A1 Refereed original research article in a scientific journal

Verifying Theoretical Models of Flux Pinning Using Heavy Ion Irradiated YBCO Thin Films




AuthorsPaturi, Petriina; Aye, Moe Moe; Soman, Arya; Notthoff, Christian; Kluth, Patrick; Strickland, Nicholas; Huhtinen, Hannu

PublisherInstitute of Electrical and Electronics Engineers (IEEE)

Publication year2025

JournalIEEE Transactions on Applied Superconductivity

Journal name in sourceIEEE Transactions on Applied Superconductivity

Article number8000105

Volume35

Issue5

ISSN1051-8223

eISSN2378-7074

DOIhttps://doi.org/10.1109/TASC.2025.3527949(external)

Web address https://doi.org/10.1109/tasc.2025.3527949(external)

Self-archived copy’s web addresshttps://research.utu.fi/converis/portal/detail/Publication/484521670(external)


Abstract
We have irradiated YBa2 Cu3O6+x (YBCO) films without artificial pinning sites with Ag+ ions with energies of 75 MeV and 150 MeV and fluences between 2-8 · 1011 ions/cm2 in order to create as controlled nanorod pinning sites as possible. The structural and superconducting properties were determined before and after the irradiation with x-ray diffraction and magnetic measurement. After the irradiation also transport and transmission electron microscopy measurements were made. It was noted that the ion tracks are all parallel to the YBCO c-axis of the sample and those done with 150 MeV ions formed continuous 5 nm diameter tracks, whereas with 75 MeV ions, the tracks were not continuous through the sample. The Tc and Jc(0,T) decreased with the irradiation, but the in-field Jc increased. The maximum increase was obtained with the 150MeV and 4· 1011 ions/cm2 sample with continuous rods, where the distance between the rods was closest to the diameter of the rods. Thus, the previous theoretical models predicting optimal pinning when the pinning site diameter is approximately equal to the distance between the pinning sites, are experimentally verified for these very pure samples, with no other external pinning sites.

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Funding information in the publication
This work was supported in part by the Jenny and Antti Wihuri Foundation and in part by the Royal Society of New Zealand under Marsden Fund under Grant VUW1805.


Last updated on 2025-25-02 at 10:47