Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T07:58:28.003Z Has data issue: false hasContentIssue false

Sequential Growth of High Quality Diamond Films from Hydrocarbon and Hydrogen Gases

Published online by Cambridge University Press:  25 February 2011

Darin S. Olson
Affiliation:
Department of Materials Science and Engineering, Stanford University, Stanford CA.
Michael A. Kelly
Affiliation:
Department of Materials Science and Engineering, Stanford University, Stanford CA.
Sanjiv Kapoor
Affiliation:
Department of Materials Science and Engineering, Stanford University, Stanford CA.
Stig B. Hagstrom
Affiliation:
Department of Materials Science and Engineering, Stanford University, Stanford CA.
Get access

Abstract

We have constructed a novel, sequential DC glow and hot filament CVD reactor, to study the influence of single parameters on the deposition of diamond thin films. This reactor is capable of growing diamond films, with independent excitation of hydrogen and methane. This is achieved by the sequential exposure of the substrate to spatially separated, chemically independent, plasma regions of hydrogen, and methane in helium. The substrate is mounted on a rotating plate above the gas sources at a variable distance, typically 0.5 – 2 mm. The plate is radiantly heated from behind to a desired temperature up to 1300 K. Using the sequential deposition chamber we have been able to deposit good quality diamond up to 8% methane in helium, without the presence of oxygen, by separating a source of atomic hydrogen and a source of methane. These experiments show that methane and atomic hydrogen do not need to be present simultaneously to grow diamond. Our results further indicate that the primary critical parameter for both quality and growth rate, in hot filament deposition of diamond, is the concentration of atomic hydrogen in the system.

Type
Research Article
Copyright
Copyright © Materials Research Society 1992

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

1. Yarbrough, W. A. and Messier, R., Science, 247, 688 (1990).Google Scholar
2. Angus, J. C, Hayman, C. C. Science, 241, 913 (1988).Google Scholar
3. Badzìan, A. R., DeVries, R. C., Mat. Res. Bull., 23. 385 (1988).Google Scholar
4. Harris, S. J., Martin, L. R., J. Mater. Res., 5, 2313 (1990).Google Scholar
5. Celii, F. G., Butler, J. E., New Diamond Science and Technology, MRS Int. Conf. Proc., 201 (1991).Google Scholar
6. Harris, S. J., Appl. Phys. Lett., 56, 2298 (1990)Google Scholar
7. Tsuda, M., Nakajima, M, Oikawa, S, J. Am. Chem. Soc., 108, 5780 (1986).Google Scholar
8. Ravi, K. V., Joshi, A., Appl. Phys. Lett., 58 (3), 246 (1991)Google Scholar
9. Olson, D., Kelly, M. A., Kapoor, S., Hagstrom, S. B., presented at 1991 MRS Fall Meeting, Boston, MA, December 5 1991.Google Scholar