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Thomas Arrow - 1C

Molecular Mechanics

Cyclopentadiene Dimers

The energies of the endo and exo conformations for a cyclopentadiene dimer were analysed by molecular mechanics simulations using the MMFF94s[1] force-field using Avogadro Version 1.1.1 [2][3].

Cyclopentadiene Dimers
Isomer Exo (1) Endo (2)
Structure
3d

The molecules analysed are displayed in the table to the right. As shown the exo form has the cyclohexene ring bent towards the bridge while the endo form has it bent away.

The reported energies for these molecules from the MMFF94s force field are tabulated below. They are broken down by the parameter with which the energy is associated. A positive value is indicative of a higher energy conformation.

Energetics of Conformations
1 2
Bond Stretching 3.54301 3.46731
Angle Bending 30.7729 33.19157
Stretch Bending -2.04139 -2.08211
Torsional -2.73414 -2.94776
Out of Plane Bending 0.0147 0.02172
Van Der Waals 12.80465 12.35789
Electrostatic 13.01375 14.18217
Total 55.37349 58.19078

It is trivial to see that the exo isomer is the more thermodynamically stable form however it is not the predominant isomer. Discrepancies in the contributions to the energy from different elements of the force-field can give us an insight into the reason for this. Particularly different are the contributions from Angle Bending and Electrostatic terms with the endo form being more strained in both cases. This is probably due to the approach of the cyclohexene ring to the bridged ring.

This suggests that the preference of endo over exo is a kinetic effect. It is often stated that this is due to better HOMO-LUMO overlap in the endo transiton state than the exo transition state[4]. Another suggested possibility is that the reaction is not concerted and the endo transition state is better at stabilising the charge build up than then exo one. [5]



Hydrogenation of Cyclopentadiene Dimers

Hydrogenated Cyclopentadiene Dimers
Isomer (3) (4)
Structure

A further analysis that was undertaken is the hydrogenation of the lower energy endo isomer. Calculations were attempted in order to determine that the hydrogenation of which C=C would result in the lowest energy product. This was also done using Avogadro and the MMFF94s force field and the results are tabulated below.

Energetics of Conformations
3 4
Bond Stretching 3.30673 2.82302
Angle Bending 30.85321 24.68566
Stretch Bending -1.92617 -1.65715
Torsional 0.07598 -0.37815
Out of Plane Bending 0.01515 0.00028
Van der Waals 13.27693 10.63680
Electrostatic 5.12098 5.14702
Total 50.72282 41.25749

It is apparent that the isomer 4 is of much lower energy than 3. This appears to be predominantly due to the reduced Angle Bending. This is because hydrogenation alpha to the bridge head results in pulling the bridge apart and greatly increasing strain.


Atropisomerism in Taxol Precursors

It is possible to investigate the stability of other types of isomer using molecular mechanics such as atropisomerism. This has been performed in a similar manner to that under taken above using Avogadro and the MMFF94s forcefield on the two atropisomers of a Taxol precursor. The structures are shown to the right. Tabulated below are the force field energetics for the molecule.

Atropisomers
Isomer (9) (10)
Structure
3d
Energetics of Conformations
9 10
Bond Stretching 14.89204 7.14091
Angle Bending 48.49693 22.75468
Stretch Bending -0.59339 -0.22705
Torsional 7.99095 -2.05224
Out of Plane Bending 2.55739 0.65304
Van Der Waals 51.13121 31.98513
Electrostatic 1.88198 0.84285
Total 126.35710 61.09732

Again, one isomer is clearly far more stable than the other. The second isomer with the carbonyl group pointing away from the bridge and methyl group is far more stable. We can see from the breakdown that this is mostly due to the Bond Stretching, Angle Bending and Van der Waals energies. This is probably due to the repulsive effects for placing the carbonyl so close to the bridge and methyl group. It is very hard to hydrogenate these because they are hyperstable alkenes. They are "less strained than the parent hydrocarbon"[6]

NMR Prediction of Taxol Isomer Precursor

The molecule shown to the right (18) is also a taxol precursor and is able to exhibit atropisomerism in the same manner as molecules 9 and 10 above.

