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Demonstrating Pressure Jumping as a Tool to Address the Pressure Gap in High Pressure Photoelectron Spectroscopy of CO and CO2 Hydrogenation on Rh(211)
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum.ORCID-id: 0000-0001-6085-2916
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum.ORCID-id: 0000-0002-0062-0643
Stockholms universitet, Naturvetenskapliga fakulteten, Fysikum.ORCID-id: 0000-0002-5297-710x
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Rekke forfattare: 72024 (engelsk)Inngår i: ChemPhysChem, ISSN 1439-4235, E-ISSN 1439-7641, Vol. 25, nr 1, artikkel-id e202300523Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

Operando probing by x-ray photoelectron spectroscopy (XPS) of certain hydrogenation reactions are often limited by the scattering of photoelectrons in the gas phase. This work describes a method designed to partially circumvent this so called pressure gap. By performing a rapid switch from a high pressure (where acquisition is impossible) to a lower pressure we can for a short while probe a remnant of the high pressure surface as well as the time dynamics during the re-equilibration to the new pressure. This methodology is demonstrated using the CO2 and the CO hydrogenation reaction over Rh(211). In the CO2 hydrogenation reaction, the remnant surface of a 2 bar pressure shows an adsorbate distribution which favors chemisorbed CHx adsorbates over chemisorbed CO. This contrasts against previous static operando spectra acquired at lower pressures. Furthermore, the pressure jumping method yields a faster acquisition and more detailed spectra than static operando measurements above 1 bar. In the CO hydrogenation reaction, we observe that CHx accumulated faster during the 275 mbar low pressure regime, and different hypotheses are presented regarding this observation.

sted, utgiver, år, opplag, sider
2024. Vol. 25, nr 1, artikkel-id e202300523
Emneord [en]
Pressure Gap, Operando Heterogenous Catalysis, Syngas, Rhodium Catalyst, Synchrotron
HSV kategori
Identifikatorer
URN: urn:nbn:se:su:diva-224231DOI: 10.1002/cphc.202300523ISI: 001103731100001PubMedID: 37877432Scopus ID: 2-s2.0-85176584003OAI: oai:DiVA.org:su-224231DiVA, id: diva2:1817221
Tilgjengelig fra: 2023-12-05 Laget: 2023-12-05 Sist oppdatert: 2025-02-20bibliografisk kontrollert

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Degerman, DavidGoodwin, ChristopherLömker, PatrickShipilin, MikhailNilsson, Anders

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