A. Gómez-Zavagliaab and R. Fausto*a
aDepartment of Chemistry, University of Coimbra, P-3004-535, Portugal
bFacultad de Farmacia y Bioquímica, Universidad de Buenos Aires, RA-1113, Argentina. E-mail: rfausto@ci.uc.pt
First published on 15th November 2002
N,N-dimethylglycine methyl ester (DMG-Me) was studied by FT-IR spectroscopy under several experimental conditions, including low temperature solid state and isolated in low temperature inert gas matrices, and by molecular orbital calculations. In agreement with the theoretical predictions, the experimental data show that in the gaseous phase the most stable conformer (ASC) has the ester group in cis configuration and the N–C–CO and Lp–N–C–C (Lp
=
lone electron pair) dihedral angles equal to 0° and 180°, respectively, while the first conformational excited state corresponds to the doubly-degenerated-by-symmetry GSC form, where the Lp–N–C–C axis is gauche-oriented (±46.5°). On the other hand, for the matrix isolated molecule as well as in both the liquid and low temperature solid states the relative stability of the two lowest energy conformers of DMG-Me is reversed, the more polar GSC form becoming the ground conformational state. This molecule is then a remarkable example of a system showing an inversion in the order of its lowest energy conformational states due to a minor perturbation by the media such as that due to the inert gas matrix. Full assignment of the spectra obtained in the different experimental conditions used is also presented.
In a previous study, we have investigated DMG isolated in low temperature inert gas matrices by FT-IR spectroscopy.8 The analysis of the experimental data was supported by extensive quantum chemical calculations undertaken at both DFT and MP2 levels of theory. In that study, the spectral signatures of the three lowest energy conformers of neutral monomeric DMG were characterized for the first time. The conformational ground state was found to be the intramolecularly O–H⋯N hydrogen-bonded GAT form, where the Lp–N–C–C and N–C–CO dihedral angles are 30° and ca. 180°, respectively, and the carboxylic group assumes a trans configuration. In the second (ASC) and third (GSC) lowest energy forms of DMG, the carboxylic moiety assumes a cis conformation, while the N–C–C
O axis adopts the syn arrangement and the conformation around the N–C bond is, respectively, anti and gauche. The presence of the intramolecular hydrogen bond was found to be essential in the stabilization of the ground conformational state in DMG.8 In DMG-Me, however, this interaction cannot operate due to the replacement of the acid hydrogen atom by the methyl ester group, and a significantly different conformational behavior can then be expected for this compound.
Taking into consideration the results for DMG, the ASC and GSC conformations (which correspond to the second and third most stable conformers in DMG8) could be expected to be the most stable structures of DMG-Me. However, in the unique structural study reported so far,9 these conformations were neglected by the authors, since they were essentially interested to determine the electron binding energies of DMG-Me and the small dipole moments of both ASC and GSC are not large enough to allow the molecule to bind an excess electron. Instead, higher energy conformations with a trans carboxylic group and a larger dipole moment were considered.9 Hence, in practical terms, DMG-Me had not yet been characterized structurally until now. Moreover, no vibrational data was reported so far.
Since the ASC and GSC conformers in DMG were found to have relatively similar energies (ΔEGSC-ASC≈
2 kJ mol−1)8 and we have been particularly interested in our laboratory to investigate the influence of media on the relative stability of nearly accidentally degenerated conformers,10–12 DMG-Me appears, also from this perspective, as a potentially interesting and challenging molecular system to be studied. In this paper we report the results of an FT-IR spectroscopic study of DMG-Me in a variety of experimental conditions, which includes the liquid phase, the low temperature solid states and the matrix-isolated species in both argon and xenon matrices. These studies were complemented with molecular orbital calculations undertaken at the density functional theory (DFT) and second order Møller–Plesset (MP2) levels.
