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Orbital Motion of Spiral Waves in Excitable Media

Source: Phys. Rev. Lett. 104, 058302 (2010); doi:10.1103/PhysRevLett.104.058302

Published 3 February 2010

PACS
  • 82.40.Ck
    Pattern formation in chemical reactions with diffusion, flow and heat transfer
  • 05.45.-a
    Nonlinear dynamics and chaos
  • 87.18.Hf
    Spatiotemporal pattern formation in cellular populations
  • 87.19.Hh
    Cardiac dynamics
  • YEAR: 2010
PUBLICATION DATA
ISSN:
1553-9628 (online)
Publisher:
AIP is a member of CrossRef APS
V. N. Biktashev
Department of Mathematical Sciences, University of Liverpool, Liverpool L69 7ZL, United Kingdom

D. Barkley
Mathematics Institute, University of Warwick, Coventry CV4 7AL, United Kingdom

I. V. Biktasheva
Department of Computer Science, University of Liverpool, Liverpool L69 3BX, United Kingdom
Spiral waves in active media react to small perturbations as particlelike objects. Here we apply asymptotic theory to the interaction of spiral waves with a localized inhomogeneity, which leads to a novel prediction: drift of the spiral rotation center along circular orbits around the inhomogeneity. The stationary orbits have fixed radii and alternating stability, determined by the properties of the bulk medium and the type of inhomogeneity, while the drift speed along an orbit depends on the strength of the inhomogeneity. Direct numerical simulations confirm the validity and robustness of the theoretical predictions and show that these unexpected effects should be observable in experiment. ©2010 The American Physical Society
History: Received 31 July 2009; published 3 February 2010
Permalink: http://link.aps.org/abstract/PRL/v104/e058302
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