Ion beam analysis and co-sputtering simulation (CO-SS) of bi-metal films produced by magnetron co-sputtering


Por: Cruz, J., Andrade, E., Muhl, S., Canto, C., de Lucio, O., Chavez, E., Rocha, M. F., Garces-Medina, E.

Publicada: 15 mar 2016
Resumen:
Magnetron sputtering is widely used to deposit thin films on different types of substrates. An important application of this method is to make multicomponent thin films using co-sputtering, where two or more elements are included in the target. The thickness and elemental composition of the films depend on the experimental parameters used, the system geometry and the spatial distribution of the elements in the target. If the target is made of two spatially separate pieces of the materials, then the composition of the deposit depends on a combination of the relative areas, the sputtering yield and the angular distribution of the emission of the sputtered flux of each material. In this work, a co-sputtering simulation program, known as CO-SS, was developed to simulate the thickness and composition of metal films produced by DC magnetron sputtering (Al) and co-sputtering (Al + Ti). The CO-SS code models the angular distribution of particles ejected by sputtering from the target, where this is assumed to vary as cosnß, where n is a free parameter and ß is the angle of ejection relative to the normal to the surface of the target, and the sputtering yield of each material. The program also takes into account other geometry factors such as the distance between the target and the substrate, and the size of the substrate. Rutherford backscattering (RBS) using 4He was employed to measure the thickness and the composition of the films deposited on glass cover slides in order to assess the CO-SS program. The film thickness was also measured by profilometry. The CO-SS code was found to accurately model the experimental results for both the Al and Ti/Al films. The CO-SS code is freely available for use from http://demonstrations.wolfram.com/CoSputteringSimulationCOSS/. © 2015 Elsevier B.V. All rights reserved.

Filiaciones:
Cruz, J.:
 Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, DF, Mexico

 Univ Nacl Autonoma Mexico, Inst Invest Mat, AP 70-360, Mexico City, DF, Mexico

Andrade, E.:
 Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, DF, Mexico

Muhl, S.:
 Univ Nacl Autonoma Mexico, Inst Invest Mat, AP 70-360, Mexico City, DF, Mexico

Canto, C.:
 Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, DF, Mexico

de Lucio, O.:
 Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, DF, Mexico

Chavez, E.:
 Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, DF, Mexico

Rocha, M. F.:
 Inst Politecn Nacl, ESIME Z, ALM Zacatenco, Mexico City 07738, DF, Mexico

Garces-Medina, E.:
 Univ Nacl Autonoma Mexico, Fac Ciencias, Lab Dinam Lineal, AP 70-360, Mexico City, DF, Mexico
ISSN: 0168583X
Editorial
Elsevier Science Publishers B.V., Amsterdam, Netherlands, PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS, Países Bajos
Tipo de documento: Article
Volumen: 371 Número:
Páginas: 268-272
WOS Id: 000373412000052