# In Situ IR Characterization of CO Interacting with Rh Nanoparticles Obtained by Calcination and Reduction of Hydrotalcite-Type Precursors

Authors: F. Basile; I. Bersani; P. Del Gallo; S. Fiorilli; G. Fornasari; D. Gary; R. Mortera; B. Onida; A. Vaccari
Journal: International Journal of Spectroscopy
 (2011)

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## Abstract

Supported Rh nanoparticles obtained by reduction in hydrogen of severely calcined Rh/Mg/Al hydrotalcite-type (HT) phases have been characterized by FT-IR spectroscopy of adsorbed CO [both at room temperature (r.t.) and nominal liquid nitrogen temperature] and Transmission Electron Microscopy (TEM). The effect of reducing temperature has been investigated, showing that Rh crystal size increases from 1.4 nm to 1.8 nm when the reduction temperature increases from 750°C to 950°C. The crystal growth favours the formation of bridged CO species and linear monocarbonyl species with respect togem-dicarbonyl species; when CO adsorbs at r.t., CO disproportionation occurs on Rh and it accompanies the formation of RhI(CO)2. The role of interlayer anions in the HT precursors to affect the properties of the final materials has been also investigated considering samples prepared from silicate-instead of carbonate-containing precursors. In this case, formation of RhI(CO)2 and CO disproportionation do not occur, and this evidence is discussed in terms of support effect.


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## Body

## 1. Introduction

Hydrotalcites or layered double hydroxides (LDH’s) belong to a large class of natural and synthetic anionic  clays. Although they are less diffuse in nature than cationic clays, they can be easily synthesized [1]. Hydrotalcites-type (HT) compounds have the general formula:(1)[M2+(1-x)M3+x(OH)2]b+(An-b/n)mH2O
The cations are present in a layer with brucite-type structure [Mg(OH)2], in which part of Mg2+ is replaced by Al3+ and, as a consequence, the positive additional charge of the cations is balanced by the insertion of anions between layers. Usually carbonates are used as anions,  even if samples with silicates have shown higher thermal and textural stability [2].The mixed oxides obtained after calcination of HT phases  at temperature above 500°C are very useful for a wide range of applications like antiacids, anion exchanger, adsorbents, catalysts, and catalyst supports because of their undeniable advantages as high surface area and structural stability [3].A further increase of the calcination temperature above 750°C gives rise to the segregation of the stoichiometric spinel phase and the formation of less defective MgO-type phase, giving rise to stable supports or catalysts for high temperature processes. In particular, the modification of the catalytic properties is possible by the substitution of part of Mg with other bivalent cation as Ni, Pt, Pd, Co, and/or part of Al ions with Rh, Fe, Cr obtaining a high variety of formulation [3, 4].The structure and surface properties of Mg-Al HT phases and of the resulting mixed oxides depend strongly on chemical composition and synthesis procedures [3].Catalytic applications take advantage of their basic and/or redox properties, as the dispersion of the cations in the hydroxylated layers is retained after calcination, thus generating well-stabilized metallic particles. This property is particularly useful for catalysts active in H2 production processes via reforming reactions. Considering that Rh is well known as one the most active metals for methane reforming, its insertion in the HT  material leads to a very active catalyst with Rh particles highly dispersed on the surface of catalyst [5].IR spectroscopy of adsorbed carbon monoxide has been widely used to characterize Rh-supported catalysts [6–11]. It is well known that three generalized types of chemisorbed CO are produced on dispersed Rh surfaces at room temperature, which are linear monocarbonyl species, Rh0(CO), bridging CO species, Rh20(CO), and gem-dicarbonyl complexes on oxidized Rh sites, RhI(CO)2. The detection of the latter is considered significant for the existence of highly dispersed Rh, whereas linear and bridged carbonyl species are usually considered to form on extended  Rh surface [6, 8, 10].Besides giving information on dispersion of  Rh, the study of interaction with CO allows to characterize the role of the support [7], which can strongly affect the catalytic activity [1]. Indeed, Rh in Rh/Mg/Al catalysts may be present in different phases. For instance, Rh/Mg/Al catalysts with high Rh content obtained by HT carbonate have been structurally characterised by sequential XRD and neutron diffraction Rietveld analysis, and Rh was shown to be present with a higher occupation factor inside the MgAl2O4 phase with respect to the MgO phase [12].The aim of the work is twofold: on the one hand, the effect of the reducing treatment on Rh metal particles produced starting from Rh/Mg/Al HT precursors (1% by weight of rhodium)  is investigated, analyzing two samples reduced at 750°C and at 950°C, respectively.On the other hand,  the effect of the support is investigated. To this purpose two materials with different M2+/M3+ ratio and different anions between layers were taken in exam: one sample was prepared with carbonate and the ratio M2+/M3+ was  about 2, and the other one was prepared with silicate and the M2+/M3+ ratio was 4. In fact, different anions give rise to different phases in the calcined system: for instance, upon calcination silicates react with part of magnesium to give forsterite-type phase [2].The characterization of supported Rh particles has been carried out by means of interaction with CO both at room temperature (r.t.) and at nominal liquid N2 temperature, being the reactivity of CO depending on temperature [6]. The study of adsorbed CO2 has been also carried out in order to characterize products of CO reaction at room temperature.IR spectroscopy data are discussed on the basis of X-ray diffraction and TEM characterization.


