Microwave properties of DyBCO monodomain in the mixed state and comparison with other RE-BCO systems
► Surface impedance measurements on Dy123 monodomains in the mixed state are presented. ► Larger London penetration depth is observed in the sample with stronger grain boundary signatures. ► The vortex viscosity of DyBCO monodomain shows same absolute values and temperature dependence as other 123 s...
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Published in: | Physica. C, Superconductivity Vol. 471; no. 21-22; pp. 854 - 858 |
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Main Authors: | , , , , , , |
Format: | Journal Article Web Resource |
Language: | English |
Published: |
Elsevier B.V
01-11-2011
Elsevier |
Subjects: | |
Online Access: | Get full text |
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Summary: | ► Surface impedance measurements on Dy123 monodomains in the mixed state are presented. ► Larger London penetration depth is observed in the sample with stronger grain boundary signatures. ► The vortex viscosity of DyBCO monodomain shows same absolute values and temperature dependence as other 123 systems.
We report on microwave measurements on DyBa2Cu3O7−δ monodomains grown by the top-seeded melt-textured technique. We measured the field increase of the surface resistance Rs(H) in the a–b plane at 48.3GHz. Measurements were performed at fixed temperatures in the range 70K–Tc with a static magnetic field μ0H<0.8T parallel to the c-axis. Low field steep increase of the dissipation, typical signature of the presence of weak links, is absent, thus indicating the single-domain behavior of the sample under study. The magnetic field dependence of Rs(H) is ascribed to the dissipation caused by vortex motion. The analysis of Xs(H) points to a free-flow regime, thus allowing to obtain the vortex viscosity as a function of temperature. We compare the results with those obtained on RE-BCO systems. In particular, we consider strongly pinned films of YBa2Cu3O7−δ with nanometric BaZrO3 inclusions. |
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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 scopus-id:2-s2.0-80055009606 |
ISSN: | 0921-4534 1873-2143 1873-2143 |
DOI: | 10.1016/j.physc.2011.05.073 |