Gianluca Ciancaleoni*a,
Alceo Macchionib,
Luca Rocchigianibc and
Cristiano Zuccacciab
aDepartamento de Química, Universidade Federal de Santa Catarina, 88040-900 Florianópolis, SC, Brazil. E-mail: g.ciancaleoni@ufsc.br
bDipartimento di Chimica, Biologia e Biotecnologie, Universitá degli Studi di Perugia, Via Elce di Sotto 8, I-06123, Perugia, Italy
cSchool of Chemistry, University of East Anglia, Norwich, NR4 7TJ, UK
First published on 18th August 2016
We demonstrate here that the Pulsed field Gradient Spin Echo (PGSE) NMR diffusion technique can be effectively used as a complementary tool for the characterization of mono- and multi-site intermolecular halogen bonding (XB) in solution. The main advantage of this technique is that it provides the possibility of unambiguously determining the stoichiometry of the supramolecular adduct, information that is particularly important when multi-site molecular systems are studied. As an example, PGSE NMR measurements in chloroform indicate that hexamethylenetetramine (HMTA), a potentially four-site XB acceptor, actually exploits only two sites for the interaction with the XB donor N-bromosuccinimide (NBS), leaving the other two nitrogen sites unoccupied. Charge displacement calculations suggest that this is due also to the anti-cooperativity of the XB interaction between HMTA and NBS.
Recently, it has been suggested9 that halogen bonding is not the only interaction that XB donors and acceptors can establish in solution, even when no other obvious interactions are possible, leading to adducts with different geometries but same stoichiometry. We recently demonstrated that 19F, 1H HOESY NMR, previously exploited with success to investigate ion pairing10 and frustrated Lewis pairs,11 can be also exploited to disclose the intermolecular structure of XB adducts.12 Furthermore, in combination with theoretical studies, it can be used to estimate the relative weights of XB and non-XB interactions.12
Concerning the equilibrium constants involved in the XB interactions, many useful titration techniques have been applied13,14 and the choice of the best one (UV-Vis, IR, NMR…) depends on the nature of the system under investigation. In all cases, the presence of more interactions is a potential complication, because the effect of each interaction on the experimental observable is, in principle, of a different magnitude, and their disentanglement is not easy. An additional layer of complexity arises when multi-site acceptors and donors are taken into account. In this case, the exact nuclearity of the adduct should be known a priori, since the fitting equation depends on the stoichiometry of the adduct (except when the different aggregation steps are clearly consecutive and with very different affinities14). Information about the latter can be derived from the Job's plot, but the general applicability of this technique is limited15 and its coupling with other methodologies is always desirable.
Here, we propose the diffusion Pulsed field Gradient Spin Echo (PGSE)16,17 NMR technique as a tool for the characterization of mono- and multi-site intermolecular halogen bonding systems, with the only requirement that NMR-active nuclei (preferably 1H, 19F or 31P) are present on at least one, but preferably both, of the components. To the best of our knowledge, such a technique has been applied only in a few recent cases, to support the formation of strong halogen-bonded adducts and to study the counterion influence on the same adduct.18,19
PGSE NMR allows information about the hydrodynamic volume (VH) of molecular species in solution to be determined.17 In the case of an aggregation process, the measured VH increases, allowing the estimation of the equilibrium constants (Ka) involved in the process.20 Remarkably, in the case of 1:1 adducts, the Ka can be evaluated by one single experiment,21 making it a useful tool for preliminary measurements.
Furthermore, since PGSE NMR is based exclusively on the VH, it takes into account all the possible aggregation processes, irrespectively from the supramolecular structure of the adduct. This offers the possibility to validate the data coming from titration techniques, where the effect of various interactions could be different on the chosen observable, with the general rule that Ka (PGSE) ≥ Ka (titration). In addition, PGSE NMR is very useful when investigating symmetric multi-site XB donors or acceptors, since it gives directly the average size of the adducts and allows the determination of the average number of units that are interacting.