## 2. Experimental

### 2.1. Materials Preparation

Carbonate and silicate-containing HT precursors were synthesized by coprecipitation method at constant pH and temperature following the method previously reported [4]. A solution of nitrate salts was added drop by drop to a basic solution containing carbonate or silicate anions. pH was kept constant at 10.5 by dropwise NaOH addition. The obtained suspension was aged  by stirring for 1 hour at 56°C, then filtered and washed with distilled water. The precipitate was dried overnight at 60°C and calcined at 900°C for 12 h.Samples obtained from the  carbonate solution (nominal composition Rh0.43Mg68Al31.57)  were reduced at 750°C for 2 h  or at 950°C for 4 h  under a 50 mL/min flow of  an  H2-Ar  mixture  (3 : 97 v/v) and from now on will be named Rh/HTCarb_750 and Rh/HTCarb_950, respectively. The material obtained from the silicate solution (nominal composition Rh0.5Mg80Al19.5)  was reduced under  a  50 mL/min flow of  an  H2-Ar  mixture  (3 : 97 v/v)  and will be  named  as Rh/HTSil_750.


### 2.2. Samples Characterization

XRD powder analyses were carried out using a Philips PW1050/81 diffractometer equipped with a graphite monochromator in the diffracted beam and controlled by a PW1710 unit (l = 0.15418 nm). A 2theta range from 5° to 80° was investigated at a scanning speed of 70°/h. In order to evaluate the particle size of phases, the silicon (plane (111)) was used to determine broadening of the X-ray reflections (FWHM). The calculation was performed with the X’Pert HighScore Program using the Scherrer’s equation.Transmission Electron Microscopy (TEM, JEOL 2010), combined with Energy Dispersive X-ray Spectrometry (EDS), was used to determine  the size of the  Rh particles  in the samples reduced at different temperatures (according to that reported above) or obtained from carbonate- or  silicate-containing HT precursors.


### 2.3. IR Study of Interaction with Probe Molecules

For IR, characterization powders were pressed into thin self-supporting pellets and then placed into a quartz IR cell. The activation treatment was carried out by connecting the cell to a vacuum-adsorption frame with a residual pressure below 10−3 mbar. In particular, prior to the adsorption measurements, all samples were activated by a treatment in H2 (200 mbar) at 750°C  (heating rate 2.5°C min−1) for 1 h, outgassed under dynamic vacuum at 650°C  for 2 h and then cooled to room temperature under Ar atmosphere.FT-IR spectra were collected by using a Bruker Equinox 55 spectrometer, equipped with MCT cryodetector, at a spectral resolution of 2 cm−1and accumulation of 32 scans. CO and CO2 (from Messer) were dosed in the pressure range from 0.1 to 35 mbar by connecting the IR cell to a vacuum  frame. The interaction with CO was studied both at r.t.  and at the nominal temperature of  −196°C  by using liquid nitrogen as coolant. The actual temperature of the sample is about  −173°C, due to the heating effect of the IR beam. Adsorption of CO2 was studied at r.t.FT-IR spectra related to different samples were normalized dividing the registered intensities by the pellet weight (mg) and multiplying by the pellet area (mm2).  For this reason, absorbance is in arbitrary units (a.u.) and values are not reported in figures. All FT-IR spectra related to the dosage of CO and CO2 are shown as difference spectra (the spectrum recorded before probe dosage was subtracted): positive bands indicate species which are formed during the in situ measurement, whereas negative bands, if present, are related to species which are consumed.


