research papers
Rietveld and pair distribution function study of Hägg carbide using synchrotron X-ray diffraction
aSasol Technology R&D, South Africa, bUniversity of Pretoria, South Africa, cUniversity of Johannesburg, South Africa, dESS AB, Stora Algatan 4, 22100 Lund, Sweden, eNMMU, Port Elizabeth 6031, South Africa, and fInstitut Laue-Langevin, BP 156, 38042 Grenoble Cedex 9, France
*Correspondence e-mail: axel.steuwer@esss.se
Fischer–Tropsch (FT) synthesis is an important process in the manufacturing of hydrocarbons and oxygenated hydrocarbons from mixtures of carbon monoxide and hydrogen (syngas). The reduced iron catalyst reacts with carbon monoxide and hydrogen to form bulk Fe5C2 Hägg carbide (χ-HC) during FT synthesis. Arguably, χ-HC is the predominant catalyst phase present in the working iron of the working catalyst can be due to oxidation of χ-HC to iron oxide, a step-wise decarburization to cementite (θ-Fe3C), carbon formation or sintering with accompanying loss of catalytic performance. It is therefore critical to determine the precise of χ-HC for the understanding of the synthesis process and for comparison with the first-principles ab initio modelling. Here the results of high-resolution synchrotron X-ray powder diffraction data are reported. The atomic arrangement of χ-HC was confirmed by and subsequent real-space modelling of the pair distribution function (PDF) obtained from direct Fourier transformation. The Rietveld and PDF results of χ-HC correspond well with that of a pseudo-monoclinic phase of Pī [a = 11.5661 (6) Å, b = 4.5709 (1) Å, c = 5.0611 (2) Å, α = 89.990 (5)°, β = 97.753 (4)°, γ = 90.195 (4)°], where the Fe atoms are located in three distorted prismatic trigonal and one octahedral arrangement around the central C atoms. The Fe atoms are distorted from the prismatic trigonal arrangement in the monoclinic structure by the change in C atom location in the structure.
Keywords: Hägg carbide; Fischer–Tropsch synthesis; crystal structure; PDF.
1. Introduction
Recent fluctuating oil prices and increasing environmental concerns have stimulated renewed interest in the production of synthetic hydrocarbons (fuels) by Fischer–Tropsch synthesis (FTS) using biomass, natural gas or coal as starting material (Dry, 1990; Riedel & Schulz, 2003a,b; Campos et al., 2010). The FTS involves a catalyst, and one of the most commonly used commercial catalyst is Fe-based, starting from oxides with small amounts of promoter substances such as Cu, K, SiO2 added to improve performance (Herranz et al., 2006; Niemantsverdriet et al., 1980). The Fe catalysts require an activation pre-treatment (using CO, syngas, hydrogen) and, in order to increase the efficiency, nanoscale oxide powders with high surface-to-bulk ratios are being used (Sarkar et al., 2007). During activation the iron oxides evolve, resulting in the formation of metallic iron and a range of carbides depending on temperature, pressure of carbon-containing gases, concentration, time of exposure, etc. Subsequent annealing results in a diffusion-determined de-carburization process forming stable cementite. Cementite and other iron carbide phases have also been observed to form via lattice-invariant deformation after carbon ion implantation into thin iron layers (Königer et al., 1997). Experimental evidence suggests that the activity (and hence performance) of the Fe-based catalyst is critically dependent on the presence and type of carbides on the surface (Herranz et al., 2006). There is a range of meta-stable and stable iron carbides, and the differences in are relatively subtle but distinct, and can be confirmed with the aid of electron diffraction (Hirotsu & Nagakura, 1972; du Plessis et al., 2007). In general, the iron carbides can be divided into carbides with C atoms on octahedral interstitial sites (O-carbides) such as ∊-Fe2C, ∊′-Fe2.2C and FexC, and carbides with C atoms on trigonal prismatic interstices such as η-Fe2C and χ-Fe5C2 (Hägg) and the (stable) cementite phase θ-Fe3C. The exact nature of the carbonaceous species on the surface and in the bulk over the catalyst has been the subject of intense investigations over recent years (Herranz et al., 2006; Steynberg et al., 2008; Faraoun et al., 2006; Mansker, 1999; Pérez-Alonso et al., 2007), but experimental evidence points at the Hägg carbide being the prevalent phase under `steady-state' FTS conditions and principally responsible for FTS activity. During FTS the of syngas is kept constant, promoters are added to aid the dissociation of carbon and oxygen on the catalyst surface, and the de-carburization process of Hägg carbide to cementite is thus limited.
