Just how difficult can it be to compute rotational barriers? Well, it turns out that for biphenyl 1, the answer is “very”!
The experimental barriers for rotation about the C1-C1’ bond of biphenyl are 6.0 ± 2.1 kcal mol-1 at 0° and 6.5 ± 2.0 kJ mol-1 at 90°.1 CCSD(T) with extrapolated basis set approximation computations by Sancho-Garcı´a and Cornil overestimate both barriers by more than 4 kJ mol-1 and, more critically in error, predict that the 0° barrier is higher in energy than the 90° barrier.2
Now Johansson and Olsen have reported a comprehensive study of the rotational barrier of biphenyl.3 They tackled a number of different effects:
- Basis sets: The cc-pVDZ basis set is simply too small to give any reasonable estimate (See Table 1).
- Correlation effects: HF, MP2, SCS-MP2 and CCSD overestimate the barriers and get the relative energies of the two barriers wrong, regardless of the basis set. While CCSD(T) does properly predict the barrier at 0° is lower than that at 90°, even this level overestimates the barrier heights (Table 1).
- Their best CCSD(T) energy using a procedure to extrapolate to infinite basis set still gives barriers that are too high, though in the right relative order: E(0°)=7.97 and E(90°) = 8.79 kJ mol-1.
- Inclusion of Core-Core and Core-Valence correlation energy reduces the 0° barrier and raises the 90° barrier a small amount. With an extrapolation for completeness in the coupled clusters expansion, their best estimates for the two barriers are 7.88 and 8.94 for the 0° and 90° barriers, respectively.
- Relativity has no effect on the barrier heights. (This is a great result – it suggests that we don’t have to worry about relativistic corrections for normal organics!)
- Intramolecular basis set superposition error might be responsible for as much a 0.4 kJ difference in the energies of the two barriers.
- Inclusion of vibrational energies along with all of the other corrections listed above leads to their best estimate of the two barriers: E(0°)=8.0 and E(90°) = 8.3 kJ mol-1, which are at least in the correct order and within the experimental error bars.
Table 1. Computed torsional barriers in kJ mol-1.
|
||||
|
MP2 |
CCSD(T) |
||
|
0° |
90° |
0° |
90° |
cc-pVDZ |
12.23 |
7.68 |
10.89 |
7.23 |
aug-cc-pVDZ |
9.68 |
7.45 |
9.23 |
6.67 |
cc-pVTZ |
9.86 |
9.13 |
8.85 |
8.50 |
aug-cc-pVTZ |
9.78 |
9.43 |
8.83 |
8.86 |
cc-pVQZ |
9.65 |
9.33 |
8.68 |
8.74 |
aug-cc-pVQZ |
9.35 |
9.31 |
8.39 |
8.76 |
|
Who would have thought this problem was so difficult?
References
(1) Bastiansen, O.; Samdal, S., "Structure and barrier of internal rotation of biphenyl derivatives in the gaseous state: Part 4. Barrier of internal rotation in biphenyl, perdeuterated biphenyl and seven non-ortho-substituted halogen derivatives," J. Mol. Struct., 1985, 128, 115-125, DOI: 10.1016/0022-2860(85)85044-4.
(2) Sancho-Garcia, J. C.; Cornil, J., "Anchoring the Torsional Potential of Biphenyl at the ab Initio Level: The Role of Basis Set versus Correlation Effects," J. Chem. Theory Comput., 2005, 1, 581-589, DOI: 10.1021/ct0500242.
(3) Johansson, M. P.; Olsen, J., "Torsional Barriers and Equilibrium Angle of Biphenyl: Reconciling Theory with Experiment," J. Chem. Theory Comput., 2008, 4, 1460-1471, DOI: 10.1021/ct800182e.
InChIs
Biphenyl 1: InChI=1/C12H10/c1-3-7-11(8-4-1)12-9-5-2-6-10-12/h1-10H
InChIKey: ZUOUZKKEUPVFJK-UHFFFAOYAV
guest responded on 15 Oct 2008 at 11:26 am #
Maybe F12 can give a better result with smaller basis set. For my knowledge, the basis set extrapolation has not been mathematical derived besides Helium, if I were correct, it is really doubtful about the validity for such extrapolation.
baoilleach responded on 16 Oct 2008 at 9:45 am #
No mention of DFT. Would be interesting to know how it compares…?
Wawrzek responded on 17 Oct 2008 at 7:47 am #
I investigated rotation barrier for pyridinium N-phenolate betaine dye and I did comparison with biphenyl, so you’ll find references to older biphenyl papers with DFT results here:
http://www.springerlink.com/content/h5446226655661x6/
Wawrzek responded on 17 Oct 2008 at 7:48 am #
Once more it me:
references 16-20 (but I’m not sure now and don’t have time to check it)