Conformations were optimized at each level of theory using the geometry direct inversion of the invariant subspace (GDIIS) method.18 Vibrational frequencies were calculated at the DFT level and the nature of the critical points on the potential energy surface resulting from optimisation was determined by inspection of the corresponding calculated Hessian matrix. All optimised structures were confirmed to be minimum energy conformations. The calculated frequencies were scaled down by a single factor (0.978) to correct them for the effects of basis set limitations, neglected part of electron correlation and anharmonicity effects, and used to assist the analysis of the experimental spectra. Normal coordinates analyses were undertaken in the internal coordinates space as described by Schachtschneider19 using the program BALGA and the optimised geometries and harmonic force constants resulting from the DFT(B3LYP)/6-311++G** calculations. Potential energy profiles for internal rotation were calculated performing a relaxed scan on the potential energy surface (PES) along the reaction coordinate and the transition state structures for conformational interconversion obtained using the synchronous transit-guided quasi-newton (STQN) method.20
In the matrix isolation experiments, a glass vacuum system and standard manometric procedures were used to deposit the matrix gas (argon, 99.99990%; xenon, 99.995%, obtained from Air Liquid). Matrices were prepared by co-deposition, onto the cooled CsI substrate of the cryostat, of the matrix gas and DMG-Me placed in a specially designed doubly termostattable Knudsen cell with shut-off possibility whose main component is a NUPRO SS-4BMRG needle valve. The temperature of the cell can be controlled separately in the valve nozzle and the sample compartment, enabling a more precise control of the saturated gas pressure over the liquid DMG-Me and a better metering function of the valve. Further details of the experimental setup can be found in ref. 21 All experiments were done on the basis of an APD Cryogenics close-cycle helium refrigeration system with a DE-202A expander. Deposition temperatures ranged from 9 to 20 K. Necessary modifications of the sample compartment of the spectrometer were made in order to accommodate the cryostat head and allow efficient purging of the instrument by a stream of dry air to remove water and CO2 vapours. After depositing the compound, annealing experiments were performed until a temperature of 30 K and 60 K for Ar and Xe, respectively.
The low temperature solid amorphous layer was prepared in the same way as matrices but with the flux of matrix gas cut off. The layer was then allowed to anneal at slowly increasing temperature up to 154 K. IR spectra were collected during this process every 10 to 20 K of temperature change. After the temperature exceeded 154 K the substrate was cooled back to 9 K and spectra collected each 10–20 K once more. Two cycles of annealing were performed by heating and cooling the sample between 9 and 154 K.
For liquid state experiments a thin film of the compound was pressed within two sealed KBr windows assembled in a SPECAC variable temperature cell controlled by a Red Lions digital temperature controller.
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Fig. 1 Lowest energy conformers of neutral DMG-Me with atom numbering scheme. For convenience, the values of main dihedral angles (degrees) and dipole moments (Debye) are included. |
Conformer | DFT(B3LYP)/6-311++G** | MP2/6-31++G** |
---|---|---|
ΔEZPE | ΔEZPEb | |
a Energies in kJ mol−1; conformers are depicted in Fig. 1.b Zero point energy corrections taken from DFT(B3LYP)/6-311++G** calculations.c Total energies with zero point vibrational energy contribution in parentheses. | ||
ASC | 0.0 (−1![]() ![]() | 0.0 (−1![]() ![]() |
GSC | 2.72 | 3.17 |
AAC | 4.93 | 4.48 |
GSkC | 6.37 | 4.66 |
GAT | 33.03 | 30.28 |
AST | 34.20 | 36.94 |
Fig. 2 shows the potential energy profile for interconversion between the two most stable conformers of DMG-Me and between the two equivalent-by-symmetry GSC conformers calculated at the DFT(B3LYP)/6-311++G** level of theory. To obtain this energy profile, the Lp–N–C–C dihedral angle was incremented by 30° and at each point all remaining geometrical parameters were optimized. The transition state structures were obtained using the synchronous transit-guided quasi-newton (STQN) method.20 The energy barriers associated with the ASC→
GSC and GSC
→
GSC′ conformational interconversions are predicted to be 28.3 kJ mol−1 and 12.8 kJ mol−1, respectively, being similar to those previously found for the corresponding isomerization reactions in N,N-dimethylglycine (29.4 kJ mol−1 and 13.6 kJ mol−18).
