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Physics theoremStatement: AI-adaptedProof: AI-adaptedPipeline-generatedverified 2026-10-22 (gpt-6.1-sol)
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Transverse far field with a uniform remainder

Physical scope

Uniform far-field limits and retarded-time Poynting flux for smooth conserved volume sources supported in one fixed spatial ball at every time. The source may have an arbitrary smooth time history; the estimates use only stated derivative suprema on bounded retarded-time intervals. The result asserts a conditional prediction of the selected classical vacuum Maxwell model, not an empirical measurement, point-source field, self-force or radiation-reaction law.

Statement

Assume Countable Choice. Use the SI laboratory chart and source conventions: ρ:R3×R→R has units C m−3 and J:R3×R→R3 has units A m−2. Let a,c,μ0>0, ε0=(μ0c2)−1, and let ρ,J be jointly C∞, vanish for ∣y∣>a, and satisfy ∂tρ+div⁡yJ=0. Let K=[u−,u+]⊂R be a nondegenerate compact interval, u−<u+, and put K♯=[u−−2a/c,u++2a/c]. For j=0,1,2, define

Mρ,j:=sup⁡B‾a×K♯∣∂tjρ∣,MJ,j:=sup⁡B‾a×K♯∣∂tjJ∣.

For n∈S2 and u∈K, define the retarded current moment and its derivative by

I(n,u):=∫BaJ(y,u+n⋅y/c) dy,V(n,u):=∂uI(n,u)=∫BaJt(y,u+n⋅y/c) dy.

Let E,B be the selected retarded fields of the preceding theorem, set S=E×B/μ0, and define

ΓE:=μ0λ3(Ba)4π(4c2Mρ,0+13caMρ,1+a2Mρ,2+3aMJ,1+a2cMJ,2),

ΓB:=μ0λ3(Ba)4π(4MJ,0+13acMJ,1+a2c2MJ,2).

Then for every n∈S2, u∈K and r≥2a, with Elead(n,u,r):=μ04πrn×(n×V(n,u)),

∣E(rn,u+r/c)−Elead(n,u,r)∣≤ΓEr2,∣B(rn,u+r/c)−n×Elead(n,u,r)c∣≤ΓBr2.

Consequently the radiation data of the preceding definition exist uniformly on S2×K and equal

Erad(n,u)=μ04πn×(n×V(n,u)),Brad(n,u)=n×Erad(n,u)c.

For each fixed retarded time u, the outward retarded-time flux has the exact limit

lim⁡r→∞∫S2r2n⋅S(rn,u+r/c) dΩ(n)=μ016π2c∫S2∣n×V(n,u)∣2 dΩ(n).

Facts & Assumptions

Given: Countable Choice; the constants and source hypotheses in the Statement; the retarded potentials of the preceding theorem; and the fixed compact retarded-time interval K with its enlargement K♯.

[A1]

Countable Choice is the measure convention used by the source integrals, divergence theorem and surface measure. (The Axiom of Countable Choice (ACω))

[F1]

The source maps are smooth volume density and current density in the fixed laboratory frame; C∞ means all iterated coordinate derivatives exist and are continuous, and their spatial support is in B‾a at every time. (Charge parameter, frame charge and current densities, volume charge and flux, and the four-current, Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields, Ck Euclidean maps and diffeomorphisms)

[F2]

For these sources the retarded potentials are smooth, satisfy the wave equations and Lorenz gauge, and generate fields satisfying the smooth vacuum Maxwell system. (Retarded Maxwell fields for spatially compact smooth histories)

[F3]

The field and energy-flux definitions are E=−∇φ−∂tA, B=curl⁡A, and S=E×B/μ0; ∇,div⁡,curl⁡ are the spatial coordinate operators at fixed time; the constants obey ε0=(μ0c2)−1. (The electric and magnetic fields as fixed-time spatial vector fields, Vacuum electromagnetic energy density and energy flux (the Poynting vector), The Jacobian matrix of partial derivatives and the gradient in the scalar-valued case, Divergence and curl of a C1 vector field, Framework-local SI units, the vacuum constants and the exact/measured status of their values)

[F4]

For a continuous integrand and its continuous time derivative on a neighborhood of a fixed compact set of finite measure, differentiation may be passed under the integral. (Differentiation under the integral sign over a compact measurable set and over a compact C1 surface)

[F7]
[F8]

The polar surface measure on S2 is the finite surface measure used in the surface-integral definition, and ∫S21 dΩ=4π. (Surface integration on compact C1 hypersurfaces, Zonal and quadratic sphere moments for the polar surface measure on S2 (d))

[F10]

Radiation data, when they exist, are the uniform limits of rE(rn,u+r/c) and rB(rn,u+r/c) on compact retarded-time intervals. (Radiation data at fixed retarded time)

[F11]

