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Retarded fields and radiation

1 · Prerequisites

2 · Summary

Objective. This page develops the retarded solution of the classical vacuum model, the fields and radiation of prescribed compact and point sources, and the honest limits of that radiation model. Everything is conditional on the stated regularity, compactness, subluminality and choice hypotheses; no dynamics (self-force, radiation reaction or mass derivation) is supplied, and no empirical claim is made. The worked examples and the reduced orbit model live on the companion page em-retarded-fields-and-radiation-examples.

Adopted retarded selection. The sourced wave system admits retarded and advanced particular solutions and free additions; the framework adopts the retarded branch with no incoming free field as an extra physical assumption with arrow-of-time content, not as a consequence of the time-reversible equations and not as a theorem or measurement (Adopted retarded solution selection: the physical branch carries no incoming free field). The postulate records the affine freedom explicitly, excludes the advanced branch and independent free fields, and extends the same selection to the separately declared weak point-source equations; existence, regularity and support must be supplied by the theorems below.

Kinematic point geometry. For a prescribed C3 uniformly subluminal worldline the retarded root s(x,t) with t−s=∣x−z(s)∣/c exists and is unique off the worldline, is C3 there, and carries the retarded data r,n,β,κ,β˙ with derivative formulas ∂ts=1/κ and ∇xs=−n/(cκ) (Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline). The definition excludes finite-history and merely pointwise subluminal curves; the companion example exhibits a smooth pointwise subluminal curve with no retarded root at one event, delimiting the uniform bound (A smooth pointwise subluminal curve with no retarded root at an event). The zonal and quadratic moments of the sphere measure used by every angular computation are proved independently as mathematics (Zonal and quadratic sphere moments for the polar surface measure on S2).

Compact smooth sources. For a smooth conserved source of compact spatial support in a compact time interval, the explicit retarded integrals are smooth, satisfy the sourced wave equations and, via the continuity equation, the Lorenz gauge condition; the four smooth Maxwell equations hold, the fields vanish before the source acts, the pair is the zero-data Cauchy solution at every earlier time, and the total charge vanishes (Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source).

Dipole radiation and point fields. The actual leading far fields of the compact branch are controlled by the shifted current moment V(n,u); replacing it by the dipole moment's second derivative p′′(u) has the explicit absolute error D(u). The theorem gives the moment identities, uniform field bounds and retarded-time radiated power with its absolute error (Controlled electric-dipole far field and retarded-time radiated power of a compact smooth source). For a prescribed point charge on a uniformly subluminal worldline the retarded potentials C/(κr) and βφ/c, the exact velocity/acceleration field split, B=n×E/c, the velocity-field bound and the uniform far-zone remainder are established off the worldline; the constructed weak point-source model satisfies the distributional Maxwell identities of the declared singular-source class, while no field value on the worldline and no nonlinear self-interaction is defined (Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder).

Emitted power. At an instantaneous-rest emission event the exact field on the emitted sphere gives the sin⁡2θ angular pattern and the Larmor power q2∣a∣2/(6πε0c3), with the uniform velocity-field remainder and a separately quantified general low-speed power and angular comparison (Instantaneous-rest Larmor power and uniform low-speed comparison for a prescribed point charge). For a general emission event the emitted power per unit emission time is defined by the κ0-weighted far-zone flux and equals q2γ06(∣a∣2−∣β0×a∣2)/(6πε0c3)=q2η(A,A)/(6πε0c3), with the uniform δ-comparison against the rest value (Relativistic emitted power of a prescribed point charge at a general emission event).

Limits of the model. For a stationary nonzero point charge the truncated electrostatic self-energy diverges, products of the singular self-field with the point current are undefined in the declared distributional source model, and the emitted-power statements are prescribed-source computations: no self-force, radiation reaction, runaway, finite-size regularization or electromagnetic mass is supplied here (Self-force, runaways and finite-size regularizations are not supplied by this page). The reduced circular-orbit model on the companion page retains its formal finite-time collapse strictly as a property of its adopted premise (Conditional radius loss of a prescribed slowly orbiting charge in a reduced quasistatic model), and the harmonic dipole computation holds inside the exact dipole law with its explicit finite-radius and flux errors (Harmonic dipole pattern and period-averaged power in the exact dipole law).

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

PostulateStatement: AI-adaptedProof: Not applicableOpen item page →

Adopted retarded solution selection: the physical branch carries no incoming free field

Physical scope

Adopted selection rule for the classical vacuum Maxwell/wave model in the framework's inertial laboratory chart and SI conventions: the physical potential pair is the retarded one with zero incoming free field, both for the smooth compact-source branch and for the separately declared weak point-source equations. Excluded: existence, uniqueness, regularity or decay claims for any source class (consuming theorems must supply them); empirical, statistical or measurement claims; the advanced branch and free fields as physical solutions; products of distributions, self-force, radiation reaction and any apparatus model.

Postulate

Adopt as a physical assumption of this framework the following solution-selection rule for the classical vacuum model on the laboratory region U≅I×Ω of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields, with the constants and SI units of Framework-local SI units, the vacuum constants and the exact/measured status of their values (so c>0, μ0>0, ε0=(μ0c2)−1).

(a) [Formulation] In the potential formulation of Maxwell's equations in potential form: the Lorenz divergence, the decoupled wave equations and residual generators with the conventions of Scalar-vector potential pairs, gauge transformation, Lorenz divergence and the wave expression, for a C2 potential pair in Lorenz gauge the sourced Maxwell system of The microscopic vacuum Maxwell equations: smooth and weak branches is equivalent to the decoupled sourced wave equations Wφ=ρ/ε0, WA=μ0J, where W=c−2∂t2−Δ. The wave expression W is invariant under t↦−t; where explicit retarded or advanced constructions for a prescribed history exist, they give distinguished particular solutions built from the corresponding forward or backward fundamental kernels. Every other solution differs from a chosen particular solution by a source-free addition; retarded and advanced particular solutions also differ by such an addition. This describes the affine free-solution freedom, not a claim that arbitrary histories have exactly two solutions or that either construction always exists.

(b) [Adopted rule] The framework adopts the retarded branch with no free field added: the physical potential pair of the model is the retarded one, that is, the one whose support and propagation lie in the forward light cones of the source and which carries no field arriving from the past independently of the source. For the zero-incoming model the selected sourced solution has no independently prescribed homogeneous addition. If nonzero Cauchy data are instead prescribed, their compatible homogeneous addition is a separate initial-data model; it is not equivalent to setting every free addition to zero. The advanced construction and independent incoming free fields are excluded by the present retarded selection.

(c) [Status and scope] This is an adopted extra temporal condition carrying the model's arrow-of-time content. It is not a theorem, not a consequence of the time-symmetric wave or Maxwell equations (which admit advanced and free solutions as mathematical objects), and not a deduction from experiment; it asserts no existence, uniqueness, regularity, support or decay for any source class, all of which must be supplied separately by theorems of this page. It selects a solution only of the models to which it is applied; it introduces no product of distributions, no source model, no self-force, no radiation reaction, no measured signal and no statistical claim. The retarded compact-source branch to which this selection applies is developed on this page as a conditional theorem, and the point-source branch is developed later on this page; neither existence statement is part of this postulate. For the separately declared point-source branch assume Countable Choice (The Axiom of Countable Choice (ACω)), as in its exact source/field interfaces, and adopt the same no-free-addition retarded selection in the weak equations of Distributional vacuum Maxwell equations for the declared point and stationary-sheet sources, for the locally integrable field and proper point-current types of Distributional Maxwell equations with point and stationary-sheet sources. This extends the selection's model scope explicitly; neither existence nor an arbitrary convolution of noncompact distributions is postulated.

Source notes

The classical treatments cited above display the retarded and advanced Green functions of the wave operator and then identify the choice of the retarded branch as additional structure imposed on the time-reversal-symmetric equations; they support the formulation of clauses (a)-(b) and the honest non-theorem status recorded in clause (c). They are not evidence for the physical correctness of the choice, and this postulate reports no experiment, measurement or statistical inference. The exact interfaces of the wave form, the gauge conventions, the smooth Maxwell system and the separately adopted weak singular-source equations are those of the cited framework items; the weak point-source extension is an explicit physical selection on the already-adopted singular-source equations, not a deduction from the smooth-only potential theorem, and a consuming theorem must construct its actual history integrals and prove weak admissibility.

DefinitionDefinition: AI-adaptedProof: Not applicableOpen item page →

Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline

Physical scope

Kinematic definition of the retarded emission data of a prescribed uniformly subluminal C3 worldline in the framework's laboratory chart: retarded root, distance, direction, speed ratio, emission-time Jacobian and emitted-sphere family off the worldline. Excluded: any field, Maxwell equation, dynamics, force law, self-force, radiation reaction, existence under a merely pointwise subluminal or finite-history curve, and every empirical or measurement claim.

Definition

Let the laboratory region, inertial chart, spatial Euclidean structure and SI units be those of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values, in particular c>0, μ0>0, ε0=(μ0c2)−1. A retarded point-geometry datum consists of a real charge parameter q∈R in coulombs (Charge parameter, frame charge and current densities, volume charge and flux, and the four-current(a)) and a prescribed map z:R→R3 of class C3 (Ck Euclidean maps and diffeomorphisms) together with a constant 0≤v∗<c such that ∣z′(s)∣≤v∗ for every s∈R (The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn); the spacetime curve s↦(z(s),s) is the laboratory reading of a prescribed massive future timelike worldline of the physical model (Worldlines, four-velocity, chart readings and the frame/observer distinction), and v∗ is a declared bound on its coordinate speed, not a measured quantity. Write Γ:={(z(s),s):s∈R} and D:={(x,t)∈R3×R:x≠z(t)} for the open off-worldline observation domain. Then:

(a) [Retarded root] For every observation event (x,t)∈D there is exactly one s=s(x,t)<t with t−s=∣x−z(s)∣/c; the map s:D→R is of class C3, and with the data of (b) below one has ∂ts=1/κ and ∇xs=−n/(cκ) (Global existence, uniqueness and differentiability of the retarded root, whose C3 branch applies because z is C3 and uniformly subluminal).

(b) [Retarded data] For (x,t)∈D define R:=x−z(s(x,t)), r:=∣R∣>0, n:=R/r, β:=z′(s(x,t))/c, κ:=1−n⋅β, β˙:=z′′(s(x,t))/c; then r=c(t−s) and κ∈[1−v∗/c, 1+v∗/c]⊆(0,∞). On D the objects r and n are of class C3, β and κ are of class C2, and β˙ is of class C1 (each is a composition of the C3 root with z or its derivatives).

(c) [Emission-event data and emitted spheres] At an emission event s0∈R and a direction n∈S2 put xr:=z(s0)+rn, tr:=s0+r/c for r>0, and β0:=z′(s0)/c, κ0:=1−n⋅β0. Then (xr,tr)∈D and s(xr,tr)=s0 for every r>0: the sphere {xr} at observation time tr is emitted at the single event s0.

(d) [Branches and scope] Only the all-time uniformly subluminal branch (a)-(c) is defined by this datum. For a curve prescribed on a finite interval J the same formulas define retarded data only at observation events for which the root equation has a solution s∈J; each consumer must assume that cone intersection explicitly. Pointwise subluminality ∣z′(s)∣<c for every finite s does not imply (a): the companion example on the examples page exhibits a smooth curve with ∣z′∣<c pointwise for which the retarded equation has no root at some event, so the uniform bound v∗<c, or an explicit cone-intersection hypothesis, is part of the datum. This definition is kinematic: it fixes the root, the retarded data and the notation, and asserts no field, no dynamics, no force law, no self-force and no empirical content. The identification of these data with the emission data of the physical field is made by the selection postulate Adopted retarded solution selection: the physical branch carries no incoming free field together with the theorems of this page.

