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184

13 Methane, ethane and hybridization

 

 

Figure 13.2. Drawing of positive axial quadrupole.

 

 

charge

in the

wave function. Figure 13.2 shows the general shape of the

 

z -axial

quadrupole with the signs of the regions. Since the moment of the molecule is

 

 

negative, we see that its signs are reversed compared to those in the figure, and the

 

individual C—H bonds are relatively positive at the H-atom ends.

 

 

 

 

We may arrive at this conclusion

another

way. In Table 13.6 the components

 

 

(x x

yy

)/2, x y ,

x z , and

yz

are zero

indicating

that the quadrupole field is

 

cylindrically

symmetric about

the

 

z -axis.

The

 

axial

moment around the

x - or

y -axis is

 

 

 

 

 

 

 

 

 

 

 

 

(2 x x yy zz )/2

= 3(x x yy )/4 (2 zz

x x yy )/4 ,

(13.6)

 

 

 

 

 

= (2 yy

x x

zz )/2 ,

 

(13.7)

 

 

 

 

 

= 0 .91485 D A

,

 

 

(13.8)

for which the positive sign again indicates the positive nature of the H end of the

 

C—H bonds. This direction of the dipole moment is the same as that

of

CH and

 

 

CH 2

, and

is again expected because of the relative predominance in the wave

 

function of the ionic term shown in Table 13.5.

 

 

 

 

 

 

 

 

 

 

 

 

 

CH

4

 

 

 

 

We expect methane to be formed by the combination of an H-atom with the remain-

 

 

ing unpaired

p z orbital of CH

3 . If the principal configuration is still that involving

 

the C

5 S

state and its nondirectional character predominates, we expect methane to

 

 

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.

13.1 CH, CH 2 , CH 3 , and CH 4 185

Table 13.7. Principal standard tableaux function structures for CH

 

 

 

 

 

 

 

4

 

 

 

 

at equilibrium bond distances.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

2

 

 

 

3

 

 

 

 

 

4

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Num.

a

 

 

1

 

 

 

 

1

 

 

 

4

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

h a

1s a

 

 

h

 

1s b

 

 

h d

h d

 

 

 

h a

1s a

 

Tab. b

 

h b

1s b

1sa a

1s

c

h a

1s

a

h

b

1s

c

 

 

h d

1s d

h

c

1s

d

h c

1s

c

h

c

1s

d

 

 

 

 

h c

1s c

 

 

h

b

h d

 

 

 

h b

1s

b

 

 

1s b

h d

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

C i (min)

0.372 037 96

 

0.155 900 88

0.129 792 00

 

 

 

0.105 365

69

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

aThe number of terms in the symmetry function that is generated from the tableau shown. (See text.)

bThese tableau symbols exclude the core orbitals.

Table 13.8. Apparent partial electronic charge on H atoms based upon lowest nonzero moment and the corresponding

calculated bond lengths, STO3G basis.

 

 

 

 

 

Molecule

Charge

R CH

A

CH

 

0.254|e |

1.231

a

CH

2

0.137

1.163

 

CH

3

0.194

1.145

 

CH

4

0.188

1.150

 

 

 

 

 

 

 

 

 

 

 

a

The H—C—H bond angle is 129.1

.

 

 

A full valence calculation on CH

4

gives 1764 standard tableaux functions, and

all of these are involved in the 164

1 A

1 symmetry functions. The second and fourth

tableaux are also present in the principal constellation and, as with the earlier cases,

these are not simple symmetry functions alone. The third tableau is ionic with the

negative charge at the C atom. As before, this contributes to the relative polarity of

the C—H bonds.

 

 

 

This is seen from a calculation of the electric moments. Methane has no nonzero

 

dipole or quadrupole moments, but the

 

x yz component of the octopole is 1.144 D A

All of the others are zero if the molecule has the orientation in the coordinate system

that is used here. The value is positive, showing the same qualitative electronic

distribution in C—H bonds as was seen for

the other

CH

n molecules we have

examined. Quantitatively, the octopole moment is equivalent to a charge of 0.204

at the H-atom nuclei.

 

 

 

For easy comparison we show in Table 13.8 the apparent charge on the H atom

 

in each of our molecules. The trend in these

charges is

broken between one

and

2 .

|e |

186

 

13

Methane, ethane and hybridization

 

 

 

 

 

Table 13.9.

