Tsukasa Takanashi,
Masazumi Tamura,
Yoshinao Nakagawa* and
Keiichi Tomishige*
Department of Applied Chemistry, School of Engineering, Tohoku University, 6-6-07, Aoba, Aramaki, Aoba-ku, Sendai 980-8579, Japan. E-mail: tomi@erec.che.tohoku.ac.jp; yoshinao@erec.che.tohoku.ac.jp; Fax: +81-22-795-7214; Tel: +81-22-795-7214
First published on 17th June 2014
The structure of Rh–In bimetallic catalysts supported on carbon for amination of alcohols was determined by XRD, TEM-EDX, XPS, CO adsorption and EXAFS. At low In/Rh ratio (In/Rh ≤ 0.2), Rh metal particles with sizes of <3 nm were observed, and the particles were partially covered with indium oxide species. With addition of more In, a tetragonal RhIn alloy with a particle size of ∼20 nm was formed. This tetragonal alloy has a structure with a = 0.315 nm and c = 0.328 nm where metal atoms are located at (0, 0, 0) and (0.5, 0.5, 0.5). The catalytic activity of the tetragonal RhIn alloy is much higher than that of Rh metal particles with or without indium oxide species. With an excess amount of In (In/Rh > 1) on the high Rh loading (20 wt%) catalyst, the cubic RhIn phase with a CsCl structure was observed instead of the tetragonal RhIn phase, and the catalytic activity was much decreased.
R–OH + NH3 → R–NH2 + H2O | (1) |
Some Rh-based bimetallic catalysts such as those using Sn, Mo, and Re have been reported to show unique activity and/or selectivity in reductive transformations of organic molecules, and the structures have been intensively investigated.8–17 On the other hand, the combination of noble metal and In has been rarely studied for catalyst materials18,19 except Pt–In system.20–24 Even for bulk material, the structure or use of Rh–In alloy system has not been so intensively studied.25,26 The known phases of Rh–In alloy are RhIn with cubic CsCl structure (a = 0.320 nm) and RhIn3 with tetragonal CoGa3 structure (a = 0.701 nm, c = 0.715 nm).27 The existence of Rh-rich Rh–In phase has been suggested; however not identified.28 In the previous paper, we characterized Rh–In/C catalyst with 5 wt% Rh and In/Rh = 1 with XRD, TEM and XPS.4 The data suggested the formation of RhIn alloy; however, because of the small loading amount and broad XRD signals it is difficult to determine the structure of catalytically active species. In this study, we investigated the structure of carbon-supported Rh–In catalysts with large Rh loadings and different In/Rh ratio in order to clarify the relationship between the structure and catalytic activity. We found a catalytically active RhIn phase with tetragonal structure that has not been reported in the literature.
The XRD patterns of the reduced catalysts were recorded on a Rigaku MiniFlex600 diffraction-meter using Cu Kα (λ = 0.154 nm) generated at 40 kV and 15 mA. The catalysts with various In/Rh molar ratios were reduced under H2 flowing at 773 K for 3 h. The reduced catalyst powders were transferred to the sample holder filled with N2 without exposing air in the glove bag. The average particle size of metal was estimated using the Scherrer equation. Dispersion of Rh particles (the ratio of surface atoms to total atoms; Rhs/Rh) was calculated by the equation: Rhs/Rh = 1.098 nm/(particle size).29 XRD pattern of model structure was calculated with CrystalDiffract for Windows ver. 1.4 software (CrystalMaker Software Ltd.).
The amount of CO chemisorption was measured in a high-vacuum system using a volumetric method. Before adsorption measurements, the catalysts were treated with H2 at 773 K for 3 h. Subsequently, the adsorption was performed at room temperature. The gas pressure at adsorption equilibrium was about 1.1 kPa. The sample weight was about 0.15 g. The dead volume of the apparatus was about 80 cm3. The adsorption amount of CO is represented as the molar ratio to Rh.
The X-ray photoelectron spectra (XPS) were recorded using a Shimadzu AXIS-ULTRA with monochromatic Al Kα irradiation (hν = 1486.6 eV). The spot size of the X-ray was ca. 700 × 300 μm2. The catalysts were reduced in flowing H2 at 773 K for 3 h, and then, the reduced catalysts were transported to the analysis chamber in N2 atmosphere. The spectra were analyzed with the program CasaXPS software, version 2.3.16. A binding energy of 284.5 eV of the C 1s level was used as an internal standard. The curve fitting of the In 3d level spectra was conducted with Voigt lineshapes and a Shirley background function.
