
Gallup G.A. - Valence Bond Methods, Theory and applications (CUP, 2002)
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184 |
13 Methane, ethane and hybridization |
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Figure 13.2. Drawing of positive axial quadrupole. |
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charge |
in the |
wave function. Figure 13.2 shows the general shape of the |
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z -axial |
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quadrupole with the signs of the regions. Since the moment of the molecule is |
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negative, we see that its signs are reversed compared to those in the figure, and the |
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individual C—H bonds are relatively positive at the H-atom ends. |
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We may arrive at this conclusion |
another |
way. In Table 13.6 the components |
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(x x |
− yy |
)/2, x y , |
x z , and |
yz |
are zero |
indicating |
that the quadrupole field is |
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cylindrically |
symmetric about |
the |
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z -axis. |
The |
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axial |
moment around the |
x - or |
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y -axis is |
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(2 x x − yy − zz )/2 |
= 3(x x − yy )/4 − (2 zz |
− x x − yy )/4 , |
(13.6) |
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= (2 yy |
− x x − |
zz )/2 , |
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(13.7) |
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= 0 .91485 D A |
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(13.8) |
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for which the positive sign again indicates the positive nature of the H end of the |
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C—H bonds. This direction of the dipole moment is the same as that |
of |
CH and |
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CH 2 |
, and |
is again expected because of the relative predominance in the wave |
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function of the ionic term shown in Table 13.5. |
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CH |
4 |
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We expect methane to be formed by the combination of an H-atom with the remain- |
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ing unpaired |
p z orbital of CH |
3 . If the principal configuration is still that involving |
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the C |
5 S |
state and its nondirectional character predominates, we expect methane to |
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be tetrahedral, thereby minimizing the repulsion energy between pairs of H atoms. This is borne out by the calculations as we see in Table 13.7.

186 |
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13 |
Methane, ethane and hybridization |
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Table 13.9. |
Statistics for 6-31G |
calculations of CH |
n . |
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Num. symm. |
Number of |
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State |
funcs. |
tableaux |
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CH |
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2 |
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213 |
546 |
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CH |
2 |
3 |
B |
1 |
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828 |
1651 |
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CH |
3 |
2 |
A |
2 |
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1597 |
9375 |
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CH |
4 |
1 |
A |
1 |
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2245 |
26 046 |
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two H atoms. The likely interpretation here is that this is the place where the most |
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important atomic configuration changes as one progresses through the list. This is |
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seen clearly in Tables 13.2, 13.3, 13.5, and 13.7, where the principal configuration |
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in the wave functions is shown. |
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In the early days of VB theory workers were concerned with the “valence state” |
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of carbon[55]. Our calculations cannot really address this question because it is well |
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defined only within a perfect pairing single tableau wave function. |
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3 |
The notion was |
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contrived to explain the relatively constant bond energies through the CH |
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n |
series, |
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while there is a requirement to pay back the ener |
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loss in having the principal |
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configuration change to higher energy. In the context of a full valence calculation |
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we may only give a somewhat more qualitative argument. The |
5 S state of |
C is |
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about 4 eV above the ground state. This suggests that each of the actual C—H bond |
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energies in CH |
2 with respect |
to |
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some hypothetical |
frozen carbon state |
is about |
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2 eV higher than the apparent calculated or measured value. We attribute this to the |
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greater effectiveness for bonding when |
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sp n |
hybrids are involved. |
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13.1.2 6-31G |
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basis |
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After our discussion of the STO3G results we, in this section, compare some of these |
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obtained with a 6-31G |
basis arranged as described in Chapter 9. As before, we find |
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that the larger basis gives more accurate results, but the minimal basis yields more |
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useful qualitative information concerning the states of the atoms involved and the |
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bonding. The statistics on the number of symmetry functions and standard tableaux |
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functions for the various calculations are given in Table 13.9. |
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From Table 13.10 we see that the bond distances are reproduced better in this case |
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than with the STO3G basis. We see that the break in the trend between CH and CH |
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2 |
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again appears, and we continue to attribute it to the change in the important atomic |
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configuration at this juncture in the |
list. The calculated |
bond |
distances are about |
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4.2% high. The success in calculating bond energies is more difficult to assess, since there is considerably more uncertainty in the experimental results.
3Even then, it is a purely theoretical concept. There appears to be no experimental approach to the energy of this state.


13.3 Conclusions |
189 |
Table 13.13. |
Energies for various hybrid orbital calculations |
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of D 3d |
and D 3 h |
ethane. |
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Ionic |
Num. symm. |
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Energy (hartree) |
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structures |
funcs. |
Tableaux |
D |
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3d |
D 3 h |
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0 |
52 |
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429 |
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−78.577 391 |
−78.575 228 |
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1 |
214 |
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2277 |
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−78.731 700 |
−78.730 171 |
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2 |
448 |
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4797 |
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−78.742 547 |
−78.741 195 |
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Table 13.14. Internal rotation barrier in ethane.
