FeSe \({}_{\mathbf{0.5}}\)掺杂CeO \({}_{\mathbf{2}}\)的\({}_{\mathbf{0.5}}\)玻璃薄膜

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY
A. V. Petrov, O. V. Snigirev, E. A. Ovchenkov, Yu. V. Blinova, N. V. Porokhov, A. R. Shevchenko, D. A. Chareev, A. G. Maresov
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引用次数: 0

摘要

发现了FeSe \({}_{0.5}\) Te \({}_{0.5}\)薄膜在含氧化铈(ceo2 \({}_{2}\))的K-208玻璃非晶衬底上的沉积模式。该薄膜的超导态转变温度\(T_{\textrm{C}}=9.5\) K高于Fischer Scientific公司的硼硅酸盐玻璃(不含CeO \({}_{2}\)),但低于目标的超导态转变温度\(T_{\textrm{C}}(M)=14\) K。这种行为与FeSe和FeSe \({}_{x}\) Te \({}_{1-x}\)家族薄膜在晶体衬底上的众所周知的特性形成对比。根据测量结果,得到了涡活化能U、临界电流密度\(j_{\textrm{C}}\)、上临界场\(H_{C2}\)和不可逆性场\(H_{\textrm{irr}}\)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

FeSe\({}_{\mathbf{0.5}}\)Te\({}_{\mathbf{0.5}}\) Films on Glass with CeO\({}_{\mathbf{2}}\) Doping

FeSe\({}_{\mathbf{0.5}}\)Te\({}_{\mathbf{0.5}}\) Films on Glass with CeO\({}_{\mathbf{2}}\) Doping

Deposition modes for thin films of FeSe\({}_{0.5}\)Te\({}_{0.5}\) on an amorphous substrate made of K-208 glass, containing cerium oxide (CeO\({}_{2}\)), have been found. The transition temperature of the film, \(T_{\textrm{C}}=9.5\) K, to the superconducting state turned out to be higher than that on borosilicate glass from Fischer Scientific, which does not contain CeO\({}_{2}\), but lower than the superconducting transition temperature of the target, \(T_{\textrm{C}}(M)=14\) K. This behavior contrasts with the well-known properties of thin films in the FeSe and FeSe\({}_{x}\)Te\({}_{1-x}\) family on crystalline substrates. Based on the measurement results, the vortex activation energy (U), the critical current density (\(j_{\textrm{C}}\)), the upper critical field (\(H_{C2}\)), and the irreversibility field (\(H_{\textrm{irr}}\)) have been obtained.

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来源期刊
Moscow University Physics Bulletin
Moscow University Physics Bulletin PHYSICS, MULTIDISCIPLINARY-
CiteScore
0.70
自引率
0.00%
发文量
129
审稿时长
6-12 weeks
期刊介绍: Moscow University Physics Bulletin publishes original papers (reviews, articles, and brief communications) in the following fields of experimental and theoretical physics: theoretical and mathematical physics; physics of nuclei and elementary particles; radiophysics, electronics, acoustics; optics and spectroscopy; laser physics; condensed matter physics; chemical physics, physical kinetics, and plasma physics; biophysics and medical physics; astronomy, astrophysics, and cosmology; physics of the Earth’s, atmosphere, and hydrosphere.
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