Haloacetonitrile-BF3 Complexes
Thin films of the bulk solids were prepared by first making a
dilute gas mixture containing nitrile, BF3, and argon on a vacuum
line. For the Cl- and F-containing species, mixtures containing
approximately 0.5% nitrile, 0.5% BF3, and 99% argon, were used,
though in some cases, a slight excess of nitrile was added to
minimize peaks due to unreacted BF3 (between 1450 and 1500
cm-1). For BrCH2CN-BF3, the mixtures were more dilute, typically
0.2% BrCH2CN and BF3, since the vapor pressure of BrCH2CN is
much lower that of FCH2CN and ClCH2CN. Films were deposited
directly onto the cold (120 K) KBr sample window by flowing the
gas mixtures into the cryostat vaccum chamber at a rate of roughly
5 mmol/h. Argon does not condense on the sample window at this
temperature; thus, only the nitrle and BF3 are deposited. Like
(CH3)3CCN-BF3 and C6H5CN-BF3,23 the spectra obtained closely
resemble low-temperature, solid-state IR spectra of CH3CN-BF3,6
indicating that the majority of the sample consists of nitrile-BF3
complexes, though the very bright vibrational bands of excess,
unreacted BF3 were also observed in some experiments.
for some MP2 calculations on FCH2CN-BF3, including those in
which we explored the relative stability of F-bonded isomeric
structures.
IV. Results and Discussion
Computational Structure Results. Initial B3LYP calcu-
lations indicated that all complexes were slightly bent about
the C-N-B linkage and, moreover, that the torsional degree
of freedom was extremely flat. Thus, to be systematic in
our search for the minimum-energy structures, we conducted
four parallel sets of optimizations, each starting with the
C-N-B angles set to 180° in either the eclipsed or staggered
conformation, and with or without enforcing Cs symmetry.
The staggered forms were found to be most stable at the
B3LYP/6-311+G** level, but by only a few calories per
mole (0.005 kcal/mol in the case of FCH2CN-BF3). Fur-
thermore, each complex was indeed bent slightly along the
C-N-B linkage by about 2°, so the conformers are not
strictly “eclipsed” or “staggered” in the formal sense.
Nonetheless, we retain these terms throughout for the sake
of simplicity.
At this point, we identified two reasons to be concerned
with these B3LYP results. First of all, B3LYP results for
CH3CN-BF3 lacked complete convergence with even larger
basis sets, up to aug-cc-pVQZ.12 Furthermore, a recent study
of amine-borane systems cast doubt on the performance of
B3LYP for B-N dative bonds.34 Thus, we conducted a
survey of various DFT methods (and MP2 with somewhat
smaller basis sets) on the equilibrium structure of staggered
FCH2CN-BF3 (Cs) under the presumption that some degree
of consistency would emerge. Table 3 lists equilibrium B-N
distances obtained in this survey, and overall, there is a
considerable degree of inconsistency among the various
methods. For the most part, however, B-N distances are a
few hundredths of an angstrom shorter when diffuse func-
tions are used (i.e., aug-cc-pVTZ), and this has been noted
in several previous instances for nitrile-BF3 systems.12,21-23
Regardless, in the absence of an experimental structure, it
was unclear which method was most reliable. To address
this ambiguity, we conducted (and recently completed) a
validation study on HCN-BF3,22 a similar and also fairly
weak complex for which an experimental structure has
been determined.14 In that work, we found that several hy-
brid DFT/HF methods (B3LYP, B3PW91, B98, and
mPW1PW91)29 yielded structures that agreed favorably with
experiment, with B3PW91 providing the best agreement,
even superior to MP2 (with the aug-cc-pVTZ basis set).
