2019
DOI: 10.1380/ejssnt.2019.169
|View full text |Cite
|
Sign up to set email alerts
|

Surface Chemistry of Carbon Dioxide on Copper Model Catalysts Studied by Ambient-Pressure X-ray Photoelectron Spectroscopy

Abstract: In-situ analysis of heterogeneous catalysts under reaction condition is indispensable to understand reaction mechanisms and nature of active sites. Ambient-pressure X-ray photoelectron spectroscopy (AP-XPS) is one of the powerful methods to investigate chemical states of catalysts and reaction intermediates adsorbed on the surface. In this review, reaction of carbon dioxide on Cu(997) and Zn-deposited Cu(997) surfaces are discussed as an example of surface chemistry of weakly adsorbed molecules, together with … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
6
0

Year Published

2020
2020
2023
2023

Publication Types

Select...
9

Relationship

4
5

Authors

Journals

citations
Cited by 13 publications
(7 citation statements)
references
References 85 publications
1
6
0
Order By: Relevance
“…On the CuO x /Cu­(111) region of the surface without zirconia (lower spectra, Figure ), the peaks associated with surface intermediates are substantially smaller and shifted in energy relative to the C­(ad) peak in the corresponding spectra with zirconia on the surface. For example, the fitted data reveal a peak at ∼285.6 eV which falls between the H x CO* and CH 3 O* features in the spectra in the zirconia region; since this peak exhibits similar intensity trends as H x CO* and CH 3 O* in the zirconia region, we assign this peak at ∼285.6 eV to H x C–O* and H x CO species, consistent with other reported values for these species on bare Cu surfaces. , The peak at ∼287.7 eV is assigned to formate (HCOO*) based on previous studies of CO 2 exposure on Cu and CuO x /Cu­(111) surfaces, although it may also overlap contributions from carboxylate (CO 2 δ− ). ,,,, Consequently, we label this peak as CO 2 δ− /HCOO*. At even higher binding energy (289.7–289.9 eV), a small peak appears between 400 and 500 K and is tentatively assigned to carbonate (*CO 3 ). ,, Overall, the carbon-based species observed in the surface region without zirconia are consistent with CO 2 interactions on Cu and CuO x surfaces and are clearly distinguishable from those in the Zr/CuO 2 /Cu­(111) surface region.…”
Section: Resultssupporting
confidence: 87%
See 1 more Smart Citation
“…On the CuO x /Cu­(111) region of the surface without zirconia (lower spectra, Figure ), the peaks associated with surface intermediates are substantially smaller and shifted in energy relative to the C­(ad) peak in the corresponding spectra with zirconia on the surface. For example, the fitted data reveal a peak at ∼285.6 eV which falls between the H x CO* and CH 3 O* features in the spectra in the zirconia region; since this peak exhibits similar intensity trends as H x CO* and CH 3 O* in the zirconia region, we assign this peak at ∼285.6 eV to H x C–O* and H x CO species, consistent with other reported values for these species on bare Cu surfaces. , The peak at ∼287.7 eV is assigned to formate (HCOO*) based on previous studies of CO 2 exposure on Cu and CuO x /Cu­(111) surfaces, although it may also overlap contributions from carboxylate (CO 2 δ− ). ,,,, Consequently, we label this peak as CO 2 δ− /HCOO*. At even higher binding energy (289.7–289.9 eV), a small peak appears between 400 and 500 K and is tentatively assigned to carbonate (*CO 3 ). ,, Overall, the carbon-based species observed in the surface region without zirconia are consistent with CO 2 interactions on Cu and CuO x surfaces and are clearly distinguishable from those in the Zr/CuO 2 /Cu­(111) surface region.…”
Section: Resultssupporting
confidence: 87%
“…97,98 The peak at ∼287.7 eV is assigned to formate (HCOO*) based on previous studies of CO 2 exposure on Cu and CuO x /Cu(111) surfaces, although it may also overlap contributions from carboxylate (CO 2 δ− ). 76,90,93,98,99 Consequently, we label this peak as CO 2 δ− /HCOO*. At even higher binding energy (289.7− 289.9 eV), a small peak appears between 400 and 500 K and is tentatively assigned to carbonate (*CO 3 ).…”
Section: Identification Of Surface Species By Irasmentioning
confidence: 99%
“…The experiments were performed at the AP-XPS endstation , at SPring-8 BL07LSU . The photon energy and flux of incident X-rays were 735 eV and 1.2 × 10 15 s –1 cm –2 , respectively.…”
Section: Methodsmentioning
confidence: 99%
“…The XPS spectra were obtained with a photon energy of 735 eV and photon flux of 1.1 × 10 15 s –1 cm –2 . The details of this endstation can be found in refs and . The samples (Ga-polar n-GaN grown on the Si substrate by metal organic chemical vapor phase epitaxy, thickness of n-GaN of 2.5 μm) used in this study, were purchased from Nuflare Technology.…”
Section: Computational and Experimental Methodologymentioning
confidence: 99%