Impact of Niobium in the Metal–Organic Framework-Mediated Synthesis of Co-Based Catalysts for Synthesis Gas Conversion
We report the use of transition metal precursors impregnated into the pores of CPO-27(Co) metal–organic framework (MOF) crystals prior to pyrolysis as a straightforward strategy for tuning the properties of MOF-derived Co-based catalysts. By adding a Nb inorganic salt prior to pyrolysis hierarchical pores are formed in the resulting carbon and the Co accessible surface area is greatly increased leading to a strong enhancement of CO hydrogenation activity.
KeywordsMetal–organic framework mediated-synthesis (MOF-MS) Heterogeneous catalysis Co Fischer–Tropsch synthesis In-situ spectroscopy High temperature XRD
Metal–organic frameworks (MOFs) are a class of porous, coordination compounds in which metal cations (or nodes) are connected to organic linker molecules forming a three-dimensional network with potential cavities . Liu et al. demonstrated in 2008 that MOFs can be used as templates for the synthesis of highly porous carbons via careful pyrolysis of the MOF crystals . This strategy has been intensively used for the preparation of metal-loaded carbon catalysts in recent years [3, 4, 5, 6]. The method presents three interesting features for the synthesis of heterogeneous catalysts, e.g. the inherent high tunability of MOFs, thus, of the properties of the resulting material; the high metal dispersion on the support; and finally, the entrapment of the metallic nanoparticles within the carbon support, which may slow down particle aggregation, a very common phenomenon in deactivation of solid catalysts during reaction conditions [7, 8].
A number of strategies of increasing complexity have been used in order to avoid full encapsulation such as creating hierarchical carbon structures  or promoting even more the growth of metal particles, in order to catalyse the formation of carbon nanotubes rather than a randomly interconnected porous network . A prominent example of MOF-templated catalyst synthesis was reported by Santos et al., who studied the formation of a Fe/FexCy/C catalyst that exhibited higher stability than benchmark Fe catalysts in the conversion of syngas, a mixture of CO and H2 [11, 12, 13, 14]. The influence of MOF hierarchical porosity and use of Na or S promoters, typically employed for Fe-catalysed Fischer–Tropsch synthesis (FTS), has been reported to profoundly impact their CO hydrogenation performance .
Contrary to the case of Fe, metal@carbon core–shell may be detrimental if the catalyst employed is Co, due to the fact that reaction is catalysed by the metallic Co0 surface, which may be covered by the aforementioned carbon matrix [16, 17, 18, 19]. One recently developed strategy to overcome this problem consisted of using the pores of ZIF-67(Co) as a nanocast for a silica precursor, which after calcination, resulted in a highly loaded Co/SiO2 catalyst . However, this method involved a hydrolysis and crystallization step of the silica precursor, and little control over the properties of the support itself. Thus, we explore the use of a simple impregnation step of a transition metal precursor into the pores of the MOF prior to pyrolysis. The use of transition metals loaded in the pores of a MOF to hierarchically structure the carbon matrix during pyrolysis has been studied . Nevertheless, to the best of our knowledge, the use of such synthetic route for the preparation of Co catalysts for FTS has not been previously investigated.
2 Experimental Section
2.1 Materials Synthesis
2.1.1 CPO-27(Co) Crystals
For the synthesis of CPO-27 (Co) crystals a previously reported procedure was used . In brief, cobalt nitrate hexahydrate (5.943 g, 20.4 mmol, 99 + %, Acros Organics) and 2,5-dihydroxyterephthalic acid (1.205 g, 6.08 mmol, 98%, Sigma-Aldrich) were introduced into 400 mL of a 1:1:1 v/v/v mixture of N,N-dimethylformamide (99.8% anhydrous, Sigma-Aldrich), ethanol (98%, VWR International) and deionized water within a 1 L sealed Schott bottle. The bottle was heated at 383 K for 24 h in an oven, then, the solution allowed to cool down to room temperature naturally. The supernatant liquid was removed by decantation and 200 mL of fresh ethanol introduced, in order to exchange the solvent within the pores. The ethanol was replaced after 4 h for other 200 mL of ethanol. After 8 h, the solid was recovered by centrifugation (3000 rpm, 5 min) and dried at 333 K in air for 16 h. Activation of the MOF prior to Nb impregnation consisted of drying under dynamic vacuum (p < 0.1 bar) at 423 K for 1 h of the framework.
2.1.2 Incipient Wetness Impregnation (IWI)
Impregnation of the evacuated materials was done by adding the necessary amount ammonium niobium oxalate (ANO, Companhia Brasileira de Metalurgia e Mineração) in ultrapure water (Metrohm Lab filtration station, 18.2 MΩ cm, 25 °C) dropwise under constant stirring of the powder in vacuum, attaining a Nb:Co atomic ratio of 0.0157.
