Primadi J.
Subintoro
and
Korey P.
Carter
*
Department of Chemistry, University of Iowa, Iowa City, IA 52242, USA. E-mail: korey-carter@uiowa.edu
First published on 15th May 2024
Molecular spin qubits have demonstrated immense potential in quantum information science research due to the addressability of electron spins using microwave frequencies, and the scalability and tunability of molecular systems. Exemplary in this regard is the holmium polyoxometalate, [Na9Ho(W5O18)2]·35H2O (HoW10), which features an accessible atomic clock transition at 9.4 GHz; however, the coherence time of this molecule is limited by spin-phonon coupling driven decoherence processes. To limit these decoherence pathways, materials need to be designed to reduce energy overlap between spin and phonon states, and this necessitates developing a better understanding on how structural modifications impact the vibrational landscape for classes of complexes. Herein we conducted a full investigation into the fundamental structural and vibrational properties of the lanthanide Lindqvist polyoxometalate series, [Na9Ln(W5O18)2]·xH2O (Ln = La(III)–Lu(III), except Pm(III)) (LnW10), to assess how structural changes effect vibrational characteristics and to elucidate pathways to improve the coherence properties of HoW10. Single crystal X-ray diffraction results revealed four distinct structural polymorphs in complexes 1–14 wherein first coordination spheres were identical, and differences manifested as changes in lattice packing. Interestingly, the subtle changes in packing exhibited by the four polymorphs were found to impact distortions away from ideal D4d symmetry for each of the LnW10 complexes. Raman and far-infrared (FIR) spectra of complexes 1–14 were collected to identify vibrational modes present in low energy regions and peak fitting assignments were made according to literature precedents. Qualitative and Partial least squares (PLS) analysis show correlations between complex structural parameters with the low energy Raman and FIR vibrational modes of interest. Overall, this investigation shows that the second coordination sphere plays an integral role in modulation of the structural and vibrational characteristics of LnW10 complexes, which makes it a viable route for tuning spin and vibrational manifolds of species within this series.
The extended coherence time in HoW10 is made possible by atomic clock transitions within the molecule,24 which are avoided level crossings with zero Zeeman slope that result from wavefunction mixing of metal-ion spin states.25 Clock transitions are a topic of significant research interest within the field of QIS due to decoupling of the coherent spin states from the surrounding magnetic environment at clock transition frequencies, which protects from spin–spin coupling based decoherence that can result from local magnetic induction.26 The clock transitions in HoW10 stem from hyperfine and crystal field induced mixing that removes the degeneracy of the MJ = ±8 ground state multiplet for Ho(III), yielding instead a tunnel split pseudodoublet of MJ = ±4 ground states.27–29 At the clock transition in HoW10, coherence times were enhanced by four times to over 8 μs, and the clock transition also allowed for coherence to be achieved without significant matrix dilution of the paramagnetic metal centers, which is crucial for the potential scalability of the system for QIS applications. A drawback of the HoW10 system is that the spin–lattice relaxation time limited the coherence time for the complex, even at low temperatures (<10 K).24,28,30 Spin–lattice relaxation times are governed by thermally activated processes involving spin states, and the changes as a function of temperature of coherence times for HoW10 indicated that the accelerated relaxation for this complex was a result of phonon coupling with the spin bath.31,32 Prolonging spin–lattice relaxation times by minimizing spin–phonon coupling is a significant synthetic challenge as it involves manipulation of the vibrational landscape to limit energy overlap between metal-ion spin states and vibrational phonons.31 In f-element POM systems, such as HoW10, this necessitates the development of a fundamental understanding of the active vibrational modes for metal–POM complexes and requires delineation of structure–property relationships so that a handle can be developed on how changes in f-element coordination environments affect active vibrational modes and the crystal field splitting of spin states. Despite multiple studies focusing on lanthanide Lindqvist POM complexes, [Ln(W5O18)2]9− (LnW10), there is limited understanding on how structural and vibrational spectroscopy characteristics of these complexes are related, even for HoW10, and there has not been a systematic structural study covering the entire LnW10 series.27,33–38
Herein we describe our findings from comprehensive structural and vibrational spectroscopy studies we conducted on the complete lanthanide Lindqvist POM series, [Na9Ln(W5O18)2]·xH2O (LnW10) (Ln = La(III)–Lu(III), except for Pm(III)). Single crystal X-ray diffraction results indicate that the entire series (complexes 1–14) is isostructural, and all structures crystallize in the triclinic P space group. There are structural differences within the LnW10 series though, as four different polymorphs were observed, three of which had not been previously identified. Differences between LnW10 polymorphs led to variations in the distortions from ideal D4d symmetry for each complex, which suggested that first and second coordination sphere structural characteristics play a significant role in modulating metal-ion point group symmetry.27,39,40 Distortions from ideal symmetry can modulate spectroscopic properties of LnW10 complexes and thus, understanding how structures have been distorted by changes in coordination chemistry and packing is pivotal to tune the vibrational landscape of these materials as the work of Shiozaki et al.41 and Blockmon and colleagues31 have illustrated. To achieve this aim, we collected both Raman and infrared (IR) spectra for the entire LnW10 series and subjected spectra to a peak fitting regime with the aim of definitively identifying the vibrational modes that were present, particularly in the low energy region (400–100 cm−1) where peaks associated with spin–phonon coupling are generally observed.24,42,43 Qualitative analysis of results showed polymorph specific trends when FIR [ν(WO5)2, ν(LnO8), and ν/ρ(LnO8)] and Raman [ν(Ln–O–W)] modes were compared to structural parameters such as ionic radii, skew angles, plane angles, and plane distances. Partial least squares (PLS) analysis confirmed the results from qualitative comparisons with the different structural parameters investigated here accounting for 37 to 86% of the variances observed in FIR and Raman vibrational modes. These results suggest tuning of structural characteristics may be a viable way to modulate the vibrational landscape of f-element POM complexes.
