Noise Smooths the Devil's Staircase ✎

Original: "Arnold maps with noise: Differentiability and non-monotonicity of the rotation number"
arXiv:1904.11744 · 2019-04-26 · arXiv non-exclusive · independent analysis · 4 min
Even under strong nonlinearity, noise makes the rotation number smooth, but monotonicity is lost.

Context

The Arnold map serves as the simplest model of the interaction between two incommensurate oscillations, such as the seasonal cycle and internal instability in the climate system. In the deterministic case, for weak nonlinearity, the rotation number forms a "devil's staircase": it is constant on frequency-locking intervals and increases monotonically. However, describing El Niño's irregularity requires strong nonlinearity and the inclusion of short-period perturbations, such as westerly wind bursts, which are modeled as additive noise. This work sits alongside studies of turbulence and quantum chaos, where noise is also considered a regularizing factor, but here the case of strong nonlinearity in the Arnold map is rigorously investigated for the first time.

Methods

The authors consider a stochastic Arnold map on the circle, where at each step an independent uniformly distributed noise is added to the deterministic shift. To prove differentiability of the rotation number, they use linear response theory: they show that the stationary measure depends smoothly on the frequency parameter if the transfer operator is mixing. Mixing is verified via computer-assisted estimates that approximate the transfer operator by a finite-dimensional operator and provide rigorous bounds on the rate of convergence to equilibrium. Non-monotonicity of the rotation number is established by certified computation of the stationary measure with a small error in the L1 norm for specific parameter values.

Results

It is proven that for nonlinearity ε ≥ 1, the rotation number ρτ is a differentiable function of the parameter τ at every point where the stochastic system is mixing. An explicit formula for the derivative is obtained via the resolvent of the transfer operator and the derivative of the stationary measure. Computer-assisted estimates confirm mixing for ε = 1.4, ξ = 0.1, and τ ∈ [0.75, 0.8], which yields differentiability on this interval. For ε = 1.4 and ξ = 0.01, the rotation number is shown to be non-monotonic: as τ increases from 0.707 to 0.716, it first decreases and then increases. Numerical experiments indicate that non-monotonicity disappears for sufficiently large noise (e.g., ξ = 0.05).

Implications

This work differs from neighboring studies in that it is the first to rigorously establish differentiability of the rotation number for strong nonlinearity in the presence of noise, whereas previously this was known only for diffeomorphisms (ε < 1). Furthermore, the discovered non-monotonicity of the rotation number for ε ≥ 1 contrasts with the monotonic behavior in the weakly nonlinear case and points to the possibility of frequency locking for disconnected parameter regions. This expands the understanding of noise as a regularizer in random dynamical systems and connects linear response theory with climate models.

Future development

The methods of computer-assisted estimates can be extended to other families of maps with noise, including systems with Gaussian noise or more complex nonlinearities. Application to intermediate-complexity climate models, where additive noise is already used to parameterize subgrid processes, is promising. It is also interesting to investigate how non-monotonicity of the rotation number affects the predictability of El Niño in models with a hierarchy of complexity.

Impact

The results may influence the modeling of El Niño and other climate oscillations, as well as the analysis of synchronization in biological systems such as cardiac arrhythmias and neural rhythms.

Next steps

The next step could be extending the differentiability proof to the case of variable noise amplitude and to maps with more general nonlinearities. It is also important to study under what conditions non-monotonicity of the rotation number arises in realistic ENSO models.

Key open problems

In dynamical systems theory, the question of smoothness of statistical properties for systems with strong nonlinearity without noise remains open. This work shows that noise can restore smoothness, but at the same time it generates new phenomena, such as non-monotonicity of the rotation number, which is related to the problem of describing the transition to chaos in random systems.

The name "devil's staircase" for the graph of the rotation number reflects its step-like structure: at every rational frequency value the rotation number is constant, and between steps there are jumps. Adding noise "smooths" this staircase, turning it into a smooth curve, but under strong nonlinearity the staircase can bend downward, breaking monotonicity.

T_{\tau,\epsilon}(x) = x + \tau - \frac{\epsilon}{2\pi}\sin(2\pi x) \mod 1
The map shifts a point on the circle by τ and adds a nonlinear sinusoidal term with amplitude ε.
X_{n+1} = T_{\tau,\epsilon}(X_n) + \Omega_n \mod 1
At each step, an independent noise Ω_n, uniformly distributed on the interval [-ξ/2, ξ/2], is added to the deterministic map.
\frac{d}{d\tau}\rho_\tau(\tau_0) = 1 + \int_{S^1} \phi_{\tau_0} d[(Id - L_{\tau_0})^{-1} \frac{\delta_{-\xi} - \delta_{\xi}}{2\xi} * L_{T_{\tau_0,\epsilon}}(\mu_{\tau_0})]
The derivative of the rotation number is expressed via the resolvent of the transfer operator and the derivative of the stationary measure, following from linear response theory.

Key numbers

  • critical nonlinearity: ε = 1
  • noise amplitude for mixing proof: ξ = 0.1
  • noise amplitude for non-monotonicity: ξ = 0.01
  • τ interval with proven mixing: [0.75, 0.8]
Concepts
ENSO El Niño index El Niño-Southern Oscillation Multivariate ENSO Index Jin-Timmermann model natural variability TAO/TRITON moorings Southern Oscillation ERSST spring predictability barrier recharge oscillator model rotation number La Niña interannual variability relative ONI seasonal cycle mixed mode oscillations reynolds number equatorial wave propagation NOAA PMEL / TAO