Francis, Samantha, Boucher, Alexandre, Jones, Glenn and Roldan, Alberto ![]() ![]() |
Preview |
PDF
- Published Version
Available under License Creative Commons Attribution. Download (3MB) | Preview |
Abstract
Sintering is one of the most common processes responsible for the loss of supported metal nanoparticle catalysts' activity. We have combined ab-initio calculations with microkinetic simulations to investigate the digestion and growth mechanism on Au clusters supported on MgO(0 0 1) following a bottom-up approach. The energy barrier for diffusing a single gold atom on the clean MgO surface was found to be 0.29 eV in full agreement with previous reports. Additionally, and as an extension to the entire energy profile related to Ostwald mechanisms, we found all of the activation energies to be below 1.05 eV in the cases investigated. An odd–even cluster trend was observed during ripening, attributed to the stability of pairing the unpaired electrons associated with the single gold atoms. Microkinetic analyses showed that Au single atoms are present on the surface of magnesia up to a temperature of 160 K. At higher temperatures, the system has enough energy for the single atom to diffuse across the surface and attach to other atoms or clusters. At temperatures akin to room temperature, the cluster undergoes ripening to form larger particles in order to achieve a more stable equilibrium.
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Advanced Research Computing @ Cardiff (ARCCA) Cardiff Catalysis Institute (CCI) Chemistry |
Publisher: | Elsevier |
ISSN: | 0169-4332 |
Funders: | EPSRC |
Date of First Compliant Deposit: | 18 October 2021 |
Date of Acceptance: | 14 September 2021 |
Last Modified: | 02 Aug 2024 13:13 |
URI: | https://orca.cardiff.ac.uk/id/eprint/144905 |
Actions (repository staff only)
![]() |
Edit Item |