Statistics for 6-31G

calculations of CH

n .

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Num. symm.

Number of

 

 

 

 

 

 

State

funcs.

tableaux

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

CH

 

2

 

 

213

546

 

 

 

 

CH

2

3

B

1

 

828

1651

 

 

 

 

CH

3

2

A

2

 

1597

9375

 

 

 

 

CH

4

1

A

1

 

2245

26 046

 

 

 

 

 

 

 

 

 

 

 

 

 

two H atoms. The likely interpretation here is that this is the place where the most

 

 

 

important atomic configuration changes as one progresses through the list. This is

 

 

 

 

seen clearly in Tables 13.2, 13.3, 13.5, and 13.7, where the principal configuration

 

 

 

in the wave functions is shown.

 

 

 

 

 

 

 

 

 

In the early days of VB theory workers were concerned with the “valence state”

 

 

 

of carbon[55]. Our calculations cannot really address this question because it is well

 

 

 

defined only within a perfect pairing single tableau wave function.

 

3

The notion was

contrived to explain the relatively constant bond energies through the CH

 

 

n

series,

while there is a requirement to pay back the ener

 

gy

loss in having the principal

 

configuration change to higher energy. In the context of a full valence calculation

 

 

 

we may only give a somewhat more qualitative argument. The

5 S state of

C is

about 4 eV above the ground state. This suggests that each of the actual C—H bond

 

 

 

 

energies in CH

2 with respect

to

 

some hypothetical

frozen carbon state

is about

 

 

 

2 eV higher than the apparent calculated or measured value. We attribute this to the

 

 

 

 

greater effectiveness for bonding when

 

 

 

sp n

hybrids are involved.

 

 

 

 

 

 

 

 

13.1.2 6-31G

 

basis

 

 

 

 

After our discussion of the STO3G results we, in this section, compare some of these

 

 

 

 

obtained with a 6-31G

basis arranged as described in Chapter 9. As before, we find

 

 

 

that the larger basis gives more accurate results, but the minimal basis yields more

 

 

 

useful qualitative information concerning the states of the atoms involved and the

 

 

 

bonding. The statistics on the number of symmetry functions and standard tableaux

 

 

 

 

functions for the various calculations are given in Table 13.9.

 

 

 

 

From Table 13.10 we see that the bond distances are reproduced better in this case

 

 

 

 

than with the STO3G basis. We see that the break in the trend between CH and CH

 

 

 

2

again appears, and we continue to attribute it to the change in the important atomic

 

 

 

 

configuration at this juncture in the

list. The calculated

bond

distances are about

 

 

 

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.

13.2 Ethane

187

 

Table 13.10.

Energies, bond distances, and bond energies of CH

 

 

n

 

 

 

 

 

 

for 6-31G

 

bases.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Bond length (A

 

)

 

 

 

D e

(eV)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Energy (au)

Calc.

 

Exp.

Dissociation

Calc.

Exp.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

C

 

37.712 51

 

 

a1.1190

 

 

 

 

 

2.978

3.462

CH

 

38.321 54

1.169

 

 

D

CH

CH

2

38.983 55

1.104

1.029

 

D

CHH

4.502

4.33

CH

3

39.624 08

1.109

1.079

 

 

D

CH

2 H

3.918

4.90

CH

4

40.295 47

1.119

1.094

 

 

D

CH

3 H

4.758

4.406

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a The H—C—H bond angle is 130.5

.

 

Table 13.11.

Various multipole moments and the apparent

charges on H atoms from 6-31G

calculations.

Moment a

Value

Charge

CH

 

D

1.20030

0.214|e |

CH

2

D

0.53033

0.119

CH

3

AQ

1.33895

0.152

CH

4

O

0.58764

0.022

 

 

 

 

 

a D, dipole; AQ, axial quadrupole; O, octopole.

The apparent charges on the H atoms in this basis are shown in Table 13.11.

 

 

These may be compared to the similar values in Table 13.8. We see that the larger

 

 

basis yields smaller values, particularly for methane. Nevertheless, we still predict

 

 

that the H atoms in these small hydrocarbons are more positive than the C atom.

