- •5.2. Validating DFT Methods for Transition States: the Walden Inversion
- •5.3. Benzene as a ”Stress Test” of the Method
- •6. CONCLUSIONS AND PROSPECTS
- •1. INTRODUCTION
- •2. THE G3/99 TEST SET
- •4. G3S THEORY
- •5. G3X THEORY
- •6. DENSITY FUNCTIONAL THEORY
- •7. CONCLUDING REMARKS
- •1. INTRODUCTION
- •2. PAIR NATURAL ORBITAL EXTRAPOLATIONS
- •3. CURRENT CBS MODELS
- •4. TRANSITION STATES
- •5. EXPLICIT FUNCTIONS OF THE INTERELECTRON DISTANCE
- •7. NEW DEVELOPMENTS
- •7.1. The SCF Limit
- •7.2. The CBS Limit for the MP2 Correlation Energy
- •7.4. Total Energies
- •8. ENZYME KINETICS AND MECHANISM
- •9. SUMMARY
- •1. INTRODUCTION
- •2. ELECTRON PROPAGATOR CONCEPTS
- •3. AN ECONOMICAL APPROXIMATION: P3
- •4. OTHER DIAGONAL APPROXIMATIONS
- •5. NONDIAGONAL APPROXIMATIONS
- •7. P3 TEST RESULTS
- •7.1. Atomic Ionization Energies
- •7.2. Molecular Species
- •8. CONCLUSIONS AND PROSPECTUS
- •1. INTRODUCTION
- •2. THEORETICAL PROCEDURES
- •3. GEOMETRIES
- •4. HEATS OF FORMATION
- •5. BOND DISSOCIATION ENERGIES
- •6. RADICAL STABILIZATION ENERGIES
- •7. REACTION BARRIERS
- •8. REACTION ENTHALPIES
- •9. CONCLUDING REMARKS
- •1. INTRODUCTION
- •2. HOMOLEPTIC CARBONYL COMPLEXES
- •4. IRON CARBONYL COMPLEXES
- •5. GROUP-10 CARBONYL COMPLEXES
- •7. NOBLE GAS COMPLEXES
- •8. TRANSITION METAL CARBENE AND CARBYNE COMPLEXES
- •12. TRANSITION METAL METHYL AND PHENYL COMPOUNDS
- •13. TRANSITION METAL NITRIDO AND PHOSPHIDO COMPLEXES
- •15. MAIN GROUP COMPLEXES OF BeO
- •16. CONCLUSION
- •1. INTRODUCTION
- •2. THEORETICAL BACKGROUND
- •3. SPECIFIC CONVENTIONS
- •4. STATISTICAL EVALUATIONS
- •5. DISCUSSION
- •Index
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small selection of the published mean absolute deviations (MADs) between computed and experimental heats of formation. Of course, the corresponding values cannot be compared directly, since they are based on different sets of reference molecules and reference data, but they should provide some indication of the errors that can be expected in such calculations. The reader should consult the original literature for further information [1-31].
5.DISCUSSION
The statistical evaluations of the preceding section indicate that the semiempirical MO methods can predict heats of formation with useful accuracy and at very low computational costs. When comparing with
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ab initio or DFT methods, the following points [32] should be kept in mind, however:
1.In general, errors tend to be more systematic at a given ab initio or DFT level and may therefore often be taken into account by suitable corrections. Errors in semiempirical calculations are normally less uniform and thus harder to correct.
2.The accuracy of the semiempirical results may be different for different classes of compounds, and there are elements that are more ”difficult” than others. Such variations in the accuracy are again less pronounced in high-level ab initio and DFT calculations.
3.Semiempirical methods can only be applied to molecules containing elements that have been parameterized, while ab initio and DFT methods are generally applicable.
4.Semiempirical parameterizations require reliable experimental or theoretical reference data and are impeded by the lack, of such data. Such problems do not occur in ab initio or DFT approaches.
In spite of these limitations, there are many areas where the established MNDO-type semiempirical methods can be applied successfully in calculations of thermochemical properties. This suggests that the underlying MNDO model includes the physically relevant interactions so that the parameterization can absorb the errors due to the MNDO approximations in an average sense. However, further improvements are clearly needed, and the inclusion of orthogonalization corrections that account for Pauli exchange repulsion indeed seems to enhance the accuracy of the calculated thermochemical properties (see the OM1 and OM2 results). This supports our belief [12] that a theoretically guided search for better models offers the most promising perspective for general-purpose semiempirical methods with better overall performance.
ACKNOWLEDGEMENTS
The author wishes to thank his coworkers for their contributions, particularly M. Kolb, A. Voityuk, and W. Weber.
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