Abstract
In this work, we have used a combination of vibrational spectroscopy (infrared, Raman and inelastic neutron scattering) and periodic density functional theory to investigate six metal methanesulfonate compounds that exhibit four different modes of complexation of the methanesulfonate ion: ionic, monodentate, bidentate and pentadentate. We found that the transition energies of the modes associated with the methyl group (C–H stretches and deformations, methyl rock and torsion) are essentially independent of the mode of coordination. The SO3 modes in the Raman spectra also show little variation. In the infrared spectra, there is a clear distinction between ionic (i.e. not coordinated) and coordinated forms of the methanesulfonate ion. This is manifested as a splitting of the asymmetric S–O stretch modes of the SO3 moiety. Unfortunately, no further differentiation between the various modes of coordination: unidentate, bidentate etc … is possible with the compounds examined. While it is likely that such a distinction could be made, this will require a much larger dataset of compounds for which both structural and spectroscopic data are available than that available here.
Keywords: methanesulfonate, inelastic neutron scattering spectroscopy, infrared spectroscopy, Raman spectroscopy, DFT
1. Introduction
Metal methanesulfonates (M(CH3SO3)x · nH2O) are compounds of interest because of the role they play as catalysts for numerous reactions in organic synthesis including (but not limited to) Mannich, Biginelli reaction, esterification and tetrahydropyranylation of alcohols and phenols [1] (figure 1). This is due to their low toxicity, low cost and low reactivity with air and water [2].
Figure 1.
Tetrahydropyranylation of an alcohol catalysed by a metal methanesulfonate.
Although these substances are rarely found naturally, some forms can be found in the sea as a result of methanesulfonic acid (CH3SO3H) being produced and emitted by marine phytoplankton (via the oxidation of dimethyl sulfide). This then undergoes chemical reactions with the cations present in sea salt e.g. Mg2+, K+, Ca2+ and Na+, to form their respective metal methanesulfonate salts [3,4]. The natural methods through which these salts form mean that they are vital to exploring the past due to nature of their deposition in ice cores, with a particular focus on Mg(CH3SO3)2· nH2O and Na(CH3SO3)2· nH2O—where the sodium salt is the most abundant [5]. It is worth noting, though, that the magnesium salt found is restricted to the Last Glacial Maximum ice which forms during the coldest period in the glacial cycle. Only during this time did the atmospheric conditions enable preservation of the salt because normally when Mg(CH3SO3)2· nH2O is deposited, it subsequently dissolves in acidic ice [3].
Metal methanesulfonate salts have also recently come into use in electrophysiological research as a common substance used for patch-clamp techniques to allow for the study of ion channels in cells. Caesium methanesulfonate is especially appropriate for this role as Cs+ can block K+ currents [6] while CH3SO3− can block Cl− channels [7]. The implications from this technique are far ranging, as it can be used to investigate many biological processes from canine atrial cells [6] to hippocampal pyramidal cells in young rats [8].
The vibrational spectra of metal methanesulfonate salts have been investigated several times [9–13]. In the present work, we use a combination of infrared, Raman and inelastic neutron scattering (INS) spectroscopies to observe all of the modes of the methanesulfonate ion in both ionic (M = Na, Cs) and complexed (M = Cu, Ag, Cd) environments. The assignments are supported by periodic density functional theory (DFT) calculations of the Na, Cs and Cu salts.
2. Experimental
2.1. Materials
The M(CH3SO3) salts, M = Na, Cs, Ag, were purchased from Aldrich and used as received, except for the Ag salt which was dried overnight at 110°C in a vacuum oven, to remove traces of adsorbed water. The Cu(H2O)4(CH3SO3)2, Cu(D2O)4(CH3SO3)2, Cd(H2O)2(CH3SO3)2, Cd(D2O)2(CH3SO3)2 and a sample of Ag(CH3SO3) were kindly provided by Durham University. These were in sealed quartz ‘lollipops’. After the Raman and INS measurements were made, the lollipops were broken open in order to measure the infrared spectra. Powder X-ray diffraction confirmed the identities of the samples. In further confirmation, the data reported here are for the Ag salt from Aldrich; however, comparison with the spectra of the Ag salt of the Durham sample showed them to be identical.