Field emission-scanning transmission electron microscope (FE-STEM) images and EDX analysis were obtained on a Hitachi spherical aberration corrected STEM/SEM HD-2700 instrument operated at 200 kV. The reduced catalyst was dispersed in ethanol in the glove bag. Then dispersed sample was deposited on a Cu grid in air. The measurement was begun within 10 minutes after deposition.
The X-ray absorption fine structure (XAFS) spectra were measured at the BL01B1 station at SPring-8 with the approval of the Japan Synchrotron Radiation Research Institute (JASRI; proposal no. 2013B1067). The storage ring was operated at 8 GeV. A Si (1 1 1) single crystal was used to obtain a monochromatic X-ray beam. Two ion chambers for I0 and I were filled with Ar for Rh and In K-edge measurement. We measured the XAFS spectra of the catalysts after reduction with flowing H2 at 773 K for 3 h. The reduced catalyst powders were transferred to the measurement cell without exposing air in the glove bag. The thickness of the cell filled with the powder was 1 cm to give an edge jump of 0.8–4.0 and 0.1–1.0 for Rh K-edge and In K-edge measurement, respectively. The XAFS data were collected in a transmission mode. For extended XAFS (EXAFS) analysis, the oscillation was first extracted from the EXAFS data using a spline smoothing method. Oscillation was normalized by the edge height around 50 eV. Fourier transformation of the k3-weighted EXAFS oscillation from the k space to the r space was performed to obtain a radial distribution function. The inversely Fourier filtered data were analyzed using a usual curve fitting method. For curve fitting analysis, the empirical phase shift and amplitude functions for the In–O bonds and metallic bonds such as Rh–Rh, In–In, Rh–In and In–Rh were extracted from data for Rh2O3 and Rh foil, respectively, because of the similar behavior of Rh and In as backscattering atoms in EXAFS and the complex structures of In metal and In2O3. Analyses of XAFS data were performed using a computer program (REX2000, ver. 2.5.9; Rigaku Corp.) for both EXAFS and XANES (X-ray adsorption near edge structure).
In/Rh in preparation | In/Rh from XRF | In loss/% |
---|---|---|
1.0 | 1.0 | 2 |
1.5 | 1.4 | 7 |
2.0 | 1.6 | 18 |
TOF (h−1) = (converted substrate (mol))/{(amount of CO adsorption (mol)) × (reaction time (h))} | (2) |
The amount of CO adsorption corresponds the amount of surface metallic Rh atoms, since In metal or metal oxides do not adsorb CO. The CO adsorption amount was gradually decreased from In/Rh = 0 to 0.5 and was rapidly decreased by further addition of In. The TOF value was much increased with increasing In amount from In/Rh = 0.2 to 1, and the catalyst with In/Rh = 1 showed the highest TOF value (14 h−1). However, further addition of In much decreased the catalytic activity: when In/Rh = 2, the catalyst showed no activity (TOF < 2.3 h−1). The catalytic performances of Rh–In/C catalysts with smaller Rh amount (5 wt%) in the same reaction conditions as those in Fig. 1 have been reported in the previous paper.4 Both series of catalysts (Rh 20 wt% and 5 wt%) have similar trends of performance when In/Rh ratio is 1 or less: the activity of Rh/C without In is very low; the catalysts with low In/Rh have low activity; the TOF value is much increased by In addition from In/Rh = 0.2 to 1; the selectivity to amino alcohols is increased with increasing In/Rh, and the ratio of 1-amino-2-propanol/2-amino-1-propanol is almost constant. It should be noted that both series of catalysts with Rh 20 wt% and 5 wt% showed similar TOF values for low In/Rh ratio (In/Rh = 0.1 and 0.2; TOF ∼3 h−1) and similar highest TOF values (14 and 15 h−1 for Rh 20 wt% and 5 wt%, respectively). The highest TOF values were obtained when In/Rh = 1 for both series. However, when In/Rh = 2, the catalysts with different Rh loadings showed different behavior: the catalyst with Rh 20 wt% (Fig. 1) showed almost no activity, while the catalyst with Rh 5 wt% has moderate activity (TOF 10 h−1). Overall, these data suggest that the structures of supported phases are similar for both series of catalysts (Rh 20 wt% and 5 wt%) when In/Rh = 1 or less.
