Jennifer
Dupont
a,
Beppo
Hartwig
b,
Katia
Le Barbu-Debus
a,
Valeria
Lepere
a,
Regis
Guillot
c,
Martin A.
Suhm
b and
Anne
Zehnacker
*a
aInstitut des Sciences Moléculaires d’Orsay (ISMO), CNRS, rue André Rivière, Université Paris-Saclay, F-91405 Orsay, France. E-mail: anne.zehnacker-rentien@universite-paris-saclay.fr
bInstitut für Physikalische Chemie, Georg-August-Universität Göttingen, Tammannstr. 6, 37077 Göttingen, Germany
cInstitut de Chimie Moléculaire et des Matériaux d’Orsay (ICMMO), 17 Av. des Sciences Université Paris-Saclay, F-91405 Orsay, France
First published on 12th March 2024
The structure and clustering propensity of a chiral derivative of cis-1,2-cyclohexanediol, namely, 1-phenyl-cis-1,2-cyclohexanediol (cis-PCD), has been studied under supersonic expansion conditions by combining laser spectroscopy with quantum chemistry calculations. The presence of the phenyl substituent induces conformational locking relative to cis-1,2-cyclohexanediol (cis-CD), and only one conformer of the bare molecule is observed by both Raman and IR-UV double resonance spectroscopy. The homochiral preference inferred for the dimer formation at low enough temperature is in line with the formation of a conglomerate in the solid state. The change in clustering propensity in cis-PCD relative to trans-1,2-cyclohexanediol (trans-CD), which shows heterochiral preference, is explained by the presence of the phenyl substituent rather than the effect of cis-trans isomerism. Indeed the transiently chiral cis-CD also forms preferentially heterodimers, whose structure is very close to that of the corresponding trans-CD dimer.
Several attempts have been reported to assess the homochiral or heterochiral preference in molecular pairs isolated in the gas phase.9,10 The gas-phase dimer structure often differs from that observed in the solid, because the isolated dimer tries to optimise the number of hydrogen bonds. In particular, alcohols or substituted alcohols have been the subjects of many studies, for example the 1-indanol11 or fluoroethanol dimer.12 Bifunctional compounds are especially interesting in this respect as they provide more anchoring points that are expected to favour chiral discrimination.13 Examples include systems with permanent chirality like the methyllactate14–16 or the protonated 1-amino-2-indanol dimers17 or systems showing transient chirality like vicinal diols or aminoalcohols. In the latter systems, the two enantiomers are interconverted by torsion around a CC bond. Tunnelling between the two enantiomers manifests itself by the splitting of the transitions observed in microwave spectroscopy.18 The torsion can be blocked by dimer formation, which allows observing both homochiral and heterochiral dimers, with a preference for heterochiral pairing in the case of the 1,2-ethanediol dimer, whose preferred structure is achiral with S4 symmetry.19 In contrast, the aminoethanol dimer shows homochiral preference.20 Trends for homochiral aggregation are also observed for transiently chiral substituted alcohols such as the trifluoroethanol dimer or large clusters of phenyl-methanol, up to the tetramer.21,22
Information has been gained recently on the chiral preference in the jet-cooled dimer of 1,2-ethanediol, by comparison with one of its cyclohexane analogues, the permanently chiral trans-1,2-cyclohexanediol (trans-CD).23trans-CD shows heterochiral pairing preference in the gas phase due to the formation of a strongly bound dimer optimising the number of hydrogen bonds. The isolated 1,2-ethanediol dimers form the same hydrogen-bond pattern, hence the same heterochiral preference in the gas phase. Heterochiral preference is also observed in the trans-CD solid, which is a racemate.24
In contrast to trans-CD, cis-1,2-cyclohexanediol (cis-CD) is only transiently chiral because of the plane of symmetry that intersects the C1C2 bond when the carbon skeleton is made planar. Moreover, the cis geometry of the substituents will influence the strength of the intramolecular hydrogen bond relative to trans-1,2-cyclohexanediol. trans CD is energetically favoured by 1.9 kJ mol−1 in terms of zero-point-corrected energy at the B3LYP-D3(BJ,abc)/ma-def2-TZVP level of theory. Adding a phenyl substituent results in 1-phenyl-cis-1,2-cyclohexanediol (cis-PCD) that is permanently chiral. Dimer formation and chiral preference are expected to differ between trans-CD, cis-CD and cis-PCD, and may be influenced by the competition between intra- and intermolecular hydrogen bonds formation.12,25 On the other hand, the aromatic π-system adds both steric hindrance and dispersion interactions in cis-PCD and acts as an efficient hydrogen bond acceptor.26 These factors result in a wealth of expected hydrogen bond patterns in the aromatic dimer.
