Origin of flux noise in superconducting devices: Size distribution of spin species from phonon-assisted spin resonance

ORAL

Abstract

While it is universally accepted that the origin of flux noise in superconducting circuits is due to spin impurities at surfaces and interfaces, the identity of the spins remains a mistery. On-chip spin resonance experiments were able to identify atoms adsorbed to the devices' surfaces, but a broad absorption background of spin impurities remained unidentified [1]. Here we show that this background can be ascribed to phonon-assisted microwave absorption, and argue that the asymmetry of the one-phonon peak provides information on the size distribution of the spin-impurity wavefunction.

[1] S. E. de Graaf, A. A. Adamyan, T. Lindström, D. Erts, S. E. Kubatkin, A. Ya. Tzalenchuk, and A. V. Danilov, Phys. Rev. Lett. 118, 057703 (2017).

*This work was supported by the Natural Sciences and Engineering Research Council of Canada (NSERC) through Discovery program grants RGPIN-2020-04328 and RGPIN-2023-05309, and the Fonds de recherche--Nature et technologies (FRQNT) of Québec.

Presenters

  • Rogério de Sousa

    • Department of Physics and Astronomy, University of Victoria, BC

Authors

  • Rogério de Sousa

    • Department of Physics and Astronomy, University of Victoria, BC
  • José Alberto Nava Aquino

    • Department of Physics and Astronomy, University of Victoria, BC
  • William A Coish

    • Department of Physics, McGill University, QC
    • McGill University