## 2.1. Materials Preparation

Carbonate and silicate-containing HT precursors were synthesized by coprecipitation method at constant pH and temperature following the method previously reported [4]. A solution of nitrate salts was added drop by drop to a basic solution containing carbonate or silicate anions. pH was kept constant at 10.5 by dropwise NaOH addition. The obtained suspension was aged  by stirring for 1 hour at 56°C, then filtered and washed with distilled water. The precipitate was dried overnight at 60°C and calcined at 900°C for 12 h.Samples obtained from the  carbonate solution (nominal composition Rh0.43Mg68Al31.57)  were reduced at 750°C for 2 h  or at 950°C for 4 h  under a 50 mL/min flow of  an  H2-Ar  mixture  (3 : 97 v/v) and from now on will be named Rh/HTCarb_750 and Rh/HTCarb_950, respectively. The material obtained from the silicate solution (nominal composition Rh0.5Mg80Al19.5)  was reduced under  a  50 mL/min flow of  an  H2-Ar  mixture  (3 : 97 v/v)  and will be  named  as Rh/HTSil_750.


## 2.2. Samples Characterization

XRD powder analyses were carried out using a Philips PW1050/81 diffractometer equipped with a graphite monochromator in the diffracted beam and controlled by a PW1710 unit (l = 0.15418 nm). A 2theta range from 5° to 80° was investigated at a scanning speed of 70°/h. In order to evaluate the particle size of phases, the silicon (plane (111)) was used to determine broadening of the X-ray reflections (FWHM). The calculation was performed with the X’Pert HighScore Program using the Scherrer’s equation.Transmission Electron Microscopy (TEM, JEOL 2010), combined with Energy Dispersive X-ray Spectrometry (EDS), was used to determine  the size of the  Rh particles  in the samples reduced at different temperatures (according to that reported above) or obtained from carbonate- or  silicate-containing HT precursors.


## 2.3. IR Study of Interaction with Probe Molecules

For IR, characterization powders were pressed into thin self-supporting pellets and then placed into a quartz IR cell. The activation treatment was carried out by connecting the cell to a vacuum-adsorption frame with a residual pressure below 10−3 mbar. In particular, prior to the adsorption measurements, all samples were activated by a treatment in H2 (200 mbar) at 750°C  (heating rate 2.5°C min−1) for 1 h, outgassed under dynamic vacuum at 650°C  for 2 h and then cooled to room temperature under Ar atmosphere.FT-IR spectra were collected by using a Bruker Equinox 55 spectrometer, equipped with MCT cryodetector, at a spectral resolution of 2 cm−1and accumulation of 32 scans. CO and CO2 (from Messer) were dosed in the pressure range from 0.1 to 35 mbar by connecting the IR cell to a vacuum  frame. The interaction with CO was studied both at r.t.  and at the nominal temperature of  −196°C  by using liquid nitrogen as coolant. The actual temperature of the sample is about  −173°C, due to the heating effect of the IR beam. Adsorption of CO2 was studied at r.t.FT-IR spectra related to different samples were normalized dividing the registered intensities by the pellet weight (mg) and multiplying by the pellet area (mm2).  For this reason, absorbance is in arbitrary units (a.u.) and values are not reported in figures. All FT-IR spectra related to the dosage of CO and CO2 are shown as difference spectra (the spectrum recorded before probe dosage was subtracted): positive bands indicate species which are formed during the in situ measurement, whereas negative bands, if present, are related to species which are consumed.