A structure for this was designed in Avogadro [2] and optimized using the MMFF94s forcefield.

The molecule was optimised and then the decoupled hydrogen and carbon NMR spectra calculated using the B3LYP level of theory and a 6-31G(d,p) basis set.[7]

The optimised molecule is shown to the right along with the NMR specta.

Structure
H NMR
C NMR

We can see that this is broadly in line with the literature[8] which lists the shifts observed as follows:

Proton NMR [9]
δ 5.21 (M, 1H), 3.00-2.70 (m, 6H), 2.70-2.35 (m,4H), 2.20-1.70 (m, 6H), 1.58 (t, J=5.4Hz, 1H) 1.50-1.20(m, 3H), 1.10 (s, 3H), 1.07 (s, 3H), 1.03 (s, 3H)
Carbon NMR[9]
211.49 148.72 120.90 74.61 60.53 51.30 50.94, 45.53, 43.28, 40.82, 38.73, 36.78, 35.47, 30.84, 30.00, 25.567, 25.35, 22.21, 21.39, 19.83

Obviously the calculated proton NMR does not exhibit any coupling and has a number of shifts which are incorrectly located. This is also due to the fact that shifts that would normally be averaged by the thermal rotation of bonds is not present resulting in more signals than expected.

The Carbon NMR on the other hand seems to match the experimental data quite closely in both value and trend. This is helped by the fact that one does not normally observe coupling in Carbon-13 NMR because it is often proton decoupled and not abundant enough to observe coupling with an adjacent carbon.



Asymmetric Epoxidation

In the 1S lab experiment it is required to epoxidise two different alkenes using two catalysts developed by Jacobsen and Shi. In this section an analysis is performed on the structures of these catalysts as well and that of the epoxides.

Structures of Asymmetric Epoxidation Catalysts

The structures of these catalysts are available in the Cambridge Crystallographic Database[10][11] which was interrogated using ConQuest[12] and then the found structures viewed using Mercury[13].

Shi Catalyst

Structure of Shi Catalyst

The structure of this molecule is shown to the right Thechnical it is a precatalyst that is oxidised to the active species that is an oxirane. It was developed by Shi et al.[14]. The crystal structure of the molecule is accessible below.


An interesting thing to note is the lengths of the anomeric carbon bonds in this molecule which are depicted below.

Anomeric Bond Lengths

Clearly some are far longer than others. This is due to the anomeric effect. I.E. in the longest bond the lone pair on the two adjacent oxygen atoms are both well able to partially donate their lone pairs into the C-O σ* orbital. The alignment for this is better in the longest bond and gradually gets worse as the bonds shorted because the lone pairs are twisted away from the σ* orbital.


Jacobsen Catalyst

Structure of Jacobsen Catalyst

The structure of this molecule is shown to the right and the crystal structure is displayed below

Distances between rings

It is interesting to note the very close approach of the tBu groups on the benzene rings as shown in the image below. This restricts the side from which the center of the molecule can be accessed by the alkene. The shorter distance ca. 2Å is less than the sum of the Van der Waals radii of hydrogen[15] and thus totally shields this side of the molecule.


NMR Spectra of Selected Epoxides

The two alkenes to be epoxidised are transβ-Methylstyrene and Stilbene. The structures of these are shown to the right.

Structures
Alkene transβ-Methylstyrene Stilbene
Structure


These can be epoxidised to the products tabulated below.