For the most part, the results in Table 3 track those
obtained for HCN-BF3,22 and thus, we chose to utilize
B3PW91/aug-cc-pVTZ as our preferred method for this
study. For completeness sake, we obtained B3LYP/aug-cc-
pVTZ and mPW1PW91/aug-cc-pVTZ results as well. Se-
lected structure parameters of both the eclipsed and staggered
conformers from all three methods are listed in Table 4, and
complete, minimum-energy B3PW91/aug-cc-pVTZ struc-
tures are displayed in Figure 2. For the F- and Cl-containing
III. Computational Methods
The HF/6-311G* orbitals displayed in Figure 1, as well as
preliminary B3LYP29 calculations on the X-CH2CN-BF3 (X )
F, Cl, Br) systems using Pople basis sets (6-31G*, 6-31+G*,
6-311G*, and 6-311+G**)29,30 were performed using SPARTAN
‘02 (Macintosh v 1.0.3, and Windows v 1.0.1).31 Aside from this
preliminary work, all other computations were performed using
Gaussian03,32 which enabled the use of several additional density
functional methods, larger basis sets, and tighter convergence
criteria for geometry optimizations. Version b.0.1 was used for MP2
and all density functional methods except O3LYP,29 for which
version c.0.3 was used. An ultrafine grid was employed for all DFT
calculations in Gaussian, and convergence criteria for optimizations
(except as noted) were set using the “opt)tight” option (which sets
the maximum and RMS forces to 1.5 × 10-5 and 1.0 × 10-5
hartrees/bohr, respectively, and the maximum and RMS displace-
ments to 6.0 × 10-5, and 4.0 × 10-5 bohr, respectively). The aug-
cc-pVTZ basis set29,33 was used for most Gaussian03 calculations,
although the cc-pVTZ basis set33 was also used for DFT calculations
on FCH2CN-BF3 to examine the effect of diffuse functions
(signified by “aug-“) on the structural results. The analogous
double-ú basis sets (cc-pVDZ, and aug-cc-pVDZ)33 were also used
(29) For a recent overview of density functional theory and other
computational methods and basis sets used in this work, see: Cramer,
C. J. Essentials of Computational Chemistry, 2nd ed.; John Wiley and
Sons: Sussex, 2004, and references therein.
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(31) SPARTAN ‘02; Wavefunction, Inc.: Irvine, CA, 2002.
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M. A.; Cheeseman, J. R.; Montgomery, J. A., Jr.; Vreven, T.; Kudin,
K. N.; Burant, J. C.; Millam, J. M.; Iyengar, S. S.; Tomasi, J.; Barone,
V.; Mennucci, B.; Cossi, M.; Scalmani, G.; Rega, N.; Petersson, G.
A.; Nakatsuji, H.; Hada, M.; Ehara, M.; Toyota, K.; Fukuda, R.;
Hasegawa, J.; Ishida, M.; Nakajima, T.; Honda, Y.; Kitao, O.; Nakai,
H.; Klene, M.; Li, X.; Knox, J. E.; Hratchian, H. P.; Cross, J. B.;
Bakken, V.; Adamo, C.; Jaramillo, J.; Gomperts, R.; Stratmann, R.
E.; Yazyev, O.; Austin, A. J.; Cammi, R.; Pomelli, C.; Ochterski, J.
W.; Ayala, P. Y.; Morokuma, K.; Voth, G. A.; Salvador, P.;
Dannenberg, J. J.; Zakrzewski, V. G.; Dapprich, S.; Daniels, A. D.;
Strain, M. C.; Farkas, O.; Malick, D. K.; Rabuck, A. D.; Raghavachari,
K.; Foresman, J. B.; Ortiz, J. V.; Cui, Q.; Baboul, A. G.; Clifford, S.;
Cioslowski, J.; Stefanov, B. B.; Liu, G.; Liashenko, A.; Piskorz, P.;
Komaromi, I.; Martin, R. L.; Fox, D. J.; Keith, T.; Al-Laham, M. A.;
Peng, C. Y.; Nanayakkara, A.; Challacombe, M.; Gill, P. M. W.;
Johnson, B.; Chen, W.; Wong, M. W.; Gonzalez, C.; Pople, J. A.
Gaussian 03, revision B.03; Gaussian, Inc.: Wallingford, CT, 2004.
(33) Woon, D. E.; Dunning, T. H., Jr. J. Chem. Phys. 1993, 98, 1358.
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