Open Access Article
Patrick A.
Julien
*ab,
Mihails
Arhangelskis
*ac,
Luzia S.
Germann
ad,
Martin
Etter
e,
Robert E.
Dinnebier
d,
Andrew J.
Morris
*f and
Tomislav
Friščić
*ag
aDepartment of Chemistry, McGill University, 801 Sherbrooke St. W., H3A 0B8 Montreal, Canada. E-mail: tomislav.friscic@mcgill.ca
bDepartment of Chemistry and Chemical Engineering, Royal Military College of Canada, 13 General Crerar Crescent, K7K 7B4 Kingston, Canada. E-mail: patrick.julien@rmc-cmr.ca
cFaculty of Chemistry, University of Warsaw, 1 Pasteura St., 02-093 Warsaw, Poland. E-mail: m.arhangelskis@uw.edu.pl
dMax-Planck Institute for Solid State Research, Heisenbergstrasse 1, D-70569 Stuttgart, Germany
eDeutsches-Elektronen Synchrotron (DESY), Notkestrasse 85, 22607 Hamburg, Germany
fSchool of Metallurgy and Materials, University of Birmingham, Birmingham, B15 2TT, UK. E-mail: a.j.morris.1@bham.ac.uk
gSchool of Chemistry, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK. E-mail: t.friscic@bham.ac.uk
First published on 12th October 2023
In pursuit of accessible and interpretable methods for direct and real-time observation of mechanochemical reactions, we demonstrate a tandem spectroscopic method for monitoring of ball-milling transformations combining fluorescence emission and Raman spectroscopy, accompanied by high-level molecular and periodic density-functional theory (DFT) calculations, including periodic time-dependent (TD-DFT) modelling of solid-state fluorescence spectra. This proof-of-principle report presents this readily accessible dual-spectroscopy technique as capable of observing changes to the supramolecular structure of the model pharmaceutical system indometacin during mechanochemical polymorph transformation and cocrystallisation. The observed time-resolved in situ spectroscopic and kinetic data are supported by ex situ X-ray diffraction and solid-state nuclear magnetic resonance spectroscopy measurements. The application of first principles (ab initio) calculations enabled the elucidation of how changes in crystalline environment, that result from mechanochemical reactions, affect vibrational and electronic excited states of molecules. The herein explored interpretation of both real-time and ex situ spectroscopic data through ab initio calculations provides an entry into developing a detailed mechanistic understanding of mechanochemical milling processes and highlights the challenges of using real-time spectroscopy.
Here, we demonstrate an integrated dual-spectroscopy approach (Fig. 1a) for time resolved in situ monitoring of milling reactions using readily accessible bench-top Raman and visible fluorescence emission spectrometers. The combination of these spectroscopic techniques with computational methods provided an opportunity to explore the potential and limitations of using highly accessible spectroscopy and modelling approaches to understand mechanochemical reaction mechanisms. Specifically, periodic time-dependent density-functional theory (TD-DFT) calculations enabled the association of spectroscopic data with the underlying molecular and extended solid-state structures of reactants and products.
In situ spectroscopy provides an attractive opportunity to detect changes in molecular structures and their solid-state environments regardless of crystallinity – including the direct observation of amorphous materials. We integrated the fluorescence spectroscopy instrumentation into an established Raman spectroscopy monitoring setup,6 enabling tandem time-resolved in situ monitoring of milling reactions without the need for synchrotron radiation. Both Raman and fluorescence spectroscopies are non-destructive, provide simultaneous sensitivity to changes in molecular and extended solid-state structure of crystalline and amorphous solids, and can be conducted with highly accessible, low-cost benchtop experimental setups capable of high sensitivity and acquisition speeds.7–10
This dual spectroscopy method is introduced as a means to investigate transformations of organic solids, specifically polymorphic transitions, cocrystallisation, as well as for the direct, real-time observation of amorphous material during milling.11,12 Amorphisation is a particularly important problem in mechanochemical processing of active pharmaceutical ingredients (APIs). Direct and real-time observation of amorphous phases during milling has remained elusive due to the well-known difficulty of quantifying amorphous content in real time by XRPD without an internal, impact-resistant diffraction standard.13–16 Research into the detection of amorphous content in milling reactions has so far largely focused on Rietveld refinement or atomic pair distribution function analysis of synchrotron X-ray data.17,18 Here, we apply both real-time Raman and fluorescence spectroscopies to directly follow amorphous phases during milling in the laboratory.