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Fig. 2 DFT(B3LYP)/6-311++G** calculated potential energy profile for internal rotation around the N4–C13 bond (ASC![]() ![]() ![]() ![]() |
It is interesting to note that in general the calculated geometries for the two most stable conformers of DMG-Me are very similar (see electronic supplementary material, Table S1†), indicating that in these conformers the main intramolecular interactions should not differ very much. The largest difference found in the geometrical parameters occurs for the C5–N4–C13, C9–N4–C13 and C1–C13–N4 angles, which are ca. 3° larger in the ASC conformer due to the closest proximity of the methyl groups from the carbonyl oxygen in this form. Indeed, the same conclusion could also be extracted by looking at the calculated Mülliken atomic charges in these two conformers (Table S2—electronic supplementary material†) that were also found to be quite similar except in the case of those of C1 and C13, which were predicted to be more positive and more negative, respectively, in the GSC conformer. These changes indicate a relatively higher charge separation in the GSC conformer, being in consonance with its larger dipole moment (1.99 D vs. 1.40 D in ASC; see Fig. 1). The N4–C13–H14 angle is also considerably different in ASC and GSC, being ca. 4° larger in the GSC conformer due to the repulsion between H14 and the closest methyl hydrogen atom H10 in this form.
![]() | ||
Fig. 3 Infrared spectra of DMG-Me trapped in argon and xenon matrices (spectra obtained immediately after deposition at 9 K) and calculated spectra for ASC and GSC conformers. |
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Fig. 4 Relevant spectral regions of the infrared spectrum of DMG-Me trapped in an argon matrix freshly prepared sample at 9 K (— nozzle temperature![]() ![]() ![]() ![]() ![]() |
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Fig. 5 Relevant spectral regions of the infrared spectrum of DMG-Me trapped in: (a) an argon matrix (— freshly prepared sample at 9 K; ![]() ![]() ![]() ![]() |
![]() | ||
Fig. 6 Infrared spectra of DMG-Me (a) in the liquid state (room temperature); (b) solid amorphous layer at 9 K; (c) amorphous layer difference spectrum (154 K–9 K); (d) annealed amorphous sample. (e) and (f) Calculated spectra for GSC and ASC monomers, respectively. |
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Fig. 7 Temperature dependence of the νC![]() |
![]() | ||
Fig. 8 Van't Hoff plot of ln [IνC![]() ![]() |
Approximate description | Conformer | Calculated frequency | Calculated intensity | Observed frequency | |
---|---|---|---|---|---|
Argon | Xenon | ||||
a Frequencies in cm−1; ν, bond stretching, δ, bending, γ rocking, ω wagging, tw, twisting, τ torsion. See Supplementary material (Tables S3–S5) for definition of symmetry coordinates, full set of calculated frequencies and intensities and PED. | |||||
νOCH3as′ | ASC | 3087.0 | 14.7 | 3036.7 | 3021.6 |
GSC | 3053.4 | 19.8 | 3007.0 | 3021.6 | |
νOCH3as″ | ASC | 3053.9 | 19.9 | 3007.0 | 3021.6 |
GSC | 3086.2 | 14.1 | 3036.7 | 3021.6 | |
νCH3as″(2) | ASC | 3017.7 | 54.4 | 2978.7 | 2974.0 |
GSC | 3062.4 | 9.4 | 3007.0 | 2988.7 | |
