• Open Access

Origin of superconductivity at nickel-bismuth interfaces

Matthew Vaughan, Nathan Satchell, Mannan Ali, Christian J. Kinane, Gavin B. G. Stenning, Sean Langridge, and Gavin Burnell
Phys. Rev. Research 2, 013270 – Published 6 March 2020

Abstract

Unconventional superconductivity has been suggested to be present at the interface between bismuth and nickel in thin-film bilayers. In this work, we study the structural, magnetic, and superconducting properties of sputter deposited Bi/Ni bilayers. As-grown, our films do not display a superconducting transition; however, when stored at room temperature, after about 14 days our bilayers develop a superconducting transition up to 3.8 K. To systematically study the effect of low temperature annealing on our bilayers, we perform structural characterization with x-ray diffraction and polarized neutron reflectometry, along with magnetometry and low-temperature electrical transport measurements on samples annealed at 70C. We show that the onset of superconductivity in our samples is coincident with the formation of ordered NiBi3 intermetallic alloy, a known s-wave superconductor. We calculate that the annealing process has an activation energy of (0.86±0.06)eV. As a consequence, gentle heating of the bilayers will cause formation of the superconducting NiBi3 at the Ni/Bi interface, which poses a challenge to studying any distinct properties of Bi/Ni bilayers without degrading that interface.

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  • Received 22 November 2019
  • Accepted 4 February 2020

DOI:https://doi.org/10.1103/PhysRevResearch.2.013270

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Matthew Vaughan1, Nathan Satchell1, Mannan Ali1, Christian J. Kinane2, Gavin B. G. Stenning2, Sean Langridge2, and Gavin Burnell1,*

  • 1School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, United Kingdom
  • 2ISIS Neutron and Muon Source, Rutherford Appleton Laboratory, Harwell, Oxon OX11 0QX, United Kingdom

  • *g.burnell@leeds.ac.uk

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Vol. 2, Iss. 1 — March - May 2020

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