| Literature DB >> 26626928 |
Anne Knorr1, Ralf Ludwig1,2.
Abstract
Direct spectroscopic evidence for H-bonding between like-charged ions is reported for the ionic liquid,Entities:
Year: 2015 PMID: 26626928 PMCID: PMC4667241 DOI: 10.1038/srep17505
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1(a) Infrared spectra of the O-H stretching vibrations of the ionic liquid 1-(2-hydroxyethyl)-3-methylimidazolium tetrafluoroborate as a function of temperature between 233 K and 413 K. The arrow indicates the increasing intensitiy of the appearing vibrational band at 3402 cm−1. (b) The IR spectrum at the lowest temperature (233K) can be properly decomposed into four contributions at 3547 cm−1, 3496 cm−1, 3402 cm−1 and 3286 cm−1, respectively.
Figure 2B3LYP-6-31G*-D3 calculated structures of possible tetrameric clusters including four ion-pairs: tetramer ca, including solely cation-anion pairs characterized by OH…F hydrogen bonds; tetramer cc, with additional cation-cation interaction resulting in cooperative hydrogen bonding OH…OH…OH…OH…F; and tetramer cc-cyc, showing a strongly cooperative H-bonded cyclic tetramer of cations via (OH…O)4 bonds.
Figure 3A plot of the calculated O-H vibrational redshifts for all cc-clusters: the linear dimer, trimer and tetramer (open circles) and the cyclic tetramer (open square).
The shifts are determined relative to the average of the O-H stretches of the corresponding ca-clusters n = 2–4. For comparison, the redhifts of the deconvoluted bands of the measured spectra are shown as grey bars (the colors of the crosses indicate the deconvoluted bands in Fig. 1b). The calculated redshifts strongly suggest that all species are present in the liquid. The dotted lines indicate the frequency shifts obtained from calculating the derivatives of the measured spectra (see SI).
Figure 4Plots of the natural logarithm of the cc to ca vibrational band intensity ratios versus inverse temperature, taken from the measured spectra in Fig. 1 between 233 K and 373 K.
Three procedures were applied: (a) Icc and Ica of the deconvoluted bands (diamonds), (b) Icc and Ica of the deconvoluted bands each weighted by the calculated intensities of the species (circles) and (c) Icc and Ica obtained from the integral intensities left and right of the frequency position, where the deconvoluted vibrational bands for the ca and the first cc species cross (squares). The solid lines represent linear fits (R2 ≥ 0.98) with a slope of ΔE/R. ΔE, the difference in energy between the two different H-bonding configurations, is determined to be (a) 2.9 ± 0.02 kJmol−1, (b) 3.4 ± 0.02 kJmol−1 and (c) 3.9 ± 0.02 kJmol−1, respectively.
Figure 5Differences of NBO calculated stabilization energies ΔE(2)n→σ* (circles) and estimated total charge transfers qTC (squares) between the clusters n = 2–4 for the two classes of H-bond configurations cc and ca, plotted versus calculated average OH redshifts.
The linear dependence indicates the strong relation between NBO stabilization energies and charge transfers with spectroscopic properties such as IR frequencies.