νCH3as″(1) | ASC | 3015.2 | 15.9 | 2974.9 | 2988.7 |
GSC | 3030.7 | 31.2 | 2983.0 | 2988.7 | |
νCH2as | ASC | 2994.3 | 8.9 | 2963.0 | 2964.0 |
GSC | 2997.9 | 12.7 | 2963.0 | 2964.0 | |
νOCH3s | ASC | 2983.2 | 20.4 | 2946.8 | 2946.5 |
GSC | 2982.8 | 35.0 | 2946.8 | 2946.5 | |
νCH3as′(2) | ASC | 2982.5 | 33.8 | 2946.8 | 2946.5 |
GSC | 2988.0 | 29.8 | 2963.0 | 2964.0 | |
νCH3as′(1) | ASC | 2982.0 | 53.2 | 2946.8/2948.1 | 2946.5 |
GSC | 2848.4 | 190.0 | 2850.6/2835.3/2823.4 | 2816.1/2843.7/2828.9 | |
νCH2s | ASC | 2959.5 | 21.5 | 2913.5 | 2934.4 |
GSC | 2832.4 | 46.8 | 2778.6 | 2770.7 | |
νCH3s(1) | ASC | 2913.0 | 69.7 | 2899.6/2888.7 | 2890.5/2881.6 |
GSC | 3006.0 | 27.2 | 2967.8 | 2974.0 | |
νCH3s(2) | ASC | 2906.5 | 66.5 | 2875.5 | 2866.8 |
GSC | 2836.9 | 47.8 | 2799.6/2794.8 | 2793.1 | |
νC![]() | ASC | 1752.3 | 208.2 | 1761.0/1751.3 | 1757.2/1754.0/1751.4 |
GSC | 1768.4 | 232.5 | 1778.0/1771.9/1769.5 | 1766.0/1763.1/1759.6 | |
δCH3as″(1) | ASC | 1493.8 | 17.3 | 1483.4 | 1480.0 |
GSC | 1478.7 | 12.5 | 1471.9 | Non obs. | |
δCH3as″(2) | ASC | 1480.1 | 3.9 | 1476.0 | Non obs. |
GSC | 1463.0 | 14.7 | 1462.8 | 1462.1 | |
δOCH3as′ | ASC | 1465.1 | 10.8 | 1465.1 | 1462.1 |
GSC | 1451.1 | 9.8 | 1449.0 | 1445.2 | |
δCH3as′(1) | ASC | 1457.3 | 16.6 | 1459.4 | 1456.7 |
GSC | 1473.6 | 12.4 | 1469.2 | 1465.7 | |
δOCH3as″ | ASC | 1450.8 | 9.7 | 1449.0 | 1445.2 |
GSC | 1465.4 | 8.9 | 1462.8 | 1462.1 | |
δCH3as′(2) | ASC | 1445.8 | 7.2 | 1458.3 | Non obs. |
GSC | 1454.5 | 13.4 | 1450.0 | 1445.2 | |
δCH3s(1) | ASC | 1441.4 | 2.8 | 1443.9 | Non obs. |
GSC | 1447.2 | 0.7 | Non obs. | Non obs. | |
δOCH3s | ASC | 1435.7 | 9.1 | 1435.1 | 1432.2 |
GSC | 1437.5 | 11.3 | 1437.8 | 1434.5 | |
δCH2 | ASC | 1411.2 | 16.7 | 1408.7 | 1404.2 |
GSC | 1424.0 | 10.2 | 1419.8/1418.1 | 1414.1 | |
δCH3(2) | ASC | 1409.3 | 1.0 | Non obs. | Non obs. |
GSC | 1409.9 | 0.6 | Non obs. | Non obs. | |
ωCH2 | ASC | 1346.7 | 6.5 | 1351.0/1365.5 | 1352.4 |
GSC | 1374.8 | 11.2 | 1383.7/1380.6/1377.6 | 1383.7/1378.8 | |
twCH2 | ASC | 1325.3 | 9.5 | 1324.5 | 1324.7 |
GSC | 1285.6 | 23.6 | 1288.0/1285.8 | 1280 | |
γCH3′(1) | ASC | 1298.3 | 26.9 | 1297.8 | 1297.3 |
GSC | 1279.6 | 13.3 | 1279.8/1277.1 | 1278.7 | |
γOCH3′ | ASC | 1182.9 | 149.0 | 1198.2/1195.2 | 1194.7 |
GSC | 1145.5 | 7.2 | 1157.7 | 1153.0 | |
νC–O | ASC | 1166.3 | 189.4 | 1182.5 | 1179.6 |
GSC | 1153.8 | 250.1 | 1168.5/1164.6/1161.5 | 1166.8 | |
νN–Cas | ASC | 1165.5 | 19.7 | 1182.5 | 1179.6 |
GSC | 1195.6 | 201.1 | 1210.2/1204.1 | 1204.8 | |
γCH3″(1) | ASC | 1146.1 | 77.6 | 1155.6 | 1153.0 |
GSC | 1147.0 | 35.8 | 1153.4 | 1155.6 | |
γOCH3″ | ASC | 1144.5 | 1.5 | 1148.5 | 1152.2 |
GSC | 1179.7 | 6.6 | 1188.8 | Non obs. | |
γCH3″(2) | ASC | 1089.7 | 7.0 | 1096.9 | 1095.0 |
GSC | 1093.3 | 5.1 | 1098.3 | 1098.7 | |
νC–N | ASC | 1067.7 | 95.4 | 1076.6/1074.3 | 1076.7 |
GSC | 1060.3 | 74.9 | 1069.9/1065.5 | 1068.8 | |
γCH3′(2) | ASC | 1046.7 | 12.5 | 1052.5/1050.3 | 1051.6 |
GSC | 1039.1 | 18.2 | 1046.7/1044.9 | 1044.5 | |
νO–C | ASC | 974.2 | 21.6 | 998.3/995.6/994.3 | 991.9 |
GSC | 984.7 | 4.0 | 1002.1 | 999.8 | |
γCH2 | ASC | 960.8 | 15.1 | 967.3/965.5/963.8 | 966.9 |
GSC | 975.3 | 10.7 | 982.4/980.3/977.4 | 980.7 | |
