Tanja
Bauer
a,
Robert
Stepic
b,
Patrick
Wolf
c,
Fabian
Kollhoff
a,
Weronika
Karawacka
a,
Christian R.
Wick
d,
Marco
Haumann
c,
Peter
Wasserscheid
cf,
David M.
Smith
de,
Ana-Sunčana
Smith
b and
Jörg
Libuda
*af
aLehrstuhl für Physikalische Chemie II, Friedrich-Alexander-Universität Erlangen-Nürnberg, Egerlandstraße 3, D-91058 Erlangen, Germany. E-mail: joerg.libuda@fau.de
bPULS Gruppe, Lehrstuhl für Theoretische Physik I, Friedrich-Alexander-Universität Erlangen-Nürnberg, Nägelsbachstraße 49b, D-91052 Erlangen, Germany
cLehrstuhl für Chemische Reaktionstechnik, Friedrich-Alexander-Universität Erlangen-Nürnberg, Egerlandstraße 3, D-91058 Erlangen, Germany
dRuđer Bošković Institute, Bijenička cesta 54, P.P. 180, HR-10002 Zagreb, Croatia
eComputer Chemie Centrum, Friedrich-Alexander-Universität Erlangen-Nürnberg, Nägelsbachstraße 25, 91052 Erlangen, Germany
fErlangen Catalysis Resource Center and Interdisciplinary Center Interface-Controlled Processes, Friedrich-Alexander-Universität Erlangen-Nürnberg, 91058 Erlangen, Germany
First published on 28th November 2017
Ru-based supported ionic liquid phase (SILP) systems efficiently catalyze the low-temperature water-gas shift reaction (WGSR). While previous studies suggest that Ru-carbonyl species play an important role in the mechanism, detailed knowledge on the catalytically active species is still missing. To identify these carbonyl complexes, we apply in situ diffuse reflectance infrared Fourier transform spectroscopy (DRIFTS) in combination with density functional theory (DFT). Investigations of an as-prepared [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/Al2O3 catalyst indicate splitting of the dimer induced by Cl−. Subsequently, an equilibrium between several [Ru(CO)xCly]n species is established, in which the IL serves as an effectively infinite Cl− reservoir. We find that the major species in the system freshly-prepared from [Ru(CO)3Cl2]2 is indeed [Ru(CO)3Cl3]−. A smaller amount of [Ru(CO)2Cl3]− and chloride-rich species [Ru(CO)2Cl4]2− or [RuCOCl4]2− are also found in the SILP. Similar Ru-carbonyl species are observed during carbonylation of RuCl3/[C4C1C1Im]Cl/Al2O3, another potential WGSR catalyst. The response of [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/Al2O3 to heating and/or CO dosing was probed in situ and the results confirm the presence of the equilibrium proposed above.
Interestingly, spectroscopic ex situ analysis of a used RuCl3/[C4C1C1Im][OTf]/Al2O3 sample indicated the presence of Ru-carbonyl species. This finding suggests that new [Ru(CO)xCly]n complexes with enhanced catalytic activity are formed during the induction period of the WGS reaction itself.9 Indeed, the desired activity and selectivity was achieved without an induction period when [Ru(CO)3Cl2]2/[C4C1C1Im][OTf]/Al2O3 was used as a catalyst.10 However, these studies did not reveal the exact nature of the catalytically active carbonyl complex. Thus, the following questions still remain unanswered to date: a) what is the exact nature and concentration of the carbonyl species present in the SILP WGSR system? b) Which of the present species shows the highest catalytic activity (in terms of TON and TOF)? It is obvious that only if the most active carbonyl complex is also the most abundant one in the SILP system under reaction conditions, the activity of the resulting SILP catalyst system it at its maximum.
