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W-Cr-C-N Nanocomposite Thin-Film Coatings via Reactive Magnetron Sputtering
Michael Walock, Yujiao Zou, Denis Lagadrillere, Corinne Nouveau, Andrei V Stanishevsky

W-Cr-C-N Nanocomposite Thin-Film Coatings via Reactive Magnetron Sputtering

Science & Mathematics Published 2011 Verification Pending

Overview & Synopsis

While binary tungsten carbide can form smooth, hard films, these suffer from low fracture toughness. Tungsten nitride films are frequently harder, but are more brittle. Chromium nitride has excellent wear and oxidation resistance, but films often form with low hardness. Composites of these binary compounds offer a possibility to tailor the material for a desired combination of properties. To this end, we have used reactive RF-magnetron sputtering with Cr and WC targets to form quaternary composites, with nitrogen as the reactive gas. The coatings were deposited on Si, Ti, and steel substrates. The nitrogen partial pressure was varied to investigate the relationship between the film properties and the deposition conditions. Energy dispersive spectroscopy showed changes in the chemical composition as a result of the change in nitrogen partial pressure. X-ray diffraction illuminated the structure as either a solid solution with a B1 NaCl structure, or a nanocomposite with the average crystallite size under 11 nm. Optical interferometer revealed low compressive stresses. And nanoindentation established that the films are hard and adherent.

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Document Information

Document Title W-Cr-C-N Nanocomposite Thin-Film Coatings via Reactive Magnetron Sputtering
Author / Organization Michael Walock, Yujiao Zou, Denis Lagadrillere, Corinne Nouveau, Andrei V Stanishevsky
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2011
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-228671
Original Source Link Visit Source Page on hal.science »