YBa<inf>2</inf>Cu<inf>3</inf>O<inf>7</inf> films grown onto SrTiO<inf>3</inf> and YSZ substrates by chemical solution deposition of trifluoroacetates
Authors
Domínguez, AB
Cornejo, HS
Osorio-Anaya, AM
Santibañez, JF
Sovero, LS
Barnes, CHW
Publication Date
2021Journal Title
Journal of Electroceramics
ISSN
1385-3449
Publisher
Springer Science and Business Media LLC
Volume
47
Issue
1
Pages
15-22
Language
en
Type
Article
This Version
VoR
Metadata
Show full item recordCitation
Domínguez, A., De Los Santos Valladares, L., Cornejo, H., Osorio-Anaya, A., Santibañez, J., Sovero, L., & Barnes, C. (2021). YBa<inf>2</inf>Cu<inf>3</inf>O<inf>7</inf> films grown onto SrTiO<inf>3</inf> and YSZ substrates by chemical solution deposition of trifluoroacetates. Journal of Electroceramics, 47 (1), 15-22. https://doi.org/10.1007/s10832-021-00256-5
Abstract
<jats:title>Abstract</jats:title><jats:p>We report the preparation and characterization of YBa<jats:sub>2</jats:sub>Cu<jats:sub>3</jats:sub>O<jats:sub>7</jats:sub> (YBCO) films grown onto SrTiO<jats:sub>3</jats:sub> and YSZ substrates by the trifluoroacetates chemical solution deposition method and following sintering with oxygen atmosphere at 860 °C. The X-ray diffraction (XRD) reveals (00ℓ) – oriented crystallites indicating epitaxial growth of the films in the <jats:italic>c</jats:italic>-direction. Despite granular morphology and the presence of Y<jats:sub>2</jats:sub>BaCuO<jats:sub>5</jats:sub> and CuO as minor secondary phases, the technique shows the successful formation of the superconducting YBCO and preventing the formation of the unwanted BaCO<jats:sub>3</jats:sub> phase. Rocking curve measurements of the (005) reflection for the YBCO/SrTiO<jats:sub>3</jats:sub> was fitted with one Gaussian function with full width at the half maximum (FWHM) of 0.44° confirming that it consists of YBCO crystallites with different texture. For the sample grown on YSZ, the rocking curve was fitted with two Gaussian functions, one corresponding to the YBCO layer (FWHM = 0.4°) and another to the substrate (FWHM = 0.3°). The magnetic measurements taken in zero field cooling and field cooling modes confirm the formation of the superconducting YBCO with critical temperatures (<jats:italic>T</jats:italic><jats:sub>C</jats:sub>) 91.8 and 85.7 K for the samples grown onto YSZ and SrTiO<jats:sub>3</jats:sub>, respectively. The critical current density (<jats:italic>J</jats:italic><jats:sub>C</jats:sub>) curves indirectly calculated by using the Bean´s model from the <jats:italic>M</jats:italic>(<jats:italic>T</jats:italic>) loops were <jats:italic>J</jats:italic><jats:sub>C</jats:sub> ~ 10<jats:sup>9</jats:sup> A/cm<jats:sup>2</jats:sup> for the sample deposited onto YSZ and <jats:italic>J</jats:italic><jats:sub>C</jats:sub> ~ 10<jats:sup>7</jats:sup>A/cm<jats:sup>2</jats:sup> for the YBCO deposited onto SrTiO<jats:sub>3</jats:sub>. Overall, the difference in <jats:italic>T</jats:italic><jats:sub>C</jats:sub> and <jats:italic>J</jats:italic><jats:sub>C</jats:sub> values between both samples could be related to their difference in oxygen content, porosity, hole concentration per Cu ion and the presence of secondary phases.</jats:p>
Keywords
YBCO, Chemical solution deposition, Superconductors, Trifluoroacetates
Identifiers
s10832-021-00256-5, 256
External DOI: https://doi.org/10.1007/s10832-021-00256-5
This record's URL: https://www.repository.cam.ac.uk/handle/1810/338224
Rights
Licence:
http://creativecommons.org/licenses/by/4.0/
Statistics
Total file downloads (since January 2020). For more information on metrics see the
IRUS guide.
Recommended or similar items
The current recommendation prototype on the Apollo Repository will be turned off on 03 February 2023. Although the pilot has been fruitful for both parties, the service provider IKVA is focusing on horizon scanning products and so the recommender service can no longer be supported. We recognise the importance of recommender services in supporting research discovery and are evaluating offerings from other service providers. If you would like to offer feedback on this decision please contact us on: support@repository.cam.ac.uk