The oxidation of iron and iron carbides to magnetite is a postulated deactivation mechanism of the catalyst, owing to the water–gas shift reaction taking place (Sarkar et al., 2007; Mansker, 1999). Molecular dynamic simulation studies of the interaction of carbon with self-interstitial clusters in α-iron indicated the octahedral site as the most stable one for the carbon interstitial and the tetrahedral site as the saddle point for carbon jump from one octahedral site to another (Tapasa et al., 2007). It was shown that the iron lattice volume expands owing to a C atom addition to self-interstitial atom clusters. At 300 K a cluster of seven self-interstitial atoms with one or two C atoms was found to be essentially immobilized. The cluster co-migrated with C atoms at 600 and 900 K. Dissociation of carbon from the iron cluster at 1200 K was reported.
The self-diffusion coefficients of carbon at 773 K were determined in both cementite and Hägg carbide under high carburizing atmospheres (Schneider & Inden, 2007). Metal dusting was applied to limit graphite deposition. The mechanism of carbon diffusion is not known and the carbon is dependent on the difference between the surfaces and interfaces of phases containing different stoichiometric abundances of carbon.
The accurate et al., 2006; Niemantsverdriet et al., 1980; du Plessis et al., 2007; Hägg, 1931; Retief, 1999; Senateur, 1962). The meta-stable carbides are very sensitive to exposure to air/water and changes in temperature, which may result in rapid deactivation of the working catalyst owing to oxidation of χ-HC to iron oxide, a step-wise decarburization to cementite (θ-Fe3C), carbon formation and/or sintering. However, the fundamental understanding of the catalysis process and the focused development towards more efficient catalyst using tools requires a better understanding of the precise interaction between carbon and iron, and the precise carbide structure and distribution during FTS.
of the carbides during FTS conditions is challenging, and further complicated by the small crystallite size of the powders (HerranzRecently, the et al., 2007). The agreement of structure factors between the calculated and experimental powder patterns was significantly improved when using the triclinic structure instead of the monoclinic structure as previously reported by Senateur (1962) of χ-HC. Small but statistically significant differences (Steynberg et al., 2008) in the parameters when using monoclinic and pseudo-monoclinic structures of χ-HC exposed the need for higher-resolution synchrotron X-ray diffraction data. The pseudo-monoclinic was re-determined from and powder X-ray diffraction by using simulated annealing, a direct-space algorithm in Topas (Coelho, 2000). It had to be determined whether the bulk structure of χ-HC extended to the surface of the particles, since this will be the interface available for FTS. Quantitative phase analysis using total-scattering analysis (PDF) was used to determine whether amorphous surface species exist on the χ-HC crystallites. In this manuscript we report on the results of the synchrotron X-ray powder diffraction experiments undertaken on beamline ID31 at the ESRF, Grenoble, France. In addition to conventional high-resolution Bragg scattering, the available range in diffraction angles (or rather Fourier space) further allowed the total-scattering analysis of the diffractogram using the PDF approach (Qiu et al., 2004).
was re-determined by laboratory powder X-ray diffraction and (du Plessis2. Experimental
A synthetic powder sample with particle sizes between 5 and 40 µm (Fig. 1) containing mainly χ-HC was prepared by carburization of iron with carbon monoxide at 603 K for 6 h. The individual grains are of the order of tens of nanometres (as determined by Rietveld refinement) and are not visible in Fig. 1.
The sample contained no catalysis promoters and can be considered to be a model Fischer–Tropsch catalyst. χ-HC was passivated at room temperature by exposing the sample to 0.5% oxygen in helium for 2 h to prevent oxidation during unloading of the iron carbide. The unloaded powder was packed in a 0.50 mm capillary. The diffraction experiment was undertaken on beamline ID31 at the ESRF. The wavelength was set to 0.3947 Å, equivalent to 31.4 keV. The diffractogram was collected to a maximum angle of 45° 2θ (0.0085° 2θ step size) to obtain the resolution required for accurate and as well as the PDF analysis. Longer counting times were used at higher Q-space values. The Q-space probed was thus 1.11 to 12.18 Å−1. A reference standard, LaB6, was measured for characterizing the experimental configuration. The software package Topas4 was used for The PDF was determined by direct Fourier transform of the total X-ray scattering data using the software PDFGetX2 (Qiu et al., 2004).
