A study of braids arising from simple choreographies of the planar Newtonian N-body problem
Yuika Kajihara, Eiko Kin, Mitsuru Shibayama
TL;DR
This work connects celestial mechanics and low-dimensional topology by studying braids generated by periodic simple choreographies in the planar Newtonian $N$-body problem with equal masses. Using braid groups, mapping class groups, and the Nielsen–Thurston classification, the authors show that for each $N\,\ge\,3$ and every $m{m{m{m{m{}}}}}\in \Omega_N$, there exists a simple choreography whose primitive braid type is $\alpha_{-\bm{m{\omega}}}=\sigma_1^{-\omega_1}\cdots\sigma_{N-1}^{-\omega_{N-1}}$ and whose full braid type is $(\alpha_{-\bm{\omega}})^N$, with pseudo-Anosov type except when $\bm{\omega}$ is all ones or all minus ones. The paper also characterizes the $m{\omega}$ that maximize or minimize the associated stretch factor, yielding concrete extremal braids such as the figure-eight ($N=3$, $\bm{\omega}=(1,-1)$) and the super-eight ($N=4$, $\bm{\omega}=(1,-1,1)$). The results rely on a detailed treatment of braids associated with compositions of integers and on recursive polynomial formulas for stretch factors, enabling explicit computation of $\lambda$ via Perron–Frobenius theory. Overall, the work provides a topological lens on the complexity of choreographies and highlights new links between dynamical celestial mechanics and mapping-class-group dynamics.
Abstract
We study periodic solutions of the planar Newtonian $N$-body problem with equal masses. Each periodic solution traces out a braid with $N$ strands in 3-dimensional space. When the braid is of pseudo-Anosov type, it has an associated stretch factor greater than 1, which reflects the complexity of the corresponding periodic solution. For each $N \ge 3$, Guowei Yu established the existence of a family of simple choreographies to the planar Newtonian $N$-body problem. We prove that braids arising from Yu's periodic solutions are of pseudo-Anosov types, except in the special case where all particles move along a circle. We also identify the simple choreographies whose braid types have the largest and smallest stretch factors, respectively.
