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 |
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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