The present study addresses mainly the first question and elucidates the existence and amount of different [Ru(CO)xCly]n species in two representative SILP systems: RuCl3/[C4C1C1Im]Cl/Al2O3 and [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/Al2O3. For this purpose, we use in situ infrared (IR) spectroscopy, a particularly powerful tool in metal carbonyl chemistry. In combination with density functional theory (DFT) calculations, this approach allows us to identify the nature of the carbonyl complexes by careful analysis of the CO stretching frequency region. Previously, even the nature of intermediates could be identified by transient IR spectroscopy.11 In this work, we aim at a detailed understanding of the species which are present during the reaction. In contrast to earlier studies,10 we utilize here 1-butyl-2,3-dimethylimidazolium chloride ([C4C1C1Im]Cl) as the IL, because the enhanced chloride content has been shown to further enhance the activity. In particular, we focus on the influence of the IL upon preparation of the active catalyst, as well as on the effects of temperature and CO on the speciation in the active catalysts.
Transmission infrared spectroscopy (TIRS) measurements were either conducted with KBr pellets or using a KBr window as IR transparent support. The solutions were drop-cast onto a KBr window which, after evaporation of the solvent, was mounted in the sample compartment on a sample holder (Pike). Evacuation of the sample compartment leads to complete removal of the solvent. The acquisition time for TIR spectra was 1 min with a spectral resolution of 2 cm−1.
All diffuse reflectance infrared Fourier transform spectroscopy (DRIFTS) experiments were carried out in a home-built reactor system, which is described in detail elsewhere.12 Briefly, a high temperature reactor chamber and praying mantis diffuse reflectance accessory (both from Harrick) are placed in the sample compartment of the spectrometer. A home-built extension of the sample compartment, equipped with all necessary electrical and gas dosing feedthroughs, allows for keeping the complete optical path evacuated during the measurements. This maximizes the stability of the system, especially for long-term experiments. The reactor is equipped with CaF2 windows and a type K thermocouple directly contacting the examined sample, which provides excellent temperature control. Currently, the setup can be operated at pressures adjustable from 1 mbar to 20 bar using three pressure controllers (PCs). Up to five different gases can be dosed via mass flow controllers (Bronkhorst, MFCs). The setup can be operated in an automated way, which allows accurate programming of temperature, pressure and gas composition. In the CO (Linde, 4.7) dosing experiments the gas dosing (30 min, 1 bar, 20 mLN min−1) was followed by evacuation to 1 mbar for 1 min and, finally, by purging with Ar (Linde 5.0, 15 min, 1 bar, 20 mLN min−1) at 1 bar. The two last steps result in efficient removal of the CO gas phase from the reactor. This procedure was carried out repeatedly, if required, at different temperatures. All DRIFT spectra were recorded using an acquisition time of 5 min and a spectral resolution of 2 cm−1.
In a first step, [C4C1C1Im]Cl was dissolved in high purity DCM (typically 30 mL) in a round-bottom Schlenk flask under Ar atmosphere. After stirring till complete dissolution of the IL (10–15 min at 25 °C), the Ru catalyst (either RuCl3 or [Ru(CO)2Cl3]2) was added followed by another stirring for 10 min. Subsequently, the γ-Al2O3 support was added and stirred quickly for 2–5 min. To avoid crushing of the particles due to mechanical stress, the stirrer bar was taken out before removal of the solvent in two steps (step 1: 3 h, 40 °C, 900 mbar; step 2: 1 h, 40 °C, <3 mbar) in a rotary evaporator. After solvent removal, free flowing SILP catalyst particles were obtained. The resulting catalyst has a Ru loading of wRu = 0.04 gRU gsupport−1 while the pore filling grade with IL is α = 0.34. The pore filling grade describes the IL volume related to the total pore volume of the support material (VILVsupport−1).
