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On some refraction billiards

Dedicated to J.L. Vázquez with great affection and admiration

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  • The aim of this work is to continue the analysis, started in [10], of the dynamics of a point-mass particle $ P $ moving in a galaxy with an harmonic biaxial core, in whose center sits a Keplerian attractive center (e.g. a Black Hole). Accordingly, the plane $ \mathbb{R}^2 $ is divided into two complementary domains, depending on whether the gravitational effects of the galaxy's mass distribution or of the Black Hole prevail. Thus, solutions alternate arcs of Keplerian hyperbolæ with harmonic ellipses; at the interface, the trajectory is refracted according to Snell's law. The model was introduced in [11], in view of applications to astrodynamics.

    In this paper we address the general issue of periodic and quasi-periodic orbits and associated caustics when the domain is a perturbation of the circle, taking advantage of KAM and Aubry-Mather theories.

    Mathematics Subject Classification: Primary: 70H08, 70H12, 37N05, Secondary: 70G75, 70F16, 70F10.

    Citation:

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  • Figure 1.  Examples of trajectories for $ \mathcal{E} = 2.5 $, $ \omega = 1 $, $ h = 2 $ and $ \mu = 2 $. Left: general trajectory for an elliptic domain with eccentricity $ e = 0.6 $. Right: quasi-periodic trajectory for a circular domain

    Figure 2.  Orbits of the first return map $ F $ for $ \mathcal{E} = 10 $, $ \omega = 1 $, $ h = 3 $, $ \mu = 44 $ (left) and $ \mu = 55 $ (right). The shift in the stability of the homothetic equilibrium is evident, as well as the presence of invariant curves far from the $ \xi $-axis in both cases

    Figure 3.  Examples of periodic and non-periodic orbits on the circle in the phase space $ \left(\xi, I\right)\in \mathbb{R}_{/2\pi\mathbb{Z}}\times\mathcal I $

    Figure 4.  Example of a non-homothetic fixed point for $ \mathcal{F} $, with $ \mathcal{E} = 7, \omega^2 = 3, h = 2, \mu = 15 $. In this case, with reference to Proposition 4.10, $ \bar{\mu} = 41.6287 $

    Figure 5.  Curve $ \Gamma_{\tilde \alpha} $ for the computation of the winding number in the perturbed case

    Figure 6.  Sketch of the perturbed dynamics in the region described by Proposition 5.6 and Theorem 5.12 in the phase plane $ (\xi, I) $. Red: the invariant curves of Diophantine rotation numbers $ \rho_0 $ and $ \rho_1 $, which are deformations of the unperturbed invariant straight lines $ I = \bar I_{\rho_0} $, $ I = \bar I_{\rho_1} $ (green) such that $ \bar\theta\left(\bar I_{\rho_0}\right) = \rho_0 $ and $ \bar\theta\left(\bar I_{\rho_1}\right) = \rho_1 $. In the striped region the map $ \mathcal F(\xi_{0}, I_0; \epsilon) $ is area-preserving and twist. The blue dashed lines denote two singular action values for the unperturbed dynamics (i.e. $ I\in\bar{\mathcal{I}} $)

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