2.2. Vibrational spectroscopy
INS spectra were recorded at less than 20 K using TOSCA [14] at ISIS (http://www.isis.stfc.ac.uk/). The spectra are available at the INS database: http://wwwisis2.isis.rl.ac.uk/INSdatabase/. Infrared spectra were recorded using a Bruker Vertex70 FTIR spectrometer, over the range 100 to 4000 cm−1 at 4 cm−1 resolution with a DLaTGS detector using 64 scans and the Bruker Diamond ATR. The use of the ultra-wide range beamsplitter enabled the entire spectral range to be recorded without the need to change beamsplitters. The spectra have been corrected for the wavelength-dependent variation in pathlength using the Bruker software. FT-Raman spectra were recorded with a Bruker MultiRam spectrometer using 1064 nm excitation, 4 cm−1 resolution, 500 mW laser power and 64 scans. Dispersive Raman spectra were recorded with a Bruker Senterra Raman spectrometer using 532 nm excitation. All the infrared and Raman spectra were measured in air at room temperature. The Raman spectra of the Cu complex have been baseline corrected to remove a broad fluorescence background.
2.3. Computational studies
The plane wave pseudopotential-based program CASTEP was used for the calculation of the vibrational transition energies and their intensities [15,16]. The generalized gradient approximation Perdew–Burke–Ernzerhof functional was used in conjunction with optimized norm-conserving pseudopotentials. In the electronic supplementary material, table S1 gives the details of the calculations. All of the calculations were converged to better than |0.0035| eV Å−1. After geometry optimization, the vibrational spectra were calculated in the harmonic approximation using density functional perturbation theory [17]. This procedure generates the vibrational eigenvalues and eigenvectors, which allows visualization of the modes within Materials Studio (http://accelrys.com/products/collaborative-science/biovia-materials-studio/) and is also the information needed to calculate the INS spectrum using either the programs ACLIMAX [18] or AbINS [19]. We emphasize that the transition energies have not been scaled.
3. Results and discussion
In this section, we will first provide a complete assignment for Cs(CH3SO3) based on a periodic DFT calculation. We will then use this to assign the internal modes of the methanesulfonate ion in the other materials.
3.1. Cs(CH3SO3)
Figure 2 shows the INS, Raman and infrared spectra of Cs(CH3SO3). Table 1 lists the transition energies and assignments, which are based on visualization of the modes from the CASTEP calculation. In the electronic supplementary material, table S2 lists all of the calculated modes with their assignments. Cs(CH3SO3) crystallizes in the orthorhombic space group Pnma (no. 62) with four formula units in the primitive cell [20], thus there are 108 modes in total comprising 3 acoustic modes, 21 optic translational modes of the ions, together with 12 librational and 72 internal modes of the methanesulfonate ion. A complete factor group analysis is given in the electronic supplementary material, table S2. The methanesulfonate ion is on a general position, however it has C3v symmetry within the accuracy of the analysis. Assuming C3v symmetry, the 18 internal modes of the isolated methanesulfonate ion can be classified as: C–H stretch (A1 + E), H–C–H bend (A1 + E), methyl rock (E), S = O stretch (A1 + E), O = S = O bend (A1 + E), C–S stretch (A1), sulfonate rock (E) and C–S torsion (A2).
Figure 2.

(a) INS, (b) FT-Raman and (c) infrared spectra of Cs(CH3SO3).
Table 1.
Transition energies (cm−1) of the internal modes of the methanesulfonate ion in the Na and Cs compounds. sh, shoulder; modes in italics are overtones or combinations.
