Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-24T05:24:42.248Z Has data issue: false hasContentIssue false

Deuteration of C60 on a highly oriented pyrolytic graphite surface

Published online by Cambridge University Press:  12 October 2020

G. Pantazidis
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
M. Scheffler
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
F. D. S. Simonsen
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
A. Cassidy
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
P. A. Jensen
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
L. Hornekær
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected] Interdisciplinary Nanoscience Center (iNANO), Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
J. D. Thrower
Affiliation:
Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Reactions on carbonaceous surfaces play an important role in processes such as H2 formation in the interstellar medium. We have investigated the adsorption of C2 molecules on a highly oriented pyrolytic graphite (HOPG) surface and then exposed them to a beam of deuterium atoms in order to investigate the formation of deuterated fullerenes. Scanning tunneling microscopy (STM) was used to probe the adsorbed molecules and their deuteration. Deuteration of C2 films results in increased thermal stability of the film, relative to films of pristine C2, along with an evolution towards higher deuterated species. The STM data provide confirmatory evidence for the formation of deuterated fullerene species.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Berné, O. & Tielens, A. G. G. M. 2012, PNAS, 109, 401 CrossRefGoogle Scholar
Campbell, E. K., Holz, M., Gerlich, D. & Maier, J. P. 2015, Nature, 523, 322 CrossRefGoogle Scholar
Löffler, D., Weis, P., Böttcher, A. & Kappes, M. 2007, J. Phys. Chem. C, 111, 17743 CrossRefGoogle Scholar
Sellgren, K., Werner, M. W., Ingalls, J. G., Smith, J. D. T., Carleton, T. M., Joblin, C. 2010, ApJL, 722, L54 CrossRefGoogle Scholar
Thrower, J. D., Jørgensen, B., Friis, E. E., Baouche, S., Mennella, V., Luntz, A. C., Andersen, M., Hammer, B., & Hornekær, L. 2012, ApJ, 752, 3 CrossRefGoogle Scholar
Thrower, J. D., Pantazidis, G., Scheffler, M., Simonsen, F. D. S., Jensen., P. A., & Hornekær, L. 2019, in proc. IAU Symp. Google Scholar
Tschersich, K. G. 2000, J. Appl. Phys., 87, 2565 CrossRefGoogle Scholar