The four LnW10 polymorphs share many similarities, especially in the metal-ion first coordination sphere, which is consistent throughout complexes 1–14. As a result, we will only describe the metal-ion local coordination for complex 10 (HoW10), which is representative of the whole Ln-Lindqvist series. Complex 10 features a single crystallographically unique eight coordinate Ho(III) metal center that has adopted slightly distorted square antiprismatic (D4d) molecular geometry. The Ho(III) ion in 10 is sandwiched by two crystallographically unique [W5O18]6− (W5) lacunary POMs that are each comprised of five edge-sharing WO6 octahedra. Four oxygen atoms from each W5 moiety bind to the Ho(III) metal center, and collectively the Ho(III) ion and the two W5 lacunary POMs can be described as a HoW10 POM cluster. The average Ho–O bond distance in 10 is 2.366 Å, and in the LnW10 series the average Ln–O bond distances (dLn–O) range from 2.5194 Å (for La(III) – complex 1) to 2.337 Å (for Lu(III) – complex 14).
POM coordination to the Ho(III) cation in 10 generated two inequivalent WO6 units in each W5 moiety (WO6 cap and WO6 belt) (Fig. S3, ESI†). Within the coordinating WO6 belt, we identified five distinct W–O bonds, W–Olanthanide, W–Ocenter, W–Obridge, W–Oterminal, and W–Ocap, and a detailed schematic highlighting each of these can be found in Fig. S3 (ESI†). In complex 10, the average W–Olanthanide distance is 1.793 Å with a range of 1.787–1.799 Å. The average W–Ocenter bond distance is 2.316 Å with a range of 2.289–2.373 Å, while W–Obelt distances are shorter at an average of 1.949 Å with a range of 1.930–1.969 Å. For W–Oterminal bonds, the average distance is 1.735 Å with a range of 1.726–1.740 Å and W–Ocap bonds are at an average distance of 2.020 Å with a range of 2.004–2.040 Å. The WO6 cap moieties are at the apex of each W5 cluster and are not involved in lanthanide coordination. These structural units feature only three unique W–O bonds, W–Ocenter, W–Oterminal, and W–Obelt, and in HoW10, the W–Ocenter and W–Oterminal bonds are at an average of 2.252 Å and 1.744 Å, respectively, while the W–Obelt bonds are at an average of 1.910 Å with a range of 1.879–1.952 Å. Overall, there are no observable correlations between changes in Ln(III) ionic radii and the different W–O bond distances, and the values exhibited by complex 10 are typical for the entire series. Beyond the first coordination sphere in 10, there is a network of nine Na(I) cations for charge balancing and 35 lattice water molecules. The varying configurations of water and Na(I) cations in the second coordination sphere are what differentiate the four polymorphs within the LnW10 series.