Indometacin (ind, Fig. 1b) was chosen as a target, as it is pharmaceutically relevant, and provides a rich landscape of solid forms that exhibit solid-state fluorescence and undergo diverse mechanochemical transformations, including amorphisation, polymorph transformations, and cocrystallisation.19–21 Separate fluorescence22 or Raman spectroscopy approaches have been reported for distinguishing and quantifying ind solid forms in static systems, including the amorphous form (am-ind); the thermodynamically stable γ-polymorph (γ-ind); the metastable α-polymorph (α-ind), and the saccharin (sac) cocrystal (ind-sac).23–32
Despite recent interest in mechanically-induced changes in luminescence via aggregation or amorphisation,33–37 the use of real-time luminescence for monitoring ball milling reactions has remained largely unexplored and limited to fluorescence coincidentally observed in Raman spectra.38 This is most likely because fluorescence spectroscopy data is challenging to interpret, owing to the broad emission profiles of organic molecules and difficulty in relating spectroscopic responses to solid-state and molecular structures. A possible opportunity to overcome this limitation, and open spectroscopic monitoring of solids to direct and ab initio structural interpretation, is offered by periodic density-functional theory (DFT) approaches. In principle, periodic DFT calculations should facilitate the development of an integrated understanding of molecular and supramolecular transformations taking place during a mechanochemical reaction, by enabling the interpretation of spectroscopic (e.g., fluorescence, Raman, infrared, solid-state nuclear magnetic resonance – ssNMR) and XRPD monitoring outputs.
As a step towards developing such integrated understanding, we now evaluate the ability of periodic time-dependent DFT to interpret in situ fluorescence and Raman spectroscopy data, using calculations of ssNMR spectra as a validation benchmark. Specifically, periodic DFT was used to assign observed Raman data to vibrational motions within the crystal structure, and our recently developed method for calculating solid-state fluorescence emission spectra of crystalline materials (using the periodic implementation of TD-DFT in the CASTEP program)39,40 allowed us to effectively reproduce experimentally measured fluorescence spectra. At the same time, it is shown that the observed enhancement and wavelength shift of emission of ind in the solid state, compared to solution, is a result of conformational constraints imposed by the crystalline periodic environment. The herein reported computational analysis of vibrational spectra is, to the best of our knowledge, the first attempt to achieve structural insight into solid phases participating in mechanochemical reactions through real-time spectroscopy.
The Raman spectra of γ-ind, α-ind, am-ind, sac, and ind-sac were consistent with previous reports25,26,28 and suggested that focusing on the 1500–1800 cm−1 region should enable reaction monitoring with minimal interference from the PMMA milling jar (Fig. S12 and S13†).
To verify the reaction profile indicated by fluorescence emission spectroscopy measurements, we compared the time-dependent normalised luminescence intensity at the fluorescence emission maximum with the reaction profiles determined by non-negative least squares (NNLS) fitting of both in situ Raman spectroscopy (Fig. 2b–d and S14†) and fluorescence emission (Fig. 2e–g and S15†).6 The resulting agreement (Fig. 2b–g) is reasonable, indicating that simple monitoring of luminescence intensity can be used to directly estimate the time-dependent reaction profile over time. This provides a simple new route to spectroscopically follow mechanochemical reactions, using a readily accessible experimental setup. Moreover, the high fluorescence intensity enables spectra acquisition rates that are considerably faster (10–500 ms) compared to either XRPD or Raman spectroscopy. Fluorescence spectroscopy is less prone to stochastic changes in intensity as the experiment measures a larger area of the sample, making it less affected by motions of the milling assembly.43 However, compared to Raman spectroscopy, both fluorescence intensity measurement and the NNLS fitting profile suggest a slightly faster conversion to the ind-sac cocrystal. We hypothesise that the strong absorption of light at the excitation wavelength by the sample results in a shallow penetration depth into the solid, with fluorescence emission therefore primarily occurring at particle surfaces. As reactions between solid particles are expected to occur at the surface,44 the apparent reaction kinetics obtained from fluorescence would be faster than that obtained from Raman spectroscopy, a method with greater sample penetration depth. Accordingly, it may be difficult to detect low fractions of ind in inhomogeneous solids using fluorescence and factors such as particle size could significantly affect the emission.22 The similarity of fluorescence emission profiles between ind and ind-sac exacerbates the challenge of modeling in situ spectra as the sum of the spectra of pure components using the NNLS fitting method, as evidenced by patterns in the calculated residuals (see ESI, Fig. S15†).
