Abstract

We consider the time-dependent dynamical system q¨a=−Γbcaq˙bq˙c−ω(t)Qa(q) where ω(t) is a non-zero arbitrary function and the connection coefficients Γbca are computed from the kinetic metric (kinetic energy) of the system. In order to determine the quadratic first integrals (QFIs) I we assume that I=Kabq˙aq˙b+Kaq˙a+K where the unknown coefficients Kab,Ka,K are tensors depending on t,qa and impose the condition dIdt=0. This condition leads to a system of partial differential equations (PDEs) involving the quantities Kab,Ka,K,ω(t) and Qa(q). From these PDEs, it follows that Kab is a Killing tensor (KT) of the kinetic metric. We use the KT Kab in two ways: a. We assume a general polynomial form in t both for Kab and Ka; b. We express Kab in a basis of the KTs of order 2 of the kinetic metric assuming the coefficients to be functions of t. In both cases, this leads to a new system of PDEs whose solution requires that we specify either ω(t) or Qa(q). We consider first that ω(t) is a general polynomial in t and find that in this case the dynamical system admits two independent QFIs which we collect in a Theorem. Next, we specify the quantities Qa(q) to be the generalized time-dependent Kepler potential V=−ω(t)rν and determine the functions ω(t) for which QFIs are admitted. We extend the discussion to the non-linear differential equation x¨=−ω(t)xμ+ϕ(t)x˙(μ≠−1) and compute the relation between the coefficients ω(t),ϕ(t) so that QFIs are admitted. We apply the results to determine the QFIs of the generalized Lane–Emden equation.

Highlights

  • The equations of motion of a dynamical system define in the configuration space a Riemannian structure with the metric of the kinetic energy

  • On the other hand a metric is fixed by its symmetries, that is, the linear collineations: Killing vectors (KVs), homothetic vectors (HVs), conformal Killing vectors (CKVs), affine collineations (ACs), projective collineations (PCs); the quadratic collineations: second order Killing tensors (KTs)

  • The relation of the Lie/Noether symmetries with the symmetries of the kinetic metric has been considered mostly in the case of point symmetries for autonomous conservative dynamical systems moving in a Riemannian space

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Summary

Introduction

The equations of motion of a dynamical system define in the configuration space a Riemannian structure with the metric of the kinetic energy (kinetic metric). In addition to the autonomous conservative systems this method has been applied to the time-dependent potentials W (t, q) = ω (t)V (q), that is, for equations of the form a qb qc − ω ( t )V ,a ( q ) (see, e.g., [6,7,8,9,10,11,12]) In this case it has been shown that the Lie qa = −Γbc point symmetries, the Noether point symmetries and the associated FIs are computed in terms of the collineations of the kinetic metric plus a set of constraint conditions involving the time-dependent potential and the collineation vectors.

The System of Equations
The Polynomial Method for Computing the QFIs
Special Cases of the QFI In
The QFI I1
The Basis Method for Computing QFIs
The Geometric Quantities of E3
The Time-Dependent Newtonian Generalized Kepler Potential
10. The General Case
11. The Time-Dependent Kepler Potential
12. The 3d Time-Dependent Oscillator
12.1. The Lewis Invariant
13. A Special Class of Time-Dependent Oscillators
14. Collection of Results
15. Integrating the Equations
16. A Class of 1d Non-Linear Time-Dependent Equations
16.1. The Generalized Lane–Emden Equation
17. Conclusions
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