Ru species | Configuration | Peak center DFT [cm−1] | Peak center exp. [cm−1] | Δ(DFT–exp) [cm−1] | E rel [kJ mol−1] |
---|---|---|---|---|---|
[RuII(CO)3Cl2]2 | trans | 2107, 2040 | 2122, ∼2045 | −15, −5 | 0 |
[RuII(CO)3Cl2] | s.-pyr. cis | 2101, 2033 + 2025 | 2122, 2055 | −21, −26 | 0 |
[RuII(CO)3Cl2] | s.-pyr. trans | 2054, 2015 | 2040, 2002 | 14, 13 | 44 |
[RuII(CO)3Cl3]− | facial | 2063, 1983 | ∼2030, ∼1950 | ∼33, ∼33 | 0 |
[RuII(CO)3Cl3]− | meridial | 1972, 2003, 2091 | — | — | 39 |
[RuII(CO)2Cl3]− | s.-pyr. cis | 2010, 1939 | 2008, 1922 | 2, 17 | 0 |
[RuII(CO)2Cl3]− | s.-pyr. trans | 1943 | — | — | 123 |
[RuII(CO)2Cl4]2− | cis | 1969, 1893 | —, ∼1900 | —, ∼−7 | 0 |
[RuII(CO)2Cl4]2− | trans | 1894 | ∼1900 | ∼6 | 88 |
[RuIICOCl4]2− | s.-pyr. | 1862 | ∼1900 | ∼38 | |
[RuII(CO)4Cl2] | cis | (2149), 2086 + 2066, 2035 | 2140, 2078, — | 9, 8, — | 0 |
[RuII(CO)4Cl2] | trans | 2060 | — | — | 40 |
[Ru0(CO)3Cl2]2− | trig.-bipyr. cis | 1910, 1803, 1787 | — | — | 25 |
[Ru0(CO)3Cl2]2− | trig.-bipyr. trans | 1777 | — | — | 0 |
[RuII(CO)2(CO–OH)HCl3] | 2025, 1953, 1704, 1678 | (1780/1730) | — | 42 | |
[RuII(CO)2(CO–OH)Cl2] + HCl | 2117, 2013, 1944, 1728 | — | — | 0 |
Fig. 1 Reference TIR spectra for; a) the as-obtained [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/Al2O3 SILP system. The assignment is given for IL bands; b) [Ru(CO)3Cl2]2/[C4C1C1Im]Cl mixtures prepared with DCM. |
To further prove this hypothesis, we prepared [C4C1C1Im]Cl:[Ru(CO)3Cl2]2 mixtures (weight ratio 2:1 and 5:1) in DCM. The TIRS spectra are displayed in Fig. 1b. All spectra are normalized to the peak at 2030–2040 cm−1, therefore no scale bar is given. The freshly prepared 2:1 mixture (black curve) shows two features at 2122 and 2043 cm−1. Based on our DFT calculation we attribute these peaks to intact [Ru(CO)3Cl2]2.23,26 Previously, Tsuchiya et al. assigned these peaks to [Ru(CO)3Cl3]−,25 which, however, would not agree with our present DFT data. The more pronounced red-shift with respect to previously published IRAS data is attributed to the solvent effects due to the increased amount of IL.20 With increasing IL concentration in the 5:1 mixture (red curve), a small feature appears at 1950 cm−1 and the intensity of the peak at 2122 cm−1 decreases. Presumably, part of the [Ru(CO)3Cl2]2 dimer is at this stage already converted to [Ru(CO)3Cl3]−. The spectrum taken of the 5:1 mixture after 5 days (blue curve) follows this trend. No peak can be seen at 2122 cm−1, which indicates that the dimer species is completely consumed. In addition to the expected features of [Ru(CO)3Cl3]− (2032 and 1950 cm−1) a new peak is visible at 1908 cm−1. It most likely corresponds to chloride-rich, di-anionic species like, i.e., [Ru(CO)2Cl4]2− or [Ru(CO)Cl4]2−, which are formed by further CO/Cl− ligand-exchange reactions. Comparison with DFT data shows that the peak matches very well the calculated position for trans-[Ru(CO)2Cl4]2−, but this complex is energetically unfavorable (88 kJ mol−1). Its corresponding cis-isomer on the other hand should lead to two peaks. The calculated spectrum of [RuCOCl4]2− shows a single peak (1862 cm−1) and could therefore also be responsible for the feature at 1908 cm−1. This would then mean that a direct ligand substitution reaction from [Ru(CO)2Cl3]− to [RuCOCl4]2− takes place. Although no unambiguous assignment of all features can be made at the moment, we summarize that chloride-rich [Ru(CO)2Cl4]2− or [RuCOCl4]2− di-anions are formed from the dimer by sequential ligand substitution reactions. The two small features at 2008 and 1922 cm−1 can be assigned to an intermediate species cis-[Ru(CO)2Cl3]−.