Nevertheless, fluorescence emission spectroscopy provided an accessible, simple means to monitor the kinetics of mechanochemical cocrystallisation, due to significant shifts in emission wavelength and intensity throughout the process. The completeness of conversion was verified by XRPD analysis of the product immediately after milling, revealing Bragg reflections consistent with the reported ind-sac structure (CSD code UFERED),24 and no starting materials (see ESI, Fig. S1 and S3†). Full conversion was also confirmed by comparing XRPD (see ESI, Fig. S3†), 13C cross-polarisation magic angle spinning (CP-MAS) ssNMR data (see ESI, Fig. S16†), and Fourier-transform infrared spectroscopy (FT-IR) spectroscopy (see ESI, Fig. S17†) for the milling product to those for a solution-made sample of ind-sac (see ESI, Fig. S19†).45 The formation of ind-sac by LAG without observable participation of bulk amorphous or solvate phases was confirmed by separate real-time synchrotron XRPD monitoring at the Deutsches Elektronen-Synchrotron (DESY) PETRA III P02.1 beamline (see ESI, Fig. S18†).
40 plane-wave DFT calculations to simulate the Raman, infrared, and ssNMR spectra from crystal structures of γ-ind, sac and ind-sac solids. Periodic DFT simulations of both FT-IR and Raman spectra were in reasonable agreement with the experiment for γ-ind, sac, and ind-sac (see ESI, Fig. S19–S24†) enabling the qualitative assignment of most Raman peaks to specific normal modes. While periodic DFT is required to incorporate the effects of supramolecular interactions in solid-state structures, less computationally intense and more accessible gas-phase DFT calculations in Gaussian 16
46 can help identify which functional groups are responsible for vibrational modes which shift over the course of a reaction. The assignment of specific Raman bands to vibrational modes was performed for both ind and sac using periodic DFT, resulting in superior correlation to experimental spectra relative to gas phase calculations (see ESI, Fig. S25 and S26†). These calculations facilitated the assignment of Raman active vibrations above 1650 cm−1 as due to carbonyl stretching, and those between 1500 and 1650 cm−1 as C–C stretching of the aromatic rings in ind and sac (see ESI, Fig. S27 and S28†). In case of pure solids, the carbonyl stretches of both γ-ind and sac overlap near 1696 cm−1, but are observed to diverge in the ind-sac cocrystal. The application of periodic DFT enables the assignment of the absorption bands which shifted to higher wavenumbers (1714 cm−1) as corresponding to the carbonyl stretching vibrations of sac, while the ind carbonyl stretching was found to shift to lower wavenumbers (1681 cm−1) (see ESI, Fig. S29†). The periodic DFT calculations are in reasonable agreement with the experimental solid-state Raman and FT-IR data for the region of 1500 to 1800 cm−1, with the calculated vibrational frequencies falling within 20 cm−1 for the C–C ring stretching vibrations and within 45 cm−1 for the carbonyl stretching without the use of a scaling factor. The magnitude of these differences is consistent with those reported in the literature, without the use of empirical scaling factors.47 The periodic DFT correctly predicted the changes in vibrational frequencies between the different crystal structures with remarkable agreement (<5 cm−1) to experimental results. During the reaction, the carbonyl stretch of ind decreases by 15 cm−1, from 1696 cm−1 to 1681 cm−1, while a shift of 17 cm−1 is predicted from periodic DFT. The carbonyl stretch of sac shifts from 1696 cm−1 to 1714 cm−1 an increase of 18 cm−1 with DFT predicting an increase of 19 cm−1. The bands corresponding to the C–C ring stretching vibrations were predicted not to shift significantly (<3 cm−1), which is consistent with the experimental spectra. Similar trends can be observed in the FT-IR data which suggests that periodic DFT is a very powerful tool for understanding changes in vibrational frequencies which occur during reactions (Fig. S19–S21†).
Finally, our periodic DFT modelling approach was validated by comparing the experimental 13C CP-MAS ssNMR chemical shifts for all three phases, with the chemical shifts calculated using the GIPAW method implemented in CASTEP.48 Reasonable agreement between the calculated and experimental values (<5 ppm difference) (Table S3, Fig. S30–S32†) for all but three 13C signals signified the accuracy of our computational model for the crystal forms of ind. A comparison of simulated 13C chemical shifts for ind-sac and either sac or γ-ind revealed that the most significant differences (see ESI, Table S4†) were consistent with the carbon atoms adjacent to short contact interactions in the cocrystal structure (see ESI, Fig. S33†). This observation emphasises the accuracy of the GIPAW method in quantifying the effect of supramolecular interactions on the ssNMR spectra of molecular crystals.