To illustrate the potential of the PGSE approach, we considered here Lewis acids and bases shown in Scheme 1, which already proved to be XB acceptors/donors,22 having different XB strength and number of sites. In particular, 1,4-diazabicyclo[2.2.2]octane (DABCO) and hexamethylenetetramine (HMTA) are commonly used in the fabrication of crystalline materials assembled by XB.23
Scheme 1 XB donors and acceptors considered in this work. In parenthesis, the respective values for the hydrodynamic volume of the single molecule (V0H) are reported. |
In both cases, the number of nitrogen atoms involved in XB interactions depends on the XB donor and the crystallization conditions. 2,4,6-Trimethylpyridine (Me3Py) is rarely used because the resulting XB adduct is very weak, so weak that other minor interactions, as lone pair/π, cannot be neglected.12 On the other hand, perfluorinated alkanes and benzenes (as perfluorohexyl-1-iodide, I1, pentafluoroiodobenzene, I2 and 2,4-diiodooctafluorobutane, I3) have always been used in XB studies,24 whereas N-bromosuccinimide (NBS) only recently revealed its potential as XB donor.22c
For this reason, we initially performed PGSE NMR experiments on solutions of increasing concentration of the single components in toluene-d8 or chloroform-d, obtaining concentration-independent (within the experimental error of ±10%) values of V0H equal to 220, 168, 128, 137, 135, 132 and 189 Å3 for I1, I2, I3, NBS, Me3Py, DABCO and HMTA, respectively (Table 1 and Scheme 1).
C | Dt | rH | VH |
---|---|---|---|
Me3Py | |||
3.1 | 16.1 | 3.18 | 135 |
38.0 | 15.9 | 3.20 | 137 |
175 | 16.2 | 3.18 | 135 |
385 | 16.1 | 3.18 | 135 |
DABCO | |||
46.0 | 16.9 | 3.17 | 133 |
262 | 17.2 | 3.14 | 130 |
I1 | |||
11.0 | 12.8 | 3.78 | 226 |
123 | 12.9 | 3.70 | 212 |
181 | 12.8 | 3.75 | 221 |
I2 | |||
17.4 | 15.3 | 3.37 | 160 |
471 | 14.5 | 3.47 | 175 |
I3 | |||
19.0 | 14.1 | 3.11 | 126 |
210.0 | 14.2 | 3.14 | 130 |
HMTA | |||
19.0 | 12.0 | 3.54 | 187 |
110 | 12.2 | 3.58 | 192 |
NBS | |||
5.4 | 14.3 | 3.20 | 137 |
61.0 | 14.3 | 3.20 | 137 |
The hydrodynamic volume of any adduct can be calculated by the sum of the V0H values of the constituents (eqn (1)), always under the spherical approximation.17
VaggH(nD, mA) = n × V0H(D) + m × V0H(A) | (1) |
C(Me3Py) | Dt(Me3Py) | Dt(I1) | VH(Me3Py) | VH(I1) |
---|---|---|---|---|
24.9 | 16.1 | 12.9 | 146 | 219 |
64.1 | 16.1 | 12.8 | 144 | 221 |
346 | 16.1 | 12.4 | 146 | 232 |
4910 | 15.7 | 10.3 | 152 | 340 |
On the other hand, the 19F NMR titration method gives a value of Ka = 0.85 ± 0.01 M−1 (Fig. S1, ESI†).25 The titration allows to rapidly collect a large number of data, minimizing the experimental error. By the way, the formation constant obtained by diffusion measurements is double with respect to that obtained by the titration method, and this can be explained with the presence of two different 1:1 adducts, as already evidenced by HOESY results:12 the observable of the titration (δF of the α fluorine atoms, –CF2I) is mainly influenced by the XB interaction established between the nitrogen of Me3Py and the iodine of I1, whereas the observable of the PGSE (VH) is influenced by all the possible interactions, including electrostatic H⋯F ones.12 Since the Ka estimated by the PGSE measurement is the sum of all the equilibrium constants active in solution, by coupling the two techniques we can conclude that the formation constant of non-XB adducts is approximately 0.75 M−1.
Remarkably, also combining 19F, 1H HOESY results with DFT calculations, the XB adducts resulted to be predominant over the non-XB ones (XB:non-XB = 78:22);12 considering the approximations used in that paper, a reasonably good agreement is obtained.
Interestingly, in the solid state only the XB can be detected,26 demonstrating that the supramolecular behavior of a pair in solution can differ from the structure of the same pair in the crystal.
Maintaining C(I1) constant at 20 mM (solvent: toluene-d8) and increasing C(DABCO) from 3.6 to 108 mM, VH(I1) increases from 239 to 338 Å3, whereas VH(DABCO) decreases from 221 to 162 Å3. As stated before, the effect of aggregation is more visible on the least abundant species, consequently when C(DABCO) < C(I1), VH(I1) is just slightly larger than V0H(I1) and VH(DABCO) is markedly larger than V0H(DABCO). On the contrary, when C(DABCO) > C(I1), the situation is the opposite, with VH(DABCO) similar to V0H(DABCO) and VH(I1) markedly higher than V0H(I1). Indeed, when the concentration ratio I1:DABCO is 20:108, V0H(I1) approaches VaggH(DABCO, I1), which is 352 Å3, evidencing an almost complete association of I1 under these conditions.
Applying eqn (S1) and (S2) (ESI†) to this single data, Ka1 was estimated to be 34 ± 10 M−1, which corresponds to a free energy of association (ΔGa1) of −2.1 kcal mol−1. The 19F NMR titration gives Ka1 = 37.2 ± 0.4 M−1 (Fig. S2, ESI†), in agreement within the experimental errors.27 In line with these findings, 19F, 1H HOESY NMR data demonstrated that non-XB interactions can be neglected for this particular pair.12 Obviously, this does not mean that non-XB interactions are absent, but simply that their effects are completely hidden by the much more intense XB interaction, as in the PGSE as in the HOESY NMR experiments.
Successively, maintaining C(DABCO) at 7 mM and increasing C(I1) from 37 to 343 mM, VH(DABCO) increases from 250 to 517 Å3 (Table 3). In the last case, the hydrodynamic volume is much higher than V0H(DABCO), even higher than the volume of the 1:1 adduct (352 Å3) and close to that of the 1:2 adduct [VaggH(DABCO, 2I1) = 572 Å3].
C(DABCO) | C(I1) | Dt(DABCO) | Dt(I1) | VH(DABCO) | VH(I1) |
---|---|---|---|---|---|
3.6 | 20.0 | 12.8 | 12.3 | 221 | 239 |
17.6 | 20.0 | 13.7 | 11.9 | 194 | 250 |
108 | 20.0 | 15.1 | 10.3 | 162 | 328 |
7.0 | 37.0 | 12.0 | — | 250 | — |
7.0 | 85.0 | 10.5 | — | 326 | — |
7.0 | 216 | 9.2 | — | 426 | — |
7.0 | 343 | 8.5 | — | 517 | — |
The data of VH(DABCO) as a function of C(I1) can be fitted considering two equilibria (Fig. 1 and eqn (S3) and (S4), ESI†),15 either imposing Ka1 = 34 M−1, as determined previously, to find the best value of Ka2 or optimizing both Ka1 and Ka2. In the former case, Ka2 = 5 ± 1 M−1 (ΔGa2 = −0.9 kcal mol−1); in the latter case, Ka1 = 17 ± 6 M−1 and Ka2 = 7 ± 2 M−1. The results of the two methodologies are qualitatively similar, even if the second one, having more degrees of freedom, better fits the experimental data (Fig. 1). In any case, Ka2 is lower than Ka1. This is likely due to the low entropy of the adduct formed by three molecules.
More importantly, the PGSE results offer an immediate and intuitive insight into the nuclearity of the adducts, at each concentration ratio (Fig. 1).
C(DABCO) | C(I2) | Dt(DABCO) | VH(DABCO) |
---|---|---|---|
8.8 | 44.0 | 13.6 | 194 |
8.8 | 177 | 11.2 | 286 |
8.8 | 403 | 10.1 | 352 |
For HMTA/NBS, the calculated hydrodynamic volumes for the 1:1, 1:2, 1:3 and 1:4 adducts are 323, 457, 591 and 729 Å3, respectively.
Using chloroform-d as solvent and keeping C(NBS) fixed at 3.9 mM, three solutions with C(HMTA) = 12.1, 50 and 179 mM have been analyzed. VH(NBS) increases as C(HMTA) increases, going from 254 to 317 Å3 (Table 5), which is very close to VaggH(HMTA, NBS). Fitting the data, Ka1 results to be 161 ± 27 M−1 (ESI†).
