Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-23T02:26:18.740Z Has data issue: false hasContentIssue false

Spatially and spectrally resolved cathodoluminescence of hot-filament chemical-vapor-deposited diamond particles

Published online by Cambridge University Press:  31 January 2011

Lawrence H. Robins
Affiliation:
National Institute of Standards and Technology, Gaithersburg, Maryland 20899
Edward N. Farabaugh
Affiliation:
National Institute of Standards and Technology, Gaithersburg, Maryland 20899
Albert Feldman
Affiliation:
National Institute of Standards and Technology, Gaithersburg, Maryland 20899
Get access

Abstract

Spectrally resolved cathodoluminescence (CL) images and spatially resolved CL spectra were obtained from two specimens grown by hot-filament chemical vapor deposition. Each specimen consisted of a large number of unconnected diamond particles with cubo-octahedral and pseudo-fivefold twinned growth habits. The growth temperature was nominally 600 °C for one specimen and 750 °C for the other. In the 1.5–3.5 eV range, the spectra are composed of four defect and impurity related bands: there are three bands with zero-phonon lines at 1.68 eV, 2.156 eV, and 2.325 eV, and one broad band centered at 2.85 eV. A weak peak at 5.27 eV, due to exciton recombination, was also observed. Spectrally resolved images of the two most intense CL bands, at 2.156 eV and 2.85 eV, were obtained for several particles. In the low-temperature specimen, bright regions in images of the 2.156 eV band are correlated with {111} facets; bright regions in images of the 2.85 eV band are correlated in some cases with the central regions of {100} facets and in other cases with {111} facets. In the intermediate-temperature specimen, bright regions in the images of both bands are correlated with {100} facets. A model of competing recombination at different types of CL centers and nonradiative centers is proposed to facilitate the interpretation of the experimental results. For the low-temperature specimen, the model suggests that the 2.156 eV CL centers are located primarily in {111} growth sectors and the 2.85 eV CL centers are distributed relatively uniformly; images of the two dominant CL bands are predicted to have a complementary relationship in particles where there are few competing nonradiative centers. For the intermediate-temperature specimens, the model suggests that nonradiative recombination is dominant, and that the CL image contrast arises primarily from a nonuniform distribution of nonradiative centers.

Type
Articles
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

1.Clark, C. D., Mitchell, E. W. J., and Parsons, B. J., in The Properties of Diamond, edited by Field, J. E. (Academic Press, London, 1979), p. 23.Google Scholar
2.Walker, J., Rep. Prog. Phys. 42, 1605 (1979).CrossRefGoogle Scholar
3.Davies, G., in The Properties of Diamond, edited by Field, J. E. (Academic Press, 1979), p. 165.Google Scholar
4.Yacobi, B. G. and Holt, D. B., J. Appl. Phys. 59, Rl (1986).CrossRefGoogle Scholar
5.Robins, L. H., Cook, L. P., Farabaugh, E. N., and Feldman, A., Phys. Rev. B 39, 13367 (1989).CrossRefGoogle Scholar
6.Robins, L. H., Cook, L. P., Farabaugh, E. N., and Feldman, A., in Diamond Optics II, edited by Feldman, A. and Holly, S., Proc. SPIE 1146, 166 (SPIE, Bellingham, WA, 1990).Google Scholar
7.Robins, L. H., Farabaugh, E. N., Feldman, A., and Cook, L. P., accepted for publication in Phys. Rev. B (1991).Google Scholar
8.Robins, L. H., Tjossem, P. J. H., Smyth, K. C., Barnes, P. Y., Farabaugh, E. N., and Feldman, A., accepted for publication in J. Appl. Phys. (1991).Google Scholar
9.Vavilov, V. S., Gippius, A. A., Zaitsev, A. M., Deryagin, B. V., Spitsyn, B. V., and Aleksenko, A. E., Fiz. Tekh. Poluprovodn. 14, 1811 (1980) [Sov. Phys. Semicond. 14, 1078 (1980)].Google Scholar
10.Collins, A. T., Kamo, M., and Sato, Y., J. Phys. D 22, 1402 (1989).CrossRefGoogle Scholar
11.Partlow, W. D., Ruan, J., Witkowski, R. E., Choyke, W. J., and Knight, D. S., J. Appl. Phys. 67, 7019 (1990).CrossRefGoogle Scholar
12.Kawarada, H., Nishimura, K., Ito, T., Suzuki, J., Mar, K., Yokota, Y., and Hiraki, A., Jpn. J. Appl. Phys. 27, L683 (1988).CrossRefGoogle Scholar
13.Kawarada, H., Yokota, Y., Mori, Y., Nishimura, K., and Hiraki, A., J. Appl. Phys. 67, 983 (1990).CrossRefGoogle Scholar
14.Farabaugh, E. N., Feldman, A., Robins, L. H., and Etz, E. S., in Diamond Optics, edited by Feldman, A. and Holly, S., Proc. SPIE 969, 24 (SPIE, Bellingham, WA, 1989).Google Scholar
15.Kanaya, K. and Okayama, S., J. Phys. D: Appl. Phys. 5, 43 (1972).CrossRefGoogle Scholar
16.Narayan, J., Srivatsa, A. R., and Ravi, K. V., Appl. Phys. Lett. 54, 1659 (1989).CrossRefGoogle Scholar
17.Collins, A. T., Stanley, M., and Woods, G. S., J. Phys. D 20, 969 (1987).CrossRefGoogle Scholar
18.Collins, A. T. and Lawson, S. C., J. Phys. Condens. Matter 1, 6929 (1989).CrossRefGoogle Scholar
19.Zaitsev, A. M., Vavilov, V. S., and Gippius, A. A., Krat. Soob. Fiz. 10, 21 (1981) [Sov. Phys.-Leb. Inst. Rep. 10, 15 (1981)].Google Scholar
20.Yamamoto, N., Spence, J. C. H., and Fathy, D., Philos. Mag. B 49, 609 (1984).CrossRefGoogle Scholar
21.Dean, P. J., Lightowlers, E. C., and Wight, D. R., Phys. Rev. 140, A352 (1965).CrossRefGoogle Scholar