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dc.contributor.authorBiktashev, V. N.en_GB
dc.contributor.authorBarkley, D.en_GB
dc.contributor.authorBiktasheva, I. V.en_GB
dc.date.accessioned2012-09-28T17:54:47Zen_GB
dc.date.accessioned2013-03-20T12:26:37Z
dc.date.issued2010-02-03en_GB
dc.description.abstractSpiral waves in active media react to small perturbations as particle-like objects. Here we apply the asymptotic theory to the interaction of spiral waves with a localized inhomogeneity, which leads to a novel prediction: drift of the spiral rotation centre along circular orbits around the inhomogeneity. The stationary orbits have alternating stability and fixed radii, 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 simulations confirm the validity and robustness of the theoretical predictions and show that these unexpected effects should be observable in experiment.en_GB
dc.identifier.citationVol. 104 (5), article 058302en_GB
dc.identifier.doi10.1103/PhysRevLett.104.058302en_GB
dc.identifier.urihttp://hdl.handle.net/10036/3767en_GB
dc.publisherAmerican Physical Societyen_GB
dc.rights© 2010 The American Physical Society
dc.titleOrbital Motion of Spiral Waves in Excitable Mediaen_GB
dc.date.available2012-09-28T17:54:47Zen_GB
dc.date.available2013-03-20T12:26:37Z
dc.identifier.journalPhysical Review Lettersen_GB


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