2206.04997
Dynamics of a Rotated Orthogonal Gravitational Wedge Billiard
K. D. Anderson
incompletemedium confidence
- Category
- Not specified
- Journal tier
- Note/Short/Other
- Processed
- Sep 28, 2025, 12:56 AM
- arXiv Links
- Abstract ↗PDF ↗
Audit review
The paper states that trajectories are dense when TA/TB is irrational and that periodic orbits occur for θ* = arctan(p/q), but the density claim is only asserted via a one-dimensional approximation and a heuristic time-map argument (equations (13)–(16)) without a rigorous torus-flow proof; it also contains minor inconsistencies (e.g., ũ(t) uses cos(ϕ) instead of cos(θ) in (8b)) and an imprecise use of tAj+1 = 2 j TA that obscures whether these are absolute times or increments . By contrast, the model cleanly constructs exact normal-distance coordinates dA, dB with constant accelerations −sin θ and −cos θ (no approximation), shows the two “clocks” evolve as a linear flow on T2, proves minimality for irrational slopes and density in the accessible set QE, and recovers the periodic case (including the p and q collision counts and the initial momentum (ū*, w̄*)) in a self-contained way, matching the formulas reported in the paper (11), (12), and (17) .
Referee report (LaTeX)
\textbf{Recommendation:} major revisions \textbf{Journal Tier:} note/short/other \textbf{Justification:} The manuscript identifies and parameterizes an integrable wedge-billiard case and provides explicit periodic orbits, but it relies on a near-wall one-dimensional approximation and figures to justify density. A short, rigorous derivation of the two independent clocks and the standard minimality of irrational linear flows on the 2-torus would remedy the main gap; correcting minor formula/notation issues would also improve clarity. With these fixes, the contribution would be sound and useful for specialists.