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...

Full description

Saved in:
Bibliographic Details
Published in:Physica. C, Superconductivity Vol. 471; no. 21-22; pp. 854 - 858
Main Authors: Pompeo, N., Rogai, R., Ausloos, M., Cloots, R., Augieri, A., Celentano, G., Silva, E.
Format: Journal Article Web Resource
Language:English
Published: Elsevier B.V 01-11-2011
Elsevier
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
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.
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