Periodic traveling waves (wavetrains) have been extensively studied for reaction-diffusion equations. One important motivation for this work has been the identification of periodic traveling wave patterns in spatiotemporal data sets in ecology. However, for many ecological populations, diffusion is no more than a rough phenomenological representation of dispersal, and spatial convolution with a dispersal kernel is more realistic. This paper concerns periodic traveling wave solutions of differential equations with nonlocal dispersal terms, and with local dynamics of lambda-omega form. These kinetics include the normal form near a standard supercritical Hopf bifurcation and are therefore significant for a wide range of applications. For general dispersal kernels, an explicit family of periodic traveling wave solutions is derived, as well as the condition for waves to be stable to perturbations of arbitrarily small wavenumber. Three specific kernels are then considered in detail: Laplace, Gaussian, and top hat. For Laplace and Gaussian kernels, it is shown that stability to perturbations of arbitrarily small wavenumber implies stability, a result that also applies for reaction-diffusion equations with lambda-omega kinetics. However, for the top hat kernel it is shown that periodic traveling waves may be stable to perturbations with small wavenumber but not to those with larger wavenumber. The wave family for the top hat kernel also shows significant qualitative differences from those for the Laplace and Gaussian kernels, and for reaction-diffusion equations with the same kinetics.Motivated by the form of PTW solutions of (1.1), I look for solutions of (2.1) with the form r = R, θ = αx + βt, where R ≥ 0, α ≥ 0, and β are constants, givingNote that (2.2) is only valid for even kernels K(.). Figure 1 shows various examples of such PTW solutions, when K(.) is the Laplace kernel (defined in (3.1) below). Figure 1. Examples of PTW solutions of (1.4) for the Laplace kernel (3.1) with a = 1, plotted as a function of space x. The functions λ(.) and ω(.) are given by (1.2) with λ1 = 1; the values of λ0 and α are as shown in the figure. Note that the values of ω0 and ω1 do not affect the PTW as a function of space. The left-and right-hand columns illustrate wave families for λ(0) < 1 and λ(0) > 1, respectively. In both cases, waves for small α have large wavelength and high amplitude, approaching a spatially homogeneous oscillation as α → 0 + . When λ(0) < 1, the wave amplitude is zero at a finite value of α, which is 2 for the value of λ0 used in the left-hand column of the figure. In contrast when λ(0) > 1 there is no upper bound on the values of α giving waves, and the wavelength → 0 with the amplitude remaining nonzero as α → ∞.Since λ(.) is strictly decreasing, (2.2) has a (unique) solution for R and β if and only if C 0 ∈ [1 − λ(0), 1]. Intuitive understanding of this is helped by considering the cases α = 0 and Downloaded 11/06/14 to 137.195.26.108. Redistribution subject to SIAM license or copyright; see
PERIODIC WAVES...