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Reduction of the central problem to the effective one-dimensional potential: μρ′′=−(UJeff)′(ρ), the energy identity, and the converse reconstruction of the planar trajectory from the radial data

Physical scope

The one-dimensional reduction of the non-radial central problem in the adopted model class for angular-momentum magnitude J>0: the radial coordinate takes values in the declared open radial interval J_0 and obeys the effective-potential equation with the centrifugal term, its energy is the constant first integral of that one-dimensional problem, and conversely every C^2 radial solution valued in J_0 together with the angular quadrature reconstructs a planar central-force trajectory with the prescribed angular momentum, hence a motion of the two-label model together with a uniform centre-of-mass motion. The result is a conditional deduction; it asserts no observation, no measured value, and no global existence for either side.

Statement

Adopt the central-force model of Adopted central-force model class: static central pair potentials, the reduced one-label problem, the fixed-centre idealization, reading conventions and exclusions clause (i) with masses m1,m2>0, reduced mass μ=m1m2/M, M=m1+m2, static central pair potential u∈C2(J0), and let x:I→Q be a motion on a time interval I with relative coordinate r, attached angular momentum j=μ r×r′, and suppose j=Je3 with J>0 for an oriented orthonormal triad (e1,e2,e3) (Two-body reduction of a static central pair-potential model: the relative coordinate is a central-force trajectory for the reduced mass, the centre of mass moves uniformly, and the reconstruction is a bijection, Oriented orthonormal triads in R3: existence over any unit vector, and the orthonormal expansion with no fourth orthogonal direction). Let (ρ,θ) be polar data for r in that triad (Polar reduction of a non-radial central-force trajectory: ρ2θ′=J/μ, the effective-potential equation and energy conservation) and put UJeff(ρ):=u(ρ)+J22μρ2(ρ∈J0), the effective potential of angular momentum J, of class C2 on J0 (Central-force trajectories: the central-force equation, angular momentum, energy and the effective potential). Then:

  1. (Radial problem.) On I: ρ2θ′=J/μ>0, the effective equation μ ρ′′=−(UJeff)′(ρ) holds, and the relative energy E=12μ∥r′∥22+u(∣r∣) satisfies E=12μ(ρ′)2+UJeff(ρ) and is constant on I; equivalently, the radial coordinate solves the one-dimensional mechanical initial-value problem of mass μ on the declared radial interval J0 (an interval contained in ρ>0) in the potential UJeff.
  2. (Reconstruction.) Conversely, let ρ∘:I→R be a C2 function with ρ∘(t)∈J0 and μ(ρ∘)′′=−(UJeff)′(ρ∘) on I, and let θ∘:I→R be a C2 function with (θ∘)′=J/(μ(ρ∘)2) on I (for instance θ∘(t)=θ0+Jμ∫t0tρ∘(s)−2ds). Then r∘(t):=ρ∘(t)(cos⁡θ∘(t) e1+sin⁡θ∘(t) e2)(t∈I) is a central-force trajectory for (μ,u) with j∘=μ r∘×(r∘)′=Je3 and constant energy 12μ((ρ∘)′)2+UJeff(ρ∘).
  3. (Mutual inversion and model reconstruction.) The assignments of clauses 1 and 2 are mutually inverse: reconstructing from the polar data of r returns r, and the polar data of the reconstructed r∘ agree with (ρ∘,θ∘) up to an additive constant of the angular coordinate. Consequently, together with an affine centre-of-mass curve X∘ with (X∘)′′=0 on I, the datum (ρ∘,θ∘) reconstructs a motion of the two-label model with angular momentum Je3, centre of mass X∘ and relative coordinate r∘ (Two-body reduction of a static central pair-potential model: the relative coordinate is a central-force trajectory for the reduced mass, the centre of mass moves uniformly, and the reconstruction is a bijection clause 4).

Facts & Assumptions

Given: The central-force model of class (i), the motion x:I→Q on the time interval I, its relative coordinate r, the nonzero constant angular momentum j=Je3, the oriented orthonormal triad, and the polar data (ρ,θ); for clause 2, the functions ρ∘,θ∘ and the curve r∘ of the statement.