To understand the emission properties of ind, we turned to TD-DFT simulations of solid γ-ind and ind-sac. While fluorescence emission of individual molecules can be readily simulated by molecular TD-DFT, cubic scaling of the calculation with system size quickly makes such approach prohibitive for modelling solid-state emission by cluster expansion. As an alternative, we developed a method for simulating solid-state fluorescence emission spectra of crystalline materials using the periodic implementation of TD-DFT in CASTEP.39 Since our method explicitly operates in a plane-wave basis set, it is capable of studying the role of non-covalent interactions, orbital overlap, and conformational effects on the emission of molecular crystals. The simulated emission spectrum of γ-ind was in excellent agreement with experiment, demonstrating the power of periodic DFT in modelling the emission behavior of crystalline solids (Fig. 3). Notably, our calculations showed consistency with respect to the choice of DFT functionals: we have tested two methods for geometry optimisation of electronic excited state (LDA and dispersion-corrected PBE)51–53 combined with each of the three hybrid functionals (B3LYP,54–57 HSE06 (ref. 52 and 58) and PBE0 (ref. 59 and 60)) for single point calculation of excitation energies. All six combinations of functionals resulted in emission maxima within 0.2 eV of each other, which corresponds to 22 nm variation in λmax. In terms of orbital contribution, it was found that the emission process originates from the S1 excited state, which is dominated by the LUMO → HOMO electron transition.
Next, we turned our attention to simulating the emission spectrum of the ind-sac cocrystal. The simulated emission spectra calculated with different functionals were, once again, in close agreement with each other (Fig. 3b and d). In terms of agreement with the experimental emission spectrum, the periodic TD-DFT calculations underestimated λmax for ind-sac by 50–70 nm, which is less accurate than for γ-ind, but is reasonable given the complexity of modelling solid-state emission from a multi-component crystal. The electronic transformation responsible for the emission behavior of both γ-ind and the ind-sac cocrystal, according to periodic TD-DFT, was found to be HOMO and LUMO of ind, same as in the case of γ-ind. Consequently, orbitals of sac were not deemed responsible for the fluorescence emission of the cocrystal. Fully periodic calculations using a range-separated functional, are not accessible in CASTEP, so molecular TD-DFT calculations using the CAM-B3LYP functional were run in Gaussian 16. These calculations were performed on a cluster containing two ind and two sac molecules (see ESI, Fig. S34†). The electronic transition originating from a mix of HOMO−1(ind) and HOMO(ind) onto LUMO(ind) has a large oscillator strength of 0.2067, whereas the hypothetical charge transfer state from HOMO−1(ind) to LUMO(sac), has a negligible oscillator strength of just 0.0013. Neither periodic nor cluster calculations suggest a charge-transfer mechanism. However, the red-shift in fluorescence emission observed experimentally upon cocrystallisation of ind and sac was not reproduced by periodic DFT, emphasising the difficulty of modeling subtle differences in underlying electronic structure responsible for the change in fluorescence emission.
An important question to be answered in the context of ind fluorescence is the extremely weak emission in solution, contrasting the strong emission of solid γ-ind. The strong solvent dependence of the Stokes shift of ind in solution was postulated to result from a dipolar singlet excited state which is produced by intramolecular charge transfer from the indole to the benzoyl group.41,61 The molecular TD-DFT calculations suggest that the electronic excitation of an isolated ind molecule is expected to be accompanied by a 40° rotation of the benzoyl group to an orientation perpendicular with respect to the plane of the indole system (see ESI, Fig. S35†). This can be explained by the redistribution of electron density from the indole system in the HOMO to the benzoyl group in the LUMO (Fig. 3e and f). For a molecule in an unconstrained environment, e.g. in solution, this rotation results in a significant reduction of the electronic transition dipole moment and quenching of the fluorescence emission.62 This is consistent with the established behavior of ind in solution.41 Conversely, in constrained environments of crystalline γ-ind and ind-sac, such a rotation is restricted to less than 10°, regardless of the functional used for TD-DFT geometry optimisation. Overall, our calculations show that the emissive behaviour of ind in the solid-state results from the close-packed crystal structure limiting the geometric distortions that a molecule can undergo in the electronic excited state.