In a second set of experiments, to a solution of HMTA (C = 2.1 mM) in chloroform-d, NBS was added to reach C(NBS) = 4.3, 38.5, 56 and 93 mM (Table 5). As before, the hydrodynamic volume of the component in excess decreases as its concentration increases [VH(NBS) goes from 150 to 131 Å3], whereas the hydrodynamic volume of the other component (VH(HMTA)) increases from 217 to 438 Å3. Noteworthy, passing from C(NBS) = 56 to 93 mM, VH(HMTA) increases of only 30 Å3, which is within the experimental error of 10%. Unfortunately, a higher concentration of NBS is not possible because of the solubility limit of the mixture, but the final value of VH(HMTA) is very close to VaggH(HMTA, 2NBS). Such a value is the average of all the volumes of the species present in solution, but considering also that the trend of VH(HMTA) vs. C(NBS) shows a plateau in the correspondence of VaggH(HMTA, 2NBS) (Fig. 2), we can deduce that Ka3 and Ka4 are likely too small to be determined. Consequently, the experimental data can be fitted with the 1:2 model, in agreement with the crystal structure of this pair.22c The absence of a plateau in this range of VHs (400–500 Å3) would have been an indication for the existence of larger adducts, as 1:3 and 1:4.
This reveals another great advantage of the diffusion NMR technique: for multi-site systems, the maximum stoichiometry is not a hypothesis, but can be derived from the trend of VH with the concentration.
Fitting the experimental data with the 1:2 model and fixing Ka1 = 161, the best value of Ka2 is 44 ± 12 M−1 (ΔGa2 = −2.2 kcal mol−1), whereas optimizing both the values the results are 90 ± 20 and 56 ± 8 M−1 for Ka1 and Ka2, respectively (ΔGa1 = −2.6 kcal mol−1; ΔGa2 = −2.4 kcal mol−1). Also in this case, both methodologies give similar results and, again, Ka1 is larger than Ka2.
In order to understand better why the 1:3 adducts are not easily accessible in solution, DFT calculations have been performed on this system. Optimizing the structure of the 1:1, 1:2 and 1:3 adducts (level of theory M06-2X/def2-TZVP, as suggested by a recent, dedicated benchmark,28 see details in the Computational details), the N⋯Br distances results to be 2.533, 2.585 and 2.628 Å, respectively. The progressive lengthening of the N⋯Br distance already indicates that the interaction is weaker as the number of NBS molecules around the central HMTA increases.
Other information can be obtained with the Charge Displacement (CD) method,29 which already proved to be useful for the characterization of coordinative30 and non-covalent bonds,11,31 including halogen bonding.32 In particular, CD results demonstrated to be correlated linearly to the formation constants of chalcogen-bonded adducts.33
In the case of 1:1 adducts, the difference of electron density (Δρ) between the adduct and the separate fragments (HMTA and NBS) is shown in Fig. 3a. It clearly shows that the nitrogen of HMTA is in a region of electron depletion, whereas a region of electron accumulation is present between the nitrogen and the bromine. As expected, a charge transfer between the two molecules exists, going from the nitrogen to the bromine. The latter shows a polarization pattern (depletion in the direction of HMTA, accumulation on the other side) and a remarkable region of electron accumulation is on the nitrogen of the NBS. The backbone of the NBS show a small charge accumulation, whereas the nitrogen atoms of the HMTA not involved in the XB show a small charge depletion, indication that the charge flux involve the entire system.
Integrating Δρ along the axis containing the nitrogen of HMTA and the bromine of NBS (z), the charge transfer (CT) can be quantified as 0.130 e (Fig. 3b).
Applying the same method to the 1:2 and 1:3 adducts, the corresponding Δρ maps reveal a qualitative similarity with the one calculated for the 1:1 adduct (Fig. 4a and S5, ESI†). This is reasonable, since in all the cases the interaction is similar. From the quantitative point of view, the integration of the Δρ functions leads to CT values of 0.110 and 0.095 for the 1:2 and 1:3 adduct, respectively. The attenuation of the CT as the number of NBS molecules around the central HMTA increases gives a framework to explain the attenuation of the formation constants: the four nitrogen atoms on the HMTA are not mutually independent, and the donation of electronic density from one nitrogen atom to a Lewis acid makes the donation properties of the non-involved nitrogen atoms lower.
This effect can be quantified applying the CD on a different axis.34 If we consider the adduct between HMTA and two NBS moieties, we obviously have two interactions between two different nitrogen atoms of the HMTA and the two molecules of NBS. They can be labeled N1⋯NBS1 and N2⋯NBS2. Taking as fragments NBS1 and HMTA/NBS2 and integrating Δρ along the axis containing N2 and the bromine of NBS2 (Fig. 4), the effect of the establishment of N1⋯NBS1 on N2⋯NBS2 can be evaluated. In this case, the analysis of the Δρ shows that, upon the formation of N1⋯NBS1, the nitrogen of NBS2 is located in a region of electron density depletion. This indicates a charge transfer from NBS2 to HMTA, leading to a XB weakening. The integration along the axis containing N2 and Br2 confirms the direction of the flux and leads to a weakening of 0.011 e (Fig. 4b).
