Surface morphology of Hägg iron carbide (χ-Fe5C2) from ab initio atomistic thermodynamics
Ab initio simulations demonstrate that the surface facetting of the most common iron carbide observed during Fischer–Tropsch synthesis depends on the gaseous environment. [Display omitted] ► Morphology of χ-Fe5C2 was investigated under CO and H2/CO pretreatment. ► CO favors stable C-rich facets, whi...
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Published in | Journal of catalysis Vol. 294; pp. 47 - 53 |
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Main Authors | , , , , , |
Format | Journal Article |
Language | English |
Published |
Amsterdam
Elsevier Inc
01.10.2012
Elsevier Elsevier BV |
Subjects | |
Online Access | Get full text |
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Summary: | Ab initio simulations demonstrate that the surface facetting of the most common iron carbide observed during Fischer–Tropsch synthesis depends on the gaseous environment. [Display omitted]
► Morphology of χ-Fe5C2 was investigated under CO and H2/CO pretreatment. ► CO favors stable C-rich facets, while H2/CO stabilizes C-poor facets. ► Low temperature and pressure favor C-rich facets under CO and H2/CO pretreatment. ► Very high H2/CO ratio makes χ-Fe5C2 phase unstable thermodynamically.
Ab initio atomistic thermodynamics is utilized to achieve the understanding of the surface structure and stability of χ-Fe5C2 under CO and synthesis gas (H2/CO) pretreatment conditions in catalyst activation for Fischer–Tropsch synthesis (FTS). On the basis of the computed surface free energy (γ) as a function of the carbon chemical potential (μC) by considering temperature, pressure, and H2/CO ratios, it is found that CO pretreatment favors stable carbon-rich facets, while small amount of H2 added into CO leads to a large decrease in μC and thus stabilizing carbon-poor facets. The high activity of surface carbon toward hydrogenation might explain the enhanced initial activity of the FTS catalysts activated from CO pretreatment. Moreover, under both CO and H2/CO pretreatments, either low temperature or low pressure can lead to stable carbon-rich facets. |
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Bibliography: | http://dx.doi.org/10.1016/j.jcat.2012.07.003 |
ISSN: | 0021-9517 1090-2694 |
DOI: | 10.1016/j.jcat.2012.07.003 |