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. 2017 Mar 29;14(128):20160968. doi: 10.1098/rsif.2016.0968

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© 2017 The Authors.

Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits unrestricted use, provided the original author and source are credited.

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Figure 5. — A parallel analysis of figure 3 to analyse AF initiation rate for longer duration of PV bursts up to 300 s. (a) Re-entry probability as a function of PV burst duration, for different model parameters. Discrete markers: simulation results; continuous curves: best fits using equation (3.3). (b) Re-entry probability as a function of model parameters, for different PV burst durations. Re-entry probability is nonlinear for all parameters, and exhibits non-monotonic dependence on BR and restitution steepness. We have joined the scatter plots in this panel for optimal visualization of the non-monotonicity in this panel.