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Finite-time weak/slow charged probe correspondence

Physical scope

Finite-time comparison for a massive charged test probe on a stationary weak metric with the exact C2 remainder bounds and prescribed electric/magnetic scalings of the mathematical supplier, with a smooth closed background two-form and the adopted action on short local-potential curve segments. It requires alpha nonzero, a sufficiently small parameter cutoff fixed by the uniform bounds, uniformly small speed, existing trajectories, common compact convex state containment in K x R3 and finite scaled duration. It imposes neither the inhomogeneous Maxwell equation nor Einstein equations and constructs no fully coupled background family.

Statement

Use the charged-probe action sector of the fixed-background model of Separately adopted fixed-background Maxwell and charged probes and let α=q/m≠0, with constant m>0, constant charge q, length scale L>0, and speed constant c>0. When the Lorentz-force form is obtained from the adopted action, the inherited ACω hypothesis of that exact action-equivalence theorem is assumed; no stronger choice axiom is used. In SI, [α]=C kg−1, [L]=m, and [c]=m s−1; ϵ, X, ϕ, e, and b are dimensionless. Choose a cutoff 0<ϵ∗≤1 sufficiently small in terms of the displayed uniform bounds below, as required by Controlled weak/slow charged test trajectory comparison, and fix 0<ϵ≤ϵ∗. On an open Ω⊆R3, let K⋐Ω be compact and convex, use length coordinates x0=ct, xi=LXi, and suppose the prescribed metric is smooth, stationary and Lorentzian on a neighborhood of Rx0×LK, with ∂0 future timelike. For a smooth dimensionless ϕ and some fixed finite Cg, assume for every spatial multi-index β with ∣β∣≤2 that

∣∂Xβr00(ϵ)∣+max⁡i,j∣∂Xβrij(ϵ)∣≤Cgϵ2,max⁡i∣∂Xβr0i(ϵ)∣≤Cgϵ3/2,

where g00(ϵ)=−(1+2ϵϕ)+r00(ϵ), gij(ϵ)=(1−2ϵϕ)δij+rij(ϵ), and g0i(ϵ)=r0i(ϵ). Prescribe smooth stationary dimensionless fields e,b with values and first derivatives bounded on K, and a smooth real closed two-form F(ϵ) on the same background neighborhood, with dF(ϵ)=0 and SI components F0i(ϵ)=−Ei(ϵ)/c, Fij(ϵ)=ϵijkBk(ϵ) and

αE(ϵ)=ϵc2Le,αB(ϵ)=ϵcLb.

Closure dF(ϵ)=0 ensures local potentials, not a global potential: in each sufficiently small open coordinate ball D about a curve point, use the smooth radial primitive of Radial primitives for closed one- and two-forms as the supplied AD with dAD=F(ϵ)∣D. Adopt fixed-endpoint action stationarity only on sufficiently short finite curve segments contained in such a ball, as in Separately adopted fixed-background Maxwell and charged probes and Stationary charged action and Lorentz force. There is no assumption that the whole trajectory lies in a single potential domain, that F(ϵ) is globally exact, or that the local potentials are stationary. No inhomogeneous Maxwell or Einstein equation is imposed on this prescribed background. The dimensionless comparison trajectory satisfies XN′=WN, WN′=−∇Xϕ(XN)+e(XN)+WN×b(XN) on [0,S∗], where primes denote S derivatives, S∗>0, and S=ϵct/L. Write ∥(X,W)∥1 for the sum of the absolute values of the six components and ∥Df∥1→1 for its induced operator norm, as in Controlled weak/slow charged test trajectory comparison. Let the six-component comparison vector field f have derivative norm at most Lf<∞ on a compact convex state set Q⊆K×R3 containing both scaled trajectories throughout [0,S∗].

Suppose a C2 future-directed proper-time worldline exists through this finite interval, obeys this local action model (equivalently the external Lorentz law on each such segment), has coordinate speed ∣w∣≤Cvϵc, has its scaled state remain in Q, and has the same initial scaled data as the comparison trajectory. Set Xϵ=x/L and Wϵ=w/(ϵc). Then for some finite Cr depending only on the displayed uniform bounds, the exact scaled motion obeys

Xϵ′=Wϵ,Wϵ′=−∇Xϕ(Xϵ)+e(Xϵ)+Wϵ×b(Xϵ)+rϵ(S),∥rϵ(S)∥1≤Crϵ,

and consequently

sup⁡0≤S≤S∗(∥Xϵ−XN∥1+∥Wϵ−WN∥1)≤CrϵS∗eLfS∗.