 

 

13.2 Ethane

 

 

Ethane presents a considerably greater challenge for calculation than the single

 

 

carbon molecules above. Even if we continue the practice of putting 1

s

electrons

in the “core” we have seven bonds and 14 electrons. A full minimal basis calcula-

 

 

tion, such as with STO3Gs, will produce 2 760 615 standard tableaux functions or

 

 

HLSP functions for the total 14-electron basis. Not all of these are

1 A 1 g

(assum-

ing D 3d symmetry) but the number would be considerable. With 14 electrons and

 

 

14 orbitals, none doubly occupied, there are 429 possible Rumer diagrams or stan-

 

 

dard tableaux functions. We will not attempt any “full” calculations with ethane,

 

 

but rather focus on basis set arrangements that are designed to yield useful results

 

 

with greater efficiency.

 

 

188

 

13 Methane, ethane and hybridization

 

 

 

 

Table 13.12.

Energies for covalent only calculations of D

3 d and D

3 h ethane.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Num. symm.

Energy (hartree)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Treatment

 

funcs.

D 3 d

D 3 h

 

Cartesian AO

 

52

78.367 895

a

 

 

78.575 229

 

Hybrid AO

 

52

78.577 391

 

Perfect pairing (hybrid)

1

78.565 885

78.563 937

 

 

 

 

 

 

 

a This was not run.

We first contrast using a Cartesian

basis with

sp 3

hybrids on the C atoms

for a

covalent-only calculation.

4 Table 13.12 shows these along with the perfect pairing

 

energy. We see that there is a considerable lowering of the energy at

 

E

from using hybrid orbitals on the C atom instead of the original Cartesian basis.

 

 

The hybrids are arranged to be pointing at the H atoms and the other C atom. We

 

 

also see that the perfect pairing wave function is not a great deal higher in energy

 

than the full covalent-only energy at

E

= 0 .313 or 0

.307 eV for the

D

geometry, respectively. The perfect pairing function is the only Rumer tableau that is a symmetry function by itself. We saw earlier that a perfect pairing function with Cartesian AOs is frequently not sensible, and this is another such case.

Because they have no ionic states, the previous covalent-only results have too high a kinetic energy contribution, as discussed in Chapter 2. Adding all possible

ionic states would lead to the very large number of basis functions quoted in the first paragraph of the discussion of ethane. We will consider the following physical arguments that may be used to limit the number of ionic state functions. This will all be done in the context of hybrid orbitals on the C atoms.

= 5.7 eV

3 d or D 3 h

1.Adjacent ionic structures are the most important. This is expected since reductions in the kinetic energy will only occur if the overlap between the orbitals is fairly sizable. This is accomplished by assigning two electrons to each pair of orbitals that are arranged to bond

in the molecule, and then requiring that this pair always have two electrons occupying them.

2.Only a few ionic bonds are required. We accomplish this by restricting the number of

doubly occupied orbitals in a structure.

 

3. Highly charged atoms

are unlikely. We accomplish this by preventing the charge depletion

or build-up on either C atom from being outside

±1.

Table 13.13 shows the energies for several treatments of ethane using these arguments. The first addition of one set of ionic structures per basis function produces

4The reader is reminded that different linear combinations of the AOs yield different energies for less than full treatments.

13.3 Conclusions

189

Table 13.13.

Energies for various hybrid orbital calculations

 

 

 

 

of D 3d

and D 3 h

ethane.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Ionic

Num. symm.

 

 

 

Energy (hartree)

 

 

 

 

 

 

 

 

 

 

 

 

structures

funcs.

Tableaux

D

 

3d

D 3 h

0

52

 

429

 

78.577 391

78.575 228

1

214

 

2277

 

78.731 700

78.730 171

2

448

 

4797

 

78.742 547

78.741 195

 

 

 

 

 

 

 

 

Table 13.14. Internal rotation barrier in ethane.

 

Ionic

 

 

Energy (eV)

 

 

 

 

 

 

 

 

 

structures

Theory

Exp.

 

 

 

 

 

 

 

 

 

 

0

0.059

 

 

 

 

1

0.042

 

 

 

 

2

0.037

0.127

a

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a See Ref. [56].

 

 

 

 

 

a lowering of

4.2 eV, or nearly 0.6 eV per bond. The second ionic structure pro-

 

 

duces only 0.04 eV more per bond. In Chapter 2 the lowering of the energy in H

2

when the ionic states are added is nearly 1 eV. The overlap there is rather greater at

 

 

0.9 than the values here, which are around 0.7 for either a C—H or a C—C bond.