For comparison, we extracted the Ru-species also from the fresh catalyst using DCM. The corresponding TIR spectra are included in Fig. 1b (in green). As expected, the spectrum obtained is similar to both the TIR spectra of the “intact” SILP (Fig. 1a) and the one obtained from the 5:1 mixture after 5 days in solution. This proves that the Cl−-induced splitting of the Ru-dimer observed without support material in solution also takes place during preparation of the SILP catalyst. We assume that the formation of monomers is a function of the IL concentration and time. As shown by the spectra of the catalyst after extraction, the Ru-carbonyls can be completely removed from the as-prepared SILP with the non-ligating solvent DCM. Therefore, one can conclude that all species are physically dissolved in the IL phase in the system.23
More detailed insight into the conversion of the dimer species to a variety of monomers in the chloride-containing IL can be gained by studying the transformation in situ. To this end, the 2:1 [C4C1C1Im]Cl:[Ru(CO)3Cl2]2 mixture was deposited on a KBr window and IR spectra were taken in vacuo every 30 min (∼1 mbar, air). The results are displayed in Fig. 2. As the features at 2047 and 2036 cm−1 lie quite close, they cannot be resolved for integration. The peak assigned to the dimer at 2121 cm−1 decreases linearly in time, while the peak related to [Ru(CO)3Cl3]− at 1951 cm−1 increases simultaneously. The integrated peak areas of the intermediate species [Ru(CO)2Cl3]− with peaks at 2009 and 1919 cm−1 increase more steeply in the first 480 min indicating that this complex forms more rapidly at the beginning. As previously observed, its amount is rather small throughout the experiment. The experiment shows the first stage of dimer splitting, therefore, no peak related to the di-anionic species is observed.
In order to prove that Cl− ions in the IL are responsible for the transformation of the dimer, we repeated the TIRS measurements with IL solutions providing lower Cl− concentration. First, a 1:1.2 mixture of [C4C1C1Im][OTf] and [C4C1C1Im]Cl was applied to prepare the solutions as described above. Second [C4C1C1Im][OTf] with no additional Cl−, apart from the intrinsic amount from [Ru(CO)3Cl2]2 was used. In contrast to the pure Cl− containing IL, the spectrum of the [OTf]−/Cl− mixture after 5 days (see Fig. 3a) shows a peak at 2125 cm−1 indicating that the dimer is indeed only partly split. In the spectra obtained from the pure [C4C1C1Im][OTf] solution no monomer peak at 1950 cm−1 is formed and the peaks of the dimer species around 2130 and 2056 cm−1 are present even after 5 days (see Fig. 3b). This proves that a smaller Cl− content is associated with a higher amount of intact dimer in the DCM solution. In the case of a chloride-free IL no transformation of [Ru(CO)3Cl2]2 takes place. Nevertheless, spectral changes are visible for the high frequency peak, which forms a shoulder at higher IL concentration. A closer look at the IL region of the spectra helps to understand these changes. Apart from the expected peaks at 1265, 1226, 1156 and 1036 cm−1, which were observed previously, additional weaker features form at 1203 and 1015 cm−1 over time. We attribute this behavior to ligand exchange with the [OTf]− anions themselves. In previous work it was already reported that in DCM solution Cl− at the RuII metal center can be substituted by [OTf]− ligands.27 Although the amount of [OTf]−-species in this previous study was very low (∼1%), the authors could obtain a crystal structure of this complex. Moreover, we were able to spectroscopically identify [OTf]− bound in a ligand-like fashion to a metal support in recent ultra-high vacuum studies with 1-ethyl-2-methylimidazolium trifluoromethanesulfonate ([C2C1Im][OTf]).28 In the [C2C1Im][OTf] monolayer, the anions interact with a Pd support via the SO3-group, leading to red-shifted νs(S–O) and νas(S–O) signals at ∼1010 and 1216 cm−1, respectively. Similar features located at 1204 and 1016 cm−1 can also be found in the TIR spectra recorded from [C4C1C1Im][OTf]:[Ru(CO)3Cl2]2 mixtures as seen in the spectrum recorded after 5 days. The band intensity of the [OTf]− ligand species is lower compared to its solvent counterpart, but its temporal evolution shows that the concentration of the RuII[OTf]− complex increases with time.
