The negative energy N-body problem has finite diameter

被引:0
|
作者
Montgomery, Richard [1 ]
机构
[1] Univ Calif Santa Cruz, Math Dept, Santa Cruz, CA 95064 USA
来源
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY | 2025年 / 137卷 / 02期
关键词
D O I
10.1007/s10569-025-10243-5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Jacobi-Maupertuis metric lets us reformulate the classical N-body problem at fixed energy E as a geodesic flow problem on a space whose metric depends parametrically on E. We only consider the case E < 0 in which case there is a non-empty Hill boundary along which the metric degenerates. Our main result is the resulting metric space has finite diameter. As a corollary the space admits no metric rays, answering a question of Burgos (Proc Amer Math Soc 150: 1729-1733, 2022). This main result is an immediate corollary of a theorem asserting that all points of the space are a fixed bounded distance from the Hill boundary. Our proof of this last theorem relies ultimately on a game of escape from the boundary of a polyhedral convex cone in a Euclidean space into the interior of said cone. Motivation for our work comes from that of Maderna (Ann Math 192: 499-550, 2020) and from the desire to right a wrong promulgated in Montgomery (Regul Chaot Dyn 28: 374-394, 2023).
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页数:15
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