Abstract
We establish the existence of chimera states, simultaneously supporting synchronous and asynchronous dynamics, in a network of two symmetrically linked star subnetworks of identical oscillators with shear and Kuramoto–Sakaguchi coupling. We show that the chimera states may be metastable or asymptotically stable. If the intra-star coupling strength is of order ɛ, the chimera states persist on time scales at least of order 1/ɛ in general, and on time-scales at least of order 1/ɛ2 if the intra-star coupling is of Kuramoto–Sakaguchi type. If the intra-star coupling configuration is sparse, the chimeras are asymptotically stable. The analysis relies on a combination of dimensional reduction using a Möbius symmetry group and techniques from averaging theory and normal hyperbolicity.
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Recommended by Dr Lev Tsimring
Footnotes
- 3
Here stands for Landau's symbols for order functions. So, is: there exists ɛ0 ⩾ 0 and K ⩾ 0 such that 0 ⩽ t ⩽ K|δ(ɛ)| for 0 ⩽ ɛ ⩽ ɛ0.
- 4
We select initial conditions satisfying the restrictions for system be in M and we add a small random uniform vector with each coordinate drawn from the interval (0, 0.01).
- 5
For all simulations involving the BA networks, we integrate the equations using an explicit Runge–Kutta method of order four.
- 6
The complete Möbius group consists of all fractional linear transformations of the complex plane such that ad − bc ≠ 0 but we only consider the subgroup that preserves the unit circle. As in related literature we refer to this subgroup as the Möbius group.
- 7
Here we mean the topological boundary, that is, .