Jozef
Lengyel
,
Milan
Ončák
,
Andreas
Herburger
,
Christian
van der Linde
and
Martin K.
Beyer
*
Institut für Ionenphysik und Angewandte Physik, Universität Innsbruck, Technikerstraße 25, 6020 Innsbruck, Austria. E-mail: martin.beyer@uibk.ac.at
First published on 6th September 2017
We present infrared multiple photon dissociation (IRMPD) spectra of (H2O)nO˙− and (H2O)nOH− cluster ensembles for ≈ 8 and 47 in the range of 2400–4000 cm−1. Both hydrated ions exhibit the same spectral features, in good agreement with theoretical calculations. Decomposition of the calculated spectra shows that bands originating from H2O⋯O˙− and H2O⋯OH− interactions span almost the whole spectral region of interest. Experimentally, evaporation of OH˙ is observed to a small extent, which requires interconversion of (H2O)nO˙− into (H2O)n–1OH˙OH−, with subsequent H2O evaporation preferred over OH˙ evaporation. The modeling shows that (H2O)nO˙− and (H2O)n–1OH˙OH− cannot be distinguished by IRMPD spectroscopy.
In contrast to the extensive literature on the IR spectroscopy of (H2O)nOH−, we have found only one IR spectrum of (H2O)nO˙− clusters in the literature, for n = 20, reported by Johnson and co-workers.22 There is, to the best of our knowledge, no comprehensive study on the (H2O)nO˙− cluster ions available in the literature. One of the reasons could be the instability of the O˙− ion in water clusters and formation of OH˙OH− in reaction with water. Ab initio calculations on small clusters23 have shown that O˙− and OH˙OH− have similar stability. In bulk water, O˙− is predicted to be the more stable isomer,24,25 in contrast to previous experiments that favored OH˙OH−.26Ab initio molecular dynamics of the reaction between N2O and sodium doped water clusters, Na(H2O)15, yielded O˙− formation mediated by a hydrated electron,27 with a subsequent reaction to produce the OH˙OH− pair on the picosecond timescale.
In this work, we combine Fourier transform ion cyclotron resonance (FT-ICR) mass spectrometry and IRMPD spectroscopy with DFT calculations to study the nature of the interaction between O˙−/OH− anions and water molecules. First, we discuss details of the hydrated ions structure by interpretation of the IRMPD spectra; second, we investigate the conversion of O˙− into OH˙OH−, which is evidenced via the evaporation of OH˙.
(H2O)nO˙− and (H2O)nOH− clusters are initially produced in two broad size distributions with mean cluster sizes of ≈ 8 and
≈ 47. The environment is at room temperature, while the clusters have an internal temperature of about 100 K, as established in calorimetric experiments by von Issendorff and co-workers.34 At each studied wavelength, a mass spectrum was taken after irradiating all clusters simultaneously, followed by recording a mass spectrum without laser irradiation. Following the approach described by Prell, O’Brien and Williams for size-selected water cluster,35 this allowed to quantify the contribution of blackbody infrared radiative dissociation (BIRD)36–41 on cluster dissociation. These measurements also minimize the influence of fluctuations of the cluster size distribution.
Since we work with an ensemble of clusters over an extended size range, we cannot employ directly the equations presented by Williams and co-workers.35 Building on the differential equations derived for nanocalorimetry of cluster ensembles,29 we can describe the change in the average cluster size dN induced by IR laser irradiation as well as BIRD, eqn (1):
![]() | (1) |
For the practical evaluation of the absolute photodissociation cross section from the IRPD spectra, we use eqn (2), which was derived by integration of eqn (1) with and without the laser irradiation term. ΔN is the difference in the average cluster size without and with IR laser irradiation, but in both cases subject to BIRD during the irradiation time t in the ICR cell. In this analysis, the cross section σ is assumed to be independent of cluster size, which is an approximation.
