2405.05897
Efficient Numerical Computation of Spiral Spectra with Exponentially-Weighted Preconditioners
Stephanie Dodson, Ryan Goh, Björn Sandstede
correcthigh confidence
- Category
- Not specified
- Journal tier
- Strong Field
- Processed
- Sep 28, 2025, 12:56 AM
- arXiv Links
- Abstract ↗PDF ↗
Audit review
The paper proves uniform weighted resolvent bounds and unweighted exponential growth/ boundedness criteria for spiral waves on large disks via radial spatial dynamics, exponential dichotomies, and a far-field/boundary-layer gluing argument. The candidate solution follows the same structure: reduction to a first-order r-flow, choice of η ∈ J0(λ) to create a dichotomy, robustness under tail perturbations, and a core–tail matching map to obtain uniform bounds away from Σ∞, plus a boundary-layer pseudomode argument when 0 ∉ J0(λ*). Minor mismatches are present (e.g., the size/decay of the tail perturbation and the exact function space), but they do not alter the logic or conclusions. Overall, the model’s solution is a faithful proof sketch of Theorems 3.8 and 3.9.
Referee report (LaTeX)
\textbf{Recommendation:} minor revisions \textbf{Journal Tier:} strong field \textbf{Justification:} The main results are correct and relevant, and the proof strategy is rigorous, blending spatial dynamics with exponential dichotomies and boundary-layer analysis. The numerical motivation is compelling. Minor clarifications about the tail perturbation size and the functional-analytic setup (transfer between X and Y) would make the exposition more accessible and avoid misinterpretation by readers who rely on heuristic phrasing.