## 3. Results and Discussion

Rh/HTCarb_750 contains a spinel-type phase and a rock-salt-type  phase, as revealed by the XRD pattern (Figure1(a)).XRD patterns of Rh/HTCarb_750 (a) and Rh/HTSil_750 (b).
(a)(b)The average particle sizes for MgO- and spinel-type  phases, calculated by means of Sherrer’s equation using the FWHM values of the most intense reflexions, are reported in Table1.  The average crystallite size of MgO-type phase  in Rh/HT_Carb750  is close to 15 nm, while the spinel-type phase shows a slightly higher crystallite size (20 nm).Table 1
Crystal size of MgO-  and MgAl2O4-type  phases (nm) as obtained by XRD analysis.
Phase (*)Rh/HTCarb_750Rh/HTSil_750MgO (200)1213MgO (220)1517MgO13.515MgAl2O4 (111)18/MgAl2O4 (220)34/MgAl2O4 (311)24/MgAl2O425/(*)Reflections used for crystal size evaluation are reported.A complex pattern is observed for Rh/HTSil_750 (Figure1(b)). Diffraction peaks assigned to a forsterite-like phase (Mg2SiO4) are indexed. Instead, no well-defined Al-containing phase (MgAl2O4) is detected [13]. In fact, only weak and broad reflections ascribable to a spinel-type phase are observed and the first two reflections at 2θ = 19 and 32°, ascribed to (111) and (220) planes, are not  discernible in the pattern. This indicates that the silicates react with MgO to give the forsterite phase, affecting the formation of the spinel-type  phase.Since the MgO-type phase is the only phase observed in Rh/HTSil_750 also present in the Rh/HTCarb_750, the crystal size is estimated only for it and it appears larger than in the case of Rh/HTCarb 750.For both Rh/HTCarb_750 and Rh/HTSil_750, no reflections due metallic Rh are observed, being its amount close to the instrumental detection limit.Figure2 reports the spectra related to increasing amount of CO adsorbed at r.t.  on Rh/HTCarb_750 in the range 2200–1300 cm−1.  At very low CO pressure (spectrum 1), a single band is observed at 2050 cm−1, assigned to the stretching mode of  linear monocarbonyl species on Rh metal particles, Rh0(CO) [14, 15]. At increasing CO pressure, two shoulders appear above and below the band at 2050 cm−1, due to, respectively, the symmetric and antisymmetric stretching modes of dicarbonyl species on oxidized Rh species, that is, RhI(CO)2  [16]. In same spectra, absorptions below 1800 cm−1 increase, with maxima discernible at 1680 cm−1 and 1313 cm−1, due to bidentate carbonates, at 1394 cm−1 and 1220 cm−1, ascribed to hydrogenocarbonate-type and at 1380 cm−1, assigned to formate-type species  [17–19].Figure 2
FT-IR spectra related to the adsorption of CO on Rh/HTCarb_750 at r.t. Section a: spectra recorded at increasing CO pressure. The inset shows the corresponding OH stretching region. Section b. Spectrum recorded after removal of CO from the IR cell at r.t. (D:gem-dicarbonyl, M: linear monocarbonyl, C: carbonate-, HC: hydrogenocarbonate-, and F: formate-type species).The spectrum recorded after removal of CO by outgassing at r.t. is reported in Figure3 (curve 1). The band due to Rh0(CO) species is clearly observed at 2050 cm−1. The weak band discernible at 2096 cm−1 is due to the  symmetric stretching mode of RhI(CO)2  species. The twin antisymmetric mode, expected at around 2030 cm−1 [14–16], is most probably hidden in the tail of the main component at 2050 cm−1, which indeed shows a low-frequency side asymmetry evidenced by the vertical broken line in the figure.Figure 3
FT-IR spectra recorded after contact of CO with Rh/HTCarb_750 at r.t. (curve a) and at liquid N2 temperature (curve b). (D: gem-dicarbonyl, M: linear monocarbonyl, C: carbonate-, HC: hydrogenocarbonate-, and F: formate-type species).In the same spectra, bands due to carbonate-, hydrogenocarbonate-, and formate-type  species are also observed.As widely reported in the literature, species RhI are generally considered to form by reaction of CO on small Rhx crystallites rather than present on the surface as such prior to contact with CO [10, 20, 21].Indeed, the spectrum of CO adsorbed at low temperature (curve 2 in Figure3) shows a single band at 2050 cm−1 due to linear monocarbonyl species on Rh0. This suggests that species able to give gem-dicarbonyl species are not present on the surface, whereas they are formed by reaction with CO at room temperature.The mechanism of formation of RhI(CO)2 species upon reaction of CO is still under debate.  It has been suggested that Rh-Rh bonds can be disrupted at r.t.  and under CO pressure, due to the higher energy of the Rh-CO bond as compared to the Rh-Rh one [22], in small Rhx particles. Some authors proposed that RhI(CO)2  may form on two-dimensional Rh “islands” or Rh-isolated  atoms [6, 23].Primet [24] proposed that CO dissociation may occur  even at −73°C on Rh, producing chemisorbed oxygen, leading to the formation of Rh+ sites which are able to adsorb two CO molecules.Moreover, the involvement of support OH species has been also proposed in a few cases [10, 25] according to the mechanism:(2)(1x)Rhx0+2CO+OH-⟶O2-+Rh+(CO)2+12H2
In the present case, the role of surface OH species, if any, is negligible, as revealed by the investigation of spectra in the OH stretching region (inset in Figure 2), where no significant modifications during reaction with CO are observed.Despite the debate concerning the formation mechanism of RhI(CO)2  species, however, the detection of gem-dicarbonyls is generally considered a strong indication of the existence of highly dispersed Rh metal particles on the catalyst surface.In the present case, the formation of RhI(CO)2  species is accompanied by the formation of carbonate-, hydrogenocarbonate-,  and formate-type species, revealing that disproportionation of CO to C and CO2 occurs. Indeed adsorption of CO2 on the catalyst gives rise to similar absorption in the IR spectrum (Figure 4).Figure 4
FT-IR spectra related to the adsorption of CO2 on Rh/HTCarb_750 at r.t. (C: carbonate-, HC: hydrogenocarbonate-, and F: formate-type species).The reaction of CO occurs on Rh, since no formation of carbonate-type species has been observed for reaction of CO with the Rh-free support (spectra not reported). Disproportionation of  CO on Rh supported on several oxides (TiO2, Al2O3, SiO2, MgO) has been reported in the literature, though at temperature higher than 25°C  [7].It is worth noting that in the spectrum of CO adsorbed at low temperature no bands due to carbonate-type  species are observed, suggesting that carbonates form when RhI(CO)2 species form. Indeed, though at temperature higher than 25°C,  CO disproportionation on supported Rh was observed to occur with no evidence of presence of dicarbonyl species [7],  some  authors [26] suggested that the dissociation-disproportionation of CO should occur in the twin form in the case of Ru catalysts, which appears a reasonable mechanism, involving two CO molecules on the same metal site.