Fig. 3 Offset and normalized reference TIRS spectra for a) [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/[OTf] mixture and b) [Ru(CO)3Cl2]2/[C4C1C1Im][OTf] mixtures (IL region included) both prepared with DCM. |
Our findings support the assumption that there is a slow time- and concentration-dependent conversion of [Ru(CO)3Cl2]2 to a series of different monomers driven by Cl− from the supporting IL phase. The major species on the freshly prepared SILP catalyst using [Ru(CO)3Cl2]2 as a precursor is [Ru(CO)3Cl3]−. In addition, we find species with a larger number of Cl− ligands, formed at lower concentration. The formation and the nature of the [Ru(CO)xCly]n species clearly depends strongly on the concentration of Cl− ions. It is expected that the speciation should have a direct influence on the catalytic properties of the SILP system.
IL | Cl−-sourcea | x(Cl−)a [—] | TOF [h−1] |
---|---|---|---|
a Other than experimentally induced Cl− source respectively Cl− content by precursor. | |||
[C4C1C1Im][OTf] | — | 0.31 | 26.1 |
[C4C1C1Im][OTf] + [C4C1C1Im]Cl | [C4C1C1Im]Cl | 0.66 | 61.4 |
[C4C1C1Im][OTf] + NaCl | NaCl | 0.84 | 33.8 |
[C4C1C1Im]Cl | [C4C1C1Im]Cl | 1.00 | 72.5 |
[C4C1C1Im]Cl + NaCl | [C4C1C1Im]Cl + NaCl | 1.70 | 61.2 |
The Ru-carbonyls identified so far can be interconverted simply by consecutive Cl−/CO ligand substitutions, therefore we conclude that an equilibrium is established between the various observed species during the catalytic reaction.
The sharp feature at 2121 cm−1 which corresponds to the [Ru(CO)3Cl2]2 dimer is quite small and increases in intensity more slowly. Previous results with the [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/Al2O3 system suggested the formation of monomers, thus, the back-reaction and formation of [Ru(CO)3Cl2]2 in the IL is implausible. One possible explanation is that no dimerization takes place, but the [Ru(CO)3Cl2] monomer is formed in small amounts. The calculated spectrum of square pyramidal (s.-pyr.) cis-[Ru(CO)3Cl2] strongly resembles the spectrum of the dimer. Although unambiguous assignment of the bands at 2121 and 2155 cm−1 may, therefore, not be possible, it is clear that upon CO dosing several of the previously identified Ru-carbonyls are formed. Similar species like [Ru(CO)3Cl2]2, fac-[Ru(CO)3Cl3]− and [Ru(CO)2Cl4]2− were also found during carbonylation of RuCl3 in refluxing ethanol/ethoxyethanol.29,30 Thus, freshly prepared [Ru(CO)3Cl2]2 (in the presence of Cl−) and carbonylated RuCl3 SILP catalysts exhibit similar Ru-species, mostly [Ru(CO)3Cl3]−. In the case of RuCl3/[C4C1C1Im]Cl/Al2O3 such carbonylated species can only be formed under reaction conditions. This explains the induction period observed in the catalytic activity.9 The new results indicate that CO dosing at ambient conditions (1 bar, RT) should give rise to a similar effect as preparation of the SILP catalyst with [Ru(CO)3Cl2]2. This finding is interesting from an economic point of view, as RuCl3 is a cheaper starting material than [Ru(CO)3Cl2]2.