Well-definedness notes

Clauses (a)-(b) are exactly the all-time uniformly subluminal C3 branch of Global existence, uniqueness and differentiability of the retarded root: that lemma supplies, for every event of R3×R, existence and uniqueness of the root, the identity of the equality case s=t with x=z(t), the strict inequality s<t on D, the derivative formulas with 1−v∗/c≤κ≤1+v∗/c, and the Ck regularity of the root on D for a Ck trajectory; no new analysis is introduced here. Clause (c) is the elementary root check tr−s0=∣xr−z(s0)∣/c=r/c combined with the uniqueness in clause (a); no boundedness of z′′ is used. Clause (d) records the branch boundaries honestly: the finite-history and nonuniform cases are left to consumers, and the failure of existence under mere pointwise subluminality is exhibited on the examples page rather than asserted here. The phrase 'prescribed worldline' is licensed by Worldlines, four-velocity, chart readings and the frame/observer distinction(a) and (c), which relate chart readings t↦r(t) of massive worldlines to the condition ∣r′(t)∣<c. The definition introduces no physical field, so no Maxwell, self-force or empirical assertion is made; the cross-reference to Adopted retarded solution selection: the physical branch carries no incoming free field records that the retarded root is the kinematic object that the adopted selection turns into an emission time. No choice principle is used in the root lemma or in these kinematic constructions; its higher-regularity branch is explicitly choice-free.

LemmaStatement: AI-adaptedProof: AI-adaptedprecheck passOpen item page →

Zonal and quadratic sphere moments for the polar surface measure on S2

Statement

Assume the Axiom of Countable Choice (ACω), as carried by the surface-measure interface below (The Axiom of Countable Choice (ACω)). Let σ be the polar surface measure on the unit sphere S2⊆R3 (The polar surface set function on the unit sphere), let e3:=(0,0,1) and write n3=n⋅e3 for n∈S2. Then:

(a) [Zonal identity] for every continuous f:[−1,1]→R, ∫S2f(n3) dσ(n)=2π∫−11f(u) du.

(b) [Linear weighted moment] for every continuous f and every a∈R3, ∫S2(n⋅a) f(n3) dσ(n)=2π a3∫−11u f(u) du.

(c) [Quadratic weighted moment] for every continuous f and every a∈R3, ∫S2(n⋅a)2f(n3) dσ(n)=2π a32∫−11u2f(u) du+π (a12+a22)∫−11(1−u2)f(u) du.

(d) [Moments] σ(S2)=4π, ∫S2n dσ=0, ∫S2ninj dσ=(4π/3)δij, and for every a∈R3 ∫S2(n⋅a)2dσ=4π3∣a∣2,∫S2∣n×a∣2dσ=8π3∣a∣2, where δij is the Kronecker symbol and × the cross product of The cross product in R3.

(e) [Scope] (a)-(d) are identities for the polar surface measure of the unit sphere with only the stated continuity of f; they assert no physical field, flux or radiation statement. The measure is finite, so all displayed integrals are absolutely convergent; f need not be nonnegative. For the uses on this page f is a rational function with denominator bounded below by 1−b>0, hence continuous on [−1,1].

Facts & Assumptions

Given: ACω (The Axiom of Countable Choice (ACω)); the polar surface measure σ on S2; a continuous f:[−1,1]→R and a∈R3; e3=(0,0,1) and n3=n⋅e3; the chart X, the parameter region D and the reflection maps η1,η2,η3 introduced in steps 1.1 and 2.1.

[F1]

For Borel E⊆S2, σ(E)=3λ3{rω:ω∈E, 0<r≤1}; under ACω, σ is a finite Borel measure on S2. (The polar surface set function on the unit sphere, Polar coordinates decompose Lebesgue measure into r^{n-1} dr d sigma)

[F2]

The chart surface measure on S2 equals σ; orthogonal transformations of R3 preserve σ; and σ(S2)=3∣B1∣. (Agreement with the existing polar sphere measure)

[F4]

A regular parametrized surface patch is a C1 map X from a compact Jordan parameter region D (the closure of its nonempty connected interior) with Xu×Xv≠0 on D∘ and no interior parameter point sharing its image with a distinct point of D; seam identifications and rank failures may occur on the boundary. For continuous q on the patch image, ∫Sq dS=∫D(q∘X)JX with JX=∣Xu×Xv∣, and boundary values may be changed on the content-zero parameter boundary without changing the integral. (Regular parametrized surface patches on compact Jordan parameter regions, Surface area and scalar surface integrals on a regular patch, The surface area density is the norm of the cross product of the parameter tangents, Content-zero parameter-boundary exceptions do not affect surface integrals)

[F5]

Sine and cosine are differentiable with sin⁡′=cos⁡, cos⁡′=−sin⁡, sin⁡0=0, cos⁡0=1; sin⁡(π/2)=1, cos⁡(π/2)=0, sin⁡π=0, cos⁡π=−1; sin⁡(−x)=−sin⁡x, cos⁡(−x)=cos⁡x, sin⁡2x+cos⁡2x=1; sine is strictly increasing on [−π/2,π/2] and strictly decreasing on [π/2,3π/2], cosine is strictly decreasing on [0,π] and strictly increasing on [π,2π], both have range [−1,1]; the addition formulas sin⁡(x+y)=sin⁡xcos⁡y+cos⁡xsin⁡y, cos⁡(x+y)=cos⁡xcos⁡y−sin⁡xsin⁡y hold; and sin⁡x=0 if and only if x=mπ for some integer m. (Intermediate value theorem, by bisection with a canonical left-half rule: a continuous function on [a,b] takes every value between f(a) and f(b), The derivatives of sine and cosine are cosine and minus sine, Quarter-turn values and shifts by pi/2 and pi, Parity and the Pythagorean identity for sine and cosine, Signs, monotonicity intervals, and ranges of sine and cosine, The addition formulas for sine and cosine, The zero sets of sine and cosine and the least positive common period 2 pi)

[F6]

Let a<b. If f:[a,b]→R is continuous and P(u)=∫auf(v) dv for u∈[a,b], then P′=f there, with one-sided derivatives at a,b; if G:[a,b]→R is differentiable there with integrable derivative (using the same endpoint convention), then ∫abG′=G(b)−G(a); and the chain rule holds for composites of totally differentiable maps. (The first fundamental theorem: if f is integrable on [a,b] and continuous at c, then F′(c)=f(c); in particular a continuous f has F as a primitive, The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a), The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a))

[F7]

In R3 with the Euclidean inner product and norm, the cross product is bilinear and alternating, ⟨u×v,w⟩=det⁡[u v w], and ∥u×v∥22=∥u∥22∥v∥22−⟨u,v⟩2. (The cross product in R3, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn, The cross product is bilinear, alternating, and orthogonal to both factors, The squared cross-product norm is the Gram determinant of two vectors)

[F8]

Finite componentwise sums and products of Ck Euclidean maps are Ck, and composites of composable Ck maps are Ck; Ck means continuous partial derivatives up to order k. (Ck Euclidean maps are closed under componentwise algebra and composition, Ck Euclidean maps and diffeomorphisms)

[F9]

On the finite measure space (S2,σ) a bounded Borel function g with ∣g∣≤M is integrable, since ∫∣g∣ dσ≤Mσ(S2)<∞; the integral is linear in the integrand. (Integrable real and complex functions, and their integrals, Monotonicity and nonnegative homogeneity of the nonnegative integral, The Lebesgue integral is linear on L1(μ))

[F10]

For a bounded Jordan set E⊆R2 and a Riemann integrable g whose sections outside a content-zero exceptional set are Jordan measurable with integrable section functions, the iterated integral over either coordinate block equals ∫Eg. (Fubini over a bounded Jordan set when all but a content-zero family of sections are integrable)

[F11]

σ is invariant under the reflection ω↦−ω, and the substitution identity ∫g dσ=∫g∘η dσ for a σ-preserving bijection η holds for indicators by definition, extends to simple functions by linearity and to bounded Borel functions by the approximation used in that proof; the first moment satisfies ∫S2ω dσ=0. (Reflection invariance and vanishing first moment of the sphere measure)

[F12]

V3(1)=π3/2/Γ(5/2); Γ(s+1)=sΓ(s) for s>0 and Γ(1/2)=π, so Γ(5/2)=3π/4 and V3(1)=4π/3. (The closed form for the volume of the unit n-ball, The real Gamma functional equation Γ(s+1)=sΓ(s), Γ(1/2)=π from the Gaussian integral)

[F13]

Under ACω, the L1 change-of-variables formula holds for C1 diffeomorphisms of open Euclidean sets; a C1 map with invertible derivative has a C1 local inverse; product Lebesgue measure agrees with Euclidean Lebesgue measure on Borel sets, and Fubini holds for integrable functions. Degenerate bounded boxes have Lebesgue measure zero, continuous functions on compact sets are bounded, and bounded Borel Riemann-integrable functions on boxes have the same Riemann and Lebesgue integrals. (A C^1 diffeomorphism satisfies the change-of-variables formula for L^1 functions, The Euclidean inverse function theorem, On Borel subsets of R^{m+n}, the product lambda_m times lambda_n agrees with lambda_{m+n}, Fubini's theorem for L^1 functions on a sigma-finite product, A box in Rn with parameters ai≤bi is Lebesgue measurable of measure ∏i<n(bi−ai), whichever of its faces are included, A continuous real-valued function on a nonempty compact metric space is bounded and attains a greatest and a least value, Borel Darboux integrands in finite dimension)

Proof

technique · direct; the sphere integral is reduced to the standard rectangular chart, evaluated by Fubini and the fundamental theorem, and the weighted moments are obtained by reflection substitution
1.1F4F5F7F8algebra

Define X(θ,φ):=(sin⁡θcos⁡φ, sin⁡θsin⁡φ, cos⁡θ) and D:=[0,π]×[0,2π]. Then D is a compact Jordan parameter region, being a closed bounded rectangle and the closure of its nonempty connected interior D∘=(0,π)×(0,2π), and X is C1 on the open neighbourhood R2 of D because its components are finite sums and products of the C1 functions sin⁡ and cos⁡ [F5, F8]. Its partial derivatives are Xθ=(cos⁡θcos⁡φ,cos⁡θsin⁡φ,−sin⁡θ) and Xφ=(−sin⁡θsin⁡φ,sin⁡θcos⁡φ,0), and the coordinate formula for the cross product gives Xθ×Xφ=(sin⁡2θcos⁡φ, sin⁡2θsin⁡φ, sin⁡θcos⁡θ)=sin⁡θ X(θ,φ), since cos⁡2φ+sin⁡2φ=1; also ∣X(θ,φ)∣2=sin⁡2θ+cos⁡2θ=1 [F5, F7]. Hence Xθ×Xφ=0 exactly when sin⁡θ=0; on the interior θ∈(0,π) one has sin⁡θ>0 by strict monotonicity and the values sin⁡0=sin⁡π=0 [F5], so the parameter cross product is nonzero on D∘.

2.1step 1.1F4F5algebra

The chart covers the sphere and is injective in its interior. If n∈S2, the intermediate value theorem between the endpoint values cos⁡0=1, cos⁡π=−1, and strict monotonicity of cosine on [0,π] gives a unique θ∈[0,π] with cos⁡θ=n3, so sin⁡θ=(n12+n22)1/2 because sin⁡θ≥0 on [0,π] and sin⁡2θ=1−cos⁡2θ [F5]. If sin⁡θ=0 then n=±e3=X(0,0) or X(π,0); otherwise put c:=n1/sin⁡θ and s:=n2/sin⁡θ, so c2+s2=1, and choose φ∈[0,π] with cos⁡φ=c when s≥0 and φ∈[π,2π] with cos⁡φ=c when s<0, possible because cosine has range [−1,1] and is strictly monotone on each interval; then sin⁡φ has the sign of s there and sin⁡2φ=1−c2=s2, so sin⁡φ=s and n=X(θ,φ). Thus X[D]=S2. Conversely, if X(θ,φ)=X(θ′,φ′) with (θ,φ)∈D∘ and (θ′,φ′)∈D, then cos⁡θ=cos⁡θ′ with both angles in [0,π], so θ=θ′ by strict monotonicity; then sin⁡θ>0 and the first two coordinates give cos⁡φ=cos⁡φ′ and sin⁡φ=sin⁡φ′, hence cos⁡(φ−φ′)=cos⁡φcos⁡φ′+sin⁡φsin⁡φ′=cos⁡2φ+sin⁡2φ=1 [F5]. Writing x:=φ−φ′∈(−2π,2π) and using cos⁡x=1−2sin⁡2(x/2), we get sin⁡(x/2)=0, so x/2=mπ for some integer m and x=2mπ; since ∣x∣<2π this forces x=0, that is φ=φ′ [F5]. Therefore no interior parameter point shares its image with a distinct point of D, and (D,X) is a regular parametrized surface patch with image S2.