[L1]

Reduction and attached objects (Two-body reduction of a static central pair-potential model: the relative coordinate is a central-force trajectory for the reduced mass, the centre of mass moves uniformly, and the reconstruction is a bijection clauses 3-4, Central-force trajectories: the central-force equation, angular momentum, energy and the effective potential, Adopted central-force model class: static central pair potentials, the reduced one-label problem, the fixed-centre idealization, reading conventions and exclusions clause (ii)): r is a central-force trajectory for (μ,u) on I with j=μr×r′=Je3 constant and energy E=12μ∥r′∥22+u(∣r∣); the reduction reconstruction with an affine X∘ is clause 4 of the cited theorem.

[L2]

Polar reduction (Polar reduction of a non-radial central-force trajectory: ρ2θ′=J/μ, the effective-potential equation and energy conservation, Oriented orthonormal triads in R3: existence over any unit vector, and the orthonormal expansion with no fourth orthogonal direction): for a central-force trajectory with constant j=Je3, J>0, there are twice differentiable ρ:I→(0,∞), θ:I→R with r=ρ(cos⁡θ e1+sin⁡θ e2); for every such pair, ρ2θ′=J/μ, μρ′′=−(UJeff)′(ρ) with UJeff=u+J2/(2μρ2), and E=12μ(ρ′)2+UJeff(ρ) is constant; the triad identity x=∑i⟨x,ei⟩ei holds.

[L3]

Differentiation rules (Differentiation of sums, scalar multiples, inner products, cross products and squared norms of differentiable curves in R3, The derivatives of sine and cosine are cosine and minus sine, The chain rule, in one line from Carathéodory: if g is differentiable at c and f is differentiable at g(c), then f∘g is differentiable at c with (f∘g)′(c)=f′(g(c)) g′(c), Sums, scalar multiples, products and quotients: (f+g)′(c)=f′(c)+g′(c), (αf)′(c)=αf′(c), (fg)′(c)=f′(c)g(c)+f(c)g′(c), and (f/g)′(c)=(f′(c)g(c)−f(c)g′(c))/g(c)2 when g(c)≠0, Parity and the Pythagorean identity for sine and cosine, Ck Euclidean maps and diffeomorphisms, The derivative and the Riemann integral of a vector-valued function: an intrinsic derivative and a componentwise integral, Every continuous function on an interval has a primitive; two primitives differ by a constant; and ∫abf=G(b)−G(a) for any primitive G): sums, differences, products, quotients with nonvanishing denominators and compositions of Ck curves are Ck with the usual derivative rules; (cos⁡)′=−sin⁡, (sin⁡)′=cos⁡, and sin⁡2+cos⁡2=1; for a continuous f:I→R on an interval with at least two points, the integral from a fixed base point defines a C1 primitive (clause 1 of Every continuous function on an interval has a primitive; two primitives differ by a constant; and ∫abf=G(b)−G(a) for any primitive G), and any two primitives of f on I differ by a constant (clause 2). The first clause supplies the angular quadrature, and the second supplies angular-phase uniqueness.

[L4]

Cross product (The cross product in R3, The cross product is bilinear, alternating, and orthogonal to both factors, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn): the cross product is bilinear and alternating, e1×e2=e3 for a positively oriented orthonormal triad, and orthonormality gives ∣r∘∣2=(ρ∘)2 for the curve of clause 2.

[L5]

The intervals: I has nonempty interior, J0⊆(0,∞) is open, and UJeff is C2 on J0 as a sum of u and a quotient with nonvanishing denominator (Intervals of R: the nine order-convex forms, nondegeneracy, and length, Central-force trajectories: the central-force equation, angular momentum, energy and the effective potential, [L3]).

Proof

technique · direct
1.1givenL1L2L5algebra

Clause 1: by [L1], r is a central-force trajectory for (μ,u) with constant j=Je3, so the hypotheses of [L2] hold and its conclusions give ρ2θ′=J/μ, μρ′′=−(UJeff)′(ρ), and E=12μ(ρ′)2+UJeff(ρ) constant on I; [L5] makes UJeff a C2 function on J0, so the displayed equation is the one-dimensional mechanical equation for the coordinate ρ on the declared radial interval J0⊆(0,∞).