A closed bounded subset of Euclidean R3 is compact; the Borel sigma-algebra contains open sets and their complements, and under Countable Choice every Borel subset is Lebesgue measurable, in particular every closed set. For a measure μ and measurable A⊆B, one has μ(A)≤μ(B). (Heine-Borel in Rn: with the Euclidean metric a subset of Rn is compact if and only if it is closed and bounded, and the proof by bisection uses no choice principle; the same holds on the real line (2), Assuming countable choice, every Borel subset of Rn is Lebesgue measurable, Measures are monotone)

Proof

technique · direct; differentiate the retarded potentials, use conservation to remove the longitudinal scalar-potential term, estimate each geometric and time-shift remainder uniformly, and pass the resulting uniform flux limit through the finite sphere integral
1.1givenF5algebraA1

Geometry of the observation point. Fix n∈S2, u∈K, r≥2a, and y∈Ba. Put σ=n⋅y, R=∣rn−y∣, N=(rn−y)/R, v=u+σ/c, and δ=(r−σ−R)/c, so u+r/c−R/c=v+δ. Since r−σ≥r−a≥r/2, the identity R2=(r−σ)2+∣y∣2−σ2 gives ∣R−(r−σ)∣=(∣y∣2−σ2)/(R+r−σ)≤a2/r; hence ∣δ∣≤a2/(rc)≤a/(2c). Also ∣r−R∣≤∣σ∣+a2/r≤3a/2, so R≥r/2, ∣N−n∣≤∣(r−R)n−y∣/R≤5a/r, ∣R−1−r−1∣=∣r−R∣/(rR)≤3a/r2, and ∣N/R−n/r∣≤∣N−n∣/R+∣R−1−r−1∣≤13a/r2. Thus all retarded source arguments and the intervals between them lie in K♯.

1.2F2F3F4F5F7F11algebraA1

Retarded-field integrals. Put Ca:=B‾a={y:∣y∣≤a}. If ∣z∣>a, the ball of radius (∣z∣−a)/2 around z is disjoint from Ca: the triangle inequality gives ∣y∣≥∣z∣−∣y−z∣>a on that ball. Thus Ca is closed. Also Ca⊂B2a since a>0, so it is bounded and hence compact by [F11]. A closed set is Borel, because its complement is open and the Borel sigma-algebra is closed under complements; under [A1], [F11] therefore makes Ca Lebesgue measurable. The open ball B2a is measurable and has finite measure by [F7]. Applying measure monotonicity [F11] to Ca⊂B2a gives λ3(Ca)≤λ3(B2a)<∞. These are exactly the compactness, measurability and finite-measure hypotheses needed for the set form of [F4]. Since ρ,J are jointly smooth and vanish for ∣y∣>a, their values and their time derivatives vanish on ∂Ba; hence the potential integrals and the integrals obtained by one x- or t-derivative have the same values over Ba and B‾a. Fix an observation event with ∣x∣>a and a product neighborhood with compact closure in the exterior region ∣x∣>a. For each observation coordinate xi and t, hold the other coordinates fixed and apply the set form of [F4] on B‾a with that coordinate as parameter. The retarded integrands and their parameter derivatives are continuous on a neighborhood of B‾a times the chosen parameter interval, since R=∣x−y∣>0 there. Apply this argument to ρ and separately to each component of J, for each spatial-coordinate and time derivative needed in ∇φ, ∂tA and curl⁡A. The chain rule and algebra of derivatives give ∇xR=N, ∇x(t−R/c)=−N/c, and ∇x(R−1)=−N/R2. Substitution in E=−∇φ−∂tA and B=curl⁡A therefore gives, at x=rn, t=u+r/c, E=μ04π∫Ba(c2NρretR2+cNρt,retR−Jt,retR)dy,B=−μ04π∫BaN×(JretR2+Jt,retcR)dy, where the subscript “ret” means evaluation at v+δ. Here R≥r−a>0 for r≥2a.

1.3givenF1F6F7algebraA1

Continuity identity for the shifted source. Fix n,u and choose R0>a. The C1 vector field y↦J(y,u+n⋅y/c) is zero near ∂BR0. Its divergence is div⁡yJ(y,v)+(n/c)⋅Jt(y,v)=−ρt(y,v)+(n/c)⋅Jt(y,v) by the chain rule and continuity. The divergence theorem gives zero for its integral over BR0, and the integrand is zero outside Ba; therefore ∫Baρt(y,v) dy=(1/c)n⋅∫BaJt(y,v) dy=(1/c)n⋅V(n,u).

2.1givenF1F4F7step 1.2algebraA1

Differentiation of the retarded current moment. Choose a bounded open interval U containing K and a compact interval K0 whose interior contains U. Since J and Jt vanish on ∂Ba by the smooth spatial-support hypothesis, the integral over Ba agrees with that over the compact measurable finite-measure set B‾a established in step 1.2. For fixed n∈S2, the map (y,u)↦J(y,u+n⋅y/c) and its u derivative Jt(y,u+n⋅y/c) are continuous on a neighborhood of B‾a×K0. Apply the set form of [F4] separately to each of the three vector components with integration set B‾a and parameter u. Thus ∂uI(n,u)=∫BaJt(y,u+n⋅y/c) dy for every u∈U, so the definition of V in the Statement is well-defined on a neighborhood of K.

