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Birkhoff attractors of dissipative billiards

Published online by Cambridge University Press:  30 September 2024

OLGA BERNARDI*
Affiliation:
Dipartimento di Matematica Tullio Levi-Civita, Università di Padova, via Trieste 63, Padova 35121, Italy
ANNA FLORIO
Affiliation:
CEREMADE-Université Paris Dauphine-PSL, Paris 75775, France (e-mail: florio@ceremade.dauphine.fr)
MARTIN LEGUIL
Affiliation:
École polytechnique, CMLS, Route de Saclay, Palaiseau Cedex 91128, France (e-mail: martin.leguil@polytechnique.edu)
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Abstract

We study the dynamics of dissipative billiard maps within planar convex domains. Such maps have a global attractor. We are interested in the topological and dynamical complexity of the attractor, in terms both of the geometry of the billiard table and of the strength of the dissipation. We focus on the study of an invariant subset of the attractor, the so-called Birkhoff attractor. On the one hand, we show that for a generic convex table with ‘pinched’ curvature, the Birkhoff attractor is a normally contracted manifold when the dissipation is strong. On the other hand, for a mild dissipation, we prove that, generically, the Birkhoff attractor is complicated, both from the topological and the dynamical points of view.

Information

Type
Original Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press
Figure 0

Figure 1The standard billiard map and its dissipative counterpart.

Figure 1

Figure 2Birkhoff attractor of a dissipative billiard map $f_{\unicode{x3bb} }$ within an ellipse of non-zero eccentricity when the dissipation is mild, that is, $\unicode{x3bb} $ is close to $1$.

Figure 2

Figure 3The geometric condition $\max _{s \in {\mathbb T}} \tau (s)\mathcal {K}(s)<-1$ in Definition D. Here, $R(s):=-{1}/{\mathcal {K}(s)}$ is the radius of curvature, and $\mathscr {C}(O(s),R(s))$ is the osculating circle at $\Upsilon (s)$.

Figure 3

Figure 4Phase transition for a $C^k$-generic domain near an ellipse of non-zero eccentricity, $k \geq 3$.

Figure 4

Figure 5The Lyapunov function $\zeta $.

Figure 5

Figure 6An example of an indecomposable continuum (L Rempe-Gillen, CC BY-SA 3.0 https://creativecommons.org/licenses/by-sa/3.0, via Wikimedia Commons).

Figure 6

Figure 7The cones $C_+(x,\beta )$ and $C_-(x,\beta )$.

Figure 7

Figure 8The lower and upper verticals.

Figure 8

Figure 9Here, $\mathscr {I}^-:=\mathrm {int}(C^-)$ is the part of the instability region $\mathscr {I}=\mathrm {int}(C)$ that lies below the zero section $\mathbb {T} \times \{0\}$, while $\mathscr {I}_{\unicode{x3bb} }^-:=\mathrm {int}(C_{\unicode{x3bb} }^-)$ is the connected component of $\mathscr {I}\setminus \Lambda _{\unicode{x3bb} }$ bounded by $\Gamma _{\phi ^-}$.

Figure 9

Figure 10Controlling the shape of $\Lambda _{\unicode{x3bb} _{\epsilon _n}}^-$.