The XRD of Rh–In/C (Rh 20 wt%, In/Rh = 1) after reaction was also measured, and the pattern was almost unchanged from that of the fresh reduced sample (Fig. S2, ESI†). The reusability of Rh–In/C catalyst has been confirmed in the previous paper.4 Therefore, the structure of reduced catalyst surely reflects the catalytic performance.
Comparison with the results of activity tests (Fig. 1) shows that the catalytic activity is in the following order: group (ii) >group (i) ≫group (iii) ∼0. The very low activity of group (iii) (Rh–In/C (Rh 20 wt%, In/Rh > 1)) indicates that the cubic RhIn species is not catalytically active. The high activity of group (ii) suggests the activity of tetragonal alloy phase; however this idea has not been fully proven because another active phase may exist which does not appear in XRD (amorphous or very small size). We further characterized each group of catalysts.
In/Rh | Particle size/nm from XRD | Rhs/Rh from XRD | CO/Rh | Rhs/Rh − CO/Rh |
---|---|---|---|---|
0 | 3.7 | 0.30 | 0.21 | 0.09 |
0.1 | 2.8 | 0.39 | 0.19 | 0.20 |
0.2 | 2.3 | 0.48 | 0.18 | 0.30 |
The In 3d XPS data are shown in Fig. 4. Each peak can be fitted by one single function, and all the peak positions (444.5 and 444.6 eV for 3d5/2; 452.0 and 452.1 eV for 3d3/2) are within the range for In(III) species (3d5/2: 444.26–444.84 eV, 3d3/2: 451.80–452.38 eV).34 The absence of In(0) signal supported the absence of Rh–In alloy. The summary of XPS data for all samples is shown in ESI (Table S1).†
Based on the data, we propose the model structure of this group of catalyst (Fig. 5). The Rh metal particles are formed on the carbon support, and all the added In atoms are located on the Rh particle surface as In(III) oxide. The comparison between the structure (Fig. 5) and catalytic activity (Fig. 1) shows that the modification of Rh metal with indium oxide generates the catalytic activity in the amination.
The state of Rh and In was also investigated with EXAFS. The results of Fourier transform and curve fitting are shown in Fig. 6 and Table 3, respectively. The EXAFS oscillation and Fourier filtered EXAFS data are shown in ESI (Fig. S3 and S4).† The Rh K-edge EXAFS data were well fitted by single Rh–Rh shell with coordination number (CN) ∼11, supporting that all Rh atoms were in the metallic state. The In K-edge EXAFS data can be fitted by In–O shell and In–Rh shell as expected by the model structure as shown in Fig. 5.
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Fig. 6 Results of Fourier transform of k3-weighted EXAFS oscillation of Rh–In/C (Rh 20 wt%, In/Rh ≤ 0.2). (a) Rh K-edge, FT range: 30–150 nm−1; (b) In K-edge, FT range: 30–120 nm−1. |
Sample (In/Rh) | Edge | Shell | CNa | Rb nm | σc/nm | ΔE0d/eV | Rfe/% | Fourier filtering range/nm |
---|---|---|---|---|---|---|---|---|
a Coordination number.b Bond distance.c Debye–Waller factor.d Difference in the origin of photoelectron energy between the reference and the sample.e Residual factor. | ||||||||
0 | Rh K | Rh–Rh | 11.1 | 0.268 | 0.0079 | 3.0 | 0.6 | 0.166–0.292 |
0.1 | Rh K | Rh–Rh (or –In) | 10.8 | 0.268 | 0.0084 | 5.3 | 1.2 | 0.166–0.292 |
In K | In–O | 2.1 | 0.211 | 0.0060 | −9.6 | 2.4 | 0.126–0.279 | |
In–O | 2.4 | 0.225 | 0.0060 | −0.3 | ||||
In–Rh (or –In) | 1.2 | 0.271 | 0.0083 | 5.5 | ||||
0.2 | Rh K | Rh–Rh (or –In) | 10.5 | 0.268 | 0.0077 | 3.4 | 1.0 | 0.166–0.292 |
In K | In–O | 1.4 | 0.211 | 0.0076 | 2.4 | 2.2 | 0.126–0.279 | |
In–O | 1.6 | 0.225 | 0.0078 | −4.6 | ||||
In–Rh (or –In) | 2.3 | 0.271 | 0.0083 | 0.4 | ||||