3.1step 1.1step 2.1F1F5F9F10F13algebra

Reduction to the chart, including its seam and poles. Let q:S2→R be continuous. Put H:={y∈R3:y2=0, y1≥0} and Y(r,θ,φ):=rX(θ,φ) on U:=(0,1)×D∘. By step 2.1, Y is a bijection from U onto the open set V:=B1(0)∖H. Its derivative has columns X,rXθ,rXφ, so det⁡DY=r2X⋅(Xθ×Xφ)=r2sin⁡θ>0 by step 1.1. The local inverse theorem [F13] makes its bijective inverse C1 locally at every point, hence Y is a C1 diffeomorphism. The omitted set H∩B1 is contained in the degenerate box [−1,1]×{0}×[−1,1] and is Lebesgue null by [F13]. The bounded Borel function q(y/∣y∣) on B1∖{0}, assigned zero at 0, is integrable by [F13]. Applying the polar formula of Polar coordinates decompose Lebesgue measure into r^{n-1} dr d sigma to its positive and negative parts gives ∫B1q(y/∣y∣)dy=13∫S2q dσ. Change of variables by Y and Fubini [F13] give the same integral as ∫01r2dr∫D∘q(X(θ,φ))sin⁡θ dθdφ. The parameter boundary is a finite union of degenerate boxes and therefore null; the integrand extends continuously to D, and its Lebesgue integral equals its Riemann integral by [F13]. Cancelling ∫01r2dr=1/3 therefore proves ∫S2q dσ=∫02π∫0πq(X(θ,φ))sin⁡θ dθdφ. This supplies the measure identification despite the seam and pole degeneracies; it does not apply an injective regular atlas chart across those degeneracies. In particular, for q=f∘n3, n3∘X=cos⁡θ gives I:=∫S2f(n3)dσ=∫02π∫0πf(cos⁡θ)sin⁡θ dθdφ.

4.1step 3.1F5F6F10algebra

Conclusion of (a). The function g(θ,φ):=f(cos⁡θ)sin⁡θ is continuous on the rectangle D [F5, F8], hence Riemann integrable, and its sections in φ are continuous; [F10] therefore gives I=∫0π(∫02πf(cos⁡θ)sin⁡θ dφ)dθ=2π∫0πf(cos⁡θ)sin⁡θ dθ. Let P(u):=∫−1uf(v) dv on [−1,1]; by [F6] P′=f, and the chain rule [F6] with cos⁡′=−sin⁡ [F5] gives (P∘cos⁡)′(θ)=−f(cos⁡θ)sin⁡θ on [0,π]. Since this derivative is continuous, the second fundamental theorem [F6] applies and ∫0πf(cos⁡θ)sin⁡θ dθ=−[P(cos⁡θ)]0π=P(1)−P(−1)=∫−11f(u) du, because cos⁡0=1 and cos⁡π=−1 [F5]. Combining with step 3.1 gives ∫S2f(n3) dσ=2π∫−11f(u) du, which is (a); all integrands here are continuous on the compact sets in question, so the displayed integrals are finite.

5.1step 4.1F2F5F9F11algebra

Conclusion of (b). Let η1(n1,n2,n3):=(−n1,n2,n3) and η2(n1,n2,n3):=(n1,−n2,n3). Each is an orthogonal bijection of R3 with ηi[S2]=S2, so each preserves σ [F2]; by the substitution identity of [F11], applied to the bounded Borel function gi(n):=nif(n3) and the fact that gi∘ηi=−gi, we get ∫S2nif(n3) dσ=−∫S2nif(n3) dσ, whence ∫S2nif(n3) dσ=0 for i=1,2 (finiteness of both integrals is [F9]). For the third component, (a) applied to the continuous function u↦uf(u) gives ∫S2n3f(n3) dσ=2π∫−11uf(u) du. Since n⋅a=a1n1+a2n2+a3n3, linearity of the σ-integral [F9] gives ∫S2(n⋅a)f(n3) dσ=2π a3∫−11uf(u) du, which is (b).

5.2step 4.1F2F5F9F11algebra

Conclusion of (c). Expanding the square, (n⋅a)2=∑i,j=13aiajninj, and by linearity [F9] the integral is the finite sum ∑i,jaiaj∫S2ninjf(n3) dσ. For i≠j the function ninjf(n3) changes sign under ηi (or ηj), so the substitution identity of [F11] gives ∫S2ninjf(n3) dσ=0. For the diagonal terms, the swap η3(n1,n2,n3):=(n2,n1,n3) is orthogonal and preserves σ [F2], so the substitution identity gives ∫S2n12f(n3) dσ=∫S2n22f(n3) dσ; with n12+n22=1−n32 [F5] and linearity, 2∫S2n12f(n3) dσ=∫S2(1−n32)f(n3) dσ=2π∫−11(1−u2)f(u) du by (a) applied to the continuous function u↦(1−u2)f(u); and (a) applied to u↦u2f(u) gives ∫S2n32f(n3) dσ=2π∫−11u2f(u) du. Substituting into the expansion yields ∫S2(n⋅a)2f(n3) dσ=2π a32∫−11u2f(u) du+π (a12+a22)∫−11(1−u2)f(u) du, which is (c).

6.1step 4.1step 5.1step 5.2F1F2F5F7F9F11F12algebra∎

Conclusion of (d) and scope (e). Taking f=1 in (a) gives σ(S2)=2π∫−11du=4π; independently [F2] gives σ(S2)=3∣B1∣=3V3(1), and [F12] evaluates V3(1)=π3/2/Γ(5/2) with Γ(5/2)=(3/2)(1/2)Γ(1/2)=3π/4, so V3(1)=4π/3 and the two routes agree. Taking f=1 in (b) gives ∫S2(n⋅a) dσ=0 for every a, hence ∫S2n dσ=0, and taking f=1 in (c) gives ∫S2(n⋅a)2dσ=2πa32⋅23+π(a12+a22)⋅43=4π3∣a∣2; choosing a=ei and a=ei+ej for i≠j reads off ∫S2ni2 dσ=4π/3 and ∫S2ninj dσ=0 for i≠j, that is ∫S2ninj dσ=(4π/3)δij. Finally the norm identity of [F7] gives ∣n×a∣2=∣n∣2∣a∣2−(n⋅a)2=∣a∣2−(n⋅a)2 for n∈S2, so by linearity [F9] and the value just computed ∫S2∣n×a∣2 dσ=4π∣a∣2−4π3∣a∣2=8π3∣a∣2. This proves all identities of (d); every integrand is continuous on the compact S2 and σ is a finite Borel measure by [F1], so the integrals are absolutely convergent, f need not be nonnegative, and no physical interpretation is asserted, which is (e).

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Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source

Physical scope

Retarded potentials and fields of a prescribed smooth conserved source of compact spatial support in a compact time interval, on the whole laboratory spacetime in the framework's inertial chart: Lorenz gauge, the smooth vacuum Maxwell equations, zero field before the source acts, the zero-data Cauchy identification and zero total charge. Excluded: point, line, sheet or non-integrable sources; weak/distributional branches; eternal isolated charges; finite-energy, decay or boundary claims; self-force and radiation reaction; and every empirical or measurement claim.

Statement

Assume the Axiom of Countable Choice (ACω) as carried by the retarded-kernel and Cauchy suppliers below (The Axiom of Countable Choice (ACω)). Let the laboratory region, chart and units be those of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values, so that c>0, μ0>0, ε0=(μ0c2)−1 and W:=c−2∂t2−Δ is the wave expression of Scalar-vector potential pairs, gauge transformation, Lorenz divergence and the wave expression. Let a>0, t0<T and let ρ:R3×R→R, J:R3×R→R3 be source fields of Charge parameter, frame charge and current densities, volume charge and flux, and the four-current that are jointly of class C∞ in the sense of Ck Euclidean maps and diffeomorphisms, vanish identically outside the compact set B‾a(0)×[t0,T], and satisfy the continuity equation ∂tρ+div⁡J=0 everywhere --- the compatibility condition that Charge continuity as a compatibility condition of the vacuum Maxwell equations shows to be forced by the Maxwell system, here assumed for the prescribed source. Define the retarded potentials by the explicit retarded integrals

φ(x,t):=14πε0∫R3ρ(y,t−∣x−y∣/c)∣x−y∣ dy,A(x,t):=μ04π∫R3J(y,t−∣x−y∣/c)∣x−y∣ dy,

and put E:=−∇φ−∂tA, B:=∇×A (Scalar-vector potential pairs, gauge transformation, Lorenz divergence and the wave expression, The electric and magnetic fields as fixed-time spatial vector fields). Then:

(a) [Smoothness and wave equations] φ and each component of A are of class C∞ on R3×R, and Wφ=ρ/ε0, WA=μ0J pointwise.

(b) [Lorenz gauge] With G:=div⁡A+c−2∂tφ one has G=0 on R3×R: the retarded pair is in Lorenz gauge, the continuity hypothesis supplies this identity and the total-charge conclusion (f).

(c) [Maxwell fields] E and B are of class C∞ and the tuple (E,B,ρ,J) satisfies the smooth branch of the vacuum Maxwell equations of The microscopic vacuum Maxwell equations: smooth and weak branches on the whole of R3×R: div⁡E=ρ/ε0, div⁡B=0, ∇×E=−∂tB, ∇×B=μ0J+c−2∂tE.

(d) [No field before the source] E=B=0 at every event with t<t0 (indeed φ=A=0 there): the selected retarded solution carries no field from before the source acted.

(e) [Zero-data Cauchy identification] For every t1<t0 the pair (φ,A) restricted to R3×[t1,∞) is the unique C2 extension solution of the wave Cauchy problem of The three-dimensional wave Cauchy problem: Kirchhoff representation, uniqueness, domain of dependence and compact support at time t1 with zero Cauchy data and sources ρ/ε0, μ0J.

(f) [Total charge] The total charge Q(t):=∫R3ρ(y,t) dy is zero for every t: a source that is smooth, compactly supported in space and restricted to a compact time interval and satisfies continuity carries zero total charge, so this branch does not model an eternal isolated nonzero charge.

(g) [Scope] This is the compact smooth branch with an adopted causal selection; it asserts nothing about point, line or sheet sources, about weak or distributional branches, about finite-energy or decay properties, about radiation reaction or self-force, and no empirical claim. In particular the fields of a prescribed isolated point charge with an eternal worldline are not covered by this theorem and are supplied separately by the point-source items of this page.

Facts & Assumptions

Given: ACω (The Axiom of Countable Choice (ACω)); the laboratory chart and SI constants of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values; constants a>0, t0<T; a jointly C∞ source pair (ρ,J) vanishing outside B‾a(0)×[t0,T] and satisfying ∂tρ+div⁡J=0; the retarded integrals φ,A of the Statement, with K denoting the retarded kernel of [F1] so that φ=ε0−1(K∗ρ) and Ak=μ0(K∗Jk).