| Na |
Cs |
|||||
|---|---|---|---|---|---|---|
| INS | Raman | infrared | INS | Raman | infrared | description |
| 3023, 3005 | 3018, 3004 | 3020, 3006 | 3021 | CH3 asymmetric stretch | ||
| 2939 | 2941 | 2942, 2931 | CH3 symmetric stretch | |||
| 2863, 2829 | 2838 | 2 × CH3 symmetric bend | ||||
| 1432, 1400 | 1453, 1435, 1413 | 1451, 1434, 1415 | 1434 | 1438 | 1430, 1421sh | CH3 asymmetric bend |
| 1325 | 1352, 1336 | 1330 | 1342, 1323 | CH3 symmetric bend | ||
| 1183 | 1218, 1204, 1195, 1169 | 1247, 1215sh, 1183 | 1191, 1176 | 1219sh, 1179, 1115sh | SO3 asymmetric stretch | |
| 1049 | 1078, 1061sh, 1052 | 1074sh, 1061, 1054 | 1055, 1036 | 1036 | SO3 symmetric stretch | |
| 981, 968 | 992sh, 986, 972, 960sh | 990, 965 | 991, 980 | 986, 972 | 988, 979 | CH3 rock |
| 784 | 799, 792sh 781 | 787, 781 | 780, 763 | 775 | 771 | C–S stretch + SO3 symmetric bend |
| 699, 644, 607 | 613 |
|
||||
| 567, 562, 552 | 578, 568sh, 560 | 574sh, 559, | 564, 556sh | 568, 552 | 553 | SO3 symmetric bend + C–S stretch |
| 531 | 544, 532 | 544, 534, 527sh | 536, 521 | 533 | 527 | SO3 asymmetric bend |
| 425 | 2 × C–S torsion (220 cm−1) | |||||
| 350, 336 | 354 | 351 | 347, 334 | 351, 345sh | 346, 337sh | SO3 rock |
| 309, 294, 270, 224, 217 | 271, 264 | C–S torsion | ||||
For a centrosymmetric molecule in the gas phase the rule of mutual exclusion (no coincidences in the infrared and Raman spectra) is strictly valid. In the solid state, this is only rigorously true for a centrosymmetric molecule in a crystal that crystallizes in a centrosymmetric system and has only one molecule in the primitive cell. A classic example is K2[PtCl6], which crystallizes in a cubic space group and the ion occupies an octahedral site [21]. For a centrosymmetric crystal with two molecules in the unit cell, the vibrations form in-phase and out-of-phase pairs; this is the factor group splitting and arises from interactions between the molecules. In the limit that the interaction is zero, the in-phase and out-of-phase pairs are accidentally degenerate. If one mode is Raman active and the other is infrared active, then even though it is a centrosymmetric system, the modes will occur at the same transition energy in both spectra. It is the degree of coupling between the species that determines the difference in the transition energies in the two forms of spectroscopy. This is explored in more detail in the electronic supplementary material, figure S1 and table S2. In the present case, although the structure is centrosymmetric, the factor group splitting is small, even though there are four molecules in the unit cell, meaning that modes occur at similar energies in both sets of spectra. There is no evidence for symmetry-breaking in this system, as has been found for other alkali metal compounds [22,23].
The spectra illustrate the complementarity of the three techniques. INS has no symmetry-based selection rules [24], however there is a strong ‘propensity’ rule that motions that involve displacement of hydrogen dominate the spectrum. This is dramatically shown by the strongest mode in the INS spectrum at approximately 270 cm−1, which is assigned to the torsion about the C–S bond. The computational study (electronic supplementary material, table S4) confirms that this mode has essentially zero intensity in both the infrared and Raman spectrum, but as a consequence of the large amplitude hydrogen motion, it is very strong in the INS spectrum. It is also notable that only the methyl modes (torsion, rock, deformations) have significant intensity in the INS spectrum. This demonstrates that the coupling between the CH3 and SO3 moieties in the ion is weak. By contrast, the strongest modes in the infrared and Raman spectra are motions of the SO3 moiety.
Figures 3, and Figures S2 and S3 in the electronic supplementary material compare the observed and calculated INS, Raman and infrared spectra of Cs(CH3SO3). It can be seen that for the INS and Raman spectra the agreement is almost quantitative in terms of both transition energy and relative intensity. For the infrared spectrum, the intensity agreement is poorer, which is a consequence of the use of the same band width for all of the calculated modes; inspection of the experimental spectrum shows that this is not the case. Nonetheless, it is clear that the calculation has provided a reliable basis for the spectral assignment and this will be used for the other salts.
Figure 3.

Comparison of experimental (purple) and calculated (blue) INS spectra of Cs(CH3SO3).
3.2. Na(CH3SO3)
Figure 4 shows the INS, Raman and infrared spectra of Na(CH3SO3). The similarities to those of the Cs salt are striking, except for the greater intricacy of the Na spectra. The structure of the Na salt is complex with 20 formula units in the primitive cell [25]. The very large number of optic modes (537) means that it is not possible to calculate the Raman spectrum in a reasonable time. However, as figure 5 shows, the calculated INS spectrum is in excellent agreement with the experimental spectrum. In the electronic supplementary material, figure S4 compares the observed and calculated infrared spectra. Table 1 lists the observed bands and their assignments.
Figure 4.

(a) INS, (b) FT-Raman and (c) infrared spectra of Na(CH3SO3).
Figure 5.

Comparison of experimental (purple) and calculated (blue) INS spectra of Na(CH3SO3).
