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Essentials of Computational Chemistry

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7.7 PARAMETERIZED METHODS 241<br />

Table 7.6 Steps in G2 and G3 theory for molecules a,b<br />

Step G2 G3<br />

(1) HF/6-31G(d) geometry optimization HF/6-31G(d) geometry optimization<br />

(2) ZPVE from HF/6-31G(d) frequencies ZPVE from HF/6-31G(d) frequencies<br />

(3) MP2(full)/6-31G(d) geometry<br />

MP2(full)/6-31G(d) geometry<br />

optimization (all subsequent<br />

optimization (all subsequent<br />

calculations use this geometry)<br />

calculations use this geometry)<br />

(4) E[MP4/6-311+G(d,p)]<br />

−E[MP4/6-311G(d,p)]<br />

E[MP4/6-31+G(d)] −E[MP4/6-31G(d)]<br />

(5) E[MP4/6-311G(2df,p)]<br />

E[MP4/6-31G(2df,p)]<br />

−E[MP4/6-311G(d,p)]<br />

−E[MP4/6-31G(d)]<br />

(6) E[QCISD(T)/6-311G(d)]<br />

E[QCISD(T)/6-31G(d)]<br />

−E[MP4/6-311G(d)]<br />

−E[MP4/6-31G(d)]<br />

(7) E[MP2/6-311+G(3df,2p)]<br />

E[MP2(full)/G3large<br />

−E[MP2/6-311G(2df,p)]<br />

−E[MP2/6-311+G(d,p)]<br />

+E[MP2/6-311G(d,p)]<br />

c ]<br />

−E[MP2/6-31G(2df,p)]<br />

−E[MP2/6-31+G(d)]<br />

+E[MP2/6-31G(d)]<br />

(8) −0.00481 × (number <strong>of</strong> valence electron −0.006386 × (number <strong>of</strong> valence<br />

pairs) −0.00019 × (number <strong>of</strong><br />

electron pairs) −0.002977 × (number<br />

unpaired valence electrons)<br />

<strong>of</strong> unpaired valence electrons)<br />

E0 = 0.8929 × (2) + E[MP4/6-311G(d,p)] + 0.8929 × (2) + E[MP4/6-31G(d)] +<br />

(4) + (5) + (6) + (7) + (8)<br />

(4) + (5) + (6) + (7) + (8)<br />

a For atoms, G3 energies are defined to include a spin-orbit correction taken either from experiment or other highlevel<br />

calculations. In addition, different coefficients are used in step (8).<br />

b In the G2 method, the 6-311G basis set and its derivatives are not defined for second-row atoms; instead, a basis<br />

set optimized by McLean and Chandler (1980) is used.<br />

c Available at http://chemistry.anl.gov/compmat/g3theory.htm. Defined to use canonical 5 d and 7 f functions.<br />

A modification <strong>of</strong> G2 by Pople and co-workers was deemed sufficiently comprehensive<br />

that it is known simply as G3, and its steps are also outlined in Table 7.6. G3 is more accurate<br />

than G2, with an error for the 148-molecule heat-<strong>of</strong>-formation test set <strong>of</strong> 0.9 kcal mol −1 .Itis<br />

also more efficient, typically being about twice as fast. A particular improvement <strong>of</strong> G3 over<br />

G2 is associated with improved basis sets for the third-row nontransition elements (Curtiss<br />

et al. 2001). As with G2, a number <strong>of</strong> minor to major variations <strong>of</strong> G3 have been proposed to<br />

either improve its efficiency or increase its accuracy over a smaller subset <strong>of</strong> chemical space,<br />

e.g., the G3-RAD method <strong>of</strong> Henry, Sullivan, and Radom (2003) for particular application<br />

to radical thermochemistry, the G3(MP2) model <strong>of</strong> Curtiss et al. (1999), which reduces<br />

computational cost by computing basis-set-extension corrections at the MP2 level instead<br />

<strong>of</strong> the MP4 level, and the G3B3 model <strong>of</strong> Baboul et al. (1999), which employs B3LYP<br />

structures and frequencies.<br />

It should be noted that G2 and G3 potentially fail to be size extensive because <strong>of</strong> the<br />

correction term in step 8. If one is studying a homolytic dissociation into two components,<br />

at what point along the reaction coordinate are the formerly paired electrons considered<br />

to be unpaired? There will be a discontinuity in the energy at that point. In addition, G3<br />

theory uses a different correction for atoms than for molecules, and this too fails to be size<br />

extensive.

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