Here, we report the spectroscopic properties of cis-PCD and its dimers under supersonic expansion conditions, as studied by resonance-enhanced multi-photon ionisation (REMPI), Raman scattering, and conformer specific vibrational spectroscopy. The vibrational spectra of the homochiral and heterochiral dimers obtained by double resonance IR-UV spectroscopy are interpreted with the help of density functional theory (DFT) calculations to shed light on the diastereomeric preference in cis-PCD. The interaction patterns observed in the gas phase are compared to those existing in the solid. The structures found thereby are compared to the non-aromatic systems cis- and trans-CD.
The Raman spectroscopy results were obtained using a slit jet at the Institut für Physikalische Chemie. In the following, we will give a description of the measurement conditions for cis-PCD. When conditions differ between cis-PCD and cis-CD, the values for the latter will be given in parentheses. Pure He was used as a carrier gas and continuously expanded at a stagnation pressure of 0.4 bar (1.4 bar for cis-CD) into low vacuum (∼ a few 10−1 mbar). Raman scattering was obtained from a 532 nm cw laser operated at 24 W, with the expansion being irradiated orthogonally 1 mm (1.25 mm for cis-CD) downstream of the nozzle. The scattered light was collected by a photo lens perpendicular to the laser, focussed towards a Czerny–Turner-monochromator and detected by a LN2 cooled CCD camera. An exposure time of 4 min was used with 18 such exposures being averaged (5 for cis-CD) to yield the experimental spectrum. The spectrum was calibrated using Ne lines. The vapour pressure of the diol was enhanced in a heatable saturator kept at 395 K (365 K for cis-CD) with the following tubing and nozzle being heated to 425 K (395 K for cis-CD) to avoid condensation.27
The electronic and vibrational spectroscopy results for cis-PCD were obtained using a pinhole jet at ISMO. The pulsed supersonic beam was produced by expanding 2 bar of helium seeded with the enantiopure or racemic cis-PCD into high vacuum (∼10−6 mbar) through a 200 μm pulsed nozzle (General Valve – Parker).28cis-PCD was put in an oven just prior the expansion and heated at 365 K for the study of the monomer and 400 K for that of the dimer. Mass-resolved electronic spectra were obtained using one-colour resonance-enhanced two-photon ionisation (RE2PI). The UV source (0.02 cm−1 resolution) was generated by doubling the output of a dye laser (Sirah equipped with C540A dye) pumped by the second harmonic of a Nd:YAG laser (Quanta Ray, Spectra Physics). The UV laser beam was mildly focused by a 1 m focal length lens and crossed the skimmed supersonic beam (skimmer of 500 μm diameter) in the interaction zone of a linear time-of-flight (TOF) mass spectrometer (Jordan, one-meter length). The ion signal was detected by a microchannel plate detector (RM Jordan, 25 mm diameter), averaged by an oscilloscope (Lecroy wavesurfer), and processed through a personal computer.