[F1]

Retarded kernel: for every h∈Cc∞(R3×R) the function (K∗h)(x,t)=∫R3h(y,t−∣x−y∣/c)/(4π∣x−y∣) dy is well defined (absolutely convergent), of class C∞ on R3×R, and satisfies W(K∗h)=h pointwise. (The retarded wave kernel is a distribution supported on the cone, solves the point-wave equation, and convolves to the retarded solution (b))

[F2]

Gauge identities and the decoupling definition: for a potential pair of class C2 jointly on an open set, div⁡E=Wφ−∂tG and curl⁡B−c−2∂tE=WA+∇G hold there, the source-free equations div⁡B=0 and curl⁡E=−∂tB hold automatically for any potential pair, and if in addition G=0 then the sourced Maxwell system of The microscopic vacuum Maxwell equations: smooth and weak branches holds if and only if Wφ=ρ/ε0 and WA=μ0J; the fields E,B, the Lorenz divergence G and the wave expression W are those of Scalar-vector potential pairs, gauge transformation, Lorenz divergence and the wave expression, and field regularity classes are those of The electric and magnetic fields as fixed-time spatial vector fields. (Maxwell's equations in potential form: the Lorenz divergence, the decoupled wave equations and residual generators (a),(c))

[F3]

Cauchy uniqueness: if v∈C2(R3×[t1,T′]) is of class C2 in the extension sense, satisfies Wv=h on R3×(t1,T′) with h∈C∞(R3×[t1,T′]) in the extension sense, and has prescribed Cauchy data at t1, then v equals the solution constructed there. (The three-dimensional wave Cauchy problem: Kirchhoff representation, uniqueness, domain of dependence and compact support (b))

[F4]

SI constants: ε0=(μ0c2)−1, so c−2ε0−1=μ0; c>0, μ0>0. (Framework-local SI units, the vacuum constants and the exact/measured status of their values)

[F5]

Source fields: smooth source fields (ρ,J) with their units, the continuity equation and the compact-support convention are those of Charge parameter, frame charge and current densities, volume charge and flux, and the four-current; the standing hypotheses of this theorem are as stated in the Given. (Charge parameter, frame charge and current densities, volume charge and flux, and the four-current)

[F6]

C1 change of variables for L1: for a C1 diffeomorphism T:U→V of open sets and f∈L1(λn), ∫Vf=∫Uf∘T ∣det⁡DT∣. (A C^1 diffeomorphism satisfies the change-of-variables formula for L^1 functions)

[F7]

Differentiation under the integral sign: if x↦f(x,s) is integrable for every s in an open interval, s↦f(x,s) is differentiable for almost every x, the extended partial derivative is measurable in x, and ∣∂sf(x,s)∣≤g(x) for an integrable g independent of s, then ∫f(x,s) dx is differentiable with derivative ∫∂sf(x,s) dx. (Differentiation under the integral sign)

[F8]

Polar coordinates: for every nonnegative Borel f on R3, ∫R3f dλ3=∫0∞∫S2f(rω)r2 dσ(ω) dr; in particular ∫Bs(0)∣z∣−1 dz=4π∫0sr dr=2πs2<∞. (Polar coordinates decompose Lebesgue measure into r^{n-1} dr d sigma)

[F9]

Linearity of the integral on L1. (The Lebesgue integral is linear on L1(μ))

[F10]

Divergence theorem for a bounded C1 Euclidean domain Ω and F∈C1(Ω‾;R3): ∫Ωdiv⁡F dx=∫∂ΩF⋅ν dS with outward normal. (Divergence on a bounded C1 Euclidean domain)

[F11]

Parameter integrals: if K is compact measurable of finite measure and f,∂tf are continuous on a neighbourhood of K×[a,b], then t↦∫Kf(x,t) dx is differentiable there with derivative ∫K∂tf(x,t) dx. (Differentiation under the integral sign over a compact measurable set and over a compact C1 surface)

[F12]

Ck means continuous partial derivatives up to order k; finite sums and products of Ck maps are Ck. (Ck Euclidean maps and diffeomorphisms)

[F13]

The framework adopts the retarded branch of Adopted retarded solution selection: the physical branch carries no incoming free field: the selected physical potential pair is the retarded one with no free addition, and the theorem below computes exactly that branch; it asserts no existence of its own. (Adopted retarded solution selection: the physical branch carries no incoming free field (b),(c))

[F14]

For C2 fields and C1 sources satisfying the smooth branch of The microscopic vacuum Maxwell equations: smooth and weak branches, the continuity equation is forced; here continuity is assumed for the prescribed source. (Charge continuity as a compatibility condition of the vacuum Maxwell equations (a))

Proof

technique · direct; identify the potentials with the retarded kernel of [F1], differentiate the kernel pairing to obtain the Lorenz gauge from continuity, read off the Maxwell system from [F2], localize the retarded integrals for the vanishing and Cauchy claims, and integrate the continuity equation for the total charge
1.1F1F4F5F12

Smoothness and wave equations. The source pair (ρ,J) is jointly C∞ and vanishes outside the compact set B‾a(0)×[t0,T], so ρ/ε0 and each h=μ0Jk belongs to Cc∞(R3×R) [F5, F12]. Applying [F1] to these functions and using the identification φ=ε0−1(K∗ρ), Ak=μ0(K∗Jk) of the Given gives that φ and every component of A are of class C∞ on R3×R, with Wφ=ρ/ε0 and WA=μ0J pointwise. This is (a).

1.2F6F7F8

Derivative identities for the retarded kernel. Fix h∈Cc∞(R3×R). For fixed (x,t) the change of variable y↦z=x−y, a C1 diffeomorphism of R3 with ∣det⁡D(x−⋅)∣=1, is legitimate for the integrable function y↦h(y,t−∣x−y∣/c)/(4π∣x−y∣) [F6], so (K∗h)(x,t)=∫h(x−z,t−∣z∣/c)/(4π∣z∣) dz. Choose bh>0 such that the spatial projection of supp⁡h lies in B‾bh(0), and let Mh be a finite global bound on the first derivatives of h (they are continuous and compactly supported). On a parameter neighbourhood ∣x∣<R, ∣t∣<R, with R>0, each differentiated integrand vanishes unless ∣x−z∣≤bh, hence unless ∣z∣<R+bh. Its absolute value is bounded by Mh1BR+bh+1(z)/(4π∣z∣), which is integrable by [F8]. The zero extension at z=0 affects a null set only; this majorant is independent of the parameter being differentiated. The derivative is measurable as a limit of measurable difference quotients, so [F7] applies once per parameter x1,x2,x3,t with the other three parameters held fixed, and gives ∂xi(K∗h)=K∗(∂yih) and ∂t(K∗h)=K∗(∂th) on R3×R, where ∂yih is the partial derivative of h in its i-th spatial argument.

1.3F4F5F9algebra

No field before the source. Suppose t<t0. For every y the retarded argument satisfies t−∣x−y∣/c≤t<t0, where ρ and J vanish identically by the support hypothesis; hence both integrands in the definitions of φ and A vanish for every y, and φ(x,t)=0, A(x,t)=0 [F9]. Therefore E=−∇φ−∂tA=0 and B=∇×A=0 at every event with t<t0, which is (d).

1.4F5F9F10F11algebra

Total charge. By the support hypothesis, Q(t)=∫R3ρ(y,t)dy=∫Ba(0)ρ(y,t)dy for every t, and Q(t)=0 for t<t0; the integral depends smoothly on t with Q′(t)=∫Ba(0)∂tρ(y,t)dy by [F11] applied to the fixed compact B‾a(0) (the integrals over the open and closed balls agree since the smooth source vanishes on the boundary) (the integrands ρ,∂tρ are continuous on a neighbourhood of B‾a(0)×[t−1,t+1]) [F5, F12]. Fix t and R>a; the continuity equation and the divergence theorem [F10] give ∫Ba(0)div⁡J(y,t)dy=∫BR(0)div⁡J(y,t)dy=∫∂BR(0)J(y,t)⋅ν dS=0, because J vanishes outside B‾a(0) and R>a; hence Q′(t)=−∫Ba(0)div⁡J(y,t)dy=0. Thus Q is constant on R and, being zero at times before t0, is identically zero, which is (f).

2.1step 1.2F4F5F9algebra

Lorenz gauge. By step 1.2 applied to each component Ji and to ρ, together with linearity of the integral [F9], div⁡A=μ0∑i=13∂xi(K∗Ji)=μ0∑i=13K∗(∂yiJi)=μ0 K∗(div⁡J),c−2∂tφ=c−2ε0−1K∗(∂tρ)=μ0 K∗(∂tρ), the second equality using c−2ε0−1=μ0 [F4]. Adding, G=div⁡A+c−2∂tφ=μ0K∗(∂tρ+div⁡J)=0 pointwise on R3×R by the assumed continuity equation and linearity of the kernel integral [F9]. This is (b); continuity is also used in step 1.4 to establish the total-charge conclusion.

2.2step 1.1step 1.3F3F12algebra

Zero-data Cauchy identification. Fix t1<t0 and T′>t0. By step 1.3, φ(⋅,t1)=0, A(⋅,t1)=0 and also ∂tφ(⋅,t1)=0, ∂tA(⋅,t1)=0 (the same vanishing argument applies to the time derivatives, whose integrands contain ρt,Jt, vanishing for retarded arguments <t0 as well). By step 1.1 the pair is C∞, hence C2, on R3×[t1,T′] in the extension sense and satisfies Wφ=ρ/ε0, WA=μ0J on R3×(t1,T′); [F3] (with its final time renamed T′ and its Cauchy data a=b=0) therefore identifies each component with the zero-data solution constructed there. As T′>t0 is arbitrary, the identification extends to R3×[t1,∞), which is (e).

3.1step 1.1step 2.1step 2.2F2F13F14algebra∎

Maxwell fields. E and B are C∞ because φ and A are [step 1.1, F12]. By [F2] with the Lorenz divergence G of step 2.1, div⁡E=Wφ−∂tG=ρ/ε0−0 and curl⁡B−c−2∂tE=WA+∇G=μ0J+0; the two source-free equations div⁡B=0 and curl⁡E=−∂tB are automatic for the potential pair [F2]. Hence the smooth branch of The microscopic vacuum Maxwell equations: smooth and weak branches holds for (E,B,ρ,J) on R3×R with E,B of class C∞, which is (c). The remaining clause (g) is scope bookkeeping: every hypothesis used above is one of the displayed compact smooth source hypotheses, no point, line, sheet or distributional source is involved, no product of distributions or self-field is formed, no finite-energy, decay, self-force or measurement claim is made, and the only choice assumption is ACω carried by the kernel, polar and Cauchy suppliers.

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Controlled electric-dipole far field and retarded-time radiated power of a compact smooth source

Physical scope

Far-zone electric-dipole radiation of a prescribed smooth conserved source of compact spatial support and compact time support: the dipole moment identities, the explicit absolute dipole-replacement error D(u), the uniform leading far fields and the retarded-time radiated power with its absolute error. Excluded: point charges; sources without the compact smooth branch; claims that slowness alone controls D(u); observation-time power and signal-speed readings; self-force, radiation reaction and every empirical or measurement claim.

Statement

Assume the setting and hypotheses of Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources and ACω as carried by its suppliers: c>0, μ0>0, a>0, t0<T, jointly C∞ fields ρ,J vanishing outside B‾a(0)×[t0,T] and satisfying ∂tρ+div⁡J=0; let φ,A be the retarded potentials and E:=−∇φ−∂tA, B:=∇×A the fields, with S:=E×B/μ0 (Vacuum electromagnetic energy density and energy flux (the Poynting vector), Local and fixed-volume electromagnetic energy balance). Adopt the causal selection Adopted retarded solution selection: the physical branch carries no incoming free field: these retarded fields are the fields of the source model (the compact smooth instance established by Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source). Define the time-dependent electric dipole moment

p(u):=∫Bay ρ(y,u) dy∈R3

(componentwise, about the fixed chart origin of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields; it is the fixed-time analogue of the static source moment of Total charge, dipole moment, Cartesian moments and traceless quadrupole of a static charge distribution), and, as in the asymptotic theorem, I(n,u):=∫BaJ(y,u+n⋅y/c) dy, V(n,u):=∂uI(n,u)=∫BaJt(y,u+n⋅y/c) dy and

D(u):=ac∫Basup⁡∣v−u∣≤a/c∣Jtt(y,v)∣ dy.

Then:

(a) [Moment identities] p∈C∞(R;R3), p′(u)=∫BaJ(y,u) dy, p′′(u)=∫BaJt(y,u) dy, ∫Baρt(y,u) dy=0 and the total charge ∫Baρ(y,u) dy vanishes for every u.

(b) [Dipole replacement error] ∣V(n,u)−p′′(u)∣≤D(u) for every n∈S2 and every u∈[t0,T]: the explicit absolute error of the dipole approximation to the source's transverse current moment.

(c) [Leading fields] With ΓE, ΓB the constants of Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources(b) (depending only on a,c,μ0 and the listed source suprema), for every n∈S2, u∈[t0,T], r≥2a:

∣E(rn,u+rc)−μ04πrn×(n×p′′(u))∣≤ΓEr2+μ0D(u)4πr,∣B(rn,u+rc)−n×E(rn,u+rc)c∣≤ΓB+ΓE/cr2.

The displayed dipole field approximates the actual leading far field Elead=μ0n×(n×V)/(4πr) with the stated absolute D(u)/r error. Equality of these leading fields requires n×(n×(V−p′′))=0; V=p′′ and, in particular, D(u)=0 are sufficient. All errors are uniform in n at fixed u.

(d) [Retarded-time radiated power] The limit of Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources(c) equals μ0∣p′′(u)∣2/(6πc)+R(u) with the explicit absolute error

∣R(u)∣≤μ0(2∣p′′(u)∣D(u)+D(u)2)4πc,solim⁡r→∞∫S2r2n⋅S(rn,u+rc)dσ=μ06πc∣p′′(u)∣2  whenever D(u)=0.