Calcination of the MOF materials was done in a fixed-bed tubular quartz reactor were ca. 250 mg were placed, under a N2 (Linde, 99.9998%) flow of 50 mL min−1 at 333 K for 1 h, then at 773 K for 4 h, by using a ramp of 5 K min−1 to heat up the reactors. No specific passivation method was used after naturally cooling down to room temperature.
2.2 Materials Characterization
X-ray diffraction (XRD) patterns were obtained by a Bruker-AXS D2 Phaser powder X-ray diffractometer using Co Kα1,2 with λ = 1.79026 Å, operated at 30 kV, the sample holder rotated at 15 rot min−1. Measurements were carried out between 5 and 70 2θ° using a step size of 0.05 2θ step−1 and a scan speed of 1 s/step. Simulated CPO-27(Co) pattern was obtained from the previously resolved structure in Ref.  (cif file, Mercury 3.7© software (Co Kα1,2 λ = 1.79026 Å, FHWM = 0.2)). In the case of the Co@C materials, XRD was measured in the 30–60 2θ° range with the same parameters and instrument described above.
CO2adsorption/desorption isotherms at 195 K was determined on an AutoSorb I (Quantachrome) instrument. The materials were previously degassed in vacuum (p < 10−5 mbar) at 473 K for 16 h prior to the sorption measurements. BET area and pore volumes were calculated according to the consistency criteria established by Rouquerol et al. . Pore size distributions were obtained by using non-local density functional theory (NLDFT) method (assuming CO2 at 195 K on Carbon Slit pores in MicroActive®, Micromeritics, version 4.06).
Scanning electron microscopy (SEM) images of the CPO-27(Co) crystals were obtained by depositing the powder sample of carbon tape (no sputtered Au or Pt was added). The images were recorded with a PhenomPro™ scanning electron microscope equipped with a back-scattering detector (BSD), a CsB filament and operated at 5 kV and a × 2800 magnification.
N2adsorption/desorption isotherm measurements at 77 K were carried out in a Micromeritics Tristar 3000 apparatus, calculation of BET, the interval between p/p0 = 0.05–0.3, and the desorption BJH method, along with the t-plot method for the calculation of external/internal surface area ratio. Samples were pretreated at 473 K under a N2 flow of 10 mL min−1 for 16 h prior to the adsorption measurements. The hysteresis loop in (a) reveals the presence of uniform mesopores as well as micropores (H-type I, according to IUPAC), while (b) only shows the presence of ill-defined micropore systems (H-type II), and a cavitation step during desorption at p/p0 = 0.5.
Thermogravimetrical analysis (TGA) was performed using a TGA Q50 equipment (TA Instruments, USA). Typically, ca. 20 mg of sample were placed in a platinum crucible under 40 cm3 min−1 air flow and heated until 1073 K (15 K min−1), 40 cm3 min−1 N2 flow was used as reference.
X-ray photoelectron spectroscopy (XPS) data were acquired on a Thermo Scientific K-Alpha spectrometer using a Al Kα (hν = 1486.6 eV) monochromatic small-spot X-ray source. Charging effects were corrected by using the adventitious carbon C1s (sp3) peak as reference for all samples at a binding energy (BE) of 284.8 eV. Analysis of the XPS spectra was done with CasaXPS, in which Shirley background was removed and the peaks assigned. Gaussian peaks were assumed for the fitting of the spectra (BE, full width at half maximum—FWHM; peak shape, peak asymmetry and number of species), which was performed with Fiytk© software, version 0.8.6. Levenberg–Marquardt fit.
Raman spectroscopy was carried out with a Renishaw InVia™ microscope equipped with a CCD detector, a 532 nm laser and a 1200 lines/mm grating. The samples were deposited on a quartz cover and measured with a laser output power of 0.24 mW (i.e., 1.12 × 10−5 W cm−2), 50 × objective, 10 accumulations with an integration time of 10 s. Savitzky-Golay filter was applied over a smooth window of 9, with a square polynomial order.
High-temperature XRD experiments were carried out in a Bruker D8 diffractometer in Bragg–Brentano geometry, equipped with a high-temperature cell, a Co Kα,β (λ = 1.79026 Ǻ) source and a LYNXEYE detector. Samples were introduced in the flat Si holder and flushed with a He flow of 20 mL·min−1 for 10 min. Then, diffractograms were recorded with 0.041° step−1 and 1 s step−1 measurement time during a temperature program starting at 298 to 773 K, with a heating ramp of 2 K min−1.