Rh foil | Rh K | Rh–Rh | 12 | 0.268 | 0.0060 | 0 | — | — |
Rh2O3 | Rh K | Rh–O | 6 | 0.206 | 0.0060 | 0 | — | — |
The TEM images and EDX analyses of Rh–In/C (Rh 20 wt%, In/Rh = 1) are shown in Fig. 8 and 9, respectively. Surprisingly, large dendritic structure was present as well as carbon-supported particles. The dendritic structure was composed of domains with the size of 10–30 nm. The particles on the support had various sizes from <5 nm to ∼20 nm. The EDX analysis was conducted with either Cliff–Lorimer method,35 which gives the average element ratio in the total field of image, or conventional line analysis. The results showed that both dendritic structure and carbon-supported particles had the In/Rh ratio of 1.0. We also measured the mapping of elemental distributions (Fig. S5, ESI†), which also confirmed the bimetallic structure. From XRD, the particle size of tetragonal Rh–In alloy in Rh–In/C (Rh 20 wt%, In/Rh = 1) was calculated to be 20 nm. In this calculation, we assumed that the broadening by the heterogeneity of alloy composition did not affect the peak width since the change of In/Rh ratio did not affect the XRD peak positions. Based on TEM-EDX and XRD, we determined the phase of both the dendritic structure and the larger particles on the support as tetragonal RhIn alloy with the atomic ratio of 1:
1. The analogy with cubic RhIn alloy with CsCl structure suggests that the Rh and In atoms in tetragonal RhIn alloy are located at (0, 0, 0) and (0.5, 0.5, 0.5), respectively, in the unit cell as similar to CsCl structure. It is not known why tetragonal RhIn alloy was formed on this catalyst rather than well-known cubic RhIn alloy. One factor may be the shortage of In. In the literature, cubic RhIn phase has been reported to exist in slightly indium-rich conditions of In + Rh system: from In/(In + Rh) = 51% to 56% at 873 K.28
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Fig. 9 TEM-EDX analysis of Rh–In/C (Rh 20 wt%, In/Rh = 1). (a) and (b): Cliff–Lorimer method for the elemental analysis in the whole area. (c) Line analysis. |
Fig. 10 and Table 4 show the Fourier transform and the curve fitting results of EXAFS, respectively. The EXAFS oscillation and Fourier filtered EXAFS data are shown in ESI (Fig. S3 and S4).† The Rh K-edge EXAFS data can be fitted by three Rh–Rh (or In) shells, which consists of one shell for fcc Rh structure (R = 0.268 nm) and two shells for bcc-like structure (R = 0.28 and 0.32 nm; ratio of CN = 8/6). The latter shells corresponded to the tetragonal RhIn alloy. The CN of Rh–Rh shell for fcc Rh structure was decreased and the CNs for RhIn alloy were increased with increasing In amount. This behavior supports the transformation of fcc Rh particles, probably modified with indium species, into RhIn alloy by addition of indium. The In(III) species detected by XPS analysis (Fig. 7) can be assigned to the In species covering the fcc Rh metal particles. The In K-edge EXAFS data can be fitted by two In–metal (metal = Rh or In) shells and In–O shell. The two In–metal shells had almost the same distances (R) as those of Rh–metal shells for the bcc-like structure. In addition, the number of In–metal bond calculated by (CN of In–metal shell) × (number of In atoms in the sample) was almost the same as the number of Rh–metal bond (= (CN of Rh–metal shell) × (number of Rh atoms in the sample)) with similar distance. These similarities further support the formation of bcc-like RhIn alloy where Rh and In are structurally equal.
