Effects of the Ion to Growth Flux Ratio on the Constitution and Mechanical Properties of Cr 1- x -Al x -N Thin Films

Cr-Al-N thin film materials libraries were synthesized by combinatorial reactive high power impulse magnetron sputtering (HiPIMS). Different HiPIMS repetition frequencies and peak power densities were applied altering the ion to growth flux ratio. Moreover, time-resolved ion energy distribution func...

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Veröffentlicht in:ACS combinatorial science 2019-12, Vol.21 (12), p.782-793
Hauptverfasser: Banko, Lars, Ries, Stefan, Grochla, Dario, Arghavani, Mostafa, Salomon, Steffen, Pfetzing-Micklich, Janine, Kostka, Aleksander, Rogalla, Detlef, Schulze, Julian, Awakowicz, Peter, Ludwig, Alfred
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Sprache:eng
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Zusammenfassung:Cr-Al-N thin film materials libraries were synthesized by combinatorial reactive high power impulse magnetron sputtering (HiPIMS). Different HiPIMS repetition frequencies and peak power densities were applied altering the ion to growth flux ratio. Moreover, time-resolved ion energy distribution functions were measured with a retarding field energy analyzer (RFEA). The plasma properties were measured during the growth of films with different compositions within the materials library and correlated to the resulting film properties such as phase, grain size, texture, indentation modulus, indentation hardness, and residual stress. The influence of the ion to growth flux ratio on the film properties was most significant for films with high Al-content ( = 50 at. %). X-ray diffraction with a 2D detector revealed hcp-AlN precipitation starting from Al-concentration ≥ 50 at. %. This precipitation might be related to the kinetically enhanced adatom mobility for a high ratio of ions per deposited atoms, leading to strong intermixing of the deposited species. A structure zone transition, induced by composition and flux ratio / , from zone T to zone Ic structure was observed which hints toward the conclusion that the combination of increasing flux ratio and Al-concentration lead to opposing trends regarding the increase in homologous temperature.
ISSN:2156-8952
2156-8944
DOI:10.1021/acscombsci.9b00123