### 3.1. Effect of the Reducing Temperature

In order to investigate the effect of reducing temperature on the system, the sample reduced at 950°C  (Rh/HTCarb_950) has been characterized following the same approach. The characterization has been completed by TEM analysis, and Figure5 shows the TEM micrographs of Rh/HTCarb_750 and Rh/HTCarb_950. The Rh is in the form of well-dispersed nanoparticles in both cases. As expected, the average particle size appears smaller for the catalyst reduced at lower temperature (1.4 nm) than for that reduced at 950°C (1.8 nm).TEM micrographs of Rh/HTCarb_750 (upper part) and Rh/HTCarb_950 (lower part).
(a)(b)Figure6  shows the spectrum recorded after contact of Rh/HTcarb_950 with CO (p = 30 mbar) at r.t.  and removal of the gas from the cell by outgassing. Spectra in presence of CO are similar and thus are not reported for sake of brevity.Figure 6
FT-IR spectrum recorded after contact of CO with Rh/HTCarb_950 at r.t. (D: gem-dicarbonyl, M: linear monocarbonyl, B: bridged-bonded CO, and C: carbonate-type species).The narrow band at 2060 cm−1 due to the Rh0(CO) species dominates the spectrum, whereas the symmetric mode of gem-dicarbonyl complexes appears as a shoulder at 2093 cm−1, accompanied by the twin peak as a tail hardly discernible at about  2030 cm−1. The relative intensity of the monocarbonyl band with respect to the symmetric gem-dicarbonyl mode is higher than for Rh/HTCarb_750, suggesting a larger population of the former species in the present case.Moreover, a broad absorption is observed at about 1910 cm−1, due to bridged-bonded carbonyl species, Rh02(CO) [25]. Both Rh0(CO) and Rh02(CO) arise from CO adsorbed on extended Rh faces. The lower amount of the former and the absence of the latter in Rh/HTCarb_750 are both in agreement with the existence of smaller Rh particles with respect to  Rh/HTCarb_950, as revealed by TEM analysis. In particular, it may seem that the limit of average crystal size above which bridged-bonded carbonyl species are formed falls in the range of 1.4–1.8 nm.Though several authors reported the formation of bridged-bond Rh2(CO) upon adsorption of CO on supported Rh, very rarely information on particle size from complementary techniques is provided. Finocchio et al. [10]  observed the occurrence of  bridged-bond Rh2(CO) on particles with estimated size of 3.2 nm.It is worth noting that in the case of Rh/HTcarb_950, only a very small amount of carbonate-like species are formed. The lower relative amount of RhI(CO)2   in the present case suggests that formation of carbonate-type  species is related to formation of gem-dicarbonyls upon reaction with CO. As observed for Rh/HTCarb_750, only monocarbonyl species are formed upon adsorption of CO at low temperature (spectrum not reported).