For polymorph 1, the nine Na(I) cations are distributed between two fragments on the periphery of the cluster (Fig. 1a). One fragment contains six sodium cations while the other contains three sodium cations, and the closest distances between Ln(III) and Na(I) (dLn–Na) cations are 5.547 Å, 4.211 Å, and 4.197 Å for complexes 1–3 (LaW10, CeW10, PrW10), respectively. Sodium cations in the lattices of complexes 1–14 generally feature octahedral coordination (NaO6) environments except for the Na(I) cation closest to the Ln(III) metal centers in complexes 2 and 3, which exhibits tetrahedral geometry. Complex 1 is also distinct amongst polymorph one species since instead of having Na(I) in this tetrahedral hole, it has a water molecule, Fig. S5 (ESI†). The number of lattice waters for complexes 1–3 are 34, 28, and 29, respectively, and it is important to note that the variance in the number of lattice water molecules may originate from the disorder of the crystal structures since the crystals readily desolvate under ambient conditions. For polymorph 2 (complex 4), the nine NaO6 moieties form a helix pattern around the cluster, Fig. 1b, with a closest dLn–Na of 4.436 Å. The number of lattice water molecules in 4 (NdW10) is 32 and notably they are packed tightly in a helical pattern resulting in a much smaller unit cell (V = 3070 Å3) compared to polymorphs 1, 3, and 4 (V = ∼3250 Å3). The close packing of polymorph 2 resulted in four partial clusters included in each unit cell instead of the two partial clusters included in unit cells for the other polymorphs, Fig. S6 (ESI†). This compactness is also reflected in closest distances between Ln(III) cations (dLn–Ln) which is 9.987 Å for polymorph 2, while for polymorphs 1, 3, and 4 dLn–Ln values range from 11.153 Å to 11.537 Å. Inspection of the asymmetric unit in polymorph 3 revealed two configurations of the NaO6 fragments, Fig. 1c and d. Complexes 5, 7, and 13 (SmW10, GdW10, YbW10) feature all nine NaO6 moieties connected to form a single fragment contained above the clusters for 5 and 13 and to the side of the cluster for 7. For complexes 6, 8, and 12 (EuW10, TbW10, TmW10) the nine NaO6 moieties form two fragments of seven and two Na(I) units that are located on the periphery of the clusters. For complexes 5–8, 12, and 13, the closest dLn–Na are 5.672 Å, 5.645 Å, 5.710 Å, 5.705 Å, 5.635 Å, and 5.716 Å, respectively, and complexes 5–7 include 36 lattice water molecules, while complexes 8, 12, and 13 feature 37, 35, and 37 lattice waters, respectively. Similar to polymorph 3, there is variance in NaO6 configurations in the structures of polymorph 4 complexes, Fig. 1e and f. For example, complexes 9 and 10 (DyW10, HoW10) feature nine NaO6 moieties connected to form a single fragment that adopts a fork-like pattern, whereas complexes 11 and 14 (ErW10, LuW10) include NaO6 units that are split into two fragments, analogous to the packing seen in polymorph 1. The closest dLn–Na for 9, 10, 11, and 14 are 5.456 Å, 5.446 Å, 5.292 Å, and 5.446 Å, respectively, and complexes 9–11 include 35 lattice water molecules, while complex 14 has 32. These dLn–Na interaction distances and lattice compositions are consistent with literature data for polymorph 4 structures.27,33,34
The differences between polymorphs 1–4 can also be seen by analyzing the patterns produced by the Na(I) cations in the unit cell when each is viewed in the same orientation, Fig. 2. Inspection of complexes that adopt the polymorph 1 configuration reveals a consistent zigzag pattern with the Ln(III) cations located within the packing motif as highlighted in Fig. 2a. The pattern produced by the Na(I) cations in complex 4 (polymorph 2) is the most complicated in the series and is best described as a mix of zigzag and hourglass patterns with a line bisecting the packing schemes, Fig. 2b. The location of the Nd(III) cations is also unique compared to the other polymorphs as they are located on the faces of the unit cell. In polymorph 3, complexes 5–8 (SmW10, EuW10, GdW10, TbW10) exhibit a mix of zigzag and hourglass patterns for the Na(I) cations with the Ln(III) cations located inside the pattern, Fig. 2c, while complexes 12 and 13 (TmW10, YbW10) feature Na(I) cations in an hourglass pattern with the Ln(III) cations located outside the pattern, Fig. 2e. Finally, for complexes 9–11 and 14 (DyW10, HoW10, ErW10, LuW10, polymorph 4) the Na(I) cations form a whirlpool pattern with the Ln(III) cations integrated into the packing motif, Fig. 2d.