2.2step 1.1step 1.2step 1.3F5F6F7algebraA1

Electric leading field and its remainder. Put Flead:=r−1(cnρt(y,v)−Jt(y,v)) inside the integrand of step 1.2. By step 1.3, its integral is r−1(n(n⋅V)−V)=r−1n×(n×V). For the first term of the exact integrand, c2∣Nρret/R2∣≤4c2Mρ,0/r2. For its second term, split cNρt,retR−cnρt(y,v)r=c(NR−nr)ρt,ret+cnr(ρt,ret−ρt(y,v)); the first summand is bounded by 13caMρ,1/r2, while the scalar mean value theorem and step 1.1 bound the second by a2Mρ,2/r2. For the third term, set Δ:=Jt,ret−Jt(y,v). If Δ≠0, put e=Δ/∣Δ∣ and apply the scalar mean value theorem to s↦e⋅Jt(y,s) between v and v+δ; Cauchy–Schwarz then gives ∣Δ∣=∣e⋅Δ∣≤MJ,2∣δ∣. The same bound is trivial for Δ=0. Hence ∣Jt,retR−Jt(y,v)r∣≤∣1R−1r∣MJ,1+1rMJ,2∣δ∣≤3aMJ,1+a2MJ,2/cr2. Integrating these bounds with [F7] and multiplying by μ0/(4π) proves the stated ΓE/r2 estimate.

3.1step 1.1step 1.2step 2.2F5F6F7algebraA1

Magnetic leading field and its remainder. By n×(n×V)=n(n⋅V)−V, one has n×Elead/c=−μ0(4πcr)−1n×V, which is the leading part of the magnetic integral in step 1.2. The Jret/R2 term has norm at most 4MJ,0/r2. For the Jt term, split its coefficient as N/(cR)−n/(cr) plus the time shift n/(cr). The geometric coefficient is bounded by 13a/(cr2). For the time shift, the vector mean value argument of step 2.2 gives ∣Jt,ret−Jt(y,v)∣≤MJ,2∣δ∣, so its contribution is at most a2MJ,2/(c2r2). The cross product with a unit vector does not increase norm by [F5], so [F7] gives the stated ΓB/r2 estimate.

4.1step 2.2step 3.1F5F10algebraA1

Radiation-data limits. Multiplying the electric estimate of step 2.2 by r gives a uniform error at most ΓE/r on S2×K, which tends to zero; thus the uniform limit in [F10] is Erad=μ0n×(n×V)/(4π). Multiplying the magnetic estimate of step 3.1 by r likewise gives the uniform limit Brad=n×Erad/c. Since n⋅(n×(n×V))=0, the leading electric field is transverse.

5.1step 2.2step 3.1step 4.1F5F7F8F9algebraA1∎

Retarded-time flux. The map (n,u)↦V(n,u) is continuous on S2×K: its integrand is continuous on the compact product B‾a×S2×K♯, hence uniformly continuous by [F9], and the integral difference is bounded by λ3(Ba) times the uniform integrand difference, using linearity and the integral triangle inequality [F7]. It is also bounded there by λ3(Ba)MJ,1. The field estimates of steps 2.2 and 3.1 yield E=Erad/r+e and B=Brad/r+b, where ∣e∣≤ΓE/r2 and ∣b∣≤ΓB/r2 uniformly on S2×K. Put CE:=μ0λ3(Ba)MJ,1/(4π) and CB:=CE/c; then ∣Erad∣≤CE and ∣Brad∣≤CB. Bilinearity and the cross-product norm bound [F5] give ∣r2n⋅S(rn,u+r/c)−1μ0n⋅(Erad×Brad)∣≤CEΓB+CBΓEμ0r+ΓEΓBμ0r2, which tends to zero uniformly for r≥2a. Bilinearity of the cross product gives r2n⋅S(rn,u+r/c)=1μ0n⋅(Erad×Brad)+R(n,u,r)=∣Erad∣2μ0c+R(n,u,r), uniformly, where ∣R(n,u,r)∣ is bounded by the preceding display. Since Brad=n×Erad/c and n⋅Erad=0, the determinant formula for the cross product gives n⋅(Erad×(n×Erad))=det⁡[Erad,n×Erad,n]=det⁡[n,Erad,n×Erad]=∣n×Erad∣2=∣Erad∣2, where the middle equality is a cyclic permutation and the last follows from [F5]. The sphere has finite area 4π by [F8], so integrating the explicit uniform remainder makes it tend to zero. Finally ∣Erad∣2=μ02∣n×V∣2/(16π2) by [F5], which gives the asserted flux limit at fixed retarded time.

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