<p>The Jacobi-Maupertuis metric lets us reformulate the classical N-body problem at fixed energy <i>E</i> as a geodesic flow problem on a space whose metric depends parametrically on <i>E</i>. We only consider the case <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="10569_2025_10243_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="46" /> </InlineMediaObject> <EquationSource Format="TEX">\(E &lt; 0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>E</mi> <mo>&lt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> 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).</p>

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The negative energy N-body problem has finite diameter

  • Richard Montgomery

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 \(E < 0\) 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).