![]() | (2) |
IR spectra and reaction energies were modelled at the B3LYP/TZVP level of theory, with Grimme's D2 dispersion correction.43 For each cluster type, (H2O)nO˙−, (H2O)n−1OH˙OH−, (H2O)nOH−, and for n = 6–11, 15 different isomers were optimized from various starting structures (i.e. 270 isomers in total). All found structures represent local minima and their energies lie within 30 kJ mol−1 with respect to the most stable structure found. This sampling approach was picked as molecular dynamics had the tendency to remain in one part of the potential energy surface, not sampling efficiently the conformational space. Vibrations were calculated within the harmonic approximation and analyzed according to their type by calculating projection onto normal modes. For this purpose, an O–H bond is defined when r(O–H) < 1.3 Å, a hydrogen bond between OdonH⋯Oacc when r(Oacc–H) < 2.5 Å and α(Odon–H–Oacc) > 120°. Vibrations were scaled by 0.96 to reproduce the position of the free OH vibration (∼3700 cm−1). The final spectra were modeled as an arithmetic average of IR spectra of individual isomers. The spectra were broadened by Lorentzian functions with the full width at half maximum of 40 cm−1; this value was selected so that the final spectrum has neither a too pronounced structure nor it becomes too blurred. At the same time, the free OH vibration is well distinguishable in the total spectrum. Zero point energy corrections are included in all reported reaction energies. All calculations were performed in the Gaussian 09 program package,44 the respective local minima are provided in the ESI.†
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Fig. 1 Experimental IRMPD spectrum of (H2O)nO˙− and (H2O)nOH− cluster ions, ![]() |
From previous studies of neutral water clusters,45–47 we can assign the broad absorption feature (3000–3600 cm−1) with a maximum around 3450 cm−1 to the O–H stretching vibrations of water molecules that are hydrogen bonded in the cluster. A sharp and, at least for the larger clusters, well-separated free O–H stretch near 3700 cm−1 is attributed to water molecules on the cluster surface. The measured absorption bands are very similar to those for amorphous water clusters46,47 that were described in detail by theoretical calculations of Buch and co-workers.45
For the current work, the 2450–2900 cm−1 region is of main interest. Here, the observed absorption signal behaves qualitatively similar for both larger and smaller clusters, a weak absorption without pronounced structure is observed. A previous study on small (H2O)nOH− clusters15 suggested that this signal originates from the hydrogen bonds of water molecules to the anion. For larger clusters, water–water interaction in the vicinity of the ion might also contribute. If one assumes that the chromophore responsible for this feature, i.e. the hydrated ion, is the same regardless of cluster size, also the absolute cross sections should be the same. This is obviously not the case, the cross sections averaged over 2450–2900 cm−1 are a factor of 2.7 larger for the ≈ 47 clusters. However, since the absolute cross sections depend sensitively on the overlap of the laser beam with the ion cloud, we cannot rule out that the
≈ 8 clusters were irradiated with significantly fewer photons. A possible reason for this could be the storage period of 8 s before irradiation started to allow the clusters to shrink to the desired size due to BIRD. Since the signal was relatively intense, space charge effects over this period lead to spatial expansion of the ion cloud, which in turn would lead to reduced overlap with the laser beam. We therefore evaluated the total oscillator strength of the O–H stretching modes in the two cluster distributions, which is proportional to the integral of the absorption spectrum from 2400 to 4000 cm−1. We obtain a factor of 15.2 for the ratio of the two integrals, while the size ratio is 47/8 = 5.9. However, if we scale the
≈ 8 spectrum by the factor of 2.7 obtained above, the ratio of the two integrals reduces to 5.6, close to the expected 47/8 ratio. We therefore conclude that the intensity of the
≈ 8 spectrum in Fig. 2a is too low. If we multiply the intensities in Fig. 2a by 2.7, see scale bar on the right, the theoretical values in Fig. 2b–d are still a factor of 6.2 too high. Given the approximations that enter the calculation of IR absorption cross sections in quantum chemistry, however, this agreement seems acceptable. Another potential source of error in the experimental cross sections is the neglect of infrared emission following absorption of an IR laser photon. In eqn (1), we assume that the absorbed laser photons contribute fully to water evaporation, which is probably an oversimplification. IR emission will become more and more relevant with the decreasing cluster size, which could also explain the discrepancy between the
≈ 47 and
≈ 8 absorption cross sections. However, for a precise comparison between experiment and theory and for a fully reliable determination of experimental absorption cross sections, detailed master equation modeling of BIRD and IR laser irradiation will be required.