Scanning Transmission Electron Microscopy-High Angle Annular Dark Field (STEM-HAADF) images and energy dispersive X-ray spectroscopy (EDX) analysis were obtained with an FEI Talos F200X transmission electron microscope, operated at 200 kV and equipped with a high-brightness field emission gun (X-FEG) and a Super-X G2 EDX detector. More than 150 particles were measured to obtain a particle size distribution. Bright field images were recorded on a FEI Tecnai 12 Icor TEM operating at 120 kV. Samples were prepared by drop-casting a colloidal solution on a carbon-coated TEM grid, which were left to dry in air.
2.3 Catalytic Testing
The evaluation of the catalytic performance was performed using a quartz glass plug-flow reactor, loaded with ca. 20 mg catalyst (sieve fraction: 38–150 μm) diluted with ca. 200 mg of SiC. The catalysts were reduced in situ at 623 K (5 K min−1, 2 h) in Ar:H2 = 2.0 v/v flow (GHSV = 190,000 h−1). After reduction, the reactor temperature was changed to 493 K (5 K min−1) and once the temperature was reached the atmosphere was changed to synthesis gas (H2:CO = 2.0 v/v, GHSV = 28,000 h−1, 1 bar). The reaction was carried out for 100 h for each catalyst. Analysis of C1 to C18 products was done with an online gas chromatograph (Varian 430 GC, CP sil-5 column).
3 Results and Discussion
For this study, CPO-27(Co) needle-like crystals of ca. 20 µm length were prepared as described in previously reported literature . Phase purity, crystallinity, morphology and porosity were confirmed by X-ray diffraction (XRD), scanning electron microscopy (SEM) and CO2 adsorption isotherms at 195 K (Sects. 1–4 of the Electronic Supplementary Information, ESI). Thereafter, the material was degassed and impregnated with an aqueous solution of ammonium niobium (V) oxalate (ANO), attaining a Nb:Co atomic ratio of 0.0157 (see ESI for details). After drying, the material was pyrolyzed in a fixed-bed reactor (773 K, ramp 5 K min−1, 4 h, 50 mL min−1 N2 flow) to obtain NbOx-Co@C composites by MOF degradation.
The presence of Nb species in the pores of CPO-27(Co) resulted in the formation of mesopores in the carbon matrix, in contrast to pristine CPO-27(Co), as demonstrated by N2 physisorption at 77 K (Fig. 1b). Co@C showed an isotherm type II (ill-defined micropores) and the BJH pore size distribution revealed the presence of 3–4 nm mesopores in the carbon matrix (Fig. 1c). In contrast, the NbOx-Co@C composite exhibited the presence of large mesopores (20–35 nm) with ca. 4 nm pores still being present, as evidenced by the isotherm type I and the pore size distribution.
BET apparent surface area of the resulting NbOx-Co@C material was 428 m2 g−1, in contrast to the non-promoted CPO-27(Co) pyrolyzed MOF, with BET surface area of 235 m2 g−1 (see Sect. 5 in the SI for details). This observation indicates that impregnation with NbOx-precursor solution leads to the formation of larger pores throughout the carbon network. Consequently, the total pore volume of the materials was found to be 0.89 and 0.21 cm3 g−1 for the NbOx-Co@C and Co@C materials, corroborating the presence of a much higher internal pore space in the case of the Nb-promoted system.
In order to study the location of Nb after pyrolysis, TEM–EDX maps of the obtained NbOx-Co@C (Fig. 2a–d) show that Nb is in close vicinity to the Co inside the C matrix. Thus, not only the porosity of the carbon supports was affected, but also the growth of the metal clusters was affected by the inclusion of ANO into the honeycomb structure of CPO-27(Co). Particle surface average diameters (d32) of both materials obtained from TEM (Fig. 2e) show a larger average size and broader size distribution for NbOx-Co@C (ca. 25 nm) compared to Co@C (ca. 11 nm), indicating that the Nb precursor has a strong effect on the growth of Co nanoparticles during pyrolysis.
Although the porosity and particle size were affected, we sought to verify if the metal nanoparticle were more accessible after pyrolysis of the Nb impregnated MOF. Indeed, the increase in porosity was critical for the accessibility to the entrapped Co nanoparticles as shown by H2 chemisorption experiments (Fig. 2d). Despite exhibiting a higher average particle size, the promoted material possesses more than four times accessible Co0 sites compared to the Co@C material, confirming our hypothesis. Additionally, TGA under air flow was used to estimate the final cobalt content of the pyrolysed materials, resulting in ~ 50 wt % for both materials (Fig. S5). Surprisingly, the increase in porosity did not result in a higher degree of oxidation of the Co particles, which are typically oxidized to CoxOy in air. X-ray diffraction of the obtained materials (Fig. S6) shows the presence of only one peak dominating the diffractogram at 51°, which corresponds to a metallic Co fcc lattice. However, it cannot be excluded that the exposed cobalt was oxidized and the fraction of the oxide was too low and/or amorphous to be detected by XRD.