3.3. Cu, Cd and Ag methanesulfonates
In contrast to the simple ionic bonding present in the alkali metal salts, the structures of the Cu [26], Cd [27] and Ag [28] compounds are more diverse and more complex. The Cu compound has square planar [Cu(H2O)4]2− ions with the apical positions occupied by an oxygen atom of the methanesulfonate ion. Each methanesulfonate ion is only coordinated to one [Cu(H2O)4]2− ion. For the Cd compound, the Cd atom is located at the inversion centre of an octahedron with the O atoms of two water molecules at the apices and the O atoms belonging to four methanesulfonato groups in the horizontal plane. The Cd atoms are bridged by the methanesulfonato groups, so forming parallel infinite chains running along the b axis. The Ag complex has an even more elaborate structure. There is no distinct molecule; the methanesulfonato groups act as pentacoordinating ligands. Thus, each Ag atom is at the centre of a very distorted trigonal bipyramid. Figure 6 shows the three structures, which exhibit monodentate, bidentate and pentadentate coordination, respectively, of the methanesulfonato ligand.
Figure 6.
Structure of: (a) Cu(H2O)4(CH3SO3)2, (b) Cd(H2O)2(CH3SO3) and (c) Ag(CH3SO3). (Colour key: white, H; grey, C; red, O; yellow, S; copper, Cu, brown, Cd; blue, Ag).
The INS spectra of the Cu, Cd and Ag materials (including the D2O isotopomers for Cu and Cd) are shown in figure 7. As with the alkali metal salts (figures 3 and 5 and table 1) the features assigned to modes of the methyl group dominate the spectra and show a remarkable constancy in position (table 2). This is consistent with the methyl groups not being involved in the bonding; in all three examples they project into vacant space in the structure. The modes due to the coordinated water molecules in the Cu and Cd compounds give rise to librational modes in the 400–900 cm−1 region [29–31]. These are relatively weak and are readily assigned because they are shifted and much weaker in the D2O-containing samples.
Figure 7.

INS spectra of: (a) Cu(H2O)4(CH3SO3)2, (b) Cu(D2O)4(CH3SO3)2, (c) Cd(H2O)2(CH3SO3)2, (d) Cd(D2O)2(CH3SO3)2 and (e) Ag(CH3SO3). Methyl modes (torsion, rock, deformations) are indicated by asterisks.
Table 2.
Transition energies (cm−1) of the internal modes of the methanesulfonate ion in the Cu, Cd and Ag compounds. sh, shoulder; modes in italics are overtones or combinations.
| Cu |
Cd |
Ag |
|||||||
|---|---|---|---|---|---|---|---|---|---|
| INS | Raman | infrared | INS | Raman | infrared | INS | Raman | infrared | description |
| 3029, 3012 | 3029, 3012 | 3037, 3025 | 3040 | 3031, 3021 | 3031, 3019 | CH3 asymmetric stretch | |||
| 2940 | 2940 | 2945 | 2950 | 2940 | 2939 | CH3 symmetric stretch | |||
| 1421 | 1422 | 1428, 1414 | 1405 | 1422, 1414sh | 1428, 1415 | 1426 | 1430, 1421 | 1434, 1415 | CH3 asymmetric bend |
| 1342 | 1339 | 1323 | 1332, 1322sh | 1328 | 1338, 1319 | CH3 symmetric bend | |||
| 1207 | 1216, 1138 | 1217, 1198sh | 1241, 1155 | 1200 | 1168, 1116 | SO3 asymmetric stretch | |||
| 1215 | 1187 | 1219 | C–S torsion + CH3 rock | ||||||
| 1123 | 1130 | 1129 | C–S stretch + SO3 rock | ||||||
| 1045 | 1043 | 1065 | 1056 | 1050 | 1014 | SO3 symmetric stretch | |||
| 963 | 964 | 966, 957 | 968 | 1002, 991, 969 | 990sh, 975, | 993, 974 | 961 | 986, 967 | CH3 rock |
| 902 | 896 | 897 | 893 | H2O libration | |||||
| 801 | 791 | 776 | 787 | 792 | 797sh, 785 | 779 | 784 | 771 | C–S stretch + SO3 symmetric bend |
| 605, 593 | 601 | 634, 586 | 658, 616 | H2O libration | |||||
| 568, 549, 536sh, 525, 516 | 551, 528 | 544, 515 | 566, 555, 545, 536, 523, 509 | 573, 541, 519 | 571, 549, 539, 509 | 560, 533, 521 | 544, 526, 515 | SO3 symmetric bend + C–S stretch | |
| 491 | 488 | 486, 474, 458 | 488 | ||||||
| 464, 453, 438 | 436 | 418 | 449, 440, 424, 415 | ||||||
| 357sh, 347 | 353 | 348 | 347, 338 | 390, 351 | 346 | 365, 347 | 353 | SO3 rock | |
| 261, 248 | 270, 254, 246 | 256, 247 | 250, 241 | C–S torsion | |||||
The Raman spectra are shown in figure 8. Again, as with the alkali metal salts, the spectra are dominated by SO3 modes. Only the S–O symmetric stretch at approximately 1050 cm−1 shows a small variation in the complexes.