3. Results
3.1. Results from Rietveld analysis
The basic χ-Hägg was re-determined by laboratory powder X-ray diffraction and selected area electron diffraction (du Plessis et al., 2007), and the current measurements on ID31 follow essentially the same approach and are therefore reported here in slightly abbreviated fashion. The fundamental parameter approach was used to deconvolute instrumental and sample broadening observed in the diffractogram. The instrumental broadening was determined by of a reference LaB6 diffractogram, using instrumental broadening parameters as available in Topas4. The instrumental broadening parameters were then fixed during of the χ-HC diffractogram. Line broadening observed for the individual crystalline phases was then modelled using the appropriate phase-dependent parameters available in Topas4. During of the final χ-Hägg carbide structure using the pseudo-monoclinic the atomic displacement parameters of all the Fe atoms in the phases were restrained as a common isotropic parameter which refined to a value of u = 0.25 (2) Å2 and the common isotropic parameter for the C atoms in the iron carbide phases refined to u = 0.01 (3) Å2. The isotropic atomic displacement parameter of the C atoms in χ-Hägg carbide was restrained with a minimum limit of 0.01 Å2, as this parameter diverged to negative values during an unconstrained All atomic sites in the crystalline phases were fully occupied (site occupancy factor = 1). The published structures of χ-HC (du Plessis et al., 2007), θ-Fe3C (Meinhardt & Krisement, 1962) and α-Fe (Swanson et al., 1955) were used. The sample contained formed during preparation of the sample and this was modelled as a single broad peak and therefore excluded from the quantitative phase analysis. The crystalline size broadening contribution to the χ-HC reflections was modelled with a Lorentzian function and the volume column height LVol (Snyder et al., 1999) was found to be 36 (1) nm from the Similarly, the strain broadening contribution was modelled using a Voigt function and the apparent strain broadening value was found to be ∊0 = 0.075 (2). The approach was as follows. The instrumental broadening contribution was determined from a of the LaB6 standard. This instrument parameter file was then used for the of the χ-HC sample. After determination of the zero error [0.004 (1) Å], this value was fixed and the lattice parameters and relative atomic coordinates of χ-HC were refined. The lattice parameters and relative atomic coordinates of θ-Fe3C and α-Fe were fixed to the published values for the initial Upon obtaining an improved fit of χ-HC to the experimental diffractogram, the θ-Fe3C and α-Fe lattice parameters and average crystallite sizes were refined. The improved values were then fixed and the final step was to refine the lattice parameter, relative atomic coordinates and average crystallite size of χ-HC. The agreement values (Young, 1995) were Rwp = 9.25%, S = 2.9% and RBragg = 4.0%, as compared with Rwp = 12.7%, S = 4.0% and RBragg = 6.6% when refining the same synchrotron diffraction data using the structure as published by Retief (1999). The experimental and theoretical diffractograms of χ-HC can be seen in Fig. 2, together with a visualization of the unit cell.
of3.2. Results from PDF analysis
Unlike most conventional X-ray diffraction data, the diffractograms collected on ID31 lend themselves to analysis via a PDF approach. The PDFs [G(r)] for χ-HC, θ-Fe3C and α-Fe were calculated and refined using PDFGui software (Farrow et al., 2007). The fit between the experimental and theoretical PDFs is shown in Fig. 3. The lattice parameters, relative abundances of the phases and relative atomic coordinates and atomic displacement parameters thereof were refined for both the monoclinic and pseudo-monoclinic structures of χ-HC. Since the bulk crystalline phases were identified and quantified during the analysis, these phases were used as starting models for the PDF analysis. The relative abundances and atomic coordinates of all the phases (χ-HC, θ-Fe3C, α-Fe) were refined as well as the isotropic atomic displacement parameters. A spherical nanoparticle shape was assumed and found to be sufficient. The peaks visible on the experimental PDF do not have an increased broadening at higher R values, indicating that there is no stacking disorder visible up to 20 Å. The PDF does not display a typical nanocrystalline decrease of peak intensities and this result correlates with the large average crystallite size obtained from i.e. 36 (1) nm. An Rwp value of 12.9% and reduced χ2 value of 15.4% was obtained when fitting the experimental and theoretical PDFs when using the pseudo-monoclinic of χ-HC, indicating that the bulk phases extended to the surface of the particles. The interatomic distances in the range 1.8–2.2 Å are assigned to iron to carbon, mainly from χ-HC, and the peak intensity and width match well, indicating that all interatomic distances of 1.8–2.2 Å in the sample are explained by the phases included in the PDF The larger interatomic distances can be assigned to iron–iron, iron–carbon and carbon–carbon interactions.