Once distortion parameters were obtained for complexes 1–14, we investigated whether any changes could be correlated to the identity of the Ln(III) cation. This was initially done by comparing SA, PA, and PD values with ionic radii of the Ln(III) cations, and these plots are shown in Fig. 3. There are no general trends observed in comparisons of distortion parameters with the entire lanthanide series; however, when we grouped the different LnW10 complexes by structural polymorph, we did note polymorph specific trends for each of structural distortion parameters. These results are presented in Fig. 3 and S7–S9 (ESI†) and based on these plots we can identify some of the characteristics that make HoW10 unique within the LnW10 series. The skew angles of polymorph 1 (complexes 1–3) range from 3.34° (3, PrW10) to 3.77° (1, LaW10) and within this group of complexes the decrease in skew angle corresponds to the decrease in ionic radii from La(III) to Pr(III) (Fig. 3 and Fig. S7, ESI†). Polymorph 2 (complex 4) has a skew angle of 6.25° that is significantly higher than what we observed for any of the other polymorphs (Fig. 3), and since this configuration is only adopted by one complex it limits what we can learn about this structure. The skew angles for polymorph three complexes (5–8, 12, and 13) decrease as lanthanide ions get smaller, consistent with polymorph one, and range from 3.98° (12, TmW10) to 4.20° (5, SmW10) (Fig. 3 and Fig. S7, ESI†). For polymorph 4 (complexes 9–11 and 14), the skew angles increase as the ionic radii decreases; however, there is an outlier to this trend in complex 11 (ErW10) which exhibits a much smaller skew angle of 1.94°. The remainder of polymorph 4 complexes have skew angles ranging from 2.09° (9, DyW10) to 2.12° (14, LuW10) (Fig. 3 and Fig. S7, ESI†), and it is the polymorph 4 configuration that is notable as these structures features the smallest skew angles amongst LnW10 complexes.
PA values for polymorph 1 complexes display a similar correlation to Ln(III) ionic radii as what was observed for SAs, specifically, there is a decrease in plane angle as metal ions get smaller with PA values ranging from 2.71° (3, PrW10) to 4.81° (1, LaW10) (Fig. 3 and Fig. S8, ESI†). For polymorph 2, the plane angle is 2.31° which falls within the range of PA values observed for other LnW10 polymorphs. PA values for polymorph 3 complexes also follow the established trend of decreasing as the lanthanide ionic radii decreases with values ranging from 1.89° (12, TmW10) to 2.35° (5, SmW10 and 6, EuW10) (Fig. 3 and Fig. S8, ESI†). Plane angles for polymorph 4 complexes also decrease as lanthanide ions get smaller with values ranging from 1.14° (14, LuW10) to 1.17° (9, DyW10); however, there is an outlier to this trend, which is complex 10 (HoW10), that has a plane angle of 1.13° (Fig. 3 and Fig. S8, ESI†). Comparing the PAs across the series, we note that polymorph 4 complexes feature the smallest plane angles, whereas polymorph 1 complexes have the largest plane angles. The plane distances for the polymorph 1 structures range from 0.003 Å to 0.023 Å (Fig. 3 and Fig. S9, ESI†). Similar to SA and PA values for polymorph 1 complexes, there is a decrease in plane distances as the Ln(III) ionic radii shrink. For polymorph 2, the plane distance (4, NdW10) is in line with other polymorphs and the PD value for this complex is 0.011 Å. The plane distances for polymorph 3 complexes have a uniform spread that ranges from 0.013 Å (7, GdW10) to 0.019 Å (6, EuW10) (Fig. 3 and Fig. S9, ESI†). Moreover, the PD values for polymorph 4 structures decrease as the metal ion ionic radii decreases, similar to the trend noted above for polymorph 1, with values ranging from 0.047 Å (14, LuW10) to 0.051 Å (10, HoW10) (Fig. 3 and Fig. S9, ESI†). Comparing the different polymorphs in the series, polymorph 4 exhibits the longest plane distances amongst the four polymorphs, while polymorphs 1–3 display relatively similar plane distances.