XPS analysis of the NbOx-Co@C catalyst in Sect. S7 of the Supporting Information showed the presence of both Co and CoxOy species. Specifically, the Co 2p XPS peaks in Fig. S8 fitted at 802.7, 796.4, 785.6 and 780.4 eV were assigned to CoO, while the Co 2p XPS peak at 792.6 eV corresponds to Co3O4 . Significant presence of reduced Co0 was confirmed by the peak at 778.2 eV, and the presence of the LMM Auger emission peak [26, 27, 28]. In addition, the XPS peaks at 209.6 and 206.9 eV, corresponding to Nb 3d3/2 and 3d5/2 lines, respectively, indicated that the promotor is present as niobium (V) oxide (Fig. S9) .
In order to further study the structure of the carbon support, both XPS and Raman spectroscopies were used. On the one hand, the XPS peaks at 284.1, 285.8 and 288.8 eV were assigned to C sp2, C–O and C=O species (i.e. acid and –OH groups) on the carbon surface, respectively (Fig. S10). On the other hand, Raman spectra of the pyrolyzed materials (irrespective of the promoter) showed the typical D and G bands (at 1365 and 1595 cm−1, respectively, with an I(D)/I(G) =0.82), as well as the absence of the second 2D’ band at 2400–2700 cm−1, indicating a disordered nanocrystalline graphitic matrix with high content of amorphous sp2 hybridized carbon (Fig. S11) [30, 31]. In addition to those Raman bands, a number of peaks at 198, 480, 522, 618 and 687 cm−1 corresponding to Co3O4 appeared for both the pristine and the Nb-loaded Co@C samples . This was in line with the TEM–EDX map in Figs. 2d, that shows an O signal around the Co particles, suggesting that the entrapped Co species consist of bulk metallic Co0 crystallites surrounded by a thin layer of CoOx oxides.
Activity and selectivity of NbOx-Co@C and Co@C in the production of long-chain hydrocarbons during Fischer–Tropsch Synthesis (FTS) at time-on-stream (TOS) = 100 h
Initial TOF (10−3 s−1)c
The product distribution was similar for both materials at TOS = 100 h (Fig. S16), despite the reported promotional effect of NbOx for C5+ formation. This could be due to the low Nb loading or the unknown crystallinity of NbOx, two features that can have a strong influence [38, 39]. As mentioned before, the carbon surface exhibited acid groups (–COO and –OH), which might as well affect the selectivity of the materials  TEM images of the catalysts after 100 h of reaction (Figs. S17 and S18) showed Co particle growth for both materials, with the largest growth in surface average diameter for the NbOx-Co@C catalyst from 25 to 34 nm compared to 11 to 12 nm for Co@C. Both materials showed bimodal particle size distributions with smaller particles within the 5–20 nm range, most likely still entrapped in the carbon matrix, and the formation of agglomerates of 20–50 nm diameters. These agglomerates are present in the NbOx-Co@C catalyst to a larger extent, suggesting that particle sintering may be the reason for the activity decrease in CO hydrogenation.
We have described how by simply impregnating a particular Metal-MOF material, namely CPO-27(Co), with a Nb precursor solution, the properties of the resulting MOF-derived Co@C material can be tuned. Although the exact mechanism remains elusive, we have demonstrated how Nb can strongly influence the porosity of the obtained carbon matrix, thus, availability of entrapped metallic nanoparticles, rendering this composite a potential catalyst for hydrogenation reactions. Despite an initial loss of activity, hydrocarbon productivity from syngas of the NbOx-Co@C material showed appreciable stability for at least 100 h of operation. Thus, we can conclude that active and stable Co-FTS catalysts can be prepared by this strategy, combining the use of transition metal promoters and metal–organic framework mediated synthesis. Moreover, we believe that this method represents an interesting alternative for the introduction of promoters in close proximity of the active, nanoparticulate phase. These findings could guide the way for the synthesis of hierarchically structured, efficient MOF-derived catalyst materials for various chemical reactions.
This project has received funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant Agreement No. 641887 (DEFNET). Companhia Brasileira de Metalurgia e Mineração (CBMM) is thanked for financial support of this research. KPdJ acknowledges the European Research Council, EU FP7 ERC Advanced Grant no. 338846. P. Vervoorts (TU München, Germany) is gratefully acknowledged for measuring CO2 adsorption. We are thankful to W. S. Lamme (Utrecht University, UU) for measuring TEM–EDX of the materials; D. Wezendonk and M. Versluijs-Helder (UU) for the in situ XRD measurements and J. L. Weber (UU) for help with the thermogravimetry analysis. We are thankful to Dr. F. E. Oropeza-Palacio, Dr. J. P. Hofmann and Prof. E. J. Hensen (all from TU Eindhoven) for measuring XPS of the promoted sample.
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