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Fig. 10 Results of Fourier transform of k3-weighted EXAFS oscillation of Rh–In/C (Rh 20 wt%, In/Rh = 0.5 and 1). (a) Rh K-edge, FT range: 30–150 nm−1; (b) In K-edge, FT range: 30–120 nm−1. |
Sample (In/Rh) | Edge | Shell | CNa | Rb nm | σc/nm | ΔE0d/eV | Rfe/% | Fourier filtering range/nm |
---|---|---|---|---|---|---|---|---|
a Coordination number.b Bond distance.c Debye–Waller factor.d Difference in the origin of photoelectron energy between the reference and the sample.e Residual factor. | ||||||||
0.5 | Rh K | Rh–Rh (or –In) | 6.0 | 0.268 | 0.0076 | 6.6 | 1.0 | 0.166–0.292 |
Rh–Rh (or –In) | 2.8 | 0.277 | 0.0068 | 3.4 | ||||
Rh–Rh (or –In) | 2.2 | 0.320 | 0.0088 | 8.8 | ||||
In K | In–O | 0.7 | 0.223 | 0.0073 | 9.9 | 2.2 | 0.126–0.279 | |
In–Rh (or –In) | 5.4 | 0.277 | 0.0077 | 6.4 | ||||
In–Rh (or –In) | 4.0 | 0.319 | 0.0087 | −8.2 | ||||
1 | Rh K | Rh–Rh (or –In) | 1.5 | 0.268 | 0.0082 | 9.9 | 2.5 | 0.166-0.292 |
Rh–Rh (or –In) | 5.4 | 0.277 | 0.0070 | 5.5 | ||||
Rh–Rh (or –In) | 4.0 | 0.319 | 0.0090 | 9.8 | ||||
In K | In–O | 0.5 | 0.223 | 0.0076 | 9.9 | 0.7 | 0.126–0.279 | |
In–Rh (or –In) | 5.5 | 0.277 | 0.0071 | 6.4 | ||||
In–Rh (or –In) | 4.1 | 0.320 | 0.0088 | −4.0 | ||||
Rh foil | Rh K | Rh–Rh | 12 | 0.268 | 0.0060 | 0 | — | — |
Rh2O3 | Rh K | Rh–O | 6 | 0.206 | 0.0060 | 0 | — | — |
The molar ratio of tetragonal RhIn alloy to total Rh can be calculated from the ratio of the CN of the shells of bcc-like tetragonal phase to the theoretical values (8 and 6 for R = 0.28 and 0.32 nm shells, respectively). We did not use the calculation from the CN of the shell of fcc Rh phase because the small particle size of fcc Rh phase could decrease the CN, while tetragonal RhIn alloy particles were large enough. The calculated ratio was 36% and 68% for In/Rh = 0.5 and 1, respectively. The amount of tetragonal RhIn phase was also calculated by In XPS: the amount of In(0) corresponded to that of tetragonal RhIn; however the amount might be underestimated because not all atoms in larger RhIn alloy particles were detected by XPS analysis. The calculated values were 25% and 65% for In/Rh = 0.5 and 1, respectively, and in fact these values were smaller than those obtained from EXAFS.
Based on the above characterizations, we propose the model structure of Rh–In/C catalyst in this group (0.2 < In/Rh ≤ 1) (Fig. 11). Small Rh metal particles (3 nm or less) partially covered with indium oxide species and large tetragonal RhIn alloy particles (∼20 nm) are present on the support carbon. In addition, the large tetragonal RhIn particles are attached together, and dendritic structure is formed. The formation of large RhIn particles may be due to the low melting point of In(0). During the reduction process, In species that did not interact with Rh particle might be reduced to liquid In metal. The drops of liquid In metal moved on the support to collect many Rh particles, and large alloy particles were formed.
From the catalysis data (Fig. 1), the catalytic activity (TOF value) was sharply increased with the formation of tetragonal RhIn phase. Therefore, we conclude that the catalytic activity of the different phases is in the following order: tetragonal RhIn alloy > Rh metal modified with indium oxide ≫ unmodified Rh metal.
In/Rh | Binding energy/eV | |
---|---|---|
Rh 3d5/2 | Rh 3d3/2 | |
0.1 | 307.40 | 312.15 |
0.2 | 307.35 | 312.10 |
0.5 | 307.32 | 312.03 |
1 | 306.81 | 311.44 |
2 | 306.69 | 311.31 |
The low activity of In/Rh = 2 catalyst (cubic RhIn alloy) is not explained by this electronic effect. Cubic RhIn alloy was formed only when excess amount of In was present, and in fact the CO adsorption amount on Rh–In/C (20 wt% Rh, In/Rh = 2) was very low. Therefore, a number of In atoms were present on the cubic RhIn alloy surface. The surface In species might block the access of substrate molecule that is much larger than CO on the surface Rh atom.
We also mention the leaching of Rh and In during the reaction. As reported in the previous paper,4 leaching of both Rh and In from Rh–In/C (In/Rh = 1) was observed during the amination reaction, especially when carbon black support was used instead of activated carbon. In fact, the leaching accompanied the change of reaction medium into turbid colloidal solution even after the filtration. Increasing the loading amount from 5 wt% Rh to 20 wt%, the solution after reaction became much more turbid: the leaching problem was more evident. Based on the results in Section 3.5, especially TEM result, a part of Rh–In alloy phase might well be detached from the support and might become colloid. In other words, the cause of leaching can be the formation of Rh–In alloy colloid. The observed leaching of Rh, which as metallic state is insoluble in water, also supports this idea.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra03984j |
This journal is © The Royal Society of Chemistry 2014 |