νCC | ASC | 863.4 | 6.0 | 879.4 | 879.7 |
GSC | 883.6 | 9.4 | 897.9/895.5 | 897.8 | |
νN–Cs | ASC | 820.6 | 3.6 | 839.7/835.2 | 836.8 |
GSC | 845.1 | 32.0 | 860.0/856.9 | 859.8 | |
δOCO | ASC | 689.2 | 27.0 | 710.5/705.2 | 704.9 |
GSC | 703.3 | 6.7 | 713.1 | 714.8 | |
γC![]() | ASC | 567.6 | 4.2 | 576.4 | 573.9 |
GSC | 587.1 | 7.2 | 593.8 | 594.5 | |
δCC![]() | ASC | 471.9 | 3.2 | 483.9 | 486.1 |
δN(CH3)2 | GSC | 475.4 | 0.2 | 483.9 | 486.1 |
Approximate description | Conformer | Calculated frequency | Observed frequency | ||
---|---|---|---|---|---|
Amorphous (T![]() ![]() | Annealed amorphousb | Liquid (room temperature) | |||
a Frequencies in cm−1; ν, bond stretching, δ, bending, γ rocking, ω wagging, tw, twisting, τ torsion. See Supplementary material (Tables S3–S5) for definition of symmetry coordinates, full set of calculated frequencies and intensities and PED.1b Annealing was carried out by performing three heating/cooling cycles in between 9 and 154 K. | |||||
νOCH3as′ | ASC | 3087.0 | 3021.7 | 3026.7 | |
GSC | 3053.4 | 2990.5 | 2998.7 | 2979.2 | |
νOCH3as″ | ASC | 3053.9 | 2990.5 | 2979.2 | |
GSC | 3086.2 | 3021.7 | 3024.6/3019.9 | 3026.7 | |
νCH3as″(2) | ASC | 3017.7 | 2968.8 | 2953.6 | |
GSC | 3062.4 | 2990.5 | 3009.0/3003.4 | 2979.2 | |
νCH3as″(1) | ASC | 3015.2 | 2968.8 | 2953.6 | |
GSC | 3030.7 | 2990.5 | 2986.6 | 2979.2 | |
νCH2as | ASC | 2994.3 | Non obs. | Non obs. | |
GSC | 2997.9 | Non obs. | Non obs. | Non obs. | |
νOCH3s | ASC | 2983.2 | 2936.0 | 2936.9 | |
GSC | 2982.8 | 2953.7 | 2954.1 | 2953.6 | |
νCH3as′(2) | ASC | 2982.5 | 2936.0 | 2936.9 | |
GSC | 2988.0 | 2953.7 | 2960.6 | 2953.6 | |
νCH3as′(1) | ASC | 2982.0 | 2936.0 | 2936.9 | |
GSC | 2848.4 | 2822.6/2794.7 | 2852.5/2845.2/2832.2/2819.7/2800.2 | 2826.8/2795.1 | |
νCH2s | ASC | 2959.5 | 2913.5 | 2906.1 | |
GSC | 2832.4 | 2739.6 | 2745.8/2731.5 | 2737.9 | |
νCH3s(1) | ASC | 2913.0 | 2871 | 2872.6 | |
GSC | 3006.0 | 2953.7 | 2967.5 | 2953.6 | |
νCH3s(2) | ASC | 2906.5 | 2871 | 2872.6 | |
GSC | 2836.9 | 2773.9 | 2774.3/2767.8 | 2774.9 | |
νC![]() | ASC | 1752.3 | 1739.8 | 1739.6 | 1739.3 |
GSC | 1768.4 | 1757.8/1749.2 | 1753.8/1746.6 | 1756.0/1749.9 | |
δCH3as″(1) | ASC | 1493.8 | 1483.9 | 1480.9 | |
GSC | 1478.7 | Non obs. | 1477.4 | 1475.4 | |
δCH3as″(2) | ASC | 1480.1 | Non obs. | Non obs. | |
GSC | 1463.0 | 1468.5 | 1463.3 | 1472.2 | |
δOCH3as′ | ASC | 1465.1 | Non obs. | 1472.2 | |
GSC | 1451.1 | 1437.5 | 1436.7/1435.3 | 1436.1 | |
δCH3as′(1) | ASC | 1457.3 | 1448.8 | 1451.3/1448.0 | 1448.0 |
GSC | 1473.6 | 1467.9 | 1471.8 | 1472.2 | |
δOCH3as″ | ASC | 1450.8 | Non obs. | 1456.8 | |
GSC | 1465.4 | 1458.5 | 1463.3 | 1456.8 | |
δCH3as′(2) | ASC | 1445.8 | 1429.3 | 1436.1 | |
GSC | 1454.5 | 1442.7 | 1443.7/1441.2 | 1436.1 | |
δCH3s(1) | ASC | 1441.4 | 1429.3 | Non obs. | |
GSC | 1447.2 | Non obs. | Non obs. | Non obs. | |
δOCH3s | ASC | 1435.7 | 1409.9 | 1413.1 | |
GSC | 1437.5 | 1417.3 | 1423.0 | 1416.3 | |
δCH2 | ASC | 1411.2 | 1409.9 | 1413.1 | |
GSC | 1424.0 | 1417.3 | 1412.0 | 1416.3 | |
δCH3(2) | ASC | 1409.3 | Non obs. | 1405.0 | |
GSC | 1409.9 | Non obs. | 1406.4 | 1405.0 | |
ωCH2 | ASC | 1346.7 | 1356.8 | 1361.4 | |
GSC | 1374.8 | 1379.6 | 1390.9/1385.3/1379.6 | 1380.2 | |
