2020
DOI: 10.1007/s10569-019-9946-9
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Numerical integration in Celestial Mechanics: a case for contact geometry

Abstract: Several dynamical systems of interest in celestial mechanics can be written in the formqFor instance, the modified Kepler problem, the spin-orbit model and the Lane-Emden equation all belong to this class. In this work we start an investigation of these models from the point of view of contact geometry. In particular we focus on the (contact) Hamiltonisation of these models and on the construction of the corresponding geometric integrators.

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Cited by 24 publications
(54 citation statements)
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“…For s = 0 and setting the appropriate initial condition p 0 = − f (q 0 ) − g(q 0 )/s 0 , p(t) derived from (18) turns out to be the slope of the tangent ds dq to the orbit of the system at each point (q(t), s(t)) of its evolution. This stems from the fact that (16)- (18) are the characteristic equations of the Hamilton-Jacobi equation for (15). Details of this derivation are in preparation by [28].…”
Section: A Contact Hamiltonian Formulation Of Liénard Systemsmentioning
confidence: 99%
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“…For s = 0 and setting the appropriate initial condition p 0 = − f (q 0 ) − g(q 0 )/s 0 , p(t) derived from (18) turns out to be the slope of the tangent ds dq to the orbit of the system at each point (q(t), s(t)) of its evolution. This stems from the fact that (16)- (18) are the characteristic equations of the Hamilton-Jacobi equation for (15). Details of this derivation are in preparation by [28].…”
Section: A Contact Hamiltonian Formulation Of Liénard Systemsmentioning
confidence: 99%
“…Contact splitting integrators are a class of geometric integrators recently introduced in the context of celestial mechanics [15]. They are the contact analogues of the well-known symplectic splitting integrators.…”
Section: Contact Splitting Integratorsmentioning
confidence: 99%
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