:
1 mixture of α- and am-ind.63 Changes observed by real-time fluorescence monitoring of γ-ind amorphisation (Fig. 4e–g) can be explained by ind molecules being more able to adopt non-emissive conformations, resulting in a red shift and a reduction in intensity of emission, readily observed by NNLS fitting of in situ data. However, NNLS fails to adequately differentiate α- and am-ind which have similar fluorescence emission profiles (see ESI, Fig. S36†). Monitoring the maximum emission intensity of each spectrum, however, does reveal a slight increase in emission intensity corresponding to the formation of α-ind, which is known to be slightly more emissive than am-ind (see ESI, Fig. S37†).22 The projected gradient method66 for non-negative matrix factorisation (NMF)67 was applied to simultaneously estimate both the component spectra and their associated profiles. The estimated component spectra are similar to both ex situ emission spectra (see ESI, Fig. S37†) and resemble the reaction profile estimated by Raman spectroscopy (see ESI, Fig. S38†). Accurately determining relative amounts of α- and am-ind only through fluorescence emission data remains challenging (Fig. 4f), highlighting the value of complementarity inherent to the dual monitoring approach. Unfortunately, the complexity of α-ind crystal structure, with three independent molecules in the unit cell and numerous intermolecular interactions, preclude the previously used cluster and periodic DFT methods both in terms of computational cost and interpretation of the result. Modeling the lack of crystalline order in am-ind is a fundamental challenge beyond the scope of this work.68 Both the Raman and fluorescence emission data sets are in agreement with a simple model proposed for amorphisation during mechanical alloying.69 In this model each impact of a milling ball can convert a small amount of γ-ind to am-ind, and the amount of material that has undergone impacts is expected to be an exponential in the form of e−kn, where n is the number of impacts and k is the amount of powder processed per impact. As milling is conducted at a constant frequency, the total number of impacts n is expected to be directly proportional to time (t), and the molar fraction (α) of γ-ind and am-ind can be expressed using the following equations:| αγ-ind(t) = e−kt | (1) |
| αam-ind(t) = 1 − e−kt | (2) |
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| Fig. 4 (a) Schematic of the monitored model transformation of neat milling solid γ-ind. The atoms of the indometacin crystal structures are displayed with the following colors: red: oxygen, blue: nitrogen, green: chlorine, grey: carbon, and white: hydrogen. (b) Normalised Raman spectra of γ-ind, α-ind, and am-ind synthesised via solution or melt protocols.63,64 (c) Time-resolved normalised Raman spectra acquired during the milling of γ-ind. (d) Relative amounts of γ-ind, α-ind, and am-ind estimated using non-negative least squares fitting of the in situ dataset using the reference spectra in (b). (e) Estimated fluorescence spectra of γ-ind, α-ind, and am-ind obtained from non-negative matrix factorisation of the real time fluorescence emission spectroscopy dataset. Due to the low emission intensity of the α- and am-forms the effect of detector baseline becomes significant. (f) Time-resolved fluorescence emission data acquired during the milling of solid ind, truncated to 10 minutes for clarity. For full data see ESI Fig. S36.† (g) Relative amounts of γ-, α-, and am-ind estimated using non-negative matrix factorisation of the in situ fluorescence emission dataset. | ||
This model assumes a homogeneous mixture of solid phases. However, recent measurements on the milling amorphisation of trehalose suggest that amorphisation preferentially occurs at particle surfaces resulting in the formation of particles with crystalline cores and amorphous shells.17 The initial kinetics of the loss of γ-ind during amorphisation via milling are fairly consistent with an exponential decay function (eqn (1)) for both Raman spectroscopy and fluorescence emission data, although the rate constant obtained by fluorescence spectroscopy (ca. 0.52 s−1) is approximately double of that found from Raman spectroscopy (ca. 0.23 s−1) data (see ESI Table S5, Fig. S39 and S40†). We hypothesise that the fluorescence emission mostly originates from the amorphous shell on particle surfaces, while Raman spectroscopy has sufficient penetrating power to observe the slower conversion of crystalline cores. Such a hypothesis is consistent with the observed discrepancy in estimated fraction of γ-ind between the two techniques for 25–70 minutes of milling. This partially amorphised state of γ-ind cores with amorphous shells appears relatively kinetically stable until around 70 minutes of milling. At that point, crystalline α-ind begins to form, with a sigmoidal crystallisation profile similar to that expected from a kinetic model previously proposed for the conversion of β- to α-mannitol during milling.18 The nucleation of α-ind from am-ind above room temperature (30 °C) has previously been observed ex situ70 with these phases reported as being close in energy.71 In this case, however, it is unclear where in the particle or in which phase this transition preferentially occurs.