Vibrational spectra were recorded using the IR-UV double resonance method.29,30 A slightly focused (0.5 m focal length lens) IR laser beam (OPO/OPA – Laser Vision – 3 cm−1 resolution) was counter-propagated relative to the UV laser beam and superimposed to it in the source region. After fixing the UV probe laser on selected vibronic transitions of the electronic spectrum, the wavelength of the IR pump laser was scanned in the 3 μm region. The IR absorption was then detected as a depletion of the UV-induced ion signal. The IR pulse was triggered ∼80 ns before the UV pulse to record ground-state vibrational spectra. Synchronisation between the lasers was controlled by a homemade gate generator. The IR spectra were recorded resorting to an active baseline scheme, by measuring the difference in ion signal produced by successive UV laser pulses (one without and one with the IR laser pulse present).31
X-ray diffraction data for compound cis-PCD were collected following the protocol described in the ESI.†
The relative stability of the different conformers was assessed by comparing their relative zero-point-corrected energies ΔE0 and their standard Gibbs free energies ΔG (we suppress the standard sign because only differences are relevant in the present work) relative to the most stable conformation at 300 K. Comparison between ΔE0 and ΔG is especially relevant for dimers, because they are formed at a temperature somewhere between that of the nozzle and the temperature where the expansion is probed. The difference between ΔE0 and ΔG may be viewed as a rough estimate of the uncertainty in the predicted energy ranking. The deformation energy was calculated as the difference in energy between the structure of the monomer in the complex and that of its most stable form.25,38,39 The deformation energy mentioned in what follows is the sum of that of the two monomers.
The nature of the first two electronic excited states and the vertical transition energies were calculated at the TD-DFT level at the same level as the ground state, using 4 excited states. The difference in electronic densities was calculated from the cube files generated by the Gaussian software and using the “cubman” facility. The resulting densities were plotted using the VMD software with an isovalue of 0.001. All these calculations were performed with the Gaussian Package (Version 16 Rev. B.01).40
For the sake of comparison with previously published work and sensitivity analysis with respect to small computational details like three-body-inclusive dispersion correction and basis set variants, the energies and harmonic frequencies were also calculated at the B3LYP-D3(BJ,abc)/ma-def2-TZVP41,42 level using the ORCA (version 5.0.3) program package.43 The theoretical spectra were simulated using the harmonic frequencies scaled by 0.963. Furthermore, a recently proposed empirical model45 was applied to the cis-PCD monomer to account for density functional deficiencies and the missing anharmonicity. Specifically, a correction of −146.0 cm−1 was used to account for the degree of substitution at the 1,2-diol subunit as well as an additional correction of −8 cm−1 due to the phenyl group. In the case of the PCD dimers, for which highly anharmonic low-frequency modes are expected, the Gibbs energy calculations were also conducted using the Quasi Rigid Rotor Harmonic Oscillator (QRRHO) approximation developed by Grimme,44 as a second measure for the uncertainty involved in such calculations. The results and discussion that follow are based on the B3LYP-D3(BJ,abc)/ma-def2-TZVP calculations, unless specified otherwise. The B3LYP-D3BJ/6-311++G(d,p) results are given in the ESI† as well as the comparison with QRRHO.
Fig. 1 Scheme and atom numbering for (a) (S,S)-(+)-1-phenylcyclohexane-cis-1,2-diol (cis-PCD) (b) (1S,2S)-trans-1,2-cyclohexanediol (trans-CD) (c) cis-1,2-cyclohexanediol (cis-CD). |
Fig. 2 (a) Raman spectrum of cis-PCD. “w” denotes a water impurity signal. (b) Double resonance spectrum of the monomer obtained by setting the UV probe on the transition origin at 37766 cm−1. (c) IR spectrum simulated for the most stable structure M1, shown in Fig. 4, obtained from the B3LYP-D3(BJ,abc)/ma-def2-TZVP empirically corrected harmonic frequencies. (d) Simulated Raman spectrum obtained from the empirically corrected harmonic B3LYP-D3(BJ,abc)/ma-def2-TZVP frequencies. The computed harmonic frequencies have been corrected by a recently proposed empirical correction model (see text and ref. 46). A Gaussian line profile is assumed with a full width at half maximum of 4 cm−1 and 1.5 cm−1 for the IR/UV and Raman spectra, respectively. Scaled B3LYP-D3(BJ,abc)/ma-def2-TZVP or B3LYP-D3(BJ)/6-311++G(d,p) harmonic frequencies calculations yield similar results. |
Fig. 3 shows the S1 ← S0 spectrum of the cis-PCD monomer. The strong transition origin at 37766 cm−1 is followed by a progression built on a low-frequency mode of 28 cm−1. The same progression appears in combination with the Herzberg–Teller allowed mode at +528 cm−1.
