Abstract
To address the problem of how cardiac muscle contraction affects the dynamics of rotating spiral waves, spiral breakup induced by mechanical deformation in excitable media is studied in two partial-differential-equation models. It is shown that spirals begin to break up at ω=0.5ω0 when we increase the amplitude of the mechanical deformation gradually. Our numerical results point to a new mechanism of transition from spirals to spatiotemporal chaos, in which the anisotropic time-dependent diffusion coefficient is essential.
Original language | English |
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Article number | 016212 |
Pages (from-to) | 016212-1-016212-5 |
Number of pages | 5 |
Journal | Physical Review E |
Volume | 70 |
Issue number | 1 |
DOIs | |
Publication status | Published - 26 Jul 2004 |
Scopus Subject Areas
- Statistical and Nonlinear Physics
- Statistics and Probability
- Condensed Matter Physics