Spectroscopic signatures of pressurized carbon dioxide in diffuse reflectance infrared spectroscopy of heterogeneous catalysts

Abstract: Using diffuse reflectance infrared Fourier transform (DRIFT) spectroscopy to study surface species of reaction intermediates on heterogeneous catalysts requires particular precautions, when assigning IR bands to intermediates apparently resulting from the reaction of H2, CO, and CO2. In accordance with earlier work, it is shown that in the investigation of the heterogeneous methanol synthesis, several gas phase bands of CO2 were misassigned in previous studies as adsorbates on the catalyst surface. Thus, several combination bands and overtones of CO2 in the 2200–750 cm−1 range – notably those at 2130, 2112, 2107, 2094, 2077, ∼2056, 1933, ∼1920, ∼1079, ∼1050, ∼973, and ∼948 cm−1 – were already misinterpreted as adsorbates/intermediates. Some of these bands exhibit similar (low) intensities as surface species and are in the range of typical adsorbed CO or methoxy/methanol vibrations. Higher pressures and temperatures, which are necessary to study industrial catalysts by in situ IR spectroscopy, even amplify this effect. In addition, due to a Fermi resonance at a CO2 partial pressure above ∼10 bar, two further bands appear at 1388 and 1285 cm−1. This is also within the range typically associated with surface adsorbates. In order to avoid misassignments of IR bands for in situ or operando DRIFT spectroscopy, those occurring at CO2 pressures up to 30 bar in the widely used Praying Mantis TM High Temperature Reaction Chamber are presented here and assigned to their origin as combination bands and overtones of gaseous CO2

Location
Deutsche Nationalbibliothek Frankfurt am Main
Extent
Online-Ressource
Notes
ChemCatChem. - 12, 9 (2020) , 2622-2629, ISSN: 1867-3899

Keyword
DRIFT-Spektroskopie
Kohlendioxid
Heterogene Katalyse
Adsorption

Event
Veröffentlichung
(where)
Freiburg
(who)
Universität
(when)
2020
Creator

DOI
10.1002/cctc.201902038
URN
urn:nbn:de:bsz:25-freidok-1552366
Rights
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Last update
14.08.2025, 10:48 AM CEST

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Time of origin

  • 2020

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