Overall, the polymorph specific trends in structural distortion parameters that were identified for complexes 1–14 indicate that the composition and packing of the lattice plays a major role in modulating the effective symmetry and tuning the crystal field of the Ln(III) metal centers. Comparisons of dLn–Na interaction distances versus ionic radii of the Ln(III) cations also reveals polymorph based correlations which further strengthens this observation, Fig. S10 (ESI†). In HoW10, the MJ = ±4 ground state was stabilized and further mixed by the distorted D4d symmetry, which facilitates the atomic clock transition that has been observed in this complex.24 Due to selection rules, tunneling between MJ states is forbidden in Kramers ions (J = non-integer), hence clock transitions can only exist in non-Kramers ions (J = integer).24,25,59 In the Ln(III) series, this includes Pr(III), Pm(III), Eu(III), Tb(III), Ho(III), and Tm(III). It has been hypothesized that the clock transition of the HoW10 complex could be re-created if the effective symmetry around the Ho(III) cation was emulated in the other non-Kramers LnW10 species.16,60 Herein we have shown that the distortion parameters for HoW10 (complex 10) are distinct from Lindqvist POM complexes with the other non-Kramers Ln(III) cations, and this provides a potential explanation for why only the HoW10 complex has displayed an accessible atomic clock transition. To re-create the effective symmetry of the HoW10 complex in other LnW10 species, alternative means for controlling structural distortion parameters and second coordination sphere packing will be necessary, and pathways for pursuing this aim include novel crystallization methods and inclusion of different charge balancing cations.27
Data collection and peak identification in FIR spectra is challenging due to signals that are overwhelmed by water absorption effects and possible mode couplings between cluster and lattice elements that can result in jagged and broad features instead of well-defined peaks. To identify FIR features for complexes 1–14, spectra were fitted with Gaussian peak profiles and the FIR spectrum of HoW10 (complex 10) was used as a representative example for the entire series. Peak assignments were made based on the calculations from Blockmon and colleagues who conducted a far-IR magnetospectroscopy study on HoW10 that included eight peaks in the spectral window of 400–100 cm−1.31 Interestingly, we only observed six peaks in the same spectral window after background subtraction (Fig. 4), and this may be due to our instrument not being able to resolve the complex vibrational features present in this region. The six peaks identified for 10 in the FIR are centered at 357 cm−1, 319 cm−1, 200 cm−1, 175 cm−1, 146 cm−1, and 120 cm−1. The peak at 354 cm−1 was assigned as a ρ/δ(HoO4) (ν = stretching, δ = bending) mode and the peak at 319 cm−1 was assigned as a ν/ρ(HoO8) (ρ = rocking) mode. The peak at 200 cm−1 was assigned to the ρ(W5O18) mode; however, this peak only shows up in spectra for complexes 9 and 10 (DyW10, HoW10), and since there are no structural features that are unique to complexes 9–10, we suspect this peak is present for all complexes and only observable for these two complexes. The two final peaks at 175 cm−1 and 146 cm−1 were assigned as ρ(HoO8) and ν(WO5)2 modes, respectively. The peak at 120 cm−1 does not match with any known stretches for this Ln POM system, yet spectra collected by Blockmon and colleagues show an unidentified peak at 113.4 cm−1, which may correspond to the peak we observe for 10.31 Raw and fitted FIR spectra for complexes 1–14 (Fig. S11–24, ESI†) as well as tables listing the peaks and peak fitting parameters for each FIR spectra (Tables S3–S17, ESI) are available in the ESI.†
Fig. 4 Background subtracted FIR spectrum (400–100 cm−1) for complex 10 (HoW10) fit to Gaussian functions. |
Raman spectra were collected for complexes 1–14 and peak identification and data fitting was based on the assignments made by Shiozaki et al. and Kazanskii and colleagues.41,61 The Raman spectrum of HoW10 (complex 10) was used as a representative example, and the fitted Raman spectrum for 10 using Lorentzian peak profiles is presented in Fig. 5, which includes twelve major peaks in the spectral window of interest (1020–100 cm−1). The sharp peaks at 952 cm−1 and 935 cm−1 were assigned as ν(WOt) modes, while the peak at 888 cm−1 was assigned to the ν(Ln–O–W) mode. The peaks centered at 834 cm−1 and 554 cm−1 were assigned as ν(W–O–W) modes. At lower energies, the peaks at 428 cm−1 and 360 cm−1 were identified as the δ(W–O–W/WO/Ln–O–W) mode, and the remaining peaks at 326 cm−1, 214 cm−1, 171 cm−1, and 137 cm−1 were attributed to deformation modes of the HoW10 POM. We also observed a significant change in select peak intensities when the orientation of the sample was changed during measurements. This implies that some of these vibrational modes are polarizable which is a characteristic sign that the vibrational modes are likely part of the A1 irreducible representation.62 More specifically, we noted that the 888 cm−1 peak, which is assigned as the ν(Ln–O–W) mode, fluctuates in intensity when different crystals of the same sample are measured (Fig. S25, ESI†). Interestingly, according to the literature this band is not supposed to be polarizable,61 and thus changes in peak intensity as a function of crystal orientation are unexpected. Moreover, we also found features in the 200 cm−1 region that fluctuate in similar manner, which is in agreement with previous observations from Kazanskii et al.61 Raw and fitted Raman spectra along with a table listing peaks observed in complexes 1–14 are available in the ESI (Fig. S26–S39, Tables S18–S32, ESI†), and overall, comparisons of the spectra for 1–14 show good agreement with the results from Shiozaki et al. and Kazanskii and colleagues wherein eight to twelve features are observed in the 1020–100 cm−1 spectral window with comparable peak locations.41,61
The MIR spectrum of ErW10 (complex 11) will be discussed in detail since this allowed for matching our spectrum assignments to those made by Radio et al. in their study on GdW10 and ErW10 complexes.34 Comparing the overall features of the MIR spectrum of 11 with literature results, we found that vibrational bands in our spectrum were consistently redshifted by approximately 10 cm−1 which may be due to our use of an Attenuated Total Reflectance (ATR) probe rather than the more traditional KBr pellet.63 The MIR features centered at 3353 cm−1, 1650 cm−1, and 1635 cm−1 were assigned to ν(O–H) and δ(H–O–H) stretches of water. The broad peak at 1357 cm−1 and the sharp peak at 968 cm−1 were assigned to the νas(NO3) and ν(NO3) modes of NaNO3, respectively. The presence of NaNO3 is expected as it is the main byproduct in our synthetic process. The peak at 921 cm−1 corresponds to the ν(WOt) mode, while peaks at 833 cm−1, 777 cm−1, 694 cm−1, 582 cm−1, 538 cm−1, and 480 cm−1 were assigned as ν(W–O–W) modes. The final peak at 405 cm−1 was assigned as the δ(W–O–W) mode. Overall, there is a good agreement between the MIR spectrum of 11 and the results from Radio and colleagues in terms of peak locations.34 Peak fitting was also conducted on the MIR spectrum of 11 from 1200–400 cm−1 and the fitted spectrum and fit details can be found in Fig. S40 and Table S33 (ESI†).