IR-UV double resonance spectra have been recorded by setting the UV probe on all the transitions marked by * in Fig. 3; that obtained by probing the transition origin is displayed in Fig. 2b. They are identical whatever the probe wavelength, showing unambiguously that only one conformer exists under pinhole jet conditions too. The spectrum shows two bands, both being down-shifted relative to a free ν(OH), at 3575 and 3613 cm−1, very close to the Raman spectroscopy values (Fig. 2a).
We are thus left with the three structures shown in Fig. 4, together with their energetics (Gibbs energy ΔG and ZPE-corrected energy ΔE0). Their energetics are summarised in Table S1 of the ESI.† They all show the phenyl and the O2H in equatorial position, and the O1H in axial position. They all involve a sterically constrained OH⋯O intramolecular interaction. We shall discuss their energetics in terms of relative Gibbs energies and ZPE-corrected energy ΔE0 at the B3LYP-D3(BJ,abc)/ma-def2-TZVP level. The energetics (relative Gibbs energy ΔG and ZPE-corrected energy ΔE0) and geometrical parameters at the B3LYP-D3BJ/6-311G++(d,p) level are listed in Table S2 of the ESI.† These structures will be called M (like monomer) with the index 1 or 2 when the OH on the carbon atom 1 or 2 is acting as a hydrogen bond donor, respectively. Both M1 and show an O1H⋯O2 interaction. They only differ by a rotation of O2H that allows a weak O2H⋯π interaction to take place in M1 and not in . M1 is thus stabilised by 6.7 kJ mol−1 relative to , in terms of ΔG. This value can be taken as an estimation of the OH⋯π interaction energy. M2 shows a hydrogen bond in the opposite direction, namely, an O2H⋯O1 interaction and is much less stable than M1 because no OH⋯π interaction is possible in M2 due to steric reasons. Notwithstanding the difference in hydrogen bond directions, the backbones are very similar in and M2. The Gibbs energy of M2 relative to M1 is 9.6 kJ mol−1, which allows roughly assessing the difference between O2H⋯O1 and O1H⋯O2 interactions to ∼3 kJ mol−1. The energy barrier for converting to M1 is calculated at 2.5 kJ mol−1 and is overcome in our experimental conditions,45 therefore only M1 is expected to be observed. The energy ranking is the same if one considers ΔE0 or the values obtained at the B3LYP-D3BJ/6-311G++(d,p) level (see Tables S1 and S2, ESI†), the values obtained with the various approaches differing by less than 10%.
The splitting of the calculated frequencies of M1 matches well the experimental one, whatever the method used. The empirical scaling model developed for diols also predicts the absolute wavenumbers very well, although cis-PCD was not part of the training set.46ν(O1H) (3574.0 for the Raman and 3575 for the IR-UV results) is much lower than its counterpart in the related structure of cis-CD (3648 cm−1),46 as expected from the presence of an O1H⋯π interaction. Moreover, also ν(O2H) (3611.5 for the Raman and 3613 for the IR-UV results) is lower in frequency, which points towards a cooperative effect between the two hydrogen bonds, as observed also for intermolecular hydrogen bonds.26,47,48 The intramolecular hydrogen bond is hindered and far from linearity (θ(O1HO2) = 115° and d(O1H⋯O2) = 2.22 Å in M1), which explains the limited downshift of ν(O1H) compared to intermolecular OH⋯O interactions.
cis/trans isomerism also influences the diol structure. The two OH substituents are in equatorial position in trans-CD, hence equivalent. Two monomers with a different orientation of the accepting OH are calculated, corresponding to an angle of 145° and 110°, respectively (M and M′ in reference,23 here renamed T′ and T for better distinction and analogy), akin to and M1 in cis-PCD, notwithstanding the axial or equatorial position. In the absence of other interactions, T and T′ are almost isoenergetic. They differ in energy by about 1 kJ mol−1 and their interconversion barrier is of the order of 4 kJ mol−1. The two of them are therefore observed under slit jet conditions.23
The spectrum of racemic cis-PCD clearly shows additional bands, which are due to the heterochiral dimer. The downshift of the S1 ← S0 transition origin of the heterochiral dimer (37511 cm−1) is smaller (255 cm−1 from the monomer origin). A low-frequency pattern similar to that of the homochiral dimer is observed near the S1 ← S0 origin, with bands at 18, 45, 57 cm−1 from the S1 ← S0 origin. An additional weak band appears at 70 cm−1. The band tentatively assigned to the S2 ← S0 origin, located at 145 cm−1 from the S1 ← S0 origin, also shows a larger down shift relative to the monomer than the homochiral dimer (110 cm−1). The same decrease in band intensity at higher energy is observed as for the homochiral dimer. Still, an intense band is observed at +257 cm−1 of the S1 ← S0 origin, a point to which we shall come back later.