The evaluation uses the sphere moment ∫S2∣n×p′′∣2dσ=(8π/3)∣p′′∣2 of Zonal and quadratic sphere moments for the polar surface measure on S2(d). The limit is at fixed retarded time u, not at fixed observation time.

(e) [Scope] The compact smooth source branch only; the dipole error is absolute and explicitly controlled by D(u), and no assertion is made that slow or 'nonrelativistic' source motion alone makes D(u) small -- that is a hypothesis on the source's time variation. No point charge, no moving point source, no radiation reaction, no self-force and no empirical or measurement content; the failure of the correspondence with an oscillator for rapidly varying sources is retained through D(u). Separately retain the sharper actual source estimate ∣B(rn,u+r/c)−n×Elead(n,u,r)/c∣≤ΓB/r2, with Elead=μ0n×(n×V)/(4πr); the bound against the actual E uses the combined constant displayed in (c).

Facts & Assumptions

Given: ACω (The Axiom of Countable Choice (ACω)); the hypotheses of Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources: constants c>0, μ0>0, a>0, t0<T, jointly C∞ sources (ρ,J) vanishing outside B‾a(0)×[t0,T] and satisfying ∂tρ+div⁡J=0; the retarded potentials and fields with S=E×B/μ0; the dipole moment p, the moments I,V and the error coefficient D of the Statement.

[F1]

Far-zone expansion of Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources (b): with I(n,u)=∫BaJ(y,u+n⋅y/c)dy, V=∂uI, Elead(n,u,r)=μ04πrn×(n×V(n,u)) and ΓE,ΓB constants depending only on a,c,μ0 and the source suprema, for all n∈S2, u∈[t0,T], r≥2a one has ∣E(rn,u+r/c)−Elead(n,u,r)∣≤ΓE/r2 and ∣B(rn,u+r/c)−n×Elead(n,u,r)/c∣≤ΓB/r2. (Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources (b))

[F2]

Retarded-time flux limit of Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources (c): for every u∈[t0,T], lim⁡r→∞∫S2r2n⋅S(rn,u+rc) dΩ(n)=μ016π2c∫S2∣n×V(n,u)∣2 dΩ(n), a limit at fixed retarded time; dΩ is the sphere surface measure, which equals the polar measure σ on S2. (Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources (c))

[F3]

Energy flux reading: S=E×B/μ0 is the Poynting energy-flux density of Vacuum electromagnetic energy density and energy flux (the Poynting vector), and the fixed-volume Poynting balance of Local and fixed-volume electromagnetic energy balance contains −∮S⋅n dS, the negative of the outward field-energy flux, in the field-energy rate. (Vacuum electromagnetic energy density and energy flux (the Poynting vector), Local and fixed-volume electromagnetic energy balance)

[F4]

Source moments: the static dipole moment and total charge of a compactly supported charge distribution about the chart origin are those of Total charge, dipole moment, Cartesian moments and traceless quadrupole of a static charge distribution(a); the present p(u) is the fixed-time analogue for the moving source. (Total charge, dipole moment, Cartesian moments and traceless quadrupole of a static charge distribution)

[F5]

Parameter integrals over a fixed compact set: if f,∂tf are continuous on a neighbourhood of K×J with K compact measurable of finite measure, then t↦∫Kf is differentiable with derivative ∫K∂tf; iterating gives C∞ dependence for C∞ integrands. (Differentiation under the integral sign over a compact measurable set and over a compact C1 surface)

[F6]

Divergence theorem on a bounded C1 domain: ∫Ωdiv⁡F=∫∂ΩF⋅ν dS for F∈C1(Ω‾;R3). (Divergence on a bounded C1 Euclidean domain)

[F7]

Mean value theorem: if f:[s1,s2]→R is continuous and differentiable in the interior, then f(s2)−f(s1)=f′(s∗)(s2−s1) for some interior s∗. (The mean value theorem, as the case g(x)=x of Cauchy's: for f continuous on [a,b] with a<b and differentiable on (a,b) there is c∈(a,b) with f(b)−f(a)=f′(c)(b−a))

[F8]

Cauchy-Schwarz: ∣e⋅w∣≤∣e∣∣w∣ for e,w∈R3. (The Cauchy-Schwarz inequality for finite sums, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn)

[F9]

Integral triangle inequality and monotonicity: ∣∫f∣≤∫∣f∣ for integrable f, and 0≤f≤g gives ∫f≤∫g for the nonnegative integral. (The modulus of an integral is bounded by the integral of the modulus, Monotonicity and nonnegative homogeneity of the nonnegative integral)

[F10]

Cross product identities: u×v is bilinear and alternating, n⋅(u×v)=det⁡(n,u,v), and for ∣n∣=1 one has n⋅(n×w)=0, n×(n×w)=n(n⋅w)−w, ∣n×(n×w)∣=∣n×w∣≤∣w∣; and for a⊥:=a−(n⋅a)n one has a⋅b−(n⋅a)(n⋅b)=a⊥⋅b⊥. (The cross product is bilinear, alternating, and orthogonal to both factors, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn)

[F11]

Shifted source moments: V(n,u)=∫BaJt(y,u+n⋅y/c)dy=∂uI(n,u). (Uniform far-zone asymptotics and retarded-time flux limit for compact conserved smooth sources (a),(b))

[F12]

Sphere moment: ∫S2∣n×a∣2 dσ(n)=8π3∣a∣2 for every a∈R3, and σ(S2)=4π. (Zonal and quadratic sphere moments for the polar surface measure on S2 (d))

[F13]

Compact smooth branch: for the same source class the retarded fields satisfy the smooth vacuum Maxwell equations and the total charge vanishes: ∫Baρ(y,u)dy=0 for every u, and the retarded pair is the adopted selected branch. (Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source (b),(f), Adopted retarded solution selection: the physical branch carries no incoming free field)

[F14]

Source support and regularity conventions: (ρ,J) are the smooth source fields of Charge parameter, frame charge and current densities, volume charge and flux, and the four-current, with the support hypothesis of the Given. (Charge parameter, frame charge and current densities, volume charge and flux, and the four-current)

Proof

technique · direct; obtain the moment identities by differentiating the dipole integral and integrating the continuity equation by parts, bound the moment replacement by the mean value theorem, transfer the far-zone expansion of [F1] to the dipole fields, and evaluate the flux limit of [F2] using the exact sphere moment [F12] and the pointwise replacement bound
1.1F4F5F6F9F13F14algebra

Moment identities (a). The moment p(u)=∫Bay ρ(y,u)dy is the fixed-time analogue of the static source moment of [F4], a convention about which moment is computed and not a dynamical identity. Since ρ is jointly C∞ and supported in the fixed compact set B‾a(0)×[t0,T], repeated application of [F5] to u↦p(u) shows p∈C∞ with p′(u)=∫Bay ρt(y,u)dy and p′′(u)=∫Bay ρtt(y,u)dy [F14]. For the first derivative, fix u and R>a: the continuity equation gives ∫Bayiρt(y,u)dy=−∫Bayidiv⁡J(y,u)dy, and since div⁡(yiJ)=Ji+yidiv⁡J, the divergence theorem [F6] on BR gives ∫BRdiv⁡(yiJ)dy=∫∂BRyiJ⋅ν dS=0 because J vanishes on ∂BR; hence ∫Bayidiv⁡J dy=−∫BaJi dy and pi′(u)=∫BaJi(y,u)dy [F9]. Differentiating this identity once more with [F5] gives p′′(u)=∫BaJt(y,u)dy, the displayed second moment identity. The same divergence theorem with weight 1 gives ∫Baρt(y,u)dy=−∫Badiv⁡J(y,u)dy=0, and the vanishing of the total charge is clause (f) of [F13] for this source class. This is (a).

2.1step 1.1F7F8F9F11F14F15algebra

Dipole replacement error (b). First D(u) is well defined and finite. For fixed u, the function gu(y):=max⁡∣v−u∣≤a/c∣Jtt(y,v)∣ attains its maximum by [F15]. Moreover ∣gu(y)−gu(y′)∣≤sup⁡∣v−u∣≤a/c∣∣Jtt(y,v)∣−∣Jtt(y′,v)∣∣, so uniform continuity on B‾a×[u−a/c,u+a/c] makes gu continuous and bounded on B‾a. It is therefore measurable and integrable on the finite-measure ball, giving the claimed finite coefficient; the same estimate after writing v=u+w also makes D continuous on compact time intervals. Fix n∈S2, u∈[t0,T] and y∈Ba, and put s1:=u, s2:=u+n⋅y/c, so ∣s2−s1∣≤a/c; the map s↦Jt(y,s) is C1 [F14]. If Δ:=Jt(y,s2)−Jt(y,s1)≠0, apply [F7] on the closed interval between s1 and s2 to the scalar function s↦e⋅Jt(y,s) with e:=Δ/∣Δ∣: there is s∗ between s1 and s2 with e⋅Δ=(e⋅Jtt(y,s∗))(s2−s1); if Δ=0 the same bound holds trivially. By [F8], ∣e⋅Jtt(y,s∗)∣≤∣Jtt(y,s∗)∣, so ∣Δ∣≤(a/c)sup⁡∣v−u∣≤a/c∣Jtt(y,v)∣ (the point s∗ lies within a/c of u). Integrating over Ba with the integral triangle inequality and monotonicity [F9], and using V(n,u)−p′′(u)=∫Ba[Jt(y,u+n⋅y/c)−Jt(y,u)]dy from step 1.1 and [F11], gives ∣V(n,u)−p′′(u)∣≤D(u). This is (b).

3.1step 2.1F1F9F10algebra

Leading fields (c). By [F1], for n∈S2, u∈[t0,T], r≥2a write E(rn,u+rc)=Elead(n,u,r)+ρE with ∣ρE∣≤ΓE/r2 and Elead=μ0 n×(n×V(n,u))/(4πr). Substituting V=p′′+(V−p′′) and using the identity ∣n×(n×w)∣=∣n×w∣≤∣w∣ of [F10] together with the bound of step 2.1, ∣E(rn,u+rc)−μ04πrn×(n×p′′(u))∣≤ΓEr2+μ04πr∣V(n,u)−p′′(u)∣≤ΓEr2+μ0D(u)4πr, which is the first displayed bound. For the magnetic field, [F1] gives ∣B(rn,u+rc)−n×Elead/c∣≤ΓB/r2, and ∣n×(E−Elead)∣/c≤∣E−Elead∣/c≤ΓE/(cr2) by [F10], so the triangle inequality [F9] gives the second displayed bound (ΓB+ΓE/c)/r2; the sharper source estimate against n×Elead/c is the supplier's own ΓB/r2 bound retained in (e). This is (c), uniformly in n at fixed u.

4.1step 2.1F2F3F8F9F10F12algebra∎

Retarded-time radiated power (d). By [F2], the limit of ∫S2r2n⋅S(rn,u+rc)dσ as r→∞ equals μ016π2c∫S2∣n×V(n,u)∣2dσ at fixed u; here the polar measure and the sphere surface measure coincide, and [F3] identifies the surface flux with the field-energy flux. For the replacement V↦p′′ put a±:=V±p′′; by [F10] the pointwise difference satisfies ∣n×V∣2−∣n×p′′∣2=a+⋅a−−(n⋅a+)(n⋅a−)=(a+)⊥⋅(a−)⊥, so its absolute value is at most ∣a+∣∣a−∣≤(∣V∣+∣p′′∣)∣V−p′′∣≤(2∣p′′∣+D)D=2∣p′′∣D+D2, using [F8], the bound of step 2.1 and monotonicity of the norm. Since σ(S2)=4π [F12], the integral changes by at most 4π(2∣p′′∣D+D2) in absolute value [F9], so the limit equals μ016π2c∫S2∣n×p′′(u)∣2dσ+R(u) with ∣R(u)∣≤μ0(2∣p′′∣D+D2)4πc. The exact integral is ∫S2∣n×p′′(u)∣2dσ=8π3∣p′′(u)∣2 by [F12], so the exact term is μ016π2c⋅8π3∣p′′(u)∣2=μ06πc∣p′′(u)∣2; whenever D(u)=0 the error vanishes by the displayed bound. This is (d). The scope clause (e) is bookkeeping: the limit is at fixed retarded time, the error is controlled by the source's time variation through D(u) alone, and no point source, no observer-time power, no radiation reaction, no self-force and no measurement claim is introduced; the only choice assumption is ACω, inherited from the supplier.