The plot of frequencies of the ν(WO5)2 mode versus the ionic radii of the Ln(III) cations is presented in Fig. 6, which shows a general decrease in the frequency of ν(WO5)2 modes as we move to larger Ln(III) cations with two clear outliers in complexes 7 and 14 (GdW10 and LuW10). We evaluated the W–O bond distances of the coordinating WO6 unit in complexes 7 and 14 to see if this was the origin of the anomalous behavior; however, these values were consistent with W–O distances throughout the LnW10 series. We also compared structural distortion parameters of 1–14 with ν(WO5)2 mode frequencies, which show correlations between the FIR mode and SA, PA, and PD values when complexes of the same polymorph are compared. A look at the relationship between the frequencies of ν(WO5)2 modes and SAs shows that there is a blueshift in mode frequency as the SA grow larger for polymorph 1 structures, whereas the trend is flipped for polymorph 3 and 4 complexes (Fig. S41, ESI†) and ν(WO5)2 mode frequencies redshift as SAs increase (Fig. S41, ESI†). In the comparison of ν(WO5) frequencies versus PAs, polymorph 1 structures exhibit a blueshift in the stretching mode as PAs increase, while polymorph 3 complexes do not display any type of correlation (Fig. S42, ESI†). Similar to what was observed in the comparison with SA values, ν(WO5)2 mode frequencies for polymorph 4 structures redshift as PAs increase with an outlier in complex 14 (Fig. S42, ESI†). In comparisons with metal complex PDs, polymorph 1 structures once again feature a redshift in ν(WO5)2 stretching frequencies as PDs increase, while polymorph 3 complexes do not display any type of clear correlation, consistent with SA and PA results described above (Fig. S43, ESI†). Interestingly, ν(WO5)2 mode frequencies for polymorph 4 structures blueshift as PDs increase, which is a change from the trends observed for SA and PA values (Fig. S43, ESI†). In general, structural distortion parameters consistently show correlations with the ν(WO5)2 mode frequencies in polymorph 1 and 4 structures, whereas no relationship between the stretching mode and polymorph 3 structural parameters is observed. This suggests that distortion parameter effects on the ν(WO5)2 frequency are distinct for each LnW10 polymorph, which indicates that secondary interactions with lattice elements play a role in tuning this FIR vibrational band.
Changes in ρ(LnO8) frequencies were compared with lanthanide ionic radii and the results are presented in Fig. 7, which shows that the frequency of this FIR spectral band blueshifts as the ionic radii of the metal center increases, except for one outlier peak corresponding to complex 7 (GdW10). It is important to note that we did not identify a peak suitable for this mode for complex 14 (LuW10), thus it is not included in this analysis. We also compared ρ(LnO8) mode frequencies with structural distortion parameters of 1–14 to gain insights into possible polymorph-based correlations and found trends in how this FIR mode shifted as a function of SA, PD, and PA values when complexes of the same polymorph are compared. A look at the relationship between the frequencies of ρ(LnO8) modes and SAs shows that for polymorph 1 and 3 complexes the mode blueshifts as SAs increase, while for polymorph 4 structures no trends were observed (Fig. S44, ESI†). In comparisons with metal complex PAs, ρ(LnO8) frequencies for polymorph 1 and 3 complexes were also found to blueshift with increasing PA values (Fig. S45, ESI†). In contrast, ρ(LnO8) modes for polymorph 4 structures redshifted in frequency with larger PA values (Fig. S45, ESI†). In the comparison of ρ(LnO8) frequencies versus PDs, similar trends to those observed with SAs were noted with polymorph 1 and 3 complexes featuring ρ(LnO8) modes that blueshift when PDs increase, whereas for polymorph 4 structures no correlations between the two parameters were identified (Fig. S46, ESI†). In general, structural distortion parameters consistently show correlations with the ρ(LnO8) mode frequencies in polymorph 1 and 3 structures, while no relationship between the stretching mode and polymorph 4 structural parameters is observed except for with PA values. These findings support the takeaway from ν(WO5)2 frequency versus distortion parameter comparisons, specifically that secondary interactions with lattice elements are capable providing a route to tune FIR vibrational modes.
