1993
DOI: 10.1103/physreve.47.3231
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Theory of interaction and bound states of spiral waves in oscillatory media

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Cited by 72 publications
(80 citation statements)
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“…k ≃ −c −1 exp(−π/|2c|) for b = 0 and |c| ≪ 1 [10]. In the parameter region where the singlespiral solution is stable and c = b, the interaction between two well-separated spirals falls off exponentially [11][12][13]. The screening was attributed to the shock lines where the waves emitted by the cores collide.…”
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“…k ≃ −c −1 exp(−π/|2c|) for b = 0 and |c| ≪ 1 [10]. In the parameter region where the singlespiral solution is stable and c = b, the interaction between two well-separated spirals falls off exponentially [11][12][13]. The screening was attributed to the shock lines where the waves emitted by the cores collide.…”
mentioning
confidence: 99%
“…The screening was attributed to the shock lines where the waves emitted by the cores collide. For relatively small b, c the interaction is monotonic, and the spirals exhibit asymptotic repulsion irrespectively of their charge ("monotonic range") [11,12]. In contrast, for larger b, c satisfying the condition (c − b)/(1 + bc) > c * ≈ 0.845 the velocity vs distance dependence is modulated ("oscillatory range"), and the spirals become keen to form a variety of long-living (but unstable) bound states [11,14].…”
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