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Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder

Physical scope

Retarded potentials and fields of a prescribed point charge with charge parameter q∈R on a uniformly subluminal C3 worldline, off the worldline: exact Lienard-Wiechert split, B=n×E/c, the velocity-field bound and the uniform-in-direction far-zone remainder at a fixed emission event; and the constructed proper point-source weak Maxwell solution with Lloc1 field representatives and distributional Lorenz-gauge potentials. Excluded: field values on the worldline and any nonlinear self-interaction (no products of distributions, no self-force, no radiation reaction); energy, flux or power (deferred to the emitted-power items of this page); uniform bounds in the emission event; and every empirical or measurement claim.

Statement

Assume the Axiom of Countable Choice (ACω) as carried by the point-source change-of-variables suppliers below (The Axiom of Countable Choice (ACω)). Let the laboratory region, chart and units be those of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values (c>0, μ0>0, ε0=(μ0c2)−1), let q∈R and let z, v∗ be a retarded point-geometry datum of Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline (a prescribed C3 uniformly subluminal worldline of a point charge, Worldlines, four-velocity, chart readings and the frame/observer distinction, with the constant C:=q/(4πε0)), write Ω:=R3×R and Γ:={(z(s),s):s∈R}, and let ρ,J be the point-source distributions of that charge on the worldline in the declared point-source class of Distributional Maxwell equations with point and stationary-sheet sources(b) (the C3 branch of the point-current construction). Let (φ,A) be the retarded history pairings of Retarded potentials of a point history as the retarded convolution of the point sources, and the off-worldline Lienard-Wiechert fields(b) -- the framework's retarded construction for this source under the adopted selection Adopted retarded solution selection: the physical branch carries no incoming free field -- and define E:=−∇φ−∂tA, B:=∇×A on the off-worldline domain Ω∖Γ (Scalar-vector potential pairs, gauge transformation, Lorenz divergence and the wave expression, The electric and magnetic fields as fixed-time spatial vector fields). Then:

(a) [Potentials] φ=C/(κr) and A=βφ/c on Ω∖Γ, where r,κ,β are the retarded data of Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline(b); the zero extensions of φ,A to Γ are locally integrable on Ω.

(b) [Exact fields] On Ω∖Γ, E=Evel+Eacc,Evel=C(1−∣β∣2)(n−β)κ3r2,Eacc=C n×((n−β)×β˙)c κ3r,B=n×Ec, and E,B are of class C1 there; the velocity part obeys ∣Evel∣≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2.

(c) [Uniform far-zone remainder] For every emission event s0 and direction n∈S2, with xr:=z(s0)+rn, tr:=s0+r/c, β0:=z′(s0)/c, β˙0:=z′′(s0)/c and κ0:=1−n⋅β0: (xr,tr)∈Ω∖Γ, s(xr,tr)=s0, and E(xr,tr)=C n×((n−β0)×β˙0)c κ03 r+ρE(s0,n,r),∣ρE(s0,n,r)∣≤∣C∣1+v∗/c(1−v∗/c)3 r−2,B(xr,tr)=n×E(xr,tr)c; the bound is uniform in n at fixed s0.

(d) [Scope] These are the stipulated retarded model fields of the prescribed charge: the item identifies, through the same adopted causal selection used by Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source for the compact branch, the point-source potentials and fields of the model, and proves their exact form and bounds. It asserts no value of the fields on the worldline Γ (where the formulas are undefined and the self-field is singular), no integral or energy statement, no self-force and no radiation reaction, and derives no mass. The uniform bound v∗<c and the exclusion of Γ are essential hypotheses; the companion example page shows that a merely pointwise subluminal curve can fail to have a retarded root, and no uniformity in the emission event s0 is claimed (z′′ is not assumed bounded). The signed constant C is retained in every displayed formula while absolute-value bounds use ∣C∣.

(e) [Constructed weak solution] Let Φ,Υ be the global regular potential distributions in (a), and let E=−∇Φ−∂tΥ, B=curl⁡Υ. By The retarded point-history pair solves wave, Lorenz and Maxwell equations distributionally, with locally integrable field representatives off the worldline, their representatives are exactly the locally integrable zero extensions of the displayed off-worldline fields. They satisfy all four identities of Distributional Maxwell equations with point and stationary-sheet sources(e) with the proper all-time point pair ρ,J; the volume source parts are zero. Thus they are an admitted point-source model of the explicit physical adoption Distributional vacuum Maxwell equations for the declared point and stationary-sheet sources, under the same retarded selection. The potentials satisfy WΦ=ρ/ε0, WΥ=μ0J and the distributional Lorenz identity. This existence and solution property is supplied by the mathematical theorem, not by the selection postulate or by the compact-source theorem. The zero extensions on the null graph give no physically defined self-field and no nonlinear products there. All original exact field, regularity and uniform far-zone branches remain as stated. On each product neighborhood disjoint from Γ the fields satisfy the smooth source-free Maxwell equations. Consequently any use of Local and fixed-volume electromagnetic energy balance by the radiation items is local on such neighborhoods, with ρ=J=0; it neither applies that smooth theorem across the point source nor forms self-work or a global finite-energy identity.

Facts & Assumptions

Given: ACω (The Axiom of Countable Choice (ACω)); the laboratory chart, units and constants of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values; a retarded point-geometry datum: q∈R, z:R→R3 of class C3 with ∣z′(s)∣≤v∗<c, and the off-worldline domain Ω∖Γ with the retarded data s,r,n,β,κ,β˙ of Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline; the constant C=q/(4πε0).

[F1]

Retarded point geometry: on Ω∖Γ the root s=s(x,t)<t solves t−s=∣x−z(s)∣/c, is C3, satisfies ∂ts=1/κ and ∇xs=−n/(cκ), and κ=1−n⋅β∈[1−v∗/c,1+v∗/c]; at an emission event s0 and direction n∈S2, the event (xr,tr)=(z(s0)+rn,s0+r/c) lies in Ω∖Γ and has root s(xr,tr)=s0. (Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline (a)-(c))

[F2]

Point-source history pairings: for the point-source distributions ρ,J attached to q and z, the retarded-history pairings Φ,Υ define distributions on Ω, are finite for every test, and satisfy ⟨Φ,ψ⟩=∫Ω∖ΓCψ/(κr) and ⟨Υ,ψ⟩=∫Ω∖Γ(β/c)Cψ/(κr) componentwise; consequently φ=C/(κr) and A=βφ/c are C2 functions off the worldline whose locally integrable zero extensions have Φ,Υ as their regular distributions. (Retarded potentials of a point history as the retarded convolution of the point sources, and the off-worldline Lienard-Wiechert fields (b))

[F3]

Exact fields: with E=−∇φ−∂tA and B=curl⁡A on Ω∖Γ, one has E=Evel+Eacc with the displayed velocity and acceleration parts, B=n×E/c, both fields C1 off the worldline, and ∣Evel∣≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2. (Complete retarded point fields: unique retarded root, the delta substitution with denominator 1−n⋅β, Liénard–Wiechert potentials and fields, and a uniform far-zone remainder (c))

[F4]

Uniform far-zone remainder: at the emission sphere E(xr,tr)=C n×((n−β0)×β˙0)/(cκ03r)+ρE with ∣ρE∣≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2 uniformly over n∈S2 at fixed s0, and B(xr,tr)=n×E(xr,tr)/c. (Complete retarded point fields: unique retarded root, the delta substitution with denominator 1−n⋅β, Liénard–Wiechert potentials and fields, and a uniform far-zone remainder (d))

[F5]

Distributional point-source Maxwell theorem: WΦ=ρ/ε0, WΥ=μ0J and div⁡Υ+c−2∂tΦ=0 in D′(Ω); the distributions E=−∇Φ−∂tΥ, B=curl⁡Υ satisfy the four distributional Maxwell identities with the point pair; and off Γ they restrict to the exact C1 fields of [F3], the locally integrable zero extensions of the field formulas being their regular representatives. (The retarded point-history pair solves wave, Lorenz and Maxwell equations distributionally, with locally integrable field representatives off the worldline (a)-(c))

[F6]

Weak source class and solution predicate: the all-time C3 uniformly subluminal worldline with its proper graph is an admitted point source, the predicate consists of the four vanishing distributional pairings with the source pairings of the declared point class, and no product of two distributions is formed anywhere. (Distributional Maxwell equations with point and stationary-sheet sources (b),(e),(f))

[F7]

Adopted singular-source physics: point-source models satisfying the weak predicate are the adopted physical models of the separate postulate, which the earlier smooth-source postulate neither covers nor implies. (Distributional vacuum Maxwell equations for the declared point and stationary-sheet sources)

[F8]

Adopted selection: the retarded branch with no free addition is the framework's selected branch, and for the point-source branch the same selection is adopted in the weak equations of the singular-source model. (Adopted retarded solution selection: the physical branch carries no incoming free field (b),(c))

[F10]

The same adopted causal selection is used by the compact-source theorem Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source for its branch, and that theorem explicitly leaves point sources to the point-source items of its page; the uniform speed bound and the exclusion of Γ are essential hypotheses of the point construction. (Retarded potentials, Lorenz gauge and Maxwell fields of a compactly supported conserved smooth source (b),(g))

[F11]

Local Poynting balance: for jointly C1 fields solving the smooth source-free vacuum Maxwell equations on a region, the local identity ∂tu+div⁡S=−J⋅E of Local and fixed-volume electromagnetic energy balance holds there, and on a product neighborhood disjoint from Γ the point pair restricts to zero. (Local and fixed-volume electromagnetic energy balance (a),(c))

Proof

technique · direct identification; clauses (a)-(d) instantiate the retarded point-geometry datum and the two point-source suppliers, and clause (e) instantiates the distributional point-source theorem and the weak solution predicate, with the physical adoption supplied separately by the postulates
1.1F1F2F9algebra

Potentials (a). By [F1] the retarded data are defined, with s,r,n of class C3 and β,κ of class C2 on Ω∖Γ with κ≥1−v∗/c>0, and C=q/(4πε0) is the stated signed constant [F9]. Clause (b) of [F2] identifies the retarded-history pairings with the exact integrals ∫Ω∖ΓCψ/(κr) and ∫Ω∖Γ(β/c)Cψ/(κr), and states that the potentials are the C2 functions φ=C/(κr) and A=βφ/c off the worldline whose zero extensions to Γ are locally integrable. This is (a).

2.1step 1.1F3F9algebra

Exact fields (b). Clause (c) of [F3] gives, at every event of Ω∖Γ, the split E=Evel+Eacc with the displayed velocity and acceleration parts, the relation B=n×E/c, the C1 regularity of both fields, and the velocity bound ∣Evel∣≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2; the fields are defined as E=−∇φ−∂tA and B=curl⁡A with the conventions of [F9], and the constant C is retained with its sign in the field formulas while the bound uses ∣C∣. This is (b).

2.2step 1.1F1F4algebra

Uniform far-zone remainder (c). Fix s0∈R and n∈S2; by F1 the event (xr,tr)=(z(s0)+rn,s0+r/c) lies in Ω∖Γ and its root is s(xr,tr)=s0, so the retarded data at that event are exactly β0,β˙0,κ0 and r. Clause (d) of [F4] then gives the displayed decomposition of E(xr,tr) with the uniform bound ∣ρE(s0,n,r)∣≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2 over n∈S2 at fixed s0, together with B(xr,tr)=n×E(xr,tr)/c. This is (c).

3.1step 1.1step 2.2F8F10algebra

Scope (d). The identification of the retarded construction of clause (a)-(b) with the model fields of the prescribed charge is the adopted causal selection of [F8], the same selection used by the compact-source theorem [F10]; nothing in steps 1.1-2.2 assigns a field value on Γ (the formulas require r>0), forms a product of the singular source with a field, or proves a self-force, radiation-reaction, energy or mass statement, and [F10] records that the compact-source branch explicitly leaves point sources to this page. The bound in (c) is uniform in n at fixed s0 only, since β˙0 and κ0−3 depend on the emission event and z′′ is not assumed bounded. This is (d).