### 3.2. Role of the Support

The effect of the support has been investigated considering the reactivity of  Rh/HTCarb_750 and Rh/HTSil_750 towards CO at r.t.   Figure7 reports the IR spectrum recorded after contact of Rh/HTSil_750 with CO (p = 30 mbar) at r.t.  and removal of the gas from the IR cell by outgassing.Figure 7
FT-IR spectrum recorded after contact of CO with Rh/HTSil_750 at r.t.  Inset: spectra recorded at increasing CO pressure.A single band is visible at 2048 cm−1, due to monocarbonyl species on Rh surfaces. No bands due to gem-dicarbonyls are present, neither absorptions due to carbonate-type  species. The results show that in  Rh/HTSil_750  Rh  is definitely less reactive towards CO with respect to Rh/HTCarb_750.The lower reactivity cannot  be ascribed to larger Rh particle size, that  from TEM analysis (image  not reported) shows a size of   1.1 nm, that is  smaller than those observed on Rh/HTCarb_750.An affect of the support may be instead envisaged, that  may not favor the formation of RhI(CO)2. The inset of  Figure 7 reports the spectra recorded upon increasing CO pressure at r.t. Besides the shifting of the monocarbonyl band to higher frequency upon increasing coverage, due to dipole-dipole coupling among adsorbed CO molecules [10], a new component increases at 2078 cm−1 (labeled by an asterisk in figure). This absorption is depleted by outgassing at r.t., and in fact it is not visible in the spectrum reported in the main body of  Figure 7, revealing that the related species is labile and adsorbed reversibly. We tentatively assign this band to monocarbonyl species on oxidized Rh, that is,  RhI(CO) species [15]. A similar species was proposed to account for a band observed at 2087 cm−1 on Rh/TiO2 catalyst during decarbonylation [27]. These authors suggested  that this species is an intermediate in the conversion of RhI(CO)2 to Rh0(CO) and  proposed that the corresponding band is frequently overlapped with the band above 2090 cm−1 due to gem-dicarbonyl species, so being indiscernible in most cases. The same band had been previously observed during initial adsorption of CO at low temperature on Rh/Al2O3 and it was assigned to RhI monocarbonyl species [28].Assuming that the mechanism of decarbonylation is the reverse of the conversion of Rh0(CO) to RhI(CO)2, we propose that the labile RhI(CO) species forms at increasing CO coverage and it is a precursor of the gem-dicarbonyl species. It most probably forms also in the case of Rh/HTCarb_750 (Figure 2), being the band at 2078 cm−1 overlapped with the symmetric mode of the RhI(CO)2, as previously suggested [19]. Indeed, upon CO removal (Figure 3) the high frequency shoulder of the monocarbonyl band at 2050 cm−1 is largely depleted, suggesting that species contributing to this adsorption are reversibly adsorbed.Unlike the case of  Rh/HTCarb_750, wheregem-dicarbonyl forms, in the Rh/HTSil_750 the RhI(CO) species do not evolve into RhI(CO)2 complexes. A possible explanation is that RhI(CO)2  species are not stabilized by the support. The role of the support in stabilizing RhI(CO)2species was previously suggested [29]; for instance,  it was reported that dicarbonyls are strongly favoured on Rh/Al2O3 compared to Rh/SiO2 [8, 21].Moreover, RhI(CO)2 were observed to be dominant species on Rh/TiO2 and Rh/Al2O3 reduced at 400°C, whereas this was not the case for Rh/SiO2 and Rh/MgO reduced at the same temperature, mostly at low CO pressure [8].Indeed, evidence of silicate forsterite-like phase (Mg2SiO4) is provided by XRD analysis, whereas no well-defined phase containing Al (MgAl2O4) is revealed, unlike  Rh/HTCarb_750. Moreover, MgO crystals are more extended in Rh/HTSil_750 than in Rh/HTCarb_750.It is worth noting that no carbonate-type  species form on Rh/HTSil_750 upon interaction with CO, strongly suggesting, together with previous data, that RhI(CO)2 are involved in CO disproportionation in these systems.The lower reactivity in CO disproportionation of Rh/HTSil_750, containing the silicate forsterite-like phase (Mg2SiO4) instead of  MgAl2O4, is in agreement with the observation that the extent of CO disproportionation on Rh catalyst follows the order Rh/Al2O3 > Rh/SiO2 > Rh/MgO [8].In conclusion, we propose that in Rh/HTCarb_750 Rh nanoparticles are affected by the Al-containing support, that is, the MgAl2O4 type phase in which the Rh has been reported to have larger solubility than for the MgO, when both phases are present  [12].  Instead, in Rh/HTSil_750 the metal is affected mainly by MgO, acting as support.Table2 summarizes IR data related to CO adsorption, together with Rh particle size obtained by TEM data analysis.Table 2
FT-IR data of  CO interaction at r.t. and Rh particle size evaluated by TEM analysis.
SampleνRh0CO (cm−1)νRhI(CO)2 (cm−1)ν(Rh2)CO (cm−1)COdisprop.cdparticles (nm)Rh/HTCarb_75020502096a—YES1.8Rh/HTCarb_95020602093,2032b1915small extent1.4Rh/HTSil_7502048——NO1.1a The asymmetric mode is overlapped with the monocarbonyl stretch.bLower relative amount with respect to Rh/HTCarb_750.cCO disproportionation as revealed by the formation of carbonate-like species.