For the frequencies of the ν/ρ(LnO8) mode, a redshift is observed as we move to larger Ln(III) cations except for complex 1 (LaW10) which is a likely outlier (Fig. 8). Consistent with trends observed for other FIR modes, plotting ν/ρ(LnO8) frequencies versus structural distortion parameters highlights polymorph based trends. When comparing ν/ρ(LnO8) mode frequencies with SAs, there is noticeable blueshift as SA values increase for polymorph 1 structures, while polymorph 3 and 4 complexes display the opposite behavior with mode frequencies redshifting as SAs increase (Fig. S47, ESI†). Comparisons of ν/ρ(LnO8) mode frequency versus PA values yield similar trends to those observed with SAs for polymorph 1 and 3 complexes, whereas for polymorph 4 structures no correlations are observed (Fig. S48, ESI†). The relationship between ν/ρ(LnO8) mode frequencies and PDs for complexes 1–14 is the most varied with polymorph 1 structures consistently displaying a blueshift in vibrational frequency with increasing PD values (Fig. S49, ESI†). For polymorph 3 complexes, we note two trends: complexes 6, 8, 12, and 13 (EuW10, TbW10, TmW10, YbW10) show the ν/ρ(LnO8) mode redshifting as the PD increases, while complexes 5 and 7 (SmW10, GdW10) display the opposite relationship (Fig. S49, ESI†). For polymorph 4 structures, the frequency of the ν/p(LnO8) mode redshifts as PDs increase, in a similar manner to how ν/p(LnO8) frequencies evolved as function of SAs for this same group of complexes (Fig. S49, ESI†).
Fig. 8 Plot of FIR ν/ρ(LnO8) frequencies versus lanthanide ionic radii for complexes 1–14. Error bars represent uncertainties of the peak center obtained from the fitting regime. |
In the Raman spectra of 1–14, two peaks centered at 360 cm−1 and 888 cm−1, corresponding to the [δ(W–O–W/WO/Ln–O–W)] and [ν(Ln–O–W)] modes, respectively, were chosen to be analyzed in further detail. The frequencies of both Raman modes were compared against lanthanide ionic radii and the results are presented in Fig. 9 and 10. A blueshift in the δ(W–O–W/WO/Ln–O–W) frequencies can be observed as Ln(III) cations increase in size. On the other hand, we observed a redshift in ν(Ln–O–W) frequencies as Ln(III) cations increase in size; however, there is variance in this trend as complexes 7–10 and 12 (GdW10, TbW10, DyW10, HoW10, TmW10) do not follow the linear decrease in frequency that is characteristic of early and late LnW10 complexes.
Fig. 9 Plot of Raman δ(W–O–W/WO/Ln–O–W) frequencies versus lanthanide ionic radii for complexes 1–14. Error bars represent uncertainties of the peak center obtained from the fitting regime. |
Fig. 10 Plot of Raman ν(Ln–O–W) frequencies versus lanthanide ionic radii for complexes 1–14. Error bars represent uncertainties of the peak center obtained from the fitting regime. |
Comparing Raman mode frequencies against structural distortion parameters did not yield any correlations for the [δ(W–O–W/WO/Ln–O–W)] mode (Fig. S50–52, ESI†), whereas plots of ν(Ln–O–W) frequencies versus SA, PA, and PD values revealed polymorph based correlations, consistent with FIR results described earlier (Fig. S53–55, ESI†). We found that ν(Ln–O–W) mode frequencies for polymorph 1 and 4 complexes redshift as SAs increase, while for polymorph 3 structures there was not any relationship between the two parameters (Fig. S53, ESI†). The analogous comparisons of ν(Ln–O–W) modes versus PAs show that polymorph 1 complexes feature redshifts in Raman frequencies as PA values increase, whereas there are not any trends for polymorph 3 and 4 structures (Fig. S54, ESI†). In the plot of ν(Ln–O–W) frequencies versus PDs, we observed that Raman modes redshift for polymorph 1 and 4 complexes as PDs increase, while for polymorph 3 structures the opposite trend is exhibited with ν(Ln–O–W) frequencies blueshifting with larger PD values (Fig. S55, ESI†). The correlations noted in Fig. 9 and the absence of similar phenomena in comparisons with structural distortion parameters for the δ(W–O–W/WO/Ln–O–W) Raman mode implies that this band is only influenced by the interaction between the Ln(III) center and the coordinating oxygen atoms. More generally, we have found that FIR and Raman vibrational modes display some correlations between their frequencies and both the ionic radii and the distortion parameters, suggesting these vibrational modes are affected by both the first and second coordination spheres within LnW10 POM complexes.
