Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...260..321k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 260, no. 1-2, p. 321-328.
Astronomy and Astrophysics
Astrophysics
10
Chemisorption, Graphite, Hydrogen Atoms, Interstellar Matter, Surface Reactions, Cosmic Dust, Perturbation Theory
Scientific paper
Using a perturbational approach we consider the chemisorption of a H-atom on a graphite (001) basal surface, having in mind that the graphite-H system reflects to some degree the interaction between an interstellar grain with graphitic parts and a H-atom. The theoretical model we have developed is based on the assumption that the graphite surface can be considered as a rigid network of identical carbon clusters representing the surface lattice geometry. We find, in agreement with previous studies, that the energetically preferred position of the chemisorbed H-atom is above a C-atom and that the wall-height between two adjacent binding sites of the H-atom is about 0.1 eV.
No associations
LandOfFree
Hydrogen chemisorption on a graphite surface does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Hydrogen chemisorption on a graphite surface, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydrogen chemisorption on a graphite surface will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1203153