 

 

We have calculated ethane in both

D 3d and

D 3 h geometries. From Table 13.13

we obtain the calculated barriers to internal rotation given in Table 13.14. It is seen

 

 

that the calculated barrier height is falling as the number of ionic states increases.

 

 

It is not yet

converged, but we do not give

the result obtained by

including three

 

 

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

 

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

 

190

 

13 Methane, ethane and hybridization

 

tableaux functions of the particular sort that is antisymmetric with respect to the

 

interchange of any of the four C orbitals 2

s , 2 p x , 2 p y , and 2

p z . The functions based

upon the other standard tableaux of the constellation correspond to the inclusion of

 

other

L S

states of the same configuration. Although not as important in the wave

 

function, these functions do enter and allow one to infer that the step suggested by

 

Slater and Pauling, the inclusion of all states of a configuration, was an important

 

addition to the VB method.

 

 

Our results in this chapter also show that using hybrid orbitals with restricted

 

bases can make an important improvement in the wave functions, at least when the

 

criterion is energy lowering.

 

 

We

also see

that the number of basis functions

grows rapidly with the number

 

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.

14

Rings of hydrogen atoms

In this chapter we examine some results for

four model systems consisting of

 

 

 

 

 

rings of H atoms. These calculations show how the number of atoms in a complex

 

 

 

 

 

reaction may influence rates of reaction, particularly through the activation energy.

 

 

 

 

 

The systems are as follows.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Four H atoms in a rectangular geometry of

 

 

 

 

 

D

2 h

symmetry. The rectangle is characterized

 

 

 

 

by two

distances,

RA

and

RB. We

map out a region of the ground state energy for this

 

 

 

 

 

four-electron system as a function of the two distances.

 

 

 

 

 

 

 

 

 

 

 

 

Six H atoms in a hexagonal geometry of

 

 

 

 

D

3h

symmetry. This is not a

regular

hexagon, in

 

 

general, but, like the system of four H atoms, is characterized by two distances we also

 

 

 

 

 

 

label

RA

and

RB. These

two

distances alternate

around

the ring. We

also calculate the

 

 

 

 

 

 

map of the ground state energy for this six-electron system.

 

 

 

 

 

 

 

 

 

 

 

Eight H atoms in an octagonal geometry of

 

 

 

 

 

D

4 h

symmetry and the specific

shape

char-

 

 

 

 

acterized by the

RA

and

RB

variables as above. For this larger system we only determine

 

 

 

 

 

 

the saddle point with respect to the same sort of variables.

 

 

 

 

 

 

 

 

 

 

 

Ten H atoms in a decagonal geometry of

 

 

 

 

 

D

5 h

symmetry and the

RA

and

RB

variables.

 

 

Again, we determine only the saddle point.

 

 

 

 

 

 

 

 

 

 

 

 

 

Since the geometries of these

systems

are in

most regions

not

regular

polygons,

 

 

 

 

 

we will symbolize them as (H

 

 

2

)n

, emphasizing the number of H

2

molecules rather

 

than the total number of atoms.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

For any of these, if

 

RA

= 0.7

A

 

RB

 

is quite large, the rings

represent 2–5

 

 

 

 

and

 

 

 

normal H

2

molecules well separated from

one another. If the roles of

 

 

RA

and

RB

are reversed, the H

2

molecules have executed a metathesis in which the molecules

 

 

 

 

 

transform into an equivalent set.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

These are, without doubt, somewhat artificial systems. For real systems, one could

 

 

 

 

 

not tell if anything happened, unless isotopic labeling could be arranged. An even

 

 

 

 

 

greater problem would occur in the gas phase, since the entropy penalty required

 

 

 

 

 

for

these

peculiar

geometries would

be

expected

to make them

very

improbable.

 

 

 

 

 

191

192 14 Rings of hydrogen atoms

Table 14.1.

Number of symmetry functions of three types for

 

 

 

 

 

 

 

H-ring calculations of (H

 

2 )2 and (H

2 )3 .

 

 

 

 

 

 

 

 

 

 

 

 

 

Base configs. Single exc.

Double exc.

Total

State

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(H 2 )2

8

17

 

33

 

58

1 A

1g

 

 

(H 2 )3

13

130

 

411

 

554

1 A

1

 

 

 

 

 

 

 

 

 

 

Table 14.2.