Stilbene Oxide
trans(R,R)-Stilbene Oxide trans(S,S)-Stilbene Oxide cis-β-Stilbene Oxide
β-Methylstyrene
trans(R,R)-β-Methylstyrene Oxide trans(S,S)-β-Methylstyrene Oxide cis(S,R)-β-Methylstyrene Oxide cis(R,S)-β-Methylstyrene Oxide

The NMR spectra of the enantiomers will be the same thus it is only necessary to calculate the spectra from one of each. This was undertaken at the B3LYP level of theory and with the 6-31G(d,p) basis set. The calculated spectra are shown below.

Stilbene Oxide

Trans-Stilbene Oxide Proton NMR Trans-Stilbene Oxide Carbon NMR
Trans-Stilbene Oxide Proton NMR Trans-Stilbene Oxide Carbon NMR
Cis-Stilbene Oxide Proton NMR Cis-Stilbene Oxide Carbon NMR
Cis-Stilbene Oxide Proton NMR Cis-Stilbene Oxide Carbon NMR

Clearly it is possible to differentiate between the two diastereomers of Stilbene oxide by NMR. For example we can observe a general increase in shielding of in the cis isomer versus the trans isomer. By comparison of these spectra with future experimental spectra it will be possible to identify which isomers are formed or if there is a mixture.

It is also beneficial to make a comparison to the literature values of these shifts to confirm the results of the calculations.

Trans-Stilbene Oxide Proton NMR (ppm)[9]
(400 MHz; CDCl3) = 7.42–7.52 (10H, m), 3.98 (2H, s)
Trans-Stilbene Oxide Carbon NMR (ppm)[9]
(100 MHz; CDCl3) = 137.7, 129.1, 128.8, 126.1, 63.3
Cis-Stilbene Oxide Proton NMR (ppm)[16]
(400 MHz; CDCl3) = 7.21(M, 10H) 4.39(S 2H)
Cis-Stilbene Oxide Carbon NMR [9]
(100 MHz; CDCl3) = 134.8, 128.7, 127.6, 127.3, 60.2

The marked deviation of the calculations from the literature is the presence of a number of highly shielded peaks. This suggests that perhaps the calculation should be rerun. All peaks in this molecule should (by common sense) be quite deshielded as they are either aromatic or part of the epoxide group.

β-Methystyrene Oxide

Trans-β-Methystyrene Oxide Proton NMR Trans-β-Methystyrene Oxide Carbon NMR
Trans-β-Methystyrene Oxide Proton NMR Trans-β-Methystyrene Oxide Carbon NMR
Cis-β-Methystyrene Oxide Proton NMR Cis-β-Methystyrene Oxide Carbon NMR
Cis-β-Methystyrene Oxide Proton NMR Cis-β-Methystyrene Oxide Carbon NMR

The literature values for comparison are given below:


Trans-β-Methystyrene Oxide Proton NMR (ppm) [17]
(100 MHz; CDCl3) = 7.36-7.24 (m, 5H),

3.57 (d, J=2.0 Hz, 1H), 3.04 (dq, J =2.0, 5.4 Hz, 1H), 1.45 (d, J =5.4 Hz, 3H)

Trans-β-Methystyrene Oxide Carbon NMR (ppm) [17]
(100 MHz; CDCl3) = 137.7, 128.4, 128.0, 125.5, 59.5, 59.0, 17.9
Cis-β-Methystyrene Oxide Carbon NMR (ppm) [17]
(400 MHz; CDCl3) = 7.37-7.27 (m, 5H),

4.06 (d, J=4.4 Hz, 1H), 3.34 (dq, J=4.4, 5.4 Hz, 1H), 1.09 (d, J=5.4Hz, 3H)

Cis-β-Methystyrene Oxide Carbon NMR (ppm) [17]
(100 MHz; CDCl3) = δ 135.5, 128.0, 127.5, 126.6, 57.5, 55.1, 12.5

Determining the Chirality of Epoxides

Determining the optical rotation of a given molecule can be performed entirely computationally and thus by taking an experimental reading of optical rotation it is possible to assign the absolute chirality of a sample.

