1996
DOI: 10.1116/1.580190
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Reactive magnetron sputter deposited CNx: Effects of N2 pressure and growth temperature on film composition, bonding, and microstructure

Abstract: Articles you may be interested inLowtemperature deposition of cubic BN:C films by unbalanced direct current magnetron sputtering of a B4C target Effects of nitrogen pressure and ion flux on the properties of direct current reactive magnetron sputtered Zr-N films J. Vac. Sci. Technol. A 13, 2808 (1995); 10.1116/1.579709Preparation and characterization of epitaxial gold films deposited on mica by direct current magnetron sputteringThe effects of growth processes on the chemical bond structure, microstructure, an… Show more

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Cited by 173 publications
(28 citation statements)
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References 12 publications
(18 reference statements)
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“…However, because of the overlap with stronger N2-C (sp 2 ) vibrations, the N1 contribution to the Raman spectrum is essentially negligible. This is in agreement with the experiment [27] .…”
Section: Raman Spectrasupporting
confidence: 93%
“…However, because of the overlap with stronger N2-C (sp 2 ) vibrations, the N1 contribution to the Raman spectrum is essentially negligible. This is in agreement with the experiment [27] .…”
Section: Raman Spectrasupporting
confidence: 93%
“…1a), WC x N y films exhibit an approximately symmetric peak at binding energy of 283.0 eV, which is similar to that for pure WC film, indicating W-C bonds are formed in WC x N y films [36,37]. It is worth noting that neither C-N/ C N/CBBN peaks, generally occur in the range of 284.5-289.9 eV [38,39], nor C-C ones at about 284.4 eV [38,39] appear in the C 1s spectra for WC x N y samples, probably meaning that no C-N/C N/ CBBN or C-C bonds are formed in the WC x N y films. This can be further verified by their N 1s spectra (Fig.…”
Section: Composition and Microstructuresupporting
confidence: 56%
“…This can be further verified by their N 1s spectra (Fig. 1b), in which only an approximately symmetric W-N peak at about 397.0 eV appears [40,41], and no C-N/C N/CBBN ones, generally occur in the range of 398.3-400.3 eV in N 1s spectra [38,39], can be observed. In the W 4f spectra (Fig.…”
Section: Composition and Microstructuresupporting
confidence: 56%
“…It can be seen that, after nitrogen-implantation, the D band position only shifts slightly, but the G band position has a pronounced downshift of $40 cm À1 . The downshift of the G band signifies the increase of sp 3 -bonding fraction at the expense of the sp 2 -bonding fraction [22,23]. Therefore, it is likely that nitrogen-implantation into a-C films is bound to a carbon atom, and promotes Nsp 3 C bonds rather than N-sp 2 C bonds.…”
Section: Methodsmentioning
confidence: 94%