journal article·2010-04Open access

Theoretical simulation and preparation of binary and ternary combinatorial libraries by thermal PVD

Sebastian Oliver Klemm, Alistair Graeme Martin, Julia Lengsfeld, Janine‐Christina Schauer, Bernd Schuhmacher, Achim Walter Hassel

physica status solidi (a)· Volume 207· Issue 4

Abstract

Abstract Binary and ternary composition spread material libraries were prepared using a thermal physical vapor deposition system with three separated heating sources and adjustable chamber geometry. In this work, we present binary Cu84‐20Al16‐80 and Zn71‐8Mg29‐92 libraries as well as a ternary Cu67‐6Ag81‐13Mg66‐12 system with a thickness around 300 nm. The composition of the obtained films was determined by automated energy dispersive X‐ray spectroscopy and the data further used to develop a mathematical model to simulate the surface. The thickness of a copper film was measured by atomic force microscopy and used to verify the theoretical model, whereas topography scans provided information on the surface roughness. The consistency between theoretical simulations and observed compositions concludes multiple source thermal co‐evaporation to be a reliable method with high variety regarding source metals and deposition rates and therefore of high value for material library fabrication.
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Research context

OpenAlex topics: Copper Interconnects and Reliability · Metal and Thin Film Mechanics · High-Temperature Coating Behaviors

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Max‐Planck‐Institut für Eisenforschung GmbH, Max‐Planck‐Str. 1, 40237 Düsseldorf, Germany

School of Chemistry, The University of Edinburgh, Edinburgh, EH9 3JJ Scotland, UK

Dortmunder OberflächenCentrum, Eberhardstr. 12, 44145 Dortmund, Germany

Institute for Chemical Technology of Inorganic Materials, Johannes Kepler University, Altenberger Str. 69, 40404 Linz, Austria

Funding

Dortmunder OberflächenCentrum, Dortmund, Germany · Deutscher Akademischer Austauschdienst

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