4.1step 1.1step 2.1step 2.2step 3.1F5F6F7F8F11algebra∎

Constructed weak solution (e) and conclusion. By F5 the potential distributions of [F2] satisfy WΦ=ρ/ε0, WΥ=μ0J and the distributional Lorenz identity, and by F5 the field distributions E,B satisfy all four distributional Maxwell identities with the point pair ρ,J; F5 identifies their representatives with the locally integrable zero extensions of the off-worldline fields of [F3] and records that the off-worldline C1 fields satisfy the source-free classical Maxwell equations. The all-time C3 uniformly subluminal worldline with its proper graph is an admitted point source of the declared class [F6], the source pairings are those of the predicate, and the volume source parts vanish; hence the four identities are exactly the solution predicate of F6 with (ρ,J), and by the explicit physical adoption [F7] under the same retarded selection [F8] these constructed weak fields are the model fields of the point charge. This is the solution property claimed in (e); it is supplied by the mathematical theorem and not by the selection postulate. No product of distributions is formed anywhere (F6), and the zero extension on the null graph gives no physically defined self-field there. Finally, on a product neighborhood disjoint from Γ the point pair restricts to the zero source so that the smooth source-free Maxwell equations of F5 hold and the local Poynting identity [F11] applies there with ρ=J=0; it is never applied across the point source and forms no self-work or global finite-energy identity. This completes (e) and, with steps 1.1-3.1, all clauses (a)-(e).

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Instantaneous-rest Larmor power and uniform low-speed comparison for a prescribed point charge

Physical scope

Exact rest-event radiation of the prescribed retarded point-source model (angular flux density, Larmor power and sin^2 pattern with the uniform velocity-field remainder) and a separately quantified general uniform low-speed power and angular comparison; no particle dynamics, self-force, radiation reaction, mass derivation or empirical claim.

Statement

Assume ACω as carried by the cited point-source suppliers. Let the laboratory region, chart and units be those of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values, let q∈R, let z,v∗ be a retarded point-geometry datum of Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline (prescribed C3 uniformly subluminal worldline, C:=q/(4πε0)), let s0 be an emission event with z′(s0)=0 (the charge is momentarily at rest in the laboratory chart), and put a:=z′′(s0) and, for n∈S2, xr:=z(s0)+rn, tr:=s0+r/c. Let E,B be the retarded fields of the charge given by Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder and S:=E×B/μ0 (Vacuum electromagnetic energy density and energy flux (the Poynting vector), Local and fixed-volume electromagnetic energy balance). Then:

(a) [Field on the emitted sphere] For every r>0 and n∈S2, E(xr,tr)=C n×(n×a)c2r+ρE(s0,n,r),∣ρE(s0,n,r)∣≤∣C∣1+v∗/c(1−v∗/c)3r−2,B(xr,tr)=n×E(xr,tr)c.

(b) [Angular flux density] The limits dPdσ(n):=lim⁡r→∞r2 n⋅S(xr,tr)=C2 ∣n×(n×a)∣2μ0c5,Pem(s0):=∫S2dPdσ(n) dσ(n), exist with the convergence uniform in n∈S2; dσ is the polar surface measure of the unit sphere (equal to the chart surface measure by Agreement with the existing polar sphere measure).

(c) [Total power] Pem(s0)=C2μ0c5⋅8π3∣a∣2=q2∣a∣26πε0c3, the Larmor power of the momentarily resting prescribed charge.

(d) [Angular distribution] For a≠0, define θ∈[0,π] by cos⁡θ=(n⋅a)/∣a∣; this angle exists uniquely because the quotient is in [−1,1] and cosine is continuous and strictly decreasing from 1 to −1 on [0,π]. When a=0 the angle is undefined and dP/dσ≡0. Then dPdσ(n)=q2∣a∣216π2ε0c3sin⁡2θ: when q≠0 and a≠0 the radiation pattern vanishes exactly along the instantaneous acceleration axis and is maximal in the perpendicular plane; when q=0 it vanishes in every direction; ∫S2dP/dσ dσ=Pem(s0). If a=0 all displayed radiation quantities vanish.

(e) [Scope and conventions] The result is exact at an emission event at which the charge is instantaneously at rest in the laboratory chart: then κ0(n)=1 for every n, so no retarded-time conversion factor appears and the displayed limits are simultaneously the fixed-sphere flux and the emitted power per unit emission time. The item uses only the prescribed worldline and the retarded model fields -- it is not a mechanical evolution law, does not assert a self-force or radiation reaction, derives no mass, and makes no empirical or measurement claim. For a general emission event the exact formula and its low-speed comparison are supplied by clause (f); 'slow' motion alone is never substituted for an error bound. The prescribed curve, the uniform subluminal bound and z′(s0)=0 are hypotheses; for a varying-velocity worldline the instantaneous rest event is a single parameter value, not an interval.

(f) [General low-speed branch] At any emission event, without imposing z′(s0)=0 for this clause, define emitted power by the weighted far-zone flux integral κ0(n) r2 n⋅S on the emitted spheres, with κ0(n)=1−n⋅β0, β0=z′(s0)/c, ∣β0∣≤v∗/c and γ0:=(1−∣β0∣2)−1/2. The same field formula and angular computation give Pem=γ06(∣a∣2−∣β0×a∣2)q26πε0c3. Put PL=q2∣a∣2/(6πε0c3). For ∣β0∣≤δ<1, PL≤Pem≤(1−δ2)−3PL,∣Pem−PL∣≤3δ2(1−δ2)−3PL. This includes q=0 or a=0 without division by PL. Uniform angular comparison is also explicit: if Nβ=n×((n−β0)×a), N0=n×(n×a) and Hβ=q2∣Nβ∣2/(16π2ε0c3κ05), H0=q2∣N0∣2/(16π2ε0c3), then ∣Hβ−H0∣≤q2∣a∣216π2ε0c3 δ[2+δ(1−δ)5+5(1−δ)6] for all n. The exact rest-event clauses (a)-(e) retain their hypotheses; this additional branch supplies the general low-speed comparison, not a mechanical loss law.

Facts & Assumptions

Given: ACω (The Axiom of Countable Choice (ACω)); the laboratory chart, units and constants of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields and Framework-local SI units, the vacuum constants and the exact/measured status of their values; a retarded point-geometry datum with the off-worldline retarded data s,r,n,β,κ,β˙ of Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline and the point charge parameter q, C=q/(4πε0); the retarded fields E,B of Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder with S=E×B/μ0; the rest event s0 with z′(s0)=0, a=z′′(s0), and in clause (f) a general emission event with β0=z′(s0)/c, ∣β0∣≤v∗/c, κ0(n)=1−n⋅β0.

[F1]

Lienard-Wiechert point fields: off the worldline E=Evel+Eacc with Evel=C(1−∣β∣2)(n−β)/(κ3r2), Eacc=C n×((n−β)×β˙)/(cκ3r), B=n×E/c, ∣Evel∣≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2; at an emission event (xr,tr)=(z(s0)+rn,s0+r/c) the retarded data are β0,β˙0=a/c,κ0 and r, and the same formulas and remainder bound hold there. (Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder (b),(c))

[F2]

Retarded emission geometry: (xr,tr) lies off the worldline, s(xr,tr)=s0, r>0, κ0=1−n⋅β0∈[1−v∗/c,1+v∗/c]. (Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline (b),(c))

[F3]

Sphere moments of the polar measure σ: ∫S2F(n3)dσ=2π∫−11F(u)du, ∫S2(n⋅a)f(n3)dσ=2πa3∫−11uf(u)du, ∫S2(n⋅a)2f(n3)dσ=2πa32∫−11u2f+π(a12+a22)∫−11(1−u2)f, and ∫S2(n⋅a)2dσ=(4π/3)∣a∣2, ∫S2∣n×a∣2dσ=(8π/3)∣a∣2, σ(S2)=4π. (Zonal and quadratic sphere moments for the polar surface measure on S2 (a)-(d))

[F4]

Cross-product and inner-product identities: u×v is bilinear and alternating, u×(v×w)=(u⋅w)v−(u⋅v)w, ∣n×(n×w)∣=∣n×w∣≤∣w∣ for ∣n∣=1, ∣u×v∣2=∣u∣2∣v∣2−(u⋅v)2, and n⋅(E×F)=(n×E)⋅F for ∣n∣=1; the Euclidean norm is that of The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn. (The cross product is bilinear, alternating, and orthogonal to both factors, The cross product in R3, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn)

[F5]

Flux and power reading: S=E×B/μ0 is the Poynting energy-flux density and the boundary flux term of the Poynting balance is the field energy leaving a volume. (Vacuum electromagnetic energy density and energy flux (the Poynting vector) (a), Local and fixed-volume electromagnetic energy balance (a),(c))

[F6]

Integral inequalities: ∣∫f∣≤∫∣f∣; monotonicity for the nonnegative integral; σ(S2)<∞. (The modulus of an integral is bounded by the integral of the modulus, Monotonicity and nonnegative homogeneity of the nonnegative integral, Zonal and quadratic sphere moments for the polar surface measure on S2 (d))

[F8]

SI relations: C=q/(4πε0), C2/(μ0c5)=q2/(16π2ε0c3), since ε0μ0c2=1. (Framework-local SI units, the vacuum constants and the exact/measured status of their values)

[F9]

One-variable calculus: the second fundamental theorem for continuous derivatives, the chain and power rules and the derivative of ym for integers m, and the mean value theorem; together with the continuity of the power functions on their domains. (The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a), The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a), 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, Continuity and derivatives of positive-base real powers, For a natural n≥1 the function x↦xn is differentiable everywhere with derivative ι(n) x n−1; for n=0 it is the constant 1, with derivative 0; for a natural n≥1 the function x↦x−n is differentiable at every x≠0 with derivative −ι(n) x−n−1; consequently every polynomial function is differentiable at every real, with the derivative computed term by term, The mean value theorem, as the case g(x)=x of Cauchy's: for f continuous on [a,b] with a<b and differentiable on (a,b) there is c∈(a,b) with f(b)−f(a)=f′(c)(b−a))

[F10]

The polar measure equals the chart surface measure on S2. (Agreement with the existing polar sphere measure)

[F11]

∣n⋅a∣≤∣a∣ for ∣n∣=1; cosine has range [−1,1] and is strictly decreasing on [0,π], with cos⁡0=1, cos⁡π=−1 and cos⁡(π/2)=0; sin⁡2θ+cos⁡2θ=1 and sine vanishes on [0,π] exactly at its endpoints. (The Cauchy-Schwarz inequality for finite sums, Intermediate value theorem, by bisection with a canonical left-half rule: a continuous function on [a,b] takes every value between f(a) and f(b), Signs, monotonicity intervals, and ranges of sine and cosine, Quarter-turn values and shifts by pi/2 and pi, Parity and the Pythagorean identity for sine and cosine, The zero sets of sine and cosine and the least positive common period 2 pi)

Proof

technique · direct; evaluate the rest-case field on the emitted sphere, convert the flux to the angular power density with the uniform remainder, integrate it with the sphere moments for the Larmor power and the $\sin^2$ pattern, and then repeat the computation for a general emission event with the weighted flux integral and explicit low-speed comparisons
1.1F1F2F8algebra

Field on the emitted sphere (a). At the rest event z′(s0)=0, so at the emitted sphere the retarded data are β=0, κ=1, β˙=a/c [F2]; [F1] then gives Evel=C(1−0)(n−0)/(1⋅r2)=Cn/r2 and Eacc=C n×((n−0)×a/c)/(c⋅1⋅r)=C n×(n×a)/(c2r), together with B=n×E/c. Writing ρE:=Cn/r2 gives E(xr,tr)=C n×(n×a)/(c2r)+ρE and ∣ρE∣=∣C∣/r2≤∣C∣(1+v∗/c)(1−v∗/c)−3r−2, because both factors in the last expression are at least 1. This is (a).

2.1step 1.1F3F4F6F10algebra

Angular flux limit (b). At the rest event the remainder is exactly ρE=Cn/r2 by step 1.1, so n×ρE=0 for either sign of C. The identity n⋅(E×(n×E))=∣n×E∣2 and B=n×E/c give n⋅S=∣n×E∣2/(μ0c). Thus ∣n×E∣=∣C∣ ∣n×a∣/(c2r) and, for every r>0, r2n⋅S(xr,tr)=C2∣n×a∣2μ0c5=C2∣n×(n×a)∣2μ0c5. The expression is independent of r and continuous in n, so its limit is uniform, and its sphere integral is finite by [F3, F6]. In particular the integral limit equals the integral of this density without a sign-dependent remainder estimate. The measures agree by [F10]. This proves (b) for all real charges, including q=0.

