Unpinning triggers for superfluid vortex avalanches

L. Warszawski, A. Melatos, and N. G. Berloff
Phys. Rev. B 85, 104503 – Published 6 March 2012

Abstract

The pinning and collective unpinning of superfluid vortices in a decelerating container is a key element of the canonical model of neutron star glitches and laboratory spin-down experiments with helium II. Here the dynamics of vortex (un-)pinning is explored using numerical Gross-Pitaevskii calculations, with a view to understanding the triggers for catastrophic unpinning events (vortex avalanches) that lead to rotational glitches. We explicitly identify three triggers: rotational shear between the bulk condensate and the pinned vortices, a vortex proximity effect driven by the repulsive vortex-vortex interaction, and sound waves emitted by moving and repinning vortices. So long as dissipation is low, sound waves emitted by a repinning vortex are found to be sufficiently strong to unpin a nearby vortex. For both ballistic and forced vortex motion, the maximum inter-vortex separation required to unpin scales inversely with pinning strength.

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  • Received 17 August 2010

DOI:https://doi.org/10.1103/PhysRevB.85.104503

©2012 American Physical Society

Authors & Affiliations

L. Warszawski1,*, A. Melatos1, and N. G. Berloff2

  • 1School of Physics, The University of Melbourne, Parkville 3010, Victoria, Australia
  • 2Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, United Kingdom

  • *lila@unimelb.edu.au

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Vol. 85, Iss. 10 — 1 March 2012

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