To improve understanding of how structural parameters impact vibrational modes relevant to spin–phonon coupling processes, partial least square (PLS) analysis was done with structural parameters (ionic radii, SA, PA, and PD) as independent variables and each vibrational mode set as the dependent variables (Fig. S56–S66, ESI†). The PLS analysis for the ν(WO5)2 FIR stretch shows only two structural parameters, ionic radii and PAs, are statistically significant which is defined by having a variable influence on projection (VIP) value of over 0.8 (Fig. S56 and 57, ESI†); however, the leave-one-out cross validation test which determined the optimal number of independent variables via calculation of the minimum root mean PRESS (predicted residual sum of squares), found only one factor, the ionic radii, to be optimal for the fit. The model constructed with only lanthanide ionic radii as the independent variable accounts for 38% of the variance in the ν(WO5)2 frequencies. If both structural parameters (ionic radii and plane angle) are included in the PLS model, this accounts for 47% of the variance observed in the frequency of this FIR mode (Fig. S58 and 59, ESI†). PLS analysis on the ρ(LnO8) FIR mode shows three structural parameters, ionic radii, PAs and SAs, are statistically significant and a cross validation test on the model confirms that ionic radii and SAs are necessary for the fit even though these two independent variables can only account for 30% of the variance in ρ(LnO8) frequencies (Fig. S60 and 61, ESI†). The low variance accountability for these modes is not surprising as the visual correlations are not strong; however, this suggests that there are other structural parameters with a more significant role in modulating these mode frequencies. PLS analysis on the ν/ρ(LnO8) FIR mode finds that three structural parameters, ionic radii, PAs, and SAs, are statistically significant and account for 86% of the variance observed (Fig. S62 and 63, ESI†), which suggests that the ν/ρ(LnO8) mode is strongly correlated with these specific structural parameters. This is notable as Blockmon et al. found significant coupling between this mode and the MJ = ±7 states of Ho(III) in HoW10.31 Moreover, as frequencies of this mode can be modulated by tuning POM structural parameters, this provides a pathway for affecting the extent of spin–phonon coupling within POM complexes by controlling the extent of distortion around the metal center. For the ν(Ln–O–W) Raman mode, PLS analysis indicates that the lanthanide ionic radii is the only statistically significant structural parameter, accounting for 51% of the variance observed in the mode frequency (Fig. S64 and 65, ESI†). This is surprising due to the presence of polymorph based correlations in comparisons between ν(Ln–O–W) mode frequencies and structural distortion parameters that, based on the results from the FIR modes, imply some involvement of the distortion parameters in modulating this mode. Finally, PLS analysis on the [δ(W–O–W/WO/Ln–O–W)] mode found that none of the structural parameters discussed were a determinant for this vibrational mode (Fig. S66, ESI†). Despite the limited accountability for the variance found in the vibrational modes that were probed using PLS analysis, the models still confirm the involvement of structural parameters in modulating these bands, except for the [δ(W–O–W/WO/Ln–O–W)] mode, which agrees with the conclusions from our qualitative analysis.
Footnote |
† Electronic supplementary information (ESI) available: Crystallographic parameters for complexes 1–14, additional structural figures, methodological details for determining structural distortion parameters, raw and fitted FIR and Raman spectra for complexes 1–14, plots comparing structural distortion parameters versus lanthanide ionic radii, plots comparing FIR and Raman vibrational modes frequencies with structural distortion parameters, methodological details for performing PLS analysis, and plots produced from PLS analysis where the relationship between FIR and Raman vibrational modes frequencies and structural distortion parameters was investigated. CCDC 2336257 (complex 9 (DyW10)), 2336260–2336262 (complexes 3 (PrW10), 8 (TbW10), and 12 (TmW10)), 2336274–2336276 (complexes 5 (SmW10), 6 (EuW10), and 13 (YbW10)), 2336278 (complex 7 (GdW10)), 2336280 (complex 11 (ErW10)), 2336284 (complex 1 (LaW10)), 2336286 (complex 2 (CeW10)), 2336288 (complex 14 (LuW10)), 2336290 (complex 4 (NdW10)), and 2336921 (complex 10 (HoW10)). For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d4dt00786g |
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