Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films
Main Author: | |
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Publication Date: | 2011 |
Other Authors: | , , , , , , , , |
Format: | Article |
Language: | eng |
Source: | Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
Download full: | https://hdl.handle.net/1822/15684 |
Summary: | The evolution of the nanoscale structure and the chemical bonds formed in Ti–C–N–O films grown by reactive sputtering were studied as a function of the composition of the reactive atmosphere by increasing the partial pressure of an O2+N2 gas mixture from 0 up to 0.4 Pa, while that of acetylene (carbon source) was constant. The amorphisation of the films observed by transmission electron microscopy was confirmed by micro- Raman spectroscopy, but it was not the only effect associated to the increase of the O2+N2 partial pressure. The chemical environment of titanium and carbon, analysed by X-ray photoemission spectroscopy, also changes due to the higher affinity of Ti towards oxygen and nitrogen than to carbon. This gives rise to the appearance of amorphous carbon coexisting with poorly crystallized titanium oxynitride. The evolution of the films colour is explained on the basis of these structural changes. |
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Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin filmsTitanium oxy-carbo-nitridesReactive sputteringTransmission electron MicroscopyRaman spectroscopyX-ray photoelectron SpectroscopyScience & TechnologyThe evolution of the nanoscale structure and the chemical bonds formed in Ti–C–N–O films grown by reactive sputtering were studied as a function of the composition of the reactive atmosphere by increasing the partial pressure of an O2+N2 gas mixture from 0 up to 0.4 Pa, while that of acetylene (carbon source) was constant. The amorphisation of the films observed by transmission electron microscopy was confirmed by micro- Raman spectroscopy, but it was not the only effect associated to the increase of the O2+N2 partial pressure. The chemical environment of titanium and carbon, analysed by X-ray photoemission spectroscopy, also changes due to the higher affinity of Ti towards oxygen and nitrogen than to carbon. This gives rise to the appearance of amorphous carbon coexisting with poorly crystallized titanium oxynitride. The evolution of the films colour is explained on the basis of these structural changes.Fundação para a Ciência e a Tecnologia (FCT) - PTDC/CTM/69362/2006, SFRH/BPD/27114/2006CRUP (Acção Integrada Luso-francesa N° F-2307) and the GRICES/CNRS collaboration (Proc. 4.1.1 França)ElsevierUniversidade do MinhoChappé, J. M.Marco de Lucas, M. C.Cunha, L.Moura, C.Pierson, J. F.Imhoff, L.Heintz, O.Potin, V.Bourgeois, S.Vaz, F.2011-10-312011-10-31T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/1822/15684eng0040-609010.1016/j.tsf.2011.06.108http://www.sciencedirect.com/info:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2025-04-12T04:32:52Zoai:repositorium.sdum.uminho.pt:1822/15684Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T15:22:11.841871Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse |
dc.title.none.fl_str_mv |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
title |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
spellingShingle |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films Chappé, J. M. Titanium oxy-carbo-nitrides Reactive sputtering Transmission electron Microscopy Raman spectroscopy X-ray photoelectron Spectroscopy Science & Technology |
title_short |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
title_full |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
title_fullStr |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
title_full_unstemmed |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
title_sort |
Structure and chemical bonds in reactively sputtered black Ti–C–N–O thin films |
author |
Chappé, J. M. |
author_facet |
Chappé, J. M. Marco de Lucas, M. C. Cunha, L. Moura, C. Pierson, J. F. Imhoff, L. Heintz, O. Potin, V. Bourgeois, S. Vaz, F. |
author_role |
author |
author2 |
Marco de Lucas, M. C. Cunha, L. Moura, C. Pierson, J. F. Imhoff, L. Heintz, O. Potin, V. Bourgeois, S. Vaz, F. |
author2_role |
author author author author author author author author author |
dc.contributor.none.fl_str_mv |
Universidade do Minho |
dc.contributor.author.fl_str_mv |
Chappé, J. M. Marco de Lucas, M. C. Cunha, L. Moura, C. Pierson, J. F. Imhoff, L. Heintz, O. Potin, V. Bourgeois, S. Vaz, F. |
dc.subject.por.fl_str_mv |
Titanium oxy-carbo-nitrides Reactive sputtering Transmission electron Microscopy Raman spectroscopy X-ray photoelectron Spectroscopy Science & Technology |
topic |
Titanium oxy-carbo-nitrides Reactive sputtering Transmission electron Microscopy Raman spectroscopy X-ray photoelectron Spectroscopy Science & Technology |
description |
The evolution of the nanoscale structure and the chemical bonds formed in Ti–C–N–O films grown by reactive sputtering were studied as a function of the composition of the reactive atmosphere by increasing the partial pressure of an O2+N2 gas mixture from 0 up to 0.4 Pa, while that of acetylene (carbon source) was constant. The amorphisation of the films observed by transmission electron microscopy was confirmed by micro- Raman spectroscopy, but it was not the only effect associated to the increase of the O2+N2 partial pressure. The chemical environment of titanium and carbon, analysed by X-ray photoemission spectroscopy, also changes due to the higher affinity of Ti towards oxygen and nitrogen than to carbon. This gives rise to the appearance of amorphous carbon coexisting with poorly crystallized titanium oxynitride. The evolution of the films colour is explained on the basis of these structural changes. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-10-31 2011-10-31T00:00:00Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
https://hdl.handle.net/1822/15684 |
url |
https://hdl.handle.net/1822/15684 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
0040-6090 10.1016/j.tsf.2011.06.108 http://www.sciencedirect.com/ |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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Elsevier |
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Elsevier |
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