## 3.1. Effect of the Reducing Temperature

In order to investigate the effect of reducing temperature on the system, the sample reduced at 950°C  (Rh/HTCarb_950) has been characterized following the same approach. The characterization has been completed by TEM analysis, and Figure5 shows the TEM micrographs of Rh/HTCarb_750 and Rh/HTCarb_950. The Rh is in the form of well-dispersed nanoparticles in both cases. As expected, the average particle size appears smaller for the catalyst reduced at lower temperature (1.4 nm) than for that reduced at 950°C (1.8 nm).TEM micrographs of Rh/HTCarb_750 (upper part) and Rh/HTCarb_950 (lower part).
(a)(b)Figure6  shows the spectrum recorded after contact of Rh/HTcarb_950 with CO (p = 30 mbar) at r.t.  and removal of the gas from the cell by outgassing. Spectra in presence of CO are similar and thus are not reported for sake of brevity.Figure 6
FT-IR spectrum recorded after contact of CO with Rh/HTCarb_950 at r.t. (D: gem-dicarbonyl, M: linear monocarbonyl, B: bridged-bonded CO, and C: carbonate-type species).The narrow band at 2060 cm−1 due to the Rh0(CO) species dominates the spectrum, whereas the symmetric mode of gem-dicarbonyl complexes appears as a shoulder at 2093 cm−1, accompanied by the twin peak as a tail hardly discernible at about  2030 cm−1. The relative intensity of the monocarbonyl band with respect to the symmetric gem-dicarbonyl mode is higher than for Rh/HTCarb_750, suggesting a larger population of the former species in the present case.Moreover, a broad absorption is observed at about 1910 cm−1, due to bridged-bonded carbonyl species, Rh02(CO) [25]. Both Rh0(CO) and Rh02(CO) arise from CO adsorbed on extended Rh faces. The lower amount of the former and the absence of the latter in Rh/HTCarb_750 are both in agreement with the existence of smaller Rh particles with respect to  Rh/HTCarb_950, as revealed by TEM analysis. In particular, it may seem that the limit of average crystal size above which bridged-bonded carbonyl species are formed falls in the range of 1.4–1.8 nm.Though several authors reported the formation of bridged-bond Rh2(CO) upon adsorption of CO on supported Rh, very rarely information on particle size from complementary techniques is provided. Finocchio et al. [10]  observed the occurrence of  bridged-bond Rh2(CO) on particles with estimated size of 3.2 nm.It is worth noting that in the case of Rh/HTcarb_950, only a very small amount of carbonate-like species are formed. The lower relative amount of RhI(CO)2   in the present case suggests that formation of carbonate-type  species is related to formation of gem-dicarbonyls upon reaction with CO. As observed for Rh/HTCarb_750, only monocarbonyl species are formed upon adsorption of CO at low temperature (spectrum not reported).