XRPD analysis of milled solid ind revealed an elevated baseline with broad signals of α-ind, consistent with the presence of amorphous material (see ESI, Fig. S2†). Attempt to characterise the sample by 13C CP-MAS ssNMR revealed signals identical to those for a separately synthesised sample of α-ind, but did not reveal any amorphous content (see ESI, Fig. S41†). The inability to observe am-ind by ssNMR suggests that the sample fully crystallised during the preparation of the ssNMR measurement a conclusion also supported by FT-IR measurements (see ESI, Fig. S42†). The recrystallisation of amorphous samples from ball milling has been previously been observed by DSC and is hypothesized to occur due to nano-sized crystalline cores in the sample.17 This highlights the need for real time approaches to understand the behaviour of amorphous solids during mechanochemical processes and for the synthesis of amorphous formulations of APIs.72
Samples of α-ind were synthesised using a modified literature procedure,64 by dissolving 300 mg of γ-ind in 5 mL of ethanol at 80 °C before adding 10 mL of room temperature distilled water and filtering the resulting precipitate.
CASTEP TD-DFT calculations can only be performed at one k-point in the Brillouin zone. The k-point offering the best approximation to the converged k-point grid was selected by calculating the singlet–triplet energy difference for a series of k-points. The special k-point found to accurately reproduce the singlet–triplet energy difference for the converged k-point grid, analogous to the idea of the so-called Baldereschi point60 was found at (1/4; −3/8; 1/8) for γ-ind and at (1/4; 1/8; 1/8) for ind-sac. Next, excited state TD-DFT calculations were performed. In the case of γ-ind the 1st excited state was optimised, which corresponded to the HOMO–LUMO transition on indometacin. In the case of ind-sac, the 1st TD-DFT excited state involved transition from HOMO(ind) to LUMO(sac), which corresponded to a low-intensity charge transfer (CT) state, known as an artefact of TD-DFT. With the aid of molecular range-separated TD-DFT calculations (see below), this was ruled out as an incorrect solution, and instead a higher rank TD-DFT excited state corresponding to the HOMO(ind)–LUMO(ind) transition was chosen. That way both γ-ind and ind-sac follow the same mechanism of fluorescence emission.
The selected excited states were geometry-optimised using CASTEP TD-DFT module. Same input settings and convergence criteria were used here as for ground-state geometry-optimisation, except for unit cell parameters which were kept fixed. The final step of the fluorescence calculation was a single point TD-DFT calculation using each of the three functionals: PBE0, B3LYP and HSE06. The hybrid calculations were performed both on the ground state- and TD-DFT-optimised geometries, the energy difference between these two geometries being used to approximate the width of the spectral line, approximated by the Gaussian curve.
For the Raman calculation the crystal structures were reoptimised with a tighter atomic force convergence criterion of 0.01 eV Å−1. Further, the standard and fine FFT grid scales were changed from their default values to 2 and 3, respectively. The vibrational frequencies at the Γ phonon q-point were calculated using the density-functional perturbation theory (DFPT) approach. The polarisability tensors were then calculated for the Raman-active modes. Spectra were simulated as using Gaussian functions for each Raman active vibration, using the calculated Raman frequencies, scattering activities, and a peak width of 6 cm−1. All spectra were normalised to via the highest intensity for plotting.
FT-IR spectra were simulated as a summation of Gaussian functions for IR active vibrational modes using a peak width of 15 cm−1, the calculated vibrational frequency, and relative peak amplitudes obtained from the CASTEP calculation. All spectra were normalised to a maximum intensity of 0.5 and converted into transmittance for comparison to experimental spectra.
The NMR parameters were calculated using the gauge including projector augmented waves (GIPAW) method. The plane-wave basis set cut-off was increased to 1000 eV, the standard and fine FFT grid scales were set to 2 and 3, respectively, and ultrasoft on-the-fly generated pseudopotentials were used.
Footnote |
| † Electronic supplementary information (ESI) available: Illustration of the experimental setup, along with additional references and relevant X-ray powder diffraction, fluorescence emission, bandgap measurement, infrared spectroscopy, ultraviolet/visible spectroscopy, Raman spectroscopy, in situ Raman and fluorescence emission spectroscopy, 13C NMR spectroscopy, in situ synchrotron X-ray powder diffraction, computational and kinetic modelling data. See DOI: https://doi.org/10.1039/d3sc04082h |
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