In the next step, we tested the response of the carbonylated RuCl3/[C4C1C1Im]Cl/Al2O3 system to a change in temperature. The experiments were performed in Ar atmosphere at 1 bar. A summary of the results is displayed in Fig. 5. Upon heating above 75 °C, the peak at 2121 cm−1 decreases in intensity until no band is visible anymore above 125 °C. Simultaneously, a peak with increasing intensity is observed at 1902 cm−1. This points to the formation of chlorine-rich Ru-carbonyls from CO-rich species. The loss of CO ligands is expected, as carbonylchlororuthenium complexes like [Ru(CO)3Cl2]2 are frequently used as CO releasing molecules (CO-RM) in, for example, medical applications.31 It was reported that up to 0.7 mole CO per mole [Ru(CO)3Cl2]2 can be released in DMSO.26 As both peaks of [Ru(CO)2Cl3]− appear rather as shoulders, it cannot be clearly deduced whether this species increases in intensity or the signal is suppressed by the increase of the more dominant features of [Ru(CO)3Cl3]− at 2032 cm−1 and [Ru(CO)2Cl4]2− or [RuCOCl4]2− at 1902 cm−1. Moreover, a new peak is formed at 1735 cm−1 upon heating which was not observed before. Our DFT calculations (see ESI†) suggest that features at such low wavenumbers are found only for carbonyl–carboxylate complexes and five-coordinated Ru0 carbonyls in trigonal-bipyramidal (trig.-bip.) configuration (see Table 1). The formation of a Ru0 species is relatively unlikely under the present conditions (see also section 3.5). The formation of carboxylates could result from the presence of water in the system, which we consider as unlikely or, potentially, from OH species arising from the Al2O3 support. However, formation of a carboxylate from one CO ligand species should influence the carbonyl peaks at higher wavenumbers, which is not observed. The definite assignment of this peak is, therefore, not possible at the present time.
Fig. 5 Top: Offset DRIFT spectra during heating the carbonylated RuCl3/[C4C1C1Im]Cl/Al2O3 sample; bottom: selected, normalized peak areas (all lines are guides to the eye). |
In general, we observe that only little peak intensity is lost while, at the same time, several peaks drastically increase in intensity. One explanation for this observation is that upon heating IL and Ru species diffuse in the porous system and – at the applied high IL loading – even some may diffuse out of the pores of the support. The change in peak intensity of the IL-related peaks, which should increase correspondingly, supports this hypothesis (see ESI†). In addition residual RuCl3 species in the catalyst pellets may react with CO and form additional [Ru(CO)3Cl3]−, which would also lead to an increase in the intensity of the respective features.
The experiments with RuCl3/[C4C1C1Im]Cl/Al2O3 confirm that an equilibrium is established between different [Ru(CO)xCly]n species present in the two SILP systems that are active for WGSR.
Upon CO dosing the amount of chloride-rich species decreases and [Ru(CO)3Cl2] or [Ru(CO)3Cl2]2 species are formed with more CO ligands bound to the Ru metal center. This observation supports the presence of a dynamic equilibrium between these species.
A closer look at the spectra reveals that a small feature at 2140 cm−1 in combination with a band at 2078 cm−1 (orange curve) develops at temperatures above ∼80 °C. As peaks located at such high wavenumbers point to CO-rich Ru-complexes, this signal pair can be assigned to [Ru(CO)4Cl2].32 The third peak expected from DFT at ∼2030 cm−1 coincides with bands from other species and, therefore, cannot easily be identified in the spectra. [Ru(CO)4Cl2] may indeed be formed from [Ru(CO)3Cl2] or the corresponding dimer in either configuration by carbonylation. It is stable above 90 °C in our experiment, whereas decreasing peaks areas of the [Ru(CO)3Cl2] conformers or dimer (green and grey curve) indicate consumption of the latter at high temperatures.
During cooling, [Ru(CO)4Cl2] re-converts to [Ru(CO)3Cl2] or [Ru(CO)3Cl2]2 complexes by loss of CO. The amount of s.-pyr. trans-[Ru(CO)3Cl2] at 2002 cm−1 decreases upon cooling, although the process seems not to be completed on the time scale of the present experiment.