The electronic energies ΔE of the 1:1, 1:2 and 1:3 adducts are −11.6, −20.5 and −28.0 kcal mol−1 (ESI†) with respect to the isolated components (see Table S1, ESI†). If we calculate ΔE/n, where n is the number of NBS involved in the adduct, it results −11.6, −10.2 and −9.3 kcal mol−1, respectively, again indicating that the interactions become weaker for larger aggregates (anti-cooperativity), in agreement with CD results. Therefore, the formation of adducts with higher stoichiometric ratios, as 1:3 and 1:4, is made difficult not only for obvious entropic reasons (each additional moiety loses its translational degree of freedom, making the ΔG more positive), but also for enthalpic ones (the charge transfer becomes weaker as the number of units increases). Interestingly, in other cases the XB resulted to be cooperative in nature.35
Applying eqn (S1) and (S2) (ESI†) to the experiments where one component is in excess [C(DABCO) = 85.8 and C(I3) = 58 mM, Table 6], Ka1 results to be 6 ± 2 and 10 ± 3 M−1, respectively (ΔGa1 = −1.2 kcal mol−1).
In particular, for the pair Me3Py/I1 the complementarity of the NMR titration and the PGSE method allowed the estimation of the formation constant of the adducts held together by interactions different from the XB (non-XB).
In the case of the ditopic halogen acceptor DABCO, both 1:1 and 1:2 adducts have been directly detected, either using aliphatic and aromatic perfluorinated XB donors (I1 and I2). The corresponding formation constants have been evaluated and the formation of the 1:2 adduct showed an equilibrium constant considerably lower than that of the 1:1 adduct. For this system, the formation constant of the 1:1 adduct evaluated by NMR titration is in agreement with that measured by PGSE, indication that non-XB adducts are negligible.
The case of HMTA is even more interesting, since it bears four symmetric nitrogen atoms and all of them potentially could establish an interaction with NBS. PGSE NMR data unequivocally demonstrate that only two nitrogen atoms are involved in the interaction with NBS and, again, the formation constant of the 1:2 adduct resulted lower than that of the 1:1 adduct. DFT and charge displacement investigations demonstrated that each molecule of NBS that binds on a nitrogen atom of the HMTA reduces the electron-donating properties of the other nitrogen atoms (anti-cooperativity).
Finally, PGSE NMR data demonstrated also that the interaction between DABCO and I3 is too weak in chloroform-d to produce aggregates larger than the 1:1 adduct, despite both the XB acceptor and donor possess two binding sites and despite the existence in the solid state of infinite chains.
In conclusion, PGSE NMR can be surely considered a powerful technique, which gives information that could be a complement for the titration methods routinely used up to now. For this reason, an integrated multi-technique approach, which include titrations, diffusion and Overhauser NMR techniques (but also DFT calculations, when needed) is highly desirable, for a complete characterization of XB systems in solution.
(2) |
The self-diffusion coefficient Dt, which is directly proportional to the slope m of the regression line obtained by plotting ln(I/I0) versus G2, was estimated by evaluating the proportionality constant for a sample of HDO (5%) in D2O [known diffusion coefficients in the range 274–318 K (ref. 38)] under the exact same conditions as the sample of interest. The solvent or TMS was taken as internal standard.
All the charge displacement29 calculations were carried out using density functional theory employing the same level of calculation used for optimizations. Such an approach relies on the integration along a given direction z (eqn (3)) of the difference of electronic density [Δρ(x, y, z)] between the adduct and its non-interacting fragments, frozen in the same positions they occupy in the adduct.
(3) |
The value of Δq(z′) defines the amount of the electronic charge that, upon formation of the adduct, has moved across a plane perpendicular to the axis through the coordinate z′. At the boundary between the fragments (the point on the z axis at which equal-valued isodensity surfaces of the isolated fragments are tangent) the value of Δq is represented by CT.
The electronic density matrices have been manipulated through the suite of tools “Cubes”.42
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c6ra17455h |
This journal is © The Royal Society of Chemistry 2016 |