The most stable calculated homochiral structure (Fig. 7a) meets these requirements. The other calculated structures are shown in Fig. S1 of the ESI,† together with their 6-311G++(d,p) energetics. Their interactive 3-D structures are given in the ESI† structures file. Their energetic data calculated at the B3LYP-D3(BJ,abc)/ma-def2-TZVP level are listed in Table S1 (ESI†). The simulated spectra are shown in Fig. S2 (ESI†).
The most stable homochiral structure is built from the most stable monomers M1 and is what we shall call an “insertion” complex. The O2H group of one of the monomers, called “guest” in what follows and denoted by the subscript “g”, inserts into the intramolecular hydrogen bond of the other monomer, called “host” and denoted by “h”. The intramolecular O1gH⋯O2g hydrogen bond of the guest is retained while its O2gH⋯π contact is disrupted to the benefit of the strong intermolecular O2gH⋯O2h interaction. The dangling O2hH interacts with the aromatic ring of the guest. The intramolecular O1hH⋯O2h hydrogen bond of the host is disrupted to the benefit of two strong intermolecular O2gH⋯O2h and O1hH⋯O2g interactions. The intramolecular hydrogen bond of the guest is hardly modified relative to the M1 monomer (θ(O1gHO2g) = 116° and d(O1g⋯HO2g) = 2.19 Å vs. 115° and 2.22 Å). In contrast, the host undergoes strong deformation, which explains the large deformation energy (10.4 kJ mol−1). The experimental spectrum is readily assigned on the basis of this geometry (Fig. 6a and b). The bands observed at 3344 and 3467 cm−1 are assigned to the ν(O1hH) and ν(O2gH), respectively. The doublet at 3554/3563 cm−1 is assigned to ν(O2hH) and ν(O1gH), respectively.
More conformational diversity is observed for the heterochiral dimer and a different vibrational spectrum is obtained for the probe set on the transition located at 257 cm−1 of the S1 ← S0 transition origin or for the probe set on the S1 ← S0 transition origin or any of the other bands. The spectrum with the probe set on the S1 ← S0 origin (Fig. 6c) shows four transitions, at 3380, 3516, 3555 and 3563 cm−1. It is attributed to the most stable (at 0 K) calculated structure (Fig. 7b), which is very similar to the homochiral dimer described above. A similar insertion structure is calculated with similar hydrogen bonds, with a deformation energy of the same order as the corresponding homochiral complex. The spectrum simulated for this structure is in excellent agreement with the experimental findings (Fig. 6c and d). The assignments of the bands at 3380 and 3516 cm−1 or the doublet at 3555/3563 cm−1 parallel that of the homochiral dimer.