twCH2 | ASC | 1325.3 | 1329.1 | 1326.3 | |
GSC | 1285.6 | 1288.7 | 1287.8/1283.8 | 1286.8 | |
γCH3′(1) | ASC | 1298.3 | 1299.2 | 1286.8 | |
GSC | 1279.6 | 1277.3 | 1276.4 | 1276.0 | |
γOCH3′ | ASC | 1182.9 | 1201.9 | 1204.7 | |
GSC | 1145.5 | Non obs. | Non obs. | Non obs. | |
νC–O | ASC | 1166.3 | 1183.4 | 1180.5 | |
GSC | 1153.8 | 1171.1 | 1172.9/1171.1/1163.6 | 1167.6 | |
νN–Cas | ASC | 1165.5 | 1183.4 | 1183.5 | |
GSC | 1195.6 | 1209.4 | 1209.4/1204.1 | 1204.7 | |
γCH3″(1) | ASC | 1146.1 | 1137.0 | 1137.1 | |
GSC | 1147.0 | 1155.0 | 1154.5 | 1151.7 | |
γOCH3″ | ASC | 1144.5 | Non obs. | Non obs. | |
GSC | 1179.7 | Non obs. | 1187.4 | Non obs. | |
γCH3″(2) | ASC | 1089.7 | 1097.1 | 1095.9 | 1099.6 |
GSC | 1093.3 | 1101.2 | 1104.7/1103.4/1099.1 | 1103.7 | |
νC–N | ASC | 1067.7 | 1075.9 | 1075.9 | 1072.0 |
GSC | 1060.3 | 1060.5 | 1071.4/1063.3 | 1064.9 | |
γCH3′(2) | ASC | 1046.7 | 1051.2 | 1052.4 | |
GSC | 1039.1 | 1045.1 | 1048.3/1042.9/1037.3 | 1044.1 | |
νO–C | ASC | 974.2 | 989.2 | 990.2 | |
GSC | 984.7 | 1015.7 | 1007.1 | 1015.9 | |
γCH2 | ASC | 960.8 | 968.5 | 970.2 | |
GSC | 975.3 | 981.6 | 981.4/980.1/973.9 | 978.6 | |
νCC | ASC | 863.4 | 881.62 | 876.8 | |
GSC | 883.6 | 899.2 | 900.4 | 894.0 | |
νN–Cs | ASC | 820.6 | 841.4 | 839.6 | |
GSC | 845.1 | 859.2 | 871.3/861.2/857.3 | 856.3 | |
δOCO | ASC | 689.2 | 707.3 | 715.8 | |
GSC | 703.3 | 717.0 | 724.3/777.0 | 738.0 | |
γC![]() | ASC | 567.6 | 578.2 | 594.9/594.5 | |
GSC | 587.1 | 597.6 | 606.5/597.6 | 594.9/594.5 | |
δCC![]() | ASC | 471.9 | 486.1 | Not studied | |
δN(CH3)2 | GSC | 475.4 | 486.1 | 486.1 | Not studied |
Infrared spectra of DMG-Me in both argon and xenon matrices obtained by co-deposition of the vapour of the compound and the matrix-gas were obtained as described in the Experimental section. Different temperatures of the valve nozzle and of the cold substrate of the cryostat were used. From the whole set of experiments on the matrix-isolated compound the following main conclusions could be extracted:
(i) Two different conformers of DMG-Me contribute to the observed spectra in both argon and xenon matrices. Comparison of the experimental data with the theoretically predicted spectra (Fig. 3) revealed that the two conformers observed experimentally are the ASC and GSC forms, i.e., the two lowest energy forms predicted by the calculations. Full assignment of the observed matrix spectra is presented in Table 2. In general, the calculated (scaled) spectra fit nicely the experimental data. The assignments to individual conformers were facilitated by the temperature dependence exhibited by the intensity of the bands, both upon annealing and changing the temperature of the vapour prior to deposition.
(ii) In consonance with the theoretical predictions, in the gaseous phase the ASC conformer was found to be the ground conformational state. Indeed, increasing the temperature of the valve nozzle led to increasing the relative population of the less stable GSC conformer. This is clearly illustrated in Fig. 4 which compares the spectra obtained for DMG-Me in argon using two different valve nozzle temperatures (25 and 200°C). The spectral regions shown correspond to those where the νC