Theoretical calculations of IR spectra (Fig. 2b and c) provide further evidence that the IR intensity in the 2450–2900 cm−1 region is induced by the presence of O˙− or OH− anions. Both calculated spectra have similar shape and reproduce well the experimental data. Spectra of O˙− clusters exhibit a slightly lower relative intensity in the 2400–2700 cm−1 region compared to OH− clusters; this difference, however, might be due to the limitations of the modeling approach.
Decomposition of the calculated IR spectra of hydrated O˙− and OH− ions into various interaction types shows that the water–water interaction fingerprint is located in the broad region starting already at about 2400–2600 cm−1, with a strong increase in intensity for higher wavenumbers. However, we can expect that the intensity in the 2400–2900 cm−1 region is induced mainly by the presence of the anion; neutral water clusters do not show any absorptions in this wavelength region, indicating that these contributions come from water–ion interactions as well as water–water interactions in the vicinity of the anion.45,48 For larger clusters, the intensity in the 2400–2900 cm−1 region will thus diminish relative to the intensity in the 3000–3600 cm−1 region, as discussed above. The region comprising interaction of water molecules with the solvated ions (OH−, O˙−) spreads among the whole 2400–3600 cm−1 region, with about similar intensity. For (H2O)nOH−, n = 1–5, the broad weak continuum absorption over the whole spectrum, 2450–3800 cm−1, was interpreted by Niedner-Schatteburg and co-workers14 as a rapid interconversion of cluster isomers. This is in agreement with our calculations as single isomers exhibit sharp peaks in the 2400–3000 cm−1 region and spectral broadening is gained by averaging. Note also that the IR spectra in Fig. 2 were calculated using a local minima approach. Therefore, the spectrum broadening arises due to the presence of different isomers; the absorption below 3000 cm−1 can be explained without invoking a mobile proton as suggested by Johnson and co-workers for protonated water clusters,49 but this does not rule out its presence in the current experiments.
Thus, the absorption intensity in the 2400–2800 cm−1 region can be attributed mainly to the signal induced by the presence of O˙−/OH− ion in the cluster while both ion-water and water–water interactions are present for higher frequencies. Finally, the free O–H vibration is located at about 3700 cm−1; this characteristic peak was used to choose the scaling factor of the calculated vibrational spectra (see Methods section).
Besides the O˙− isomer considered above, the (H2O)nO˙− clusters can also undergo the proton transfer reaction (3), forming the (H2O)n−1OH˙OH− structure which might be formed in two forms, with OH moieties forming contact or solvent separated pairs. In our calculations, these two forms have almost the same occurrence.
(H2O)nO˙− → (H2O)n−1OH˙OH− | (3) |
In agreement with an ab initio study on small (H2O)nO˙− and (H2O)n−1OH˙OH− clusters, n = 1–5,23 our calculations at the B3LYP+D2/TZVP level show that for n = 6–11, both isomers lie close in energy (within 7 kJ mol−1, see Table 1). However, while calculations on small clusters found that (H2O)nO˙− are generally preferred, no clear trend is seen in our case.
