Linear stability analysis of rotating spiral waves in excitable media

Dwight Barkley
Phys. Rev. Lett. 68, 2090 – Published 30 March 1992
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Abstract

Fast numerical methods are used to solve the equations for periodically rotating spiral waves in excitable media, and the associated eigenvalue problem for the stability of these waves. Both equally and singly diffusive media are treated. Rotating-wave solutions are found to be discretely selected by the system and an isolated, complex-conjugate pair of eigenmodes is shown to cause instability of these waves. The instability arises at the point of zero curvature on the spiral interface and results in wavelike disturbances which propagate from this point along the interface.

  • Received 16 December 1991

DOI:https://doi.org/10.1103/PhysRevLett.68.2090

©1992 American Physical Society

Authors & Affiliations

Dwight Barkley

  • Program in Applied and Computational Mathematics, Princeton University, Princeton, New Jersey 08544

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Vol. 68, Iss. 13 — 30 March 1992

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