A comparative study of accuracy and rollout stability of temporal surrogate models
For researchers in computational physics and dynamical systems, this work provides a fair comparison of architectures for long-horizon prediction stability, but the findings are incremental as they confirm known advantages of integrator-like updates.
This study compares several deep neural network architectures for temporal surrogate modeling of chaotic dynamical systems, finding that models with integrator-like updates exhibit lower bias and perturbation amplification, leading to more stable long-horizon rollouts and accurate predictions.
Temporal surrogate models are effective for predicting chaotic dynamical systems where computational cost can be prohibitive. Several deep neural network architectures can be used for such purposes. In this work, a few commonly used architectures are compared using a common training protocol. The objective is to fairly assess the impact of model architectures for long-horizon prediction stability. Experiments are carried out for three problems, the double pendulum, the Kuramoto-Sivashinsky equations, and the Kolmogorov flow. The experiments are carried out with matching model capacity. Analysis is also carried out for a scenario where each model is individually optimized. It is observed that in both scenarios, the models exhibit categorical differences in long-horizon rollouts. For a concrete quantification, stepwise error injections and perturbation amplifications are analyzed using metrics such as local jacobian, relative one-step bias, and finite-time Lyapunov growth. Additionally, an attractor analysis is also conducted to assess how well the learned models replicate the underlying system geometry. An ablation study to isolate the impact of each component of a continuous-update architecture is also carried out. It is concluded that models that having integrator-like updates show lower bias and perturbation amplification yielding stable long-horizon rollout and more accurate predictions.