Reaction | n | |||||
---|---|---|---|---|---|---|
6 | 7 | 8 | 9 | 10 | 11 | |
(H2O)nO˙− → (H2O)n−1OH˙OH− | −2.0 | 0.5 | 1.6 | 2.9 | −1.8 | −6.4 |
(H2O)nO˙− → (H2O)n−1O˙− + H2O | 64.5 | 49.7 | 56.9 | 50.4 | 54.8 | |
(H2O)nO˙− → (H2O)n−1OH− + OH˙ | 72.5 | 56.9 | 63.3 | 58.5 | 55.4 | |
(H2O)nOH− → (H2O)n−1OH− + H2O | 65.3 | 50.5 | 55.1 | 58.0 | 45.6 |
The presence of the OH˙OH− isomer in the current experiment can be deduced directly from OH˙ evaporation. If the OH˙OH− motif is present, loss of the OH˙ radical, reaction (4), competes with loss of H2O, reaction (5).
(H2O)nOH˙OH− → (H2O)nOH− + OH˙ | (4) |
(H2O)nOH˙OH− → (H2O)n−1OH˙OH− + H2O | (5) |
Under the present experimental conditions, IR irradiation of (H2O)nO˙− and (H2O)nOH− cluster ions with ≈ 47 at the absorption maximum leads to evaporation of about 10 water molecules per second (see Fig. S1 in the ESI†). If the OH˙ radical is evaporated, the ratio of (H2O)nO˙−
:
(H2O)nOH− abundance in the mass spectrum decreases. Fig. 3 documents the change of normalized intensities of (H2O)nO˙− ions after IR irradiation with respect to BIRD, calculated viaeqn (6).
![]() | (6) |
![]() | ||
Fig. 3 Change of the normalized intensity of (H2O)nO˙− cluster ions for the size of ![]() |
The decrease in (H2O)nO˙− intensity starts to appear in the region of high absorption cross section of the OH stretches and matches well with the IRMPD spectrum of the corresponding clusters from 2900 cm−1 to 3700 cm−1. The OH˙ radical evaporation induced by IRMPD, i.e. corrected for BIRD effects, takes place in the absorption region, with the average decrease of (H2O)nO˙− intensity reaching 2% at the absorption maximum.
By analyzing the relative probability of OH˙ dissociation with respect to H2O dissociation, we can estimate the difference in activation energy for evaporation of OH˙ and H2O. We assume that the (H2O)n−1OH˙OH− isomer is exclusively present and consider that there are on average 46 water molecules per OH˙. Within dissociation of 10 H2O molecules, there is a probability of 2% to dissociate an OH˙ radical. Then, we obtain the following ratio between the rates kOH˙ and kH2O (see ESI† for details):
![]() | (7) |
![]() | (8) |
Table 1 summarizes reaction energies of H2O and OH˙ dissociation calculated for n = 7–11. OH˙ dissociation is consistently higher in energy than H2O dissociation, in agreement with experiment. OH˙ dissociation requires about 61 kJ mol−1, dissociation of a water molecule from both (H2O)nO˙− and (H2O)nOH− clusters has comparable energy of about 55 kJ mol−1. The difference between OH˙ and H2O dissociation can be tentatively assigned to the electronic structure of the radical causing subtle differences in the strength of the hydrogen bond.
Fig. 3 shows that the OH˙OH− isomer is formed prior to evaporation, but it does not reveal when it is formed. Reaction (3) might proceed quantitatively directly after O˙− formation, but there may as well be an equilibrium between the almost isoenergetic O˙− and OH˙OH− ions, with rapid interconversion in both directions. It is interesting to note that during the course of the geometry optimization, interconversion between O˙− and OH˙OH− was occasionally observed. This indicates that the equilibrium between the isomers depends on the topology of the hydrogen bonded network, rather than on the presence of O˙− or OH˙OH− in the starting geometry. The ongoing making and breaking of hydrogen bonds in the clusters stored in the ICR cell and exposed to room temperature black-body radiation might thus induce the isomerization between O˙− and OH˙OH−.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c7cp04577h |
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