The presence of 1–2 wt% α-iron (reactant) was detected in the synchrotron X-ray diffractogram when carrying out the which was not visible using laboratory X-ray data, probably owing to the small crystallite size (44 nm, from Rietveld refinement) and peak overlap of the (011) reflection of α-iron with the χ-HC (121) reflection. The α-iron phase was included during a trial of the laboratory X-ray data, but refined to zero. The (011) reflection of α-iron in the synchrotron X-ray diffractogram is indicated by a red arrow in Fig. 4.
However, using the PDF approach (Farrow et al., 2007; Qiu et al., 2004) it was possible to refine the nanocrystalline structure of χ-HC, which confirmed the triclinic structure to be prevalent in the synthetically prepared χ-HC. The lattice parameters, relative abundances, atomic displacement parameters and relative atomic coordinates of χ-HC were optimized during the PDF refinements. A comparison of the relative abundances of the crystalline phases obtained from the Rietveld refinements (using the C2/c and crystal structures of χ-HC) and the agreement values are listed in Table 1; it is clear from the table that the of χ-HC is indeed , as indicated by improved agreement values.
|
4. Discussion
Theoretically, the optimal packing of Fe atoms around the central C atoms in the monoclinic structure is simple trigonal prisms (Hirotsu & Nagakura, 1972; Dirand & Afqir, 1983). In the both the Fe and C atoms are allowed additional positional freedom during the This provided a better fit of the experimental diffractogram and suggests that the Fe atoms in the are arranged in three different types of distorted trigonal prisms and an octahedron around the central C atoms (compare Fig. 5).
The PDF approach was used to refine the nanocrystalline structure of χ-HC. From the agreement between the Rietveld and PDF refinements it can be deduced that the bulk structure probably extends to the surface of the powder particles. Differences in relative abundances between Rietveld and PDF quantitative refinements usually indicate local structural disorder (Egami & Billinge, 2003). The distortions of the trigonal prisms are thus not due to local disorder but are possibly due to the mobility of carbon in the bulk structure. The relative atomic coordinates as fractions of the of χ-HC are listed in Table 2. The values Δx, Δy and Δz indicate the deviations in the relative atomic coordinates of the atoms from those in the monoclinic structure (C2/c). These relative atomic coordinate displacement values suggest that the C atoms could be mobile in the χ-HC crystal structure.
|
To summarize, high-resolution synchrotron X-ray diffraction data were obtained on beamline ID31 at the ESRF and confirmed the pseudo-monoclinic structure of χ-HC. In addition to confirmation of the true of χ-HC, the presence of 1–2 wt% iron was detected in the sample using synchrotron X-rays, which was not visible using laboratory X-ray diffraction. Using the PDF approach it was also possible to refine the nanocrystalline structure of χ-HC, which proved the triclinic structure to be prevalent in the unloaded catalysts. It is also clear from comparing Rietveld and PDF quantitative phase analyses that the bulk χ-HC structure extends to the surface of the χ-HC particles. The Fe atoms are located in three distorted prismatic trigonal and one octahedral arrangement around the central C atoms, an arrangement which is significantly different from the monoclinic structure of χ-HC as described and reported previously.
Acknowledgements
We gratefully acknowledge Sasol Technology R&D Pty Ltd, South Africa, for funding, and acknowledge the ESRF (Grenoble, France) for provision of beam time on the high-resolution powder diffraction beamline ID31.
