Flux pinning by columnar defects in high-temperature superconducting crystals

M. Konczykowski, Y. Yeshurun, L. Klein, E. R. Yacoby, N. Chikumoto, V. M. Vinokur, M. V. Feigel'man

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12 Scopus citations

Abstract

Y-Ba-Cu-O:123 and Bi-Sr-Ca-Cu-O:2212 crystals were irradiated with 5.8 GeV Pb ions. The columnar defects, produced by this irradiation are expected to yield the strongest possible pinning energy. Indeed, there is an apparent increase in the width of the magnetization curves. However, the results of magnetic relaxation experiments indicate the energy barrier for flux creep from the columnar defects much smaller than expected pinning energy. This effect is explained in terms of nucleation of vortex loop mechanism of flux creep. The estimate of pinning energy of columnar defect can be obtained from measurement of the angular dependence of the magnetization curves.

Original languageEnglish
Pages (from-to)407-410
Number of pages4
JournalJournal of Alloys and Compounds
Volume195
Issue numberC
DOIs
StatePublished - 10 May 1993

Bibliographical note

Funding Information:
The authors thank Florence Rullier-Albenque and Serge Bouffard for help in irradiation. V.M.V. acknowledges support from Argonne National Laboratory through US Department of Energy, BES-Material Sciences under Contract #W-31-109-ENG-38, and through the NSF founded Science and Technology Center for Superconductivity under Grant No. DMR88-09854.The work in Israel is partially suppported by the Ministry of Science and Technolodgy.

Funding

The authors thank Florence Rullier-Albenque and Serge Bouffard for help in irradiation. V.M.V. acknowledges support from Argonne National Laboratory through US Department of Energy, BES-Material Sciences under Contract #W-31-109-ENG-38, and through the NSF founded Science and Technology Center for Superconductivity under Grant No. DMR88-09854.The work in Israel is partially suppported by the Ministry of Science and Technolodgy.

FundersFunder number
BES-Material Sciences-31-109-ENG-38
NSF founded Science and Technology Center for SuperconductivityDMR88-09854
U.S. Department of Energy
Argonne National Laboratory

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