Examples of nearly integrable systems on $\mathbb{A}^3$ with   asymptotically dense projected orbits
  Given an integer $\kappa\geq2$, we introduce a class of nearly integrable systems on $\mathbb{A}^3$, of the form $$ H_n(\theta,r)=\frac12 \Vert r\Vert ^2+\tfrac{1}{n} U(\theta_2,\theta_3)+f_n(\theta,r) $$ where $U\in C^\kappa(\mathbb{T}^2)$ is a generic potential function and $f_n$ a $C^{\kappa-1}$ additional perturbation such that $\Vert f_n\Vert_{C^{\kappa-1}(\mathbb{A}^3)}\leq \tfrac{1}{n}$, so that $H_n$ is a perturbation of the completely integrable system $h(r)=\frac12\Vert r\Vert ^2$.   Let $\Pi:\mathbb{A}^3\to\mathbb{R}^3$ be the canonical projection. We prove that for each $\delta>0$, there exists $n_0$ such that for $n\geq n_0$, the system $H_n$ admits an orbit $\Gamma_n$ at energy $\frac12$ whose projection $\Pi(\Gamma_n)$ is $\delta$-dense in $\Pi(H_n^{-1}(\tfrac{1}{2}))$, in the sense that the $\delta$-neighborhood of $\Pi(\Gamma_n)$ in $\mathbb{R}^3$ covers $\Pi(H_n^{-1}(\frac{1}{2}))$. 
Jean-Pierre Marco and Lara Sabbagh
math.DS math.SG