References
Campos, A., Lohitarn, N., Roy, A., Lotero, E., Goodwin, J. G. Jr & Spivey, J. J. (2010). Appl. Catal. A, 375, 12–16. CrossRef CAS Google Scholar
Coelho, A. A. (2000). J. Appl. Cryst. 33, 899–908. Web of Science CrossRef CAS IUCr Journals Google Scholar
Dirand, M. & Afqir, L. (1983). Acta Metall. 31, 1089–1107. CrossRef CAS Google Scholar
Dry, M. E. (1990). Catal. Lett. 7, 241–252. CrossRef CAS Web of Science Google Scholar
Egami, T. & Billinge, S. J. L. (2003). Underneath the Bragg Peaks: Structural Analysis of Complex Materials. Oxford: Pergamon/Elsevier. Google Scholar
Faraoun, H. I., Zhang, Y. D., Esling, C. & Aourag, H. (2006). J. Appl. Phys. 99, 093508. Web of Science CrossRef Google Scholar
Farrow, C. L., Juhas, P., Liu, J. W., Bryndin, D., Bozin, E. S., Bloch, J., Proffen, T. & Billinge, S. J. L. (2007). J. Phys. Condens. Matter, 19, 335219. Web of Science CrossRef PubMed Google Scholar
Hägg, G. (1931). Phys. Chem. B12, 33–56. Google Scholar
Herranz, T., Rojas, S., Perez-Alonso, F. J., Ojeda, M., Terreros, P. & Fierro, J. L. G. (2006). J. Catal. 243, 199–211. CrossRef CAS Google Scholar
Hirotsu, Y. & Nagakura, S. (1972). Acta Metall. 20, 645–655. CrossRef CAS Google Scholar
Königer, A., Hammerl, C., Zeitler, M. & Rauschenbach, B. (1997). Phys. Rev. B, 55, 8143–8147. Google Scholar
Mansker, L. D. (1999). PhD thesis, The University of New Mexico, NM, USA. Google Scholar
Meinhardt, D. & Krisement, O. (1962). Arch. Eisenhuettenwes. 33, 493–499. CAS Google Scholar
Niemantsverdriet, J. W., Van der Kraan, A. M., Van Dijk, W. L. & Van der Baan, H. S. (1980). J. Phys. Chem. 84, 3363–3370. CrossRef CAS Web of Science Google Scholar
Pérez-Alonso, F. J., Herranz, T., Rojas, S., Ojeda, M., López Granados, M., Terreros, P., Fierro, J. L. G., Gracia, M. & Gancedo, J. R. (2007). Green Chem. 9, 663–670. Google Scholar
Plessis, H. E. du, de Villiers, J. P. R. & Kruger, G. J. (2007). Z. Kristallogr. 222, 211–217. Google Scholar
Qiu, X., Thompson, J. W. & Billinge, S. J. L. (2004). J. Appl. Cryst. 37, 678. CrossRef IUCr Journals Google Scholar
Retief, J. J. (1999). Powder Diffr. 14, 130–132. CrossRef CAS Google Scholar
Riedel, T. & Schulz, H. (2003a). Topics Catal. 26, 1–4. Google Scholar
Riedel, T. & Schulz, H. (2003b). Topics Catal. 26, 41–54. Web of Science CrossRef CAS Google Scholar
Sarkar, A., Seth, D., Dozier, A. K., Neathery, J. K., Hamdeh, H. H. & Davis, B. H. (2007). Catal. Lett. 117, 1–17. Web of Science CrossRef CAS Google Scholar
Schneider, A. & Inden, G. (2007). CALPHAD, 31, 141–147. CrossRef CAS Google Scholar
Senateur, J. P. (1962). C. R. Acad. Sci. 255, 1615–1616. CAS Google Scholar
Snyder, R. L., Bunge, H. J. & Fiala, J. (1999). Editors. Microstructure Analysis from Diffraction, pp. 94–124. Oxford University Press. Google Scholar
Steynberg, P. J., van den Berg, J. A. & Janse van Rensburg, W. (2008). J. Phys. Condens. Matter, 20, 064238. Web of Science CrossRef PubMed Google Scholar
Swanson, H. E., Fuyat, R. K. & Ugrinic, G. M. (1955). Standard X-ray Diffraction Powder Patterns, National Bureau of Standards Circular 539, IV, p. 75. Washington, DC: National Bureau of Standards. Google Scholar
Tapasa, K., Barashev, A. V., Bacon, D. J. & Osetsky, Y. N. (2007). J. Nucl. Mater. 361, 52–61. Web of Science CrossRef CAS Google Scholar
Young, R. A. (1995). Editor. The Rietveld Method. Oxford University Press. Google Scholar
© International Union of Crystallography. Prior permission is not required to reproduce short quotations, tables and figures from this article, provided the original authors and source are cited. For more information, click here.