INFLUENCE OF OXYGEN ON THE NUCLEATION AND GROWTH OF DIAMOND FILMS

Citation
C. Gomezaleixandre et al., INFLUENCE OF OXYGEN ON THE NUCLEATION AND GROWTH OF DIAMOND FILMS, Thin solid films, 303(1-2), 1997, pp. 34-38
Citations number
13
Categorie Soggetti
Physics, Applied","Material Science","Physics, Condensed Matter
Journal title
ISSN journal
00406090
Volume
303
Issue
1-2
Year of publication
1997
Pages
34 - 38
Database
ISI
SICI code
0040-6090(1997)303:1-2<34:IOOOTN>2.0.ZU;2-1
Abstract
The addition of oxygen to a diluted methane/hydrogen gas mixture (2% C H4 in H-2) activated by a microwave discharge during diamond film depo sition has been studied. We have observed that oxygen addition at very low concentrations (< 2%) to the methane/hydrogen gas mixture makes t he nucleation of diamond crystals more difficult, by causing a sharp d ecrease in the deposition rate of the diamond film. For increasing oxy gen concentrations, in the [O-2] = 0.25-1% range, the diamond and grap hite deposition rates remain nearly constant, showing a slight decreas e in the graphite deposition rate for [O-2] = 1%. By contrast, for hig her oxygen concentrations (1% < [O-2] < 2.5%) thinner films of a high quality are deposited (diamond content > 84%). These facts have been e xplained by an abrupt change in the chemical processes when the oxygen is fed to the CH4 + H-2 mixture, even in a small concentration We ass ume that the role of the atomic oxygen is two-fold: (i) formation of O H radicals, which etch the diamond and graphite phases at high rates. and (ii) direct etching of the initial carbon layer formed during the nucleation stage, producing CO molecules. However, for [O-2] greater t han or equal to 2.5% the carbon etching rate (for all the phases) is s o high that no continuous film can be deposited, In this paper we pres ent the relative variation of the formation, in the 0-2.5% oxygen rang e. for both the diamond and non-diamond phases, as determined by Raman spectroscopy and scanning electron microscopy. The results have been related to the changes in the plasma composition (mainly the OH, O and CO species), as detected by optical emission spectroscopy and mass sp ectrometry. (C) 1997 Elsevier Science S.A.