SearcharxivSearch

arXiv subjects

Caleb C. Moxley

Publications and source records attributed to Caleb C. Moxley.

2 recordsLinked to original sources

Homotopical Complexity of a 3D Billiard Flow

In this paper we study the homotopical rotation vectors and the homotopical rotation sets for the billiard flow on the unit flat torus with three, mutually intersecting and mutually orthogonal cylindrical scatterers removed from it. The natural habitat for these objects is the infinite cone erected upon the Cantor set $\text{Ends}(\textbf{F}_3)$ of all "ends" of the hyperbolic group $\textbf{F}_3=π_1(\mathbf{Q})$. An element of $\text{Ends}(\textbf{F}_3)$ describes the direction in (the Cayley graph of) the group $\textbf{F}_3$ in which the considered trajectory escapes to infinity, whereas the height function $s$ ($s\ge 0$) of the cone gives us the average speed at which this escape takes place. The main results of this paper claim that the orbits can only escape to infinity at a speed not exceeding $\sqrt{3}$, and in any direction $e\in\text{Ends}(\mathbf{F}_3)$ the escape is feasible with any prescribed speed $s$, $0\leq s\leq 1/3$. This means that the radial upper and lower bounds for the rotation set $R$ are actually pretty close to each other. Furthermore, we prove the convexity of the set $AR$ of constructible rotation vectors, and that the set of rotation vectors of periodic orbits is dense in $AR$. We also provide effective lower and upper bounds for the topological entropy of the studied billiard flow.

math.DS

Homotopical Complexity of a Billiard Flow on the 3D Flat Torus with Two Cylindrical Obstacles

We study the homotopical rotation vectors and the homotopical rotation sets for the billiard flow on the unit flat torus with two, disjoint and orthogonal cylindrical scatterers removed from it. The natural habitat for these objects is the infinite cone erected upon the Cantor set $\text{Ends}(G)$ of all "ends" of the hyperbolic group $G=π_1(\mathbf{Q})$. An element of $\text{Ends}(G)$ describes the direction in (the Cayley graph of) the group $G$ in which the considered trajectory escapes to infinity, whereas the height function $s$ ($s\ge 0$) of the cone gives us the average speed at which this escape takes place. The main results of this paper claim that the orbits can only escape to infinity at a speed not exceeding $\sqrt{3}$, and in any direction $e\in\text{Ends}(π_1(\mathcal{Q}))$ the escape is feasible with any prescribed speed $s$, $0\leq s\leq\dfrac{1}{\sqrt{6}+2\sqrt{3}}$. This means that the radial upper and lower bounds for the rotation set $R$ are actually pretty close to each other. Furthermore, we prove the convexity of the set $AR$ of constructible rotation vectors, and that the set of rotation vectors of periodic orbits is dense in $AR$. We also provide effective lower and upper bounds for the topological entropy of the studied billiard flow.

math.DS