The spectrum obtained when probing the band at +257 cm−1 (band marked with an encircled asterisk in Fig. 5) shows a different pattern, with a smaller down-shift of the ν(OH) frequencies. Four bands appear at 3428, 3513, 3542, 3603 cm−1. Based on agreement between simulated and experimental frequencies, it is assigned to an addition complex (linear structure), which is high in energy at 0 K but predicted to become competitive at higher temperature (see Fig. 8 and Table S1, ESI†). The other calculated heterochiral structures are shown in Fig. S2 of the ESI,† together with their 6-311G++(d,p) energetics. Their interactive 3-D structures are given in the ESI† structures file. The addition complex is built from a M1 monomer acting as a donor, which adds to a M1 monomer via a strong intermolecular hydrogen bond. The donor and the acceptor will be denoted by the subscript “d” or “a”, respectively. They both keep their intramolecular hydrogen bond O1H⋯O2 intact. Because the geometry of the monomer within the complex is very close to that of the bare monomers (no disruption of the intramolecular hydrogen bonds), the deformation energy is very low (3.3 kJ mol−1). The dangling O2dH of the donor is involved in a strong intermolecular O2dH⋯O1a hydrogen bond while that of the acceptor is involved in the same OH⋯π interaction as the monomer. There is a rather large uncertainty in energy ranking as the addition dimer is less stable by 8.0 kJ mol−1 in terms of ΔE0 but more stable by 3.7 kJ mol−1 than the insertion heterodimer in terms of Gibbs energy at 300 K. This uncertainty mainly arises from the fact that the insertion complexes are tighter than addition complexes; the evolution of the Gibbs free energy as a function of the temperature is in favour of the latter as one can already see from the large discrepancy between ΔG and ΔE0 provided in Fig. 7. The temperature at which the complexes are formed in the out-of-equilibrium supersonic expansion is not known but the fact that we see both heterochiral complexes, the insertion one being dominant, seems to indicate that the temperature at which the complexes are formed is higher than 100 K (see Fig. 8). As expected for rigid complexes, the insertion and double insertion dimers show little variation of their relative ΔG as a function of the temperature. This contrasts to the addition complexes, in particular the heterochiral addition O2H2 → O1 (M1 + M1) dimer to which one of the experimentally observed spectra is assigned. The observation of this dimer provides an indirect measurement of the jet conformational temperature, which can be estimated at similar values using different basis set; a switch from ma-def2-TZVP to 6-311G++(d,p) would suggest a slightly different conformational temperature (175 K vs. 150 K). However, one should not overestimate the robustness of this estimate, as a different way of dealing with the entropy of very low frequency vibrations44 would suggest very different conformational temperature. Resorting to the QRRHO corrections would result in a less realistic temperature above 300 K (dashed lines in Fig. 8).
The calculated value of the chirodiastaltic energy is different whether ΔE0 or ΔG is considered (see Fig. 8 and Table S1, ESI†), and also depends on the level of theory used. Homochiral preference is obtained at 0 K whatever the method used; ΔE0(hom-het) amounts to 1.6 kJ mol−1 at the B3LYP-D3(BJ,abc)/ma-def2-TZVP level and 1.7 kJ mol−1 for B3LYP-D3BJ/6-311G++(d,p), respectively. Note that when ΔE0 is considered, the most stable homo- and heterochiral complexes are both insertion structures but when ΔG at 300 K is considered the most stable heterochiral structure is the addition dimer that would energetically win over the homochiral dimer by 1.3 kJ mol−1 at 300 K. Changing the basis set from ma-def2-TZVP to 6-311G++(d,p) reverses this trend and retrieves the homochiral preference (by 2.3 kJ mol−1) at 300 K.
The frequencies located on O2gH and O1hH are lower in the homochiral than the heterochiral dimer, suggesting stronger hydrogen bonds in the former. Non-covalent (NCI) calculations59,60 indeed indicate a slightly larger electron density for the intermolecular hydrogen bonds of the homochiral dimer (0.199 and 0.177 vs. 0.197 and 0.175 for the heterochiral dimer). This observation is compatible with a larger stability of the homochiral dimer, although it should be taken with caution as stronger hydrogen bonds do not always correlate with an overall larger stability.61 Introducing the QRRHO approximation allows retrieving a chirodiastaltic Gibbs free energy in favour of the homochiral dimer (1.8 kJ mol−1), and an insertion heterochiral complex more stable than the addition structure, but would suggest a conformational temperature in the jet close to room temperature. Still, there are concordant indications in favour of a homochiral preference, although each taken separately (energy at 0 K, relative intensities in the electronic spectrum, down shift of the ν(OH)) is not sufficiently conclusive.