Calculations were performed on one of each of the enantiomeric pairs of chiral molecules (but not on the cis-Stilbene Oxide which is an achiral meso compound) using Gaussian at the CAM-B3LYP[18] level with the 6-311++g(2df,p) basis set. It was assumed that for speed the other enantiomer of each pair will rotate the same angle in the other direction however with more time it may be interesting to check this.

Stilbene Oxide

Isomer RR SS
Literature 250.8°[19],239.2°[20] -205.2°[21]
Calculated 298.21°[22] Not Calculated

In this case the literature is in general accordance with the calculated data but not precisely the same. It is at least of the correct sign.

cis-β-Methylstyrene Oxide

Isomer SR RS
Literature 38.6°[17] 37.8°[21]
Calculated 37.42°[23] Not Calculated

Clearly there is a very close correlation between the literature data and the calculated data in this case.

trans-β-Methylstyrene Oxide

Isomer RR SS
Literature 45.7°[24] -43.6°[24]
Calculated Not Calculated -46.77° [25]

Again, the literature is in good accordance suggesting a successful calculation.

In general this means that calculating optical rotation at the B3LYP-CAM level seems to be a good way of predicting the rotation in reality. It is an easy and efficient way to determine the absolute stereochemistry of a molecule with optical rotation data available.

Analysis of Transition States

It is also possible to predict the result of an epoxidation of a given alkene with a given catalyst entirely in sillico by modelling the various possible transition states and then looking for the lowest energy path way. In this project this has not been done exhaustively because it would require determining all likely transition states and then comparing the energy surfaces. However an example of methods that could be used to undertake this are shown using transition states that have been precomputed by H Rzepa.

Relative Energies of β-Methylstyrene Transition States

The table below shows the relative energies of the transitions states of a Shi catalyst epoxidation calculated by H Rzepa.

RR SS
-1343.022970(Ha)[26] -1343.017942(Ha)[27]
-1343.019233(Ha)[28] -1343.015603(Ha)[29]
-1343.029272(Ha)[30] -1343.023766(Ha)[31]
-1343.032443(Ha)[32] -1343.024742(Ha)[33]


These can all then be converted into kJ/mol using 1Ha=2.63*106Jmol-1[34] From this it is possible to find the relative rates of population of each transition state at 300K using ΔG=-RTlnK. We can then find the ratio of the transition states that lead to each isomer and finally convert to enantiomeric excess.

Energy in kJ/mol
RR SS
-3532150411 -3532137187
-3532140583 -3532131036
-3532166985 -3532152505
-3532175325 -3532155071
Energy in kJ/mol normalised to lowest energy transition state
RR SS
24913.99 38137.63
34742.3 44289.2
8339.73 22820.51
0 20253.63
K values at 300K
RR SS
2.19E+04 4.40E+06
1.13E+06 5.19E+07
2.84E+01 9.45E+03
1.00E+00 3.38E+03
Enantiomeric Excess
RR SS
Sum of Ks 1.15E+06 5.63E+07
Mol Fraction 2.00E-02 9.80E-01
Enantiomeric excess 96%

Weak interactions in the Shi transition state

Below is a QTAIM analysis of an SS transition state of β-Methylstyrene with the Shi catalyst[33]. This shows as yellow spheres the bond critical points which are the points where the turning points of electron density with respect to all spacial dimensions lie. This allows a visualization of the length of possible weak interactions.

QTAIM Image

Also performed on the same transition state[33] is a Non-Covalent interaction analysis. This shows areas of positive electronic interactions in green and repulsive interactions in red. You can see the large number of green interactions guiding in the alkene.

View NCI

Other Alkenes

A search using Reaxys was conducted to find alternative small size alkenes with a small optical rotation that could potentially be used in future labs.

A possible alkene to use would be hex-1-ene which would result in (1,2)epoxy hexane. This has an optical rotation of ca. 11°[35]

References

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