Figure 8.

Raman spectra of: (a) Cu(H2O)4(CH3SO3)2, (b) Cu(D2O)4(CH3SO3)2, (c) Cd(H2O)2(CH3SO3)2, (d) Cd(D2O)2(CH3SO3)2 and (e) Ag(CH3SO3).
The infrared spectra of Cu(H2O)4(CH3SO3)2, Cd(H2O)2(CH3SO3)2 and Ag(CH3SO3) in the fingerprint region are shown in figure 9. (The complete 0–4000 cm−1 spectra of these compounds and those of Cu(D2O)4(CH3SO3)2 and Cd(D2O)2(CH3SO3)2 are shown in the electronic supplementary material, figure S5). For the alkali metal salts, the spectra are consistent with local C3v symmetry, the degenerate modes only show a small or no splitting. This is not the case here; the asymmetric S–O stretch mode is both strongly perturbed and is downshifted with respect to the M = Na and Cs salts. It can be seen that the degeneracy of the S–O asymmetric stretch is lifted and two modes appear. (For the Cd salt, this manifests as a broadening of the band; compare the width of the symmetric and asymmetric S–O stretches.) Unfortunately, there is no apparent correlation between the degree of splitting and the type of coordination as there is, for example, with carbonate complexes [32].
Figure 9.

Infrared spectra of: (a) Cu(H2O)4(CH3SO3)2, (b) Cd(H2O)2(CH3SO3)2 and (c) Ag(CH3SO3). The dashed lines show the transition energies of the symmetric (left) and asymmetric (right) S–O stretch modes in Cs(CH3SO3).
4. Conclusion
At the outset of this work, it was hoped that the mode of coordination of the methanesulfonate ion would show characteristic patterns in the vibrational spectra. These could then be used as a fingerprint for the type of coordination, as found for other ions, e.g. nitrite, sulfate and carbonate [32]. We have studied six compounds that exhibit four different modes of coordination. We found that the transition energies of the modes associated with the methyl group (C–H stretches and deformations, methyl rock and torsion) are essentially independent of the mode of coordination. The SO3 modes in the Raman spectra also show little variation. In the infrared spectra, there is a clear distinction between ionic (i.e. not coordinated) and coordinated forms of the methanesulfonate ion. This is manifested as a splitting of the asymmetric S–O stretch modes of the SO3 moiety. Unfortunately, no further differentiation between the various modes of coordination, unidentate, bidentate etc. … , is possible with the compounds examined. While it is likely that such a distinction could be made, this will require a much larger dataset of compounds for which both structural and spectroscopic data is available than that used here.
Supplementary Material
Acknowledgements
The authors wish to thank Drs Joseph Howard and Douglas Graham, Chemistry Department, Durham University, UK, for the gift of the Cu, Cd and Ag salts. The STFC Rutherford Appleton Laboratory is thanked for access to neutron beam facilities. Computing resources (time on the SCARF compute cluster for the CASTEP calculations) was provided by STFC's e-Science facility. This research has been performed with the aid of facilities at the Research Complex at Harwell, including the FT-Raman spectrometer. The authors would like to thank the Research Complex for access and support to these facilities and equipment.
Data accessibility
The data which underpin this work are available via TopCat, the ISIS Facility's open access online data repository at: https://data.isis.stfc.ac.uk/doi/investigation/88613665.
Authors' contributions
L.Z. measured the infrared and Raman spectra and helped draft the manuscript; S.F.P. measured the INS spectra, carried out the DFT calculations and wrote the manuscript. Both authors gave final approval for publication.
Competing interests
We declare we have no competing interests.
Funding
This work is supported by the Science and Technologies Research Council (STFC).
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Associated Data
This section collects any data citations, data availability statements, or supplementary materials included in this article.
Supplementary Materials
Data Availability Statement
The data which underpin this work are available via TopCat, the ISIS Facility's open access online data repository at: https://data.isis.stfc.ac.uk/doi/investigation/88613665.


