Enviar artigo por via de e-mail Research of Titanium Saturation with Gas and Feature of Ceramic Layer Formation Using the Oxidative Constructing Approach
- Autores: Zufman V.Y.1, Shokodko A.V.1, Kovalev I.A.1, Ashmarin A.A.1, Ogarkov A.I.1, Ovsyannikov N.A.1, Klimov A.A.2, Klimaev S.N.1, Kochanov G.P.1, Shokodko E.A.3, Chesnokov A.A.1, Chernyavskii A.S.1, Solntsev K.A.1
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Afiliações:
- Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
- LLC Aurora Borealis
- National Research Moscow State University of Civil Engineering
- Edição: Volume 10, Nº 5 (2019)
- Páginas: 1171-1176
- Seção: General-Purpose Materials
- URL: https://journals.rcsi.science/2075-1133/article/view/208094
- DOI: https://doi.org/10.1134/S2075113319050381
- ID: 208094
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Abstract—Samples made of titanium grade BT 1-0 in the form of disks were subjected to isothermal aging at 875°C with access to atmospheric air for 2, 4, 6, 7, and 13 days. As a result of XRD, it was established that the oxide layer is rutile TiO2. The metal blank absorbs oxygen and nitrogen from atmospheric air, which are concentrated in the surface layer. The increase in the mass of oxygen going to the formation of rutile is 96–98 wt % of the total amount of gas absorbed. The rest of the absorbed gas (2–4 wt %) is contained in the metal blank in the form of solid solutions. The gas absorption rate of a titanium blank is proportional to the rate of rutile formation. The process kinetics for each of the sample surfaces (side and end), which is described by an exponential law, is determined. At the initial stage of the oxidation process, the surface geometry does not affect the rate of formation of the ceramic layer of rutile; subsequently, there is an “acceleration” of rutile growth on the end surface.
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Sobre autores
V. Zufman
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: vzufman@imet.ac.ru
Rússia, Moscow, 119334
A. Shokodko
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: ashokodko@imet.ac.ru
Rússia, Moscow, 119334
I. Kovalev
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: ikovalev@imet.ac.ru
Rússia, Moscow, 119334
A. Ashmarin
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: aashmarin@imet.ac.ru
Rússia, Moscow, 119334
A. Ogarkov
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: aogarkov@imet.ac.ru
Rússia, Moscow, 119334
N. Ovsyannikov
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: novsyannikov@imet.ac.ru
Rússia, Moscow, 119334
A. Klimov
LLC Aurora Borealis
Email: ksolntsev@imet.ac.ru
Rússia, Moscow, 121205
S. Klimaev
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: sklimaev@imet.ac.ru
Rússia, Moscow, 119334
G. Kochanov
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: gkochanov@imet.ac.ru
Rússia, Moscow, 119334
E. Shokodko
National Research Moscow State University of Civil Engineering
Email: ksolntsev@imet.ac.ru
Rússia, Moscow, 129337
A. Chesnokov
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Email: ksolntsev@imet.ac.ru
Rússia, Moscow, 119334
A. Chernyavskii
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: aschernyavskiy@imet.ac.ru
Rússia, Moscow, 119334
K. Solntsev
Baikov Institute of Metallurgy and Materials Science, Russian Academy of Sciences
Autor responsável pela correspondência
Email: ksolntsev@imet.ac.ru
Rússia, Moscow, 119334
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