1.2givenL3L4algebra

Clause 2, construction and equations: define n:=cos⁡θ∘e1+sin⁡θ∘e2 and n⊥:=−sin⁡θ∘e1+cos⁡θ∘e2, and r∘:=ρ∘n. By [L3], r∘ is C2 with n′=(θ∘)′n⊥, n⊥′=−(θ∘)′n and (r∘)′=(ρ∘)′n+ρ∘(θ∘)′n⊥, hence (r∘)′′=((ρ∘)′′−ρ∘((θ∘)′)2)n+(2(ρ∘)′(θ∘)′+ρ∘(θ∘)′′)n⊥. With (θ∘)′=J/(μ(ρ∘)2) the second coefficient is 1ρ∘((ρ∘)2(θ∘)′)′=0, and the radial equation gives μ((ρ∘)′′−ρ∘((θ∘)′)2)=μ(ρ∘)′′−J2μ(ρ∘)3=−u′(ρ∘), since −(UJeff)′(ρ∘)=−u′(ρ∘)+J2μ(ρ∘)3. Therefore μ(r∘)′′=−u′(ρ∘)n=−u′(∣r∘∣)∣r∘∣r∘, the last equality by ∣r∘∣=ρ∘ and r∘=ρ∘n from [L4].

2.1step 1.2L2L3L4algebra

Clause 2, consequences: ∣r∘∣=ρ∘ takes values in J0 and ρ∘ is positive, so step 1.2 exhibits r∘ as a central-force trajectory for (μ,u) in the sense of the definition, with r∘×(r∘)′=(ρ∘)2(θ∘)′ (n×n⊥)=(ρ∘)2(θ∘)′e3=Jμe3 by [L4] and n×n⊥=e3; hence j∘=μ r∘×(r∘)′=Je3. Its energy is 12μ∥(r∘)′∥22+u(ρ∘)=12μ((ρ∘)′)2+J22μ(ρ∘)2+u(ρ∘)=12μ((ρ∘)′)2+UJeff(ρ∘) by [L3] and orthonormality. Since step 1.2 establishes that r∘ is a central-force trajectory with nonzero constant j∘=Je3, the energy conservation conclusion of [L2] applies and shows that this displayed energy is constant on I.

3.1step 1.1step 1.2step 2.1L1L2L3algebra∎

Clause 3: if (ρ,θ) are the polar data of a trajectory r as in clause 1, the construction of clause 2 applied to (ρ,θ) returns ρ(cos⁡θ e1+sin⁡θ e2)=r. Conversely, if r∘ is constructed from (ρ∘,θ∘) and (ρ~,θ~) is any polar data of r∘ supplied by [L2], then ρ~=∣r∘∣=ρ∘ and ρ~2θ~′=J/μ=ρ~2(θ∘)′, so θ~ and θ∘ are primitives of the same continuous function f(t)=J/(μ(ρ∘(t))2) on the nondegenerate interval I. By [L3], clause 2 of Every continuous function on an interval has a primitive; two primitives differ by a constant; and ∫abf=G(b)−G(a) for any primitive G, the two angle functions differ by a constant. Combining with [L1] clause 4, the pair (ρ∘,θ∘) together with any affine X∘ with (X∘)′′=0 on I reconstructs a motion of the two-label model with relative coordinate r∘ and centre of mass X∘, and by step 2.1 that motion has angular momentum Je3. This completes the proof.

Remarks

  • The barrier is not a force. UJeff=u+J2/(2μρ2) collects the potential and the centrifugal term of the angular motion; the term is a bookkeeping device of the reduced one-dimensional problem, and no new interaction is introduced.

  • Energy is the first integral used later. The page's later orbit statements consume the radial equation and the constancy of E from clause 1; clause 2 is what makes the reduction lossless up to the angular phase.

  • No global existence. Neither clause asserts that a solution of the radial equation exists for all times or that it avoids ρ→0; those are separate questions examined by the subsequent items and the scope remark.

Depends on

Dependency tree · 2 levels

Sources