This is a finite-duration conditional model prediction. It does not construct the trajectories, prove common compact containment, solve Maxwell's equations for the prescribed field, or establish a coupled Einstein–Maxwell family. The magnetic scaling may violate a coupled stress hierarchy unless additional matter scales are supplied.

Facts & Assumptions

Given: The fixed prescribed metric and field model of Separately adopted fixed-background Maxwell and charged probes, the uniform metric and field bounds above, the sufficiently small cutoff required by [F2], α≠0, a proper-time Lorentz-force curve satisfying the speed bound, and both scaled trajectories' existence and containment in the compact convex set Q⊆K×R3 with matched initial data on [0,S∗]. The smooth background two-form is closed, so smooth potentials are supplied by the radial formula on short coordinate-ball segments; no global potential is assumed. When the Lorentz-force form is obtained from the adopted action, assume the exact inherited ACω hypothesis of that action-equivalence result; no stronger choice axiom is used.

[F1]

Separately adopted fixed-background Maxwell and charged probes: the background metric and external Maxwell field are prescribed independently; the massive probe is governed on each finite local-potential segment by the adopted action and, under its exact equivalence theorem hypotheses including its stated ACω assumption, by ∇UU=αF♯(U). This is countable choice only, not arbitrary-index choice. No inhomogeneous Maxwell or Einstein equation for this background is assumed; the closure needed for local potentials is explicit.

[F2]

Controlled weak/slow charged test trajectory comparison: under the exact C2 metric-remainder bounds, field scaling, α≠0, speed bound, derivative bound on a compact convex Q⊆K×R3, and existing scaled trajectories contained in Q with matched initial data stated there, the exact coordinate equation has an O(ϵ2c2/L) acceleration remainder and yields the displayed CrϵS∗eLfS∗ finite-time error bound after ϵ∗ is chosen sufficiently small in terms of its uniform bounds. Its theorem is mathematical and conditional; it does not assert a physical Maxwell/Einstein solution.

[F3]

Radial primitives for closed one- and two-forms: on an open coordinate domain D⊂R4 star-shaped about p, every smooth real closed two-form F has the smooth primitive Ab(x)=∫01t(x−p)aFab(p+t(x−p)) dt, with dA=F. This is a local formula and does not require global exactness.

[F4]

Stationary charged action and Lorentz force: under ACω, on a finite C2 future-timelike proper-time segment contained in a supplied C2 local potential domain with F=dA, stationarity of the adopted fixed-endpoint external charged action is equivalent to m∇UU=qF♯(U). It asserts no global potential or trajectory existence.

[A1]

All uniform bounds, proper-time curve hypotheses, and finite-interval existence and containment in Q⊆K×R3 in the Statement are assumptions. They are not consequences of the test-field postulate.

Proof

1.1givenF1F2F3F4A1algebra

At each interior point of the proper-time curve, choose a sufficiently small coordinate ball D in the open prescribed-background region, centered at p. The form F(ϵ) is smooth and closed there, so the explicit radial formula [F3] supplies a smooth real AD with dAD=F(ϵ)∣D. Continuity of the curve places a sufficiently short finite segment about that point in D. Its fixed-endpoint local action variations have the regularity and supplied-potential hypotheses of [F4]; the adopted stationarity in [F1] and the stated ACω assumption therefore give the Lorentz law at that point. Applying this pointwise proves the force equation along the curve; continuity gives it at its finite interval endpoints. On overlapping potential balls the same equation depends only on dAD=F(ϵ), so no global action or potential gluing is used, and no extra choice principle is introduced. No bound or stationarity assumption on the potentials enters the comparison estimate. The metric expansion, stationary prescribed field, SI components, nonzero α, speed bound, derivative bound on the compact convex state set Q, and existence/containment assumptions in [A1] match the hypotheses of [F2] exactly: because Q⊆K×R3, both scaled positions stay in K, where the uniform metric and field bounds apply; in particular the field is not assumed to satisfy Maxwell or Einstein equations.

2.1F2A1step 1.1∎

Applying the complete conditional mathematical result [F2] to these inputs gives the scaled coordinate equation with ∥rϵ∥1≤Crϵ and, because the initial data match and both scaled curves remain in the compact convex set Q⊆K×R3, the stated finite-time comparison bound. Those conclusions inherit all the existence, containment and prescribed-background qualifications in [A1]; no infinite-duration or coupled-solution claim follows.

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