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Ionic |
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Energy (eV) |
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structures |
Theory |
Exp. |
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0 |
0.059 |
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1 |
0.042 |
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2 |
0.037 |
0.127 |
a |
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a See Ref. [56]. |
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a lowering of |
≈4.2 eV, or nearly 0.6 eV per bond. The second ionic structure pro- |
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duces only 0.04 eV more per bond. In Chapter 2 the lowering of the energy in H |
2 |
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when the ionic states are added is nearly 1 eV. The overlap there is rather greater at |
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≈0.9 than the values here, which are around 0.7 for either a C—H or a C—C bond. |
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We have calculated ethane in both |
D 3d and |
D 3 h geometries. From Table 13.13 |
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we obtain the calculated barriers to internal rotation given in Table 13.14. It is seen |
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that the calculated barrier height is falling as the number of ionic states increases. |
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It is not yet |
converged, but we do not give |
the result obtained by |
including three |
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ionic structures in the basis functions. The interested reader can work this out. The trend here with the addition of ionic states runs counter to predictions using another method published by Pophristic and Goodman[57].
In addition it appears that this minimal basis calculation is unable to give a result close to the experimental value for the rotation barrier. We do not pursue this further here, but leave it as an open question.
13.3 Conclusions |
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In its original form VB theory was proposed using only states of atoms like the |
5 S |
for C that we have invoked in describing our results. These are produced by standard |
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190 |
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13 Methane, ethane and hybridization |
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tableaux functions of the particular sort that is antisymmetric with respect to the |
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interchange of any of the four C orbitals 2 |
s , 2 p x , 2 p y , and 2 |
p z . The functions based |
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upon the other standard tableaux of the constellation correspond to the inclusion of |
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other |
L S |
states of the same configuration. Although not as important in the wave |
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function, these functions do enter and allow one to infer that the step suggested by |
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Slater and Pauling, the inclusion of all states of a configuration, was an important |
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addition to the VB method. |
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Our results in this chapter also show that using hybrid orbitals with restricted |
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bases can make an important improvement in the wave functions, at least when the |
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criterion is energy lowering. |
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We |
also see |
that the number of basis functions |
grows rapidly with the number |
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of electrons. In Chapter 16 we will discuss another method for dealing with the escalation of basis size with greater numbers of atoms and electrons.
192 14 Rings of hydrogen atoms
Table 14.1. |
Number of symmetry functions of three types for |
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H-ring calculations of (H |
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2 )2 and (H |
2 )3 . |
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Base configs. Single exc. |
Double exc. |
Total |
State |
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(H 2 )2 |
8 |
17 |
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33 |
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58 |
1 A |
1g |
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(H 2 )3 |
13 |
130 |
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411 |
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554 |
1 A |
1 |
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Table 14.2. |
Number of symmetry functions for saddle point |
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calculations of (H |
2 )4 |
and (H |
2 )2 . |
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Num. Symm. Funcs. |
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Num. tab. |
State |
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(H 2 )4 |
146 |
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1134 |
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1 A |
1g |
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(H 2 )5 |
768 |
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7602 |
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1 A |
1 |
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Nevertheless, the results have considerable interest, bearing, as they do, on the same sort of considerations as the Woodward–Hoffman rules[58].
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14.1 Basis set |
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The calculations were all performed with an “ |
s ”-only basis of a 1 |
s |
and a “2 |
s ” at each |
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center. These are written in terms of the Huzinaga 6-Gaussian function as (6 |
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/42). |
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This is the |
s part of the basis used in Chapter 2 for the H |
2 molecule and is shown in |
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Table 2.2. It will be recalled that the “2 |
s ” orbital is not a real H2 |
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s orbital, |
but the |
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second eigenfunction for this basis. As such it provides orbital breathing flexibility |
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in the wave function. We show some statistics for these calculations in Table 14.1. |
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Ionic states are restricted to |
±1 at any center. The saddle point calculations for the |
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larger two systems were carried out with more restricted bases involving valence- |
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only covalent and single-, and double-ionic structures. The statistics for these are |
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shown in Table 14.2. |
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14.2 |
Energy surfaces |
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The energy surface for (H |
2 )2 , divided by 2, is shown in Fig. 14.1, and that for (H |
2 )3, |
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divided by 3, is in Fig. 14.2. |
Because of the division by the number of H |
2 |
molecules, |
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the energy goes to |
−1 hartree as |
RA |
and |
RB |
both grow large. Examination of the |
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two surfaces shows clearly that they are quite different. The (H |
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2 )2 energy |
surface |
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has a fairly sharp ridge between the two stable valleys. This is completely missing |
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in the (H |
2 )3 case. The difference between the energies |
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E H 4 /2 − E H 6 /3
