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Circular orbits of a non-radial central-force trajectory: the critical-point condition and the squared frequency of the linearised radial equation

Statement

Let μ>0, let J0⊆(0,∞) be an open interval, let U:J0→R be of class C2, let I be an interval with at least two points, and let r:I→R3 be a central-force trajectory for (μ,U) with constant nonzero angular momentum j=Je3, J>0, and polar data (ρ,θ) as in Polar reduction of a non-radial central-force trajectory: ρ2θ′=J/μ, the effective-potential equation and energy conservation, so that ρ2θ′=J/μ and μρ′′=−(UJeff)′(ρ) on I. Fix r0∈J0. Then:

  1. (Necessity.) If ρ≡r0 is constant on I, then (UJeff)′(r0)=0 and θ′≡J/(μr02) is constant; the trajectory is the uniform rotation r(t)=r0(cos⁡θ(t) e1+sin⁡θ(t) e2).
  2. (Existence.) Conversely, if (UJeff)′(r0)=0, then for every θ0∈R the curve r∘(t):=r0(cos⁡(θ0+ωt) e1+sin⁡(θ0+ωt) e2),ω:=Jμr02, is a central-force trajectory for (μ,U) defined on R, with angular momentum j=Je3 and constant energy E=12μr02ω2+U(r0)=UJeff(r0).
  3. (Linearised radial equation.) Let ρ be a solution of the reduced equation μρ′′=−(UJeff)′(ρ) on I with (UJeff)′(r0)=0, and put δ:=ρ−r0. Then μδ′′=−(UJeff)′′(r0) δ+g(δ),g(x):=(UJeff)′′(r0)x−(UJeff)′(r0+x), where g(x)/x→0 as x→0; if moreover (UJeff)′′(r0)>0, then the associated linearised equation μδ′′=−(UJeff)′′(r0)δ has exactly the solutions δ(t)=Acos⁡(ωlin(t−t0))+Bsin⁡(ωlin(t−t0)) with A,B∈R and ωlin:=(UJeff)′′(r0)/μ>0, for any t0∈I. This is a statement about the quadratic radial approximation; no nonlinear stability of the circular orbit is asserted.

Facts & Assumptions

Given: The central-force data with constant nonzero angular momentum j=Je3 and polar data (ρ,θ) from Polar reduction of a non-radial central-force trajectory: ρ2θ′=J/μ, the effective-potential equation and energy conservation, a radius r0∈J0, and the functions n(θ):=cos⁡θ e1+sin⁡θ e2, n⊥(θ):=−sin⁡θ e1+cos⁡θ e2.

[L1]

Polar reduction: r=ρ n(θ) with ρ=∣r∣, ρ2θ′=J/μ, μρ′′=−(UJeff)′(ρ), and the energy is constant (Polar reduction of a non-radial central-force trajectory: ρ2θ′=J/μ, the effective-potential equation and energy conservation).

[L3]

sin⁡2+cos⁡2=1; and for the linearised equation: the solutions of v′′+ω2v=0 on an interval with ω>0 are exactly Acos⁡(ω(t−t0))+Bsin⁡(ω(t−t0)) (Parity and the Pythagorean identity for sine and cosine, Solutions of v′′+ω2v=0 are exactly the functions Acos⁡(ω(t−t0))+Bsin⁡(ω(t−t0)), Ck Euclidean maps and diffeomorphisms).

[L4]

The derivative of (UJeff)′ at r0 is (UJeff)′′(r0): for every ε>0 there is η>0 with ∣(UJeff)′(r0+x)−(UJeff)′(r0)−(UJeff)′′(r0)x∣≤ε∣x∣ for ∣x∣<η (The derivative f′(c)=lim⁡x→cf(x)−f(c)x−c of f:A→R at a point c∈A that is a limit point of A, and differentiability on a set, Limit point, isolated point, adherent point, derived set, and dense subset of R, Intervals of R: the nine order-convex forms, nondegeneracy, and length).

Proof

technique · direct
1.1givenL1algebra

Clause 1: if ρ≡r0 then ρ′′=0, so the reduced equation of [L1] gives (UJeff)′(r0)=0; and θ′=J/(μρ2)=J/(μr02) is constant by [L1].

1.2givenL2L3algebraconstruct

Clause 2, the kinematics: for r∘(t)=r0 n(θ0+ωt) with ω=J/(μr02), [L2] gives (r∘)′=r0ω n⊥(θ0+ωt) and (r∘)′′=−r0ω2 n(θ0+ωt); hence j=μ r∘×(r∘)′=μr02ω e3=Je3 and ∥(r∘)′∥22=r02ω2, using [L2] and [L3].

1.3givenL1L4algebra

Clause 3, the remainder: by [L4] applied to (UJeff)′ at r0, for every ε>0 there is η>0 with ∣g(x)∣≤ε∣x∣ for ∣x∣<η, where g(x)=(UJeff)′′(r0)x−(UJeff)′(r0+x) and (UJeff)′(r0)=0; that is, g(x)/x→0. Substituting ρ=r0+δ into the reduced equation of [L1] and expanding gives μδ′′=−(UJeff)′(r0+δ)=−(UJeff)′′(r0)δ+g(δ).

2.1givenstep 1.2L1algebra

Clause 2, the equation of motion: from step 1.2 and ω2=J2/(μ2r04), μ(r∘)′′=−μr0ω2n=−J2μr03 n, while −(U′(r0)/r0)r∘=−U′(r0) n; the two agree because (UJeff)′(r0)=0 means U′(r0)=J2/(μr03). The energy is 12μr02ω2+U(r0)=J22μr02+U(r0)=UJeff(r0), and it is constant because the equation is satisfied and the trajectory is periodic; more directly it equals the constant right-hand side of clause 4 of [L1] along this motion.

3.1step 1.3L3algebra∎

Clause 3, the linearised solutions: if (UJeff)′′(r0)>0 then ωlin2=(UJeff)′′(r0)/μ>0 and the linearised equation reads δ′′+ωlin2δ=0; by [L3] its solutions on I are exactly the displayed trigonometric functions for any t0∈I.

Depends on

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