Abstract:
The Jacobi–Maupertuis metric allows one to reformulate Newton's equations as geodesic equations for a Riemannian metric which degenerates at the Hill boundary. We prove that a JM geodesic which comes sufficiently close to a regular point of the boundary contains pairs of conjugate points close to the boundary. We prove the conjugate locus of any point near enough to the boundary is a hypersurface tangent to the boundary. Our method of proof is to reduce analysis of geodesics near the boundary to that of solutions to Newton's equations in the simplest model case: a constant force. This model case is equivalent to the beginning physics problem of throwing balls upward from a fixed point at fixed speeds and describing the resulting arcs, see Fig. 2.
\Bibitem{Mon14}
\by Richard~Montgomery
\paper Who's Afraid of the Hill Boundary?
\jour SIGMA
\yr 2014
\vol 10
\papernumber 101
\totalpages 11
\mathnet{http://mi.mathnet.ru/sigma966}
\crossref{https://doi.org/10.3842/SIGMA.2014.101}
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This publication is cited in the following 4 articles:
Luca Asselle, Stefano Baranzini, “On the Zoll deformations of the Kepler problem”, Bulletin of London Math Soc, 2025
L. Di Cairano, M. Gori, M. Pettini, “Coherent Riemannian-geometric description of Hamiltonian order and chaos with Jacobi metric”, Chaos, 29:12 (2019), 123134
S. Chanda, G. W. Gibbons, P. Guha, “Jacobi–Maupertuis metric and Kepler equation”, Int. J. Geom. Methods Mod. Phys., 14:7 (2017), 1730002
Cuervo-Reyes E., Movassagh R., “Non-Affine Geometrization Can Lead To Non-Physical Instabilities”, J. Phys. A-Math. Theor., 48:7 (2015), 075101