Evolution of sp{sup 2} networks with substrate temperature in amorphous carbon films: Experiment and theory

The evolution of sp{sup 2} hybrids in amorphous carbon (a-C) films deposited at different substrate temperatures was studied experimentally and theoretically. The bonding structure of a-C films prepared by filtered cathodic vacuum arc was assessed by the combination of visible Raman spectroscopy, x-...

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Veröffentlicht in:Physical review. B, Condensed matter and materials physics Condensed matter and materials physics, 2005-07, Vol.72 (1)
Hauptverfasser: Gago, R., Centro de Micro-Analisis de Materiales, Universidad Autonoma de Madrid, Campus de Cantoblanco, 28049 Madrid, Vinnichenko, M., Physics Department, Kyiv Taras Shevchenko University, 01033 Kyiv, Jaeger, H.U., Maitz, M.F., Belov, A.Yu, Jimenez, I., Huang, N., Sun, H.
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Sprache:eng
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Zusammenfassung:The evolution of sp{sup 2} hybrids in amorphous carbon (a-C) films deposited at different substrate temperatures was studied experimentally and theoretically. The bonding structure of a-C films prepared by filtered cathodic vacuum arc was assessed by the combination of visible Raman spectroscopy, x-ray absorption, and spectroscopic ellipsometry, while a-C structures were generated by molecular-dynamics deposition simulations with the Brenner interatomic potential to determine theoretical sp{sup 2} site distributions. The experimental results show a transition from tetrahedral a-C (ta-C) to sp{sup 2}-rich structures at {approx}500 K. The sp{sup 2} hybrids are mainly arranged in chains or pairs whereas graphitic structures are only promoted for sp{sup 2} fractions above 80%. The theoretical analysis confirms the preferred pairing of isolated sp{sup 2} sites in ta-C, the coalescence of sp{sup 2} clusters for medium sp{sup 2} fractions, and the pronounced formation of rings for sp{sup 2} fractions >80%. However, the dominance of sixfold rings is not reproduced theoretically, probably related to the functional form of the interatomic potential used.
ISSN:1098-0121
1550-235X
DOI:10.1103/PhysRevB.72.014120