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Defect formation in the Swift-Hohenberg equation

Tobias Galla and Esteban Moro
Phys. Rev. E 67, 035101(R) – Published 12 March 2003
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Abstract

We study numerically and analytically the dynamics of defect formation during a finite-time quench of the two-dimensional Swift-Hohenberg (SH) model of Rayleigh-Bénard convection. We find that the Kibble-Zurek picture of defect formation can be applied to describe the density of defects produced during the quench. Our study reveals the relevance of two factors: the effect of local variations of the striped patterns within defect-free domains and the presence of both pointlike and extended defects. Taking into account these two aspects we are able to identify the characteristic length scale selected during the quench and to relate it to the density of defects. We discuss possible consequences of our study for the analysis of the coarsening process of the SH model.

  • Received 26 November 2002

DOI:https://doi.org/10.1103/PhysRevE.67.035101

©2003 American Physical Society

Authors & Affiliations

Tobias Galla1,* and Esteban Moro1,2,†

  • 1Theoretical Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP, United Kingdom
  • 2Departamento de Matemáticas and GISC, Universidad Carlos III de Madrid, Avenida Universidad 30, 28911 Leganés, Spain

  • *Electronic address: galla@thphys.ox.ac.uk
  • Electronic address: emoro@math.uc3m.es

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Vol. 67, Iss. 3 — March 2003

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