Furthermore, the spectral region at lower wavenumbers shows an interesting behavior. Firstly, the peak at 1736 cm−1 develops upon heating, as expected from the heating experiment of carbonylated RuCl3. Secondly, the peak intensity decreases above 90 °C and a new peak at 1782 cm−1 is formed at the same time. The cooling ramp shows that this behavior is reversible. As discussed above the corresponding bands may be attributed to carbonyl–carboxylate or Ru0 species. We tentatively assign the low frequency peaks to carbonyl–carboxylate species formed with OH species from the Al2O3 support, as both the appreciable presence of water and reversible formation of Ru0 carbonyl species seem quite unlikely.
In the context of CO dosing, the question arises whether full carbonylation to Ru3(CO)12 is possible under the present conditions. The infrared spectrum of Ru3(CO)12 on Al2O3 shows a broad vibrational structure between 1900 and 2100 cm−1.32 On one hand, this could explain the broad smeared-out structure, which develops upon heating exactly in this spectral region. On the other hand, it has been reported that the presence of halide anions readily leads to CO displacement in Ru3(CO)12, especially in solvents which increase the nucleophilicity of Cl−.33 Still, these experiments have not been conducted in CO atmosphere.
In comparison with the CO dosing experiments performed at RT we conclude that at elevated temperatures carbonylation of chloride-rich species is possible even up to formation of [Ru(CO)4Cl2]. This species was previously not observed in the presented experiments and seems to be associated with appreciable concentration only at temperatures above 80 °C.
1) It is shown that the [Ru(CO)xCly]n SILP is a dynamic system, with a speciation that responds to the reaction conditions. In particular, we investigated the role of the reaction temperature and the CO pressure.
2) With the help of DFT calculations, several species that are present under reaction conditions have been identified. Their nature is summarized in Fig. 8. Specifically, we identify the following species: fac-[Ru(CO)3Cl3]− (major species in the freshly prepared catalyst), cis-[Ru(CO)2Cl3]−, cis-/trans-[Ru(CO)2Cl4]2−, [Ru(CO)Cl4]2−, s.-pyr. cis-/trans-[Ru(CO)3Cl2] and cis-[Ru(CO)4Cl2].
3) Successive elimination/addition steps lead to principle groups of intermediates. In this reaction sequence, the applied chloride IL acts as an effectively infinite reservoir of chloride ligands.
4) Upon preparation of [Ru(CO)3Cl2]2/[C4C1C1Im]Cl/Al2O3 by impregnation in DCM, the Ru dimer splits and a [Ru(CO)3Cl3]− monomer is formed, together with a small amount of [Ru(CO)2Cl3]−, [Ru(CO)2Cl4]2− and [RuCOCl4]2−.
5) The same species are found, if the catalyst is prepared from RuCl3/[C4C1C1Im]Cl/Al2O3 followed by subsequent CO dosing at room temperature.
6) Heating leads to CO release and an increasing fraction of chloride-rich di-anionic species (right-hand side in Fig. 8), whereas CO dosing drives the equilibrium to the CO-rich (left-hand) side. CO dosing at elevated temperatures enhances this transformation and leads even to formation of CO-rich species such as [Ru(CO)4Cl2].
7) In addition to Ru-complexes with varying numbers of Cl− and CO ligands, different conformers of the [Ru(CO)3Cl2] monomer have been identified. Some of the species observed are present only at elevated temperatures in CO atmosphere.
8) The beneficial effect of Cl− addition on the equilibria between different Ru-chloro-carbonyl species is also reflected in the catalytic activity. Higher Cl− concentrations in the IL layer result in more active WGS catalysts.
The presented experiments show that a variety of Ru-complexes can be identified by in situ DRIFTS in combination with DFT. Further experiments are planned involving the influence of water in operando mode. In this way, it should be feasible to assign catalytic activities in an even more reliable fashion.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c7cy02199b |
This journal is © The Royal Society of Chemistry 2018 |