O, νC–C and νN–C sym stretching modes are predicted to occur in both conformers; the figure also shows the calculated spectra for the two forms, for comparison. Note that the observed features exhibit site splitting. Matrix site splitting was found to be more pronounced in argon than in xenon (see Table 2). This result may indicate that in argon the solute molecules are not allowed to relax so efficiently as in xenon in order to adjust themselves as best as possible to fit the matrix packing requirements.
The band at ca. 1740 cm−1 in the νCO stretching region (Fig. 4) deserves a further comment. This band increases in intensity with the nozzle temperature. Since both AAC and GSkC conformers (the third and fourth more stable conformers of DMG-Me) are predicted to give rise to a νC
O band at a lower frequency than both ASC and GSC forms, this band could then be assigned to these conformers. However, there is no further experimental evidence of the presence of either AAC or GSkC in the matrices and the assignment of this band to the first overtone of the νC–C stretching vibration of the GSC form, whose fundamental appears at ca. 895 cm−1
(Table 2), seems to be more plausible.
(iii) Annealing of the matrices (both argon and xenon) led to partial conversion of the ASC conformer into the GSC form (Fig. 5). This result indicates that in the matrices the order of stability of the two conformers changes relatively to the gaseous phase, the GSC conformer becoming the ground conformational state. The GSC conformer has a larger dipole moment than the ASC form (1.99 vs. 1.40 D; see Fig. 1) and thus it could be expected to be stabilized in the matrices with regard to the gaseous phase. Nevertheless, this molecule is a remarkable example of a system showing an inversion in the order of its lowest energy conformational states due to a relatively minor perturbation by the media, such as that due to the inert gas matrix.
(iv) The relative populations of the ASC and GSC conformers observed in argon and xenon matrices prepared using the same experimental conditions (valve nozzle and substrate temperatures; concentration; matrix-gas flux) were found to differ considerably, with the GSC form showing a larger relative population in xenon than in argon (see Fig. 3). This is in consonance with the known better trapping ability of argon when compared with xenon or, in other words, with the generally greater conformational cooling effects observable when xenon is used as the matrix gas.12,22 Note that in the present case, the consequences of a more important conformational cooling effect in xenon are different from the usually observed phenomena when the conformational ground state is the same in both the gaseous phase and in the matrices. In the trivial situation, the most abundant conformer in the gas phase has its relative population further increased in the xenon matrix due to the conformational cooling; in DMG-Me, due to the inversion of the relative stability of the two conformational states, the most abundant conformer in the gaseous phase has its relative population decreased in the xenon matrix due to the conformational cooling.
