Abstract
Diamond films were deposited via microwave plasma chemical vapor deposition on lithium niobate (LN) substrates. Characterization of the interfacial regions formed between diamond films and LN substrates was carried out by several techniques. Secondary ion mass spectroscopy (SIMS) was used to determine the depth profiles of carbon, lithium, niobium, and oxygen in the LN substrate covered with diamond nuclei and in the substrate without nucleation. Results indicate that the diamond nuclei promoted growth of diamond, and in addition, a reduced depth of the lithium deficient zone formed in the LN substrate was observed. Grazing incidence x-ray diffraction and transmission electron microscopy observations corroborated the results obtained by SIMS. Residual stresses determined experimentally by an x-ray method or by the shift in the characteristic diamond peak in Raman spectroscopy were much smaller than the calculated thermal residual stresses. The results further emphasize that the interfacial phases are responsible for relieving the thermal stresses generated during cooling of the layered structure. The thickness of the interfacial region was found to be well below for attenuation of the surface acoustic waves in the gigahertz frequency surface acoustic wave devices.
Original language | English |
---|---|
Article number | 020606JVA |
Pages (from-to) | 2105-2112 |
Number of pages | 8 |
Journal | Journal of Vacuum Science and Technology, Part A: Vacuum, Surfaces and Films |
Volume | 24 |
Issue number | 6 |
DOIs | |
State | Published - 2006 |
Externally published | Yes |
Funding
The present research results are based upon work supported by the National Science Foundation, ECS Division under Grant No. 0139712. Part of this research is sponsored by the Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Transportation Technologies, as part of the High Temperature Materials Laboratory User Program, ORNL, managed by UT-Battelle, LLC, for the U.S. Department of Energy under Contract No. DE-AC05-000R22725. The authors wish to thank N. Stoddard for help in preliminary TEM examination, O. B. Cavin for help in x-ray characterization, and Nagraj Kulkarni for advice on thermodynamic analysis.