Hostname: page-component-7c8c6479df-hgkh8 Total loading time: 0 Render date: 2024-03-28T14:29:17.095Z Has data issue: false hasContentIssue false

Epitaxial Growth of Co3O4 Films by Low Temperature, Low Pressure Chemical Vapor Deposition

Published online by Cambridge University Press:  10 February 2011

K. Shalini
Affiliation:
Materials Research Centré, Indian Institute of Science, Bangalore -560 012, INDIA
Anil U. Mane
Affiliation:
Materials Research Centré, Indian Institute of Science, Bangalore -560 012, INDIA
R. Lakshmi
Affiliation:
Materials Research Centré, Indian Institute of Science, Bangalore -560 012, INDIA
S.A. Shivashankar
Affiliation:
Materials Research Centré, Indian Institute of Science, Bangalore -560 012, INDIA
M. Rajeswari
Affiliation:
Department of Physics, University of Maryland, College Park, MD, USA
S. Choopun
Affiliation:
Department of Physics, University of Maryland, College Park, MD, USA
Get access

Abstract

The growth of strongly oriented or epitaxial thin films of metal oxides generally requires relatively high growth temperatures or infusion of energy to the growth surface through means such as ion bombardment. We have grown high quality epitaxial thin films of Co3O4 on different substrates at a temperature as low as 450°C by low-pressure metal-organic chemical vapor deposition (MOCVD) using cobalt(II) acetylacetonate as the precursor. With oxygen as the reactant gas, polycrystalline Co3O4 films are formed on glass and Si(100) in the temperature range 350-550°C. Under similar conditions of growth, highly oriented films of Co3O4 are formed on SrTiO3(100) and LaAlO3(100). The film on LaAlO3(100) grown at 450°C show a rocking curve FWHM of 1.61°, which reduces to 1.32° when it is annealed in oxygen at 725°C. The film on SrTiO3(100) has a FWHM of 0.330 (as deposited) and 0.29° (after annealing at 725°C). The ø-scan analysis shows cube-on-cube epitaxy on both these substrates. The quality of epitaxy on SrTiO3(100) is comparable to the best of the pervoskite-based oxide thin films grown at significantly higher temperatures.

Type
Research Article
Copyright
Copyright © Materials Research Society 2000

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] McDonald, G.E., Thin Solid Films, 72, 83 (1980).Google Scholar
2] Patil, P.S., Kadam, L.D., and Lokhande, C.D., Thin Solid Films, 272, 29 (1996).Google Scholar
3] Fujü, E., Torü, H., Tomozawa, A., Takayama, R., and Hirao, T., J. Mater. Sci., 30, 6013 (1995).Google Scholar
4] Cook, J.G. and Meer, M.P. van der, Thin Solid Films, 144, 165 (1986).Google Scholar
5] Kennedy, R.J., IEEE Transactions on Magnetics, 31, 3829 (1995).Google Scholar
6] Barrera, E., Viveros, T., Avila, A., Quintana, P., Morales, M., and Batina, N., Thin Solid Films, 346, 138 (1999).Google Scholar
7] Maruyama, T. and Nakai, T., Solar Energy Materials, 23, 25 (1991).Google Scholar
8] Maruyama, T. and Arai, S., J. Electrochem. Soc., 143, 1383 (1996).Google Scholar
9] Lu, P., He, S., Li, F.X., and Jia, Q.X., Thin Solid Films, 340, 140 (1999).Google Scholar
10] Schieber, M., Han, S.C., Ariel, Y., Chokron, S., Tsach, T., Maharizi, M., Deutscher, C., Racah, D., Raizman, A., and Rotter, S., J. Cryst. Growth, 115, 31 (1991).Google Scholar
11] Lind, D.M., Berry, S.D., Chern, G., Mathias, H., and Testardi, L.R., Phys. Rev. B, 45, 1838 (1992).Google Scholar
12] Li, Z., Fisher, E.S., Liu, J.Z., and Nevitt, M.V., J. Mater. Sci., 26, 2621 (1991).Google Scholar
13] Mane, Anil U., Shalini, K., and Shivashankar, S. A. (to be published).Google Scholar