The spectrum of the low temperature amorphous layer obtained by deposition of the vapour of the compound onto the cold substrate of the cryostat (at 9 K) does also reveal the presence of both ASC and GSC conformers. This spectrum is compared with the calculated spectra for the two forms in Fig. 6. Assignments are presented in Table 3. Fig. 6 also shows the difference spectrum obtained by subtracting from the spectrum of the annealed (T=
154 K) amorphous layer the spectrum of the freshly prepared amorphous (T
=
9 K) layer. In the difference spectrum, the bands pointing upwards are due to the GSC conformer, while those pointing to the bottom belong to the ASC form. Hence, annealing the amorphous layer to higher temperatures leads to increase the population of the GSC conformer relatively to ASC. Upon reaching 154 K, the sample was cooled again to 9 K without observation of any substantial change in the spectrum. However, the subsequent rewarming of the sample further increases the relative population of the GSC conformer, in such a way that the bands due to ASC practically vanish (see spectrum d, in Fig. 6). These results can be interpreted as follows: upon deposition of the vapour into the cold substrate, the conformers present in the gaseous phase are frozen, contributing to the spectrum of the freshly prepared amorphous layer; annealing of the sample enables the molecules of the compound to relax and attain the conformation that is most stable under these conditions, which corresponds to the most polar GSC conformer; on cooling, no changes occur, but, when subjected to a new warming cycle, the sample can further relax and attain a quasi-crystalline state, where almost all molecules assume the GSC conformation.
In the liquid state spectra at room temperature (spectrum a, in Fig. 6), features due to the two conformers can also be clearly identified. Indeed, the spectrum of the liquid closely resembles that of the amorphous state (trace b, in Fig. 6). It is, however, easily noticed that the population of the GSC conformer is higher in the room temperature liquid than in the freshly prepared amorphous layer. For example, the carbonyl stretching band appears as a doublet in both spectra, with the higher frequency component, ascribable to the GSC form, being more intense than the lower component band in the spectrum of the liquid, while the opposite situation occurs in the spectrum of the amorphous layer. Since the amorphous results from the frozen vapour of the compound and in the gaseous phase ASC is the most stable form, whereas in the liquid phase the more polar GSC form is the minimum energy conformer, the observed data can be easily understood.
The temperature dependence of the carbonyl stretching bands is presented in Fig. 7. Since the ASC form is the higher energy conformer of DMG-Me in the liquid, its relative population must increase relatively to that of the GSC conformer upon increasing the temperature. Accordingly, the intensity of the band appearing at ca. 1740 cm−1, ascribed to ASC increases with temperature relatively to that due to the same mode in the GSC form, which is observed at ca. 1750 cm−1. The integrated intensities of the νCO bands due to each conformer were obtained after being subjected to deconvolution (see Fig. 7) and from these a Van't Hoff plot of ln(IASC/IGSC)
vs. the reciprocal temperature was obtained (Fig. 8), yielding an enthalpy difference between the conformers in the liquid phase of 5.13 kJ mol−1, favouring the GSC form This value may be compared with the theoretical value obtained for the gas: ca. 3 kJ mol−1, favouring the ASC form. Hence, a stabilization of ca. 8 kJ mol−1 of the more polar GSC conformer relative to the ASC form occurs upon going from the gas phase to the liquid state due to intermolecular interactions (dipolar interactions are certainly the prevalent effects). With all probability, a similar stabilization of the GSC form relative to the ASC conformer should also occur in the case of the amorphous solid state.
Taking into consideration the theoretically predicted spectra for the two experimentally observed conformers and the different experiments undertaken (e.g., temperature variation studies in different conditions; change of matrix gas, valve nozzle and of deposition temperatures) full assignment of the spectra obtained for the compound in the various phases studies could be made successfully.
Footnotes |
† Electronic supplementary information (ESI) available: calculated geometries and rotational constants for the most stable conformers of dimethylglycine methyl ester. See http://www.rsc.org/suppdata/cp/b2/b209311c/ |
‡ Calculated geometries and rotational constants for the higher energy conformers are available from the corresponding author upon request. |
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