The heterochiral dimer shows more conformational flexibility than the homochiral one as it exists in two forms. A larger conformational flexibility has been observed already for the less stable configuration of chiral systems, for example heterochiral peptides, or protonated methyl tartrate dimers,52,62,63 or the homochiral 1-indanol dimer.11 A larger conformational flexibility of the homochiral adduct was observed as well for the trans-CD dimer for which the most stable calculated dimer is heterochiral.23
The Raman spectrum of cis-CD,46 taken with experimental conditions optimised for dimer formation, is shown in Fig. 12. It has one dominant band at 3419 cm−1, which is predicted to arise mainly from the most stable transiently heterochiral dimer, whereas the most likely similarly abundant transiently homochiral dimer is spread over several conformations and weaker transitions at lower and mostly at higher wavenumber. The lack of conformational selectivity prevents any further spectral assignment, but the calculations suggest that the homo- and heterochiral dimers have a very different hydrogen bond topology. Similar to trans-CD, a heterochiral quadruple insertion dimer is predicted to be the most stable dimer with other hetero- and homochiral dimers being significantly higher in energy, although not quite as pronounced as for trans-CD (ΔE0(hom-het) for cis-CD is 3.8 kJ mol−1vs. 6.6 kJ mol−1 for trans-CD at the B3LYP-D3/ma-def2-TZVP level). The analogy to trans-CD also holds for the homochiral dimers with the most stable ones being close in energy as well as structurally related. Of these four dimers a cyclic structure (two intermolecular and two intramolecular hydrogen bonds) is energetically favoured. The somewhat surprising similarity between cis-CD and trans-CD can be explained by the fact that the O–C–C–O dihedral angles of the diol subunit are still quite similar. Hence, the fact that the chiral preference in cis-PCD is inverted can most likely be attributed to the introduction of the phenyl group. The most stable homochiral cyclic (double addition) pattern contrasts to that at play in the homochiral cis-PCD dimer that involves two intermolecular and one intramolecular OH⋯O interactions. This is because the aromatic ring electrons compete with the oxygen as a hydrogen bond acceptor; both homochiral and heterochiral cis-PCD insertion dimers involve indeed an OH⋯π interaction.
Fig. 12 Comparison between the experimental (top) and simulated (bottom) Raman spectrum of cis-CD in 1.4 bar of helium. The saturator (365 K) and nozzle (385 K) temperatures have been optimised for dimer formation. Reasonable agreement can be found between the simulation and the experiment. See Fig. 13 for depiction of the corresponding structures. For the simulation, it is assumed that homo- and heterochiral dimers are formed with equal likelihood. Furthermore, the three most stable homo-dimers are assumed to be isoenergetic and therefore the homo population is equally spread among them. Since the most stable heterochiral dimer is energetically unrivalled one arrives at statistical weights of 1:1/3:1/3:1/3 (quadruple insertion: cyclic: double insertion: double insertion A). Such an approach was previously successfully used for trans-CD. The simulation assumes Gaussian profile with a FWHM of 8 cm−1. |
Calculations confirm that there is little similarity between the most stable complexes of cis-PCD and cis-CD in a 10 kJ mol−1 window (see Fig. 11 and Fig. 13). The conformational locking induced by the phenyl on the cis-PCD monomer also exists for its dimers, as shown by the much higher density of structures for cis-CD. The insertion dimer is indeed the only homochiral stable structure in a 5 kJ mol−1 window at low temperature (see Fig. 8). In cis-PCD, the chirodiastaltic energy favours the homochiral complex. This contrasts to what is calculated for trans-CD or cis-CD for which the most stable calculated dimer is the heterochiral one (ΔE0 = 6.6 kJ mol−1 and 3.8 kJ mol−1, respectively, at the B3LYP-D3/ma-def2-TZVP level) due to its structure (quadruple insertion) that optimises the number of hydrogen bonds.
The energetics sketched in Fig. 11 illustrate the main points of the comparison between the different systems. The lesser density of structures for cis-PCD, independently of chirality, illustrates the conformational locking induced by the aromatic ring. Both cis- and trans-CD show heterochiral preference with a quadruple insertion structure, which contrast with cis-PCD that shows homochiral preference. On a common energy scale where the most stable dimer irrespective of relative chirality is aligned, the most stable homochiral dimer of cis-CD is destabilised by ∼5 kJ mol−1 when adding an aromatic ring, because of the steric hindrance brought by the latter. Conversely, the most stable homochiral cis-PCD dimer is stabilised by ∼9 kJ mol−1 relative to the equivalent in CD.
Footnote |
† Electronic supplementary information (ESI) available. CCDC 2277624. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d4cp00351a |
This journal is © the Owner Societies 2024 |