Abstract
A model for the low-temperature catalysis of hydrogen molecules on graphene and graphite, relevant for interstellar chemistry, is proposed: hydrogen atoms are either chemisorbed at the edges, or physisorbed on graphene and transported to a chemisorbed state at the edges. A second atom can then produce a molecule via a hot atom or an Eley-Rideal process. Since much of the energy is needed to desorb the molecule from the tightly-bound chemisorbed state, the desorbing molecules have only low internal excitation energy, in agreement with astronomical observations.
| Original language | English |
|---|---|
| Pages (from-to) | 117-120 |
| Number of pages | 4 |
| Journal | Chemical Physics |
| Volume | 439 |
| DOIs | |
| Publication status | Published - 17 Aug 2014 |
| Externally published | Yes |
Keywords
- Coupled-channel calculations
- Graphene
- Graphite
- Heterogeneous catalysis at surfaces
- Hydrogen production
- Interplanetary dust and gas
Fingerprint
Dive into the research topics of 'Graphene and graphite, low-temperature catalysts producing weakly-excited hydrogen molecules'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver