2019
DOI: 10.1090/tran/7589
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Periodic solutions and regularization of a Kepler problem with time-dependent perturbation

Abstract: We consider a Kepler problem in dimension two or three, with a timedependent T -periodic perturbation. We prove that for any prescribed positive integer N , there exist at least N periodic solutions (with period T ) as long as the perturbation is small enough. Here the solutions are understood in a general sense as they can have collisions. The concept of generalized solutions is defined intrinsically and it coincides with the notion obtained in Celestial Mechanics via the theory of regularization of collision… Show more

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Cited by 19 publications
(46 citation statements)
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“…Recently, a different point of view has been proposed in [12], where a suitable definition of generalized solution to (1) was given. We recall it below for the reader's convenience.…”
Section: Introduction and Statement Of The Main Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Recently, a different point of view has been proposed in [12], where a suitable definition of generalized solution to (1) was given. We recall it below for the reader's convenience.…”
Section: Introduction and Statement Of The Main Resultsmentioning
confidence: 99%
“…However, while in these papers a generalized solution is just meant as an H 1 -function attaining the value x = 0 on a zero-measure set (and solving the equation on the complementary set), Definition 1.1 requires a precise behavior at the collisions instants: that is, both the collision direction x(t) |x(t)| and the collision energy 1 2 |ẋ(t)| 2 − 1 |x(t)| are continuous functions. As shown in [12], this is a very natural definition of solution for equation (1), since it corresponds to the notion of solution provided by the well known Levi-Civita regularization for the planar Kepler problem (see [34] for some basic references about the theory of regularization in Celestial Mechanics and [24] for an application of regularization techniques to a Kepler problem with linear drag).…”
Section: Introduction and Statement Of The Main Resultsmentioning
confidence: 99%
“…For the purposes of this work, we need to take into account different definitions of solutions, allowing for collisions (cf. also [14,16]). Definition 1.3.…”
Section: Definementioning
confidence: 88%
“…From the energy equation in (16), the boundary of the Hill's region for this problem is the closed curve parametrized by polar coordinates in this way…”
Section: Homothetic Solutions For the Anisotropic Kepler Problemmentioning
confidence: 99%
“…We hope that the extended LLC variables can be useful in the studies of periodically perturbed motion, where radial orbits are of interest, forming the collision manifold (e.g. Boscaggin et al 2017). In particular, this formulation may be beneficial for planar, elliptic restricted three body problem and its special cases, like the Hill problem.…”
Section: Discussionmentioning
confidence: 99%