## 3.2. Role of the Support

The effect of the support has been investigated considering the reactivity of  Rh/HTCarb_750 and Rh/HTSil_750 towards CO at r.t.   Figure7 reports the IR spectrum recorded after contact of Rh/HTSil_750 with CO (p = 30 mbar) at r.t.  and removal of the gas from the IR cell by outgassing.Figure 7
FT-IR spectrum recorded after contact of CO with Rh/HTSil_750 at r.t.  Inset: spectra recorded at increasing CO pressure.A single band is visible at 2048 cm−1, due to monocarbonyl species on Rh surfaces. No bands due to gem-dicarbonyls are present, neither absorptions due to carbonate-type  species. The results show that in  Rh/HTSil_750  Rh  is definitely less reactive towards CO with respect to Rh/HTCarb_750.The lower reactivity cannot  be ascribed to larger Rh particle size, that  from TEM analysis (image  not reported) shows a size of   1.1 nm, that is  smaller than those observed on Rh/HTCarb_750.An affect of the support may be instead envisaged, that  may not favor the formation of RhI(CO)2. The inset of  Figure 7 reports the spectra recorded upon increasing CO pressure at r.t. Besides the shifting of the monocarbonyl band to higher frequency upon increasing coverage, due to dipole-dipole coupling among adsorbed CO molecules [10], a new component increases at 2078 cm−1 (labeled by an asterisk in figure). This absorption is depleted by outgassing at r.t., and in fact it is not visible in the spectrum reported in the main body of  Figure 7, revealing that the related species is labile and adsorbed reversibly. We tentatively assign this band to monocarbonyl species on oxidized Rh, that is,  RhI(CO) species [15]. A similar species was proposed to account for a band observed at 2087 cm−1 on Rh/TiO2 catalyst during decarbonylation [27]. These authors suggested  that this species is an intermediate in the conversion of RhI(CO)2 to Rh0(CO) and  proposed that the corresponding band is frequently overlapped with the band above 2090 cm−1 due to gem-dicarbonyl species, so being indiscernible in most cases. The same band had been previously observed during initial adsorption of CO at low temperature on Rh/Al2O3 and it was assigned to RhI monocarbonyl species [28].Assuming that the mechanism of decarbonylation is the reverse of the conversion of Rh0(CO) to RhI(CO)2, we propose that the labile RhI(CO) species forms at increasing CO coverage and it is a precursor of the gem-dicarbonyl species. It most probably forms also in the case of Rh/HTCarb_750 (Figure 2), being the band at 2078 cm−1 overlapped with the symmetric mode of the RhI(CO)2, as previously suggested [19]. Indeed, upon CO removal (Figure 3) the high frequency shoulder of the monocarbonyl band at 2050 cm−1 is largely depleted, suggesting that species contributing to this adsorption are reversibly adsorbed.Unlike the case of  Rh/HTCarb_750, wheregem-dicarbonyl forms, in the Rh/HTSil_750 the RhI(CO) species do not evolve into RhI(CO)2 complexes. A possible explanation is that RhI(CO)2  species are not stabilized by the support. The role of the support in stabilizing RhI(CO)2species was previously suggested [29]; for instance,  it was reported that dicarbonyls are strongly favoured on Rh/Al2O3 compared to Rh/SiO2 [8, 21].Moreover, RhI(CO)2 were observed to be dominant species on Rh/TiO2 and Rh/Al2O3 reduced at 400°C, whereas this was not the case for Rh/SiO2 and Rh/MgO reduced at the same temperature, mostly at low CO pressure [8].Indeed, evidence of silicate forsterite-like phase (Mg2SiO4) is provided by XRD analysis, whereas no well-defined phase containing Al (MgAl2O4) is revealed, unlike  Rh/HTCarb_750. Moreover, MgO crystals are more extended in Rh/HTSil_750 than in Rh/HTCarb_750.It is worth noting that no carbonate-type  species form on Rh/HTSil_750 upon interaction with CO, strongly suggesting, together with previous data, that RhI(CO)2 are involved in CO disproportionation in these systems.The lower reactivity in CO disproportionation of Rh/HTSil_750, containing the silicate forsterite-like phase (Mg2SiO4) instead of  MgAl2O4, is in agreement with the observation that the extent of CO disproportionation on Rh catalyst follows the order Rh/Al2O3 > Rh/SiO2 > Rh/MgO [8].In conclusion, we propose that in Rh/HTCarb_750 Rh nanoparticles are affected by the Al-containing support, that is, the MgAl2O4 type phase in which the Rh has been reported to have larger solubility than for the MgO, when both phases are present  [12].  Instead, in Rh/HTSil_750 the metal is affected mainly by MgO, acting as support.Table2 summarizes IR data related to CO adsorption, together with Rh particle size obtained by TEM data analysis.Table 2
FT-IR data of  CO interaction at r.t. and Rh particle size evaluated by TEM analysis.
SampleνRh0CO (cm−1)νRhI(CO)2 (cm−1)ν(Rh2)CO (cm−1)COdisprop.cdparticles (nm)Rh/HTCarb_75020502096a—YES1.8Rh/HTCarb_95020602093,2032b1915small extent1.4Rh/HTSil_7502048——NO1.1a The asymmetric mode is overlapped with the monocarbonyl stretch.bLower relative amount with respect to Rh/HTCarb_750.cCO disproportionation as revealed by the formation of carbonate-like species.


## 4. Conclusions

Rh metal particles obtained by reduction in diluted  H2 of Rh/Mg/Al calcined HT precursors have been characterized by FT-IR  analysis of adsorbed CO and TEM. The particle size increases from 1.4 nm to 1.8 nm when reduction temperature increases from 750°C to 950°C. The crystal growth causes, upon interaction with CO at r.t., the formation of bridged CO species and the increase of population of linear monocarbonyl in comparison to gem-dicarbonyl species.Disproportionation of CO occurs on Rh at r.t.,  giving rise to carbonate-, hydrogenocarbonate- and formate-type  species, and it accompanies the formation of RhI(CO)2, whereas no gem-dicarbonyl species and CO disproportionation are observed for reaction with CO at nominal liquid N2 temperature.The formation of RhI(CO)2 and disproportionation of CO at r.t.  do not occur for the sample obtained  from the silicate-containing HT precursor. A band at 2078 cm−1 is ascribed to a labile RhI(CO) species, which does not evolve into  gem-dicarbonyl species. This is attributed to an effect of the support, which, at variance with the system prepared from carbonate solution, does not contain a well-defined spinel phase. Instead, it contains a silicate forsterite-like phase, besides the MgO phase which acts as support.



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*Source: 458089-2011-08-22.xml*