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Thin Films of Niobium Tin by Codeposition
Thin films of niobium tin were deposited by the simultaneous condensation of niobium and tin vapor from two separate evaporation sources in a vacuum system. The composition and structure of the deposit was examined as a function of substrate temperature and the relative impingement rate of niobium t...
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Published in: | Journal of applied physics 1964-12, Vol.35 (12), p.3599-3603 |
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Main Author: | |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Thin films of niobium tin were deposited by the simultaneous condensation of niobium and tin vapor from two separate evaporation sources in a vacuum system. The composition and structure of the deposit was examined as a function of substrate temperature and the relative impingement rate of niobium to tin.
If this rate ratio is near 3:1, the cubic phase Nb3Sn is the predominant product, regardless of substrate temperature, even if it is much below the temperature where Nb3Sn forms in the bulk. For a ratio of 3:2, and at substrate temperatures less than 800°C, formation of Nb3Sn is almost entirely suppressed, and phases higher in tin predominate. Annealing at 900°C converts the phases high in tin to Nb3Sn.
The superconducting critical temperature of codeposited niobium tin films is below 14°K before annealing and above 14°K after annealing at 900°C. The superconducting energy gap is the order of 1 meV at 4.2°K, considerably below the value predicted by the BCS theory. This suggests that the material on the surface of the films has a lower critical temperature than in the interior. |
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ISSN: | 0021-8979 1089-7550 |
DOI: | 10.1063/1.1713278 |