Abstract

Tailoring mechanical properties of transition metal carbides by substituting carbon with nitrogen atoms is a highly interesting approach, as thereby the bonding state changes towards a more metallic like character and thus ductility can be increased. Based on ab initio calculations we could prove experimentally, that up to a nitrogen content of about 68% on the non-metallic sublattice, Ta-C-N crystals prevail a face centered cubic structure for sputter deposited thin films. The cubic structure is partly stabilized by non-metallic as well as Ta vacancies – the latter are decisive for nitrogen rich compositions. With increasing nitrogen content, the originally super-hard fcc-TaC0.71 thin films soften from 40 GPa to 26 GPa for TaC0.33N0.67, accompanied by a decrease of the indentation modulus. With increasing nitrogen on the non-metallic sublattice (hence, decreasing C) the damage tolerance of Ta-C based coatings increases, when characterized after the Pugh and Pettifor criteria. Consequently, varying the non-metallic sublattice population allows for an effective tuning and designing of intrinsic coating properties.

Details

Title
Tuning structure and mechanical properties of Ta-C coatings by N-alloying and vacancy population
Author
Glechner, T 1 ; Mayrhofer, P H 1 ; Holec, D 2 ; Fritze, S 3   VIAFID ORCID Logo  ; Lewin, E 3   VIAFID ORCID Logo  ; Paneta, V 4 ; Primetzhofer, D 4 ; Kolozsvári, S 5 ; Riedl, H 1   VIAFID ORCID Logo 

 Institute of Materials Science and Technology, TU Wien, Wien, Austria 
 Department of Materials Science, Montanuniversität Leoben, Leoben, Austria 
 Department of Chemistry - Ångström Laboratory, Uppsala University, Uppsala, Sweden 
 Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden 
 Plansee Composite Materials GmbH, Lechbruck am See, Germany 
Pages
1-11
Publication year
2018
Publication date
Dec 2018
Publisher
Nature Publishing Group
e-ISSN
20452322
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2150518991
Copyright
© 2018. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.