Number of symmetry functions for saddle point

 

 

 

 

 

 

 

calculations of (H

2 )4

and (H

2 )2 .

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Num. Symm. Funcs.

 

Num. tab.

State

 

 

 

 

 

 

 

 

 

 

 

 

 

(H 2 )4

146

 

 

 

1134

 

1 A

1g

 

(H 2 )5

768

 

 

7602

 

1 A

1

 

 

 

 

 

 

 

 

 

 

 

 

Nevertheless, the results have considerable interest, bearing, as they do, on the same sort of considerations as the Woodward–Hoffman rules[58].

 

 

14.1 Basis set

 

 

 

 

The calculations were all performed with an “

s ”-only basis of a 1

s

and a “2

s ” at each

center. These are written in terms of the Huzinaga 6-Gaussian function as (6

 

 

 

/42).

This is the

s part of the basis used in Chapter 2 for the H

2 molecule and is shown in

 

Table 2.2. It will be recalled that the “2

s ” orbital is not a real H2

 

s orbital,

but the

second eigenfunction for this basis. As such it provides orbital breathing flexibility

 

 

 

 

in the wave function. We show some statistics for these calculations in Table 14.1.

 

 

 

 

Ionic states are restricted to

±1 at any center. The saddle point calculations for the

 

 

larger two systems were carried out with more restricted bases involving valence-

 

 

 

 

only covalent and single-, and double-ionic structures. The statistics for these are

 

 

 

 

shown in Table 14.2.

 

 

 

 

 

 

 

14.2

Energy surfaces

 

 

The energy surface for (H

2 )2 , divided by 2, is shown in Fig. 14.1, and that for (H

2 )3,

divided by 3, is in Fig. 14.2.

Because of the division by the number of H

2

molecules,

the energy goes to

1 hartree as

RA

and

RB

both grow large. Examination of the

 

two surfaces shows clearly that they are quite different. The (H

 

2 )2 energy

surface

has a fairly sharp ridge between the two stable valleys. This is completely missing

 

in the (H

2 )3 case. The difference between the energies

 

 

 

E H 4 /2 E H 6 /3

14.2 Energy surfaces

193

Energy (hartree)

0.6 0.7 0.8 0.9 1.0 1.1 1.2

0.4 0.6 0.8

1.0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

2.2

RA (Å)

1.2

 

 

 

 

 

1.8 2.0

1.4

 

 

 

 

1.6

 

 

1.6

 

 

 

1.4

 

 

 

1.82.0

 

 

0.8 1.0 1.2

 

 

 

 

 

0.6

RB (Å)

 

 

 

2.2

0.4

 

 

 

 

 

 

 

 

 

 

 

 

 

Figure 14.1. energy is per H

The energy surface for the conversion of 2H

2 2H 2 in D 2 h geometries. The

2 molecule.

 

Energy (hartree)

0.6 0.7 0.8 0.9 1.0 1.1 1.2

0.4 0.6 0.8

1.0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

2.2

RA (Å)

1.2

 

 

 

 

 

1.8 2.0

1.4

 

 

 

 

1.6

 

 

1.6

 

 

 

1.4

 

 

 

1.82.0

 

 

0.8 1.0 1.2

 

 

 

 

 

0.6

RB (Å)

 

 

 

2.2

0.4

 

 

 

 

 

 

 

 

 

 

 

 

 

Figure 14.2.

The energy surface for the conversion of 3H

 

2 3H 2 in

D

3h

geometries. The

energy is per H

2

molecule.

 

 

 

 

 

 

 

 

for the two surfaces is plotted in Fig. 14.3. This is everywhere

 

 

>0.001 eV within

the region of the plot. Thus

 

E H

4 /2 is always relatively higher.

 

 

 

In Table 14.3 we show the saddle points and activation energies of the four

 

 

 

systems. It is seen that there is a tendency for the quantities to alternate between

 

 

 

higher and

lower

values

as the number

of

H

 

2

molecules is either

even

or

odd.

The differences decrease, however, as

the rings become larger, and

it

appears

 

 

 

that further calculations might show that the effect levels out. Nevertheless, the

 

 

 

activation energy for the (H

2

)2

system is almost three times higher than that of the

 

 

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