3.1step 2.1F3F4F8algebra

Total power (c). By [F4], ∣n×(n×a)∣2=∣n×a∣2=∣a∣2−(n⋅a)2; integrating over S2 with [F3] gives ∫S2∣n×(n×a)∣2dσ=4π∣a∣2−(4π/3)∣a∣2=(8π/3)∣a∣2. Substituting into step 2.1, Pem=C2μ0c5⋅8π3∣a∣2; and C2μ0c5=q216π2ε02μ0c5=q216π2ε0c3 by [F8] (using ε0μ0c2=1), so Pem=q2∣a∣26πε0c3. This is (c).

4.1step 2.1step 3.1F3F4F8F11algebra

Angular distribution (d). For a≠0 use the uniquely defined angle of (d), whose existence follows from the intermediate value theorem between the stated cosine endpoints and whose uniqueness follows from strict monotonicity [F11]. By [F4], ∣n×(n×a)∣2=∣a∣2−(n⋅a)2=∣a∣2(1−cos⁡2θ)=∣a∣2sin⁡2θ; since sin⁡2θ=0 exactly for θ∈{0,π} [F11], when q≠0 the pattern vanishes precisely along ±a and is maximal where sin⁡2θ=1, i.e. in the plane perpendicular to a; its coefficient is C2μ0c5=q216π2ε0c3 [F8]. If a=0 or q=0, the displayed density is zero for every n, so dP/dσ≡0 and Pem=0 by (c). Finally ∫S2dPdσdσ=Pem(s0) is (c). This is (d).

5.1step 2.1step 4.1F1F2F6F7algebra

General far-zone limit and weighted power (f, first part). Now let s0 be an arbitrary emission event with β0:=z′(s0)/c, ∣β0∣≤v∗/c, and a:=z′′(s0); the same computation as steps 1.1-2.1 applies with β0 in place of 0 and κ0 in place of 1 [F2]. By [F1], Elead:=C n×((n−β0)×a)/(c2κ03r) is the acceleration part and Evel is the remainder with ∣Evel∣≤DEr−2; writing Nβ:=n×((n−β0)×a) and repeating the flux identity of step 2.1, r2n⋅S=C2∣Nβ∣2μ0c5κ06+Rr(n) with ∣Rr(n)∣≤K′r−1 for r≥1, uniformly in n and with K′ independent of n; here 1−v∗/c≤κ0≤1+v∗/c keeps every power of κ0 bounded on the compact S2 [F2, F6]. Hence κ0(n) r2n⋅S→Hβ(n):=C2∣Nβ∣2μ0c5κ05 uniformly, and the weighted emitted power Pem:=∫S2κ0lim⁡r→∞(r2n⋅S) dσ=C2μ0c5∫S2∣Nβ∣2κ05 dσ is the dominated-convergence limit of the weighted fluxes, the weight κ0 being bounded and continuous [F6, F7].

6.1step 5.1F3F4F8F9F10algebra

Evaluation of the weighted angular integral (f, second part). By [F4], Nβ=(n⋅a)(n−β0)−(1−n⋅β0)a, so with b:=∣β0∣∈[0,v∗/c] and u:=n⋅β0/b (any unit vector e3 along β0 when b>0; the case b=0 is step 3.1) one gets ∣Nβ∣2=−(1−b2)(n⋅a)2+2(1−bu)b a∥(n⋅a)+(1−bu)2∣a∣2, where a∥ is the component of a along β0. Choose orthonormal spatial coordinates with third unit vector β0/b when b>0 (when b=0, choose any standard unit vector), and put a∥=a⋅e3 and a⊥=a−a∥e3; this coordinate change preserves the polar measure by [F10], and a⊥2 below abbreviates ∣a⊥∣2. Averaging the φ-dependence over the sphere with [F3] (the linear term in the tangential component of n integrates to 0, and the square of that component integrates to π∫(1−u2)f), the parallel coefficient of ∣Nβ∣2/(1−bu)5 reduces to 1−u2 and the perpendicular coefficient to (1−bu)2−1−b22(1−u2). Hence, with J5:=∫−11(1−u2)(1−bu)−5du and J3:=∫−11(1−bu)−3du, ∫S2∣Nβ∣2κ05dσ=2πa∥2J5+2πa⊥2[J3−1−b22J5]. The substitution y=1−bu (for b>0, with du=−dy/b) and the second fundamental theorem [F9], with the antiderivatives −y−2/2 and b−3[(1−b2)y−4/4−2y−3/3+y−2/2], give J3=2/(1−b2)2 and J5=4/(3(1−b2)3); at b=0 the same formulas follow by direct integration (J3=2, J5=4/3) and all expressions are continuous in b, so no division by b is needed in the conclusion. Therefore ∫S2∣Nβ∣2κ05dσ=8π3[a∥2(1−b2)−3+a⊥2(1−b2)−2]=8π3γ06(∣a∣2−∣β0×a∣2), because (1−b2)−1=γ02, (1−b2)−3=γ06 and ∣a∣2−∣β0×a∣2=a∥2+(1−b2)a⊥2 by [F4]. Substituting into step 5.1 and converting the constant with [F8] gives Pem=γ06(∣a∣2−∣β0×a∣2)q26πε0c3, the displayed general formula.

7.1step 6.1F2F4F9algebra

Uniform low-speed comparisons (f, third part). Write PL=q2∣a∣2/(6πε0c3) and Pem=γ06(a∥2+γ0−2a⊥2)q26πε0c3 [step 6.1]. Since γ0≥1, one has γ06a∥2≥a∥2 and γ04a⊥2≥a⊥2, so Pem≥PL; and γ06a∥2+γ04a⊥2≤γ06∣a∣2, so Pem≤γ06PL. If b=∣β0∣≤δ<1 then γ02=(1−b2)−1≤(1−δ2)−1, hence PL≤Pem≤(1−δ2)−3PL. Moreover Pem−PL=[(γ06−1)a∥2+(γ04−1)a⊥2]q26πε0c3≤(γ06−1)PL≤[(1−δ2)−3−1]PL≤3δ2(1−δ2)−3PL, where the last step is the elementary inequality (1−t)−3−1≤3t(1−t)−3 at t=δ2; all these inequalities are valid also when a=0 or q=0, with both sides zero, and no division by PL is performed. For δ=0 the angular densities coincide identically. For 0<δ<1, fix n and use coordinates with n=e3: writing p=(a1,a2), h=(β0,1,β0,2), t=a3 and β0,3, one has N0=−p and Nβ=−(κ0p+th) by [F4], so with D:=∣Nβ∣2κ0−5−∣N0∣2, D=∣p∣2(κ0−3−1)+2κ0−4t(p⋅h)+κ0−5t2∣h∣2. Since 1−δ≤κ0≤1+δ, the mean value theorem [F9] gives ∣κ0−3−1∣≤3δ(1−δ)−4 and ∣κ0−4∣≤(1−δ)−4, κ0−5≤(1−δ)−5; also ∣h∣≤δ and ∣p∣,∣t∣≤∣a∣, and 2∣t∣∣p∣≤∣t∣2+∣p∣2. Hence ∣D∣≤∣a∣2[4δ(1−δ)−4+δ2(1−δ)−5], and this is at most ∣a∣2δ[(2+δ)(1−δ)−5+5(1−δ)−6] because, after dividing by δ(1−δ)−4, the inequality reduces to 4−3δ≤2+δ+5(1−δ)−1, whose left side is at most 4 and whose right side exceeds 5. Multiplying by q216π2ε0c3 gives the displayed bound on ∣Hβ−H0∣.

8.1step 1.1step 3.1step 5.1step 7.1F2F5F10algebra∎

Scope and conclusion (e). At a rest event z′(s0)=0 one has κ0(n)=1−n⋅0=1 for every n∈S2 [F2], so the emission-time Jacobian is identically 1 and no retarded-time conversion factor appears: the limits of (b) are simultaneously the fixed-sphere flux and the emitted power per unit emission time, and the angular and total powers of (c)-(d) are the emitted quantities of the rest event. The computation used only the prescribed worldline, the retarded model fields and the adopted causal selection of Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder and Adopted retarded solution selection: the physical branch carries no incoming free field; it forms no product of distributions, asserts no self-force, radiation reaction, mass derivation or mechanical evolution law, and makes no empirical or measurement claim, while clause (f) records the general low-speed comparison as a separate quantified statement rather than a loss law. Steps 1.1-7.1 together with this clause prove (a)-(f).

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Relativistic emitted power of a prescribed point charge at a general emission event

Physical scope

Emitted power per unit emission time of a prescribed point charge at a general emission event on a uniformly subluminal C3 worldline: the κ-weighted far-zone flux, the closed form q2γ6(∣a∣2−∣β×a∣2)/(6πε0c3)=q2η(A,A)/(6πε0c3) and the uniform δ-comparison with the instantaneous-rest Larmor value. Excluded: dynamical evolution, self-force, radiation reaction, mass derivation, coordinate-time loss rates, uniformity in the emission event and every empirical or measurement claim.

Statement

Assume ACω as carried by the cited point-source suppliers. Let the setting be that of Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder: a charge q∈R (C:=q/(4πε0)) on a prescribed C3 uniformly subluminal worldline z in the laboratory chart of Laboratory geometry: a restricted inertial chart, its spatial slices and fixed-time fields with the units of Framework-local SI units, the vacuum constants and the exact/measured status of their values, with retarded fields E,B off the worldline and the uniform far-zone remainder of that item; let S:=E×B/μ0 (Vacuum electromagnetic energy density and energy flux (the Poynting vector)). Let s0 be an emission event, β0:=z′(s0)/c, γ0:=(1−∣β0∣2)−1/2, a:=z′′(s0), and for n∈S2 put xr:=z(s0)+rn, tr:=s0+r/c, κ0(n):=1−n⋅β0. Define the emitted power at the emission event s0 by the κ0-weighted far-zone flux

Pem(s0):=lim⁡r→∞∫S2κ0(n) r2 n⋅S(xr,tr) dσ(n),

dσ the polar surface measure (equal to the chart surface measure). The weight κ0 is the emission-time/observation-time conversion factor of the retarded root, ∂ts=1/κ, equivalently the moving-boundary correction S⋅n−(z′⋅n)u at leading radiation order, where u=∣S∣/c for the transverse far field. Then:

(a) [Weighted flux limit] The limit exists and Pem(s0)=C2μ0c5∫S2∣n×((n−β0)×a)∣2κ0(n)5 dσ(n).

(b) [Closed form and four-acceleration form] If b:=∣β0∣<1 and a=a∥e3+a⊥ is decomposed along β0=∣β0∣e3 and perpendicular to it, then Pem(s0)=q2γ066πε0c3(∣a∣2−∣β0×a∣2)=q26πε0c3 η(A,A), where A is the four-acceleration of the worldline at s0 and η(A,A)=γ04∣a∣2+γ06(β0⋅a)2=γ06(∣a∣2−∣β0×a∣2) (Norms of four-velocity and four-acceleration, and the observer rest-space decomposition(e)). At β0=0 the weight is 1 and (b) reduces to the instantaneous-rest Larmor power of Instantaneous-rest Larmor power and uniform low-speed comparison for a prescribed point charge.

(c) [Low-speed comparison] For every δ∈(0,1) and every emission event with ∣β0∣≤δ, q2∣a∣26πε0c3≤Pem(s0)≤(1−δ2)−3q2∣a∣26πε0c3,hence∣Pem(s0)−q2∣a∣26πε0c3∣≤3δ2(1−δ2)3q2∣a∣26πε0c3, a comparison uniform over the events with ∣β0∣≤δ. In particular the instantaneous-rest formula is the exact δ=0 case, and no term of the comparison is asserted to be small without the explicit hypothesis ∣β0∣≤δ.

(d) [Scope] Pem(s0) is the power emitted at the single retarded event s0 per unit emission time, defined by the weighted far-zone flux; it is not a coordinate-time loss rate of a dynamical particle, and no dynamics (self-force, radiation reaction, mass), no uniformity in s0, and no empirical or measurement claim is made. The near fields are O(r−2) with their uniform remainder as in Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder(c), so their contribution to the weighted r2 flux vanishes; the κ0-weighting is part of the definition of emitted power and is not an additional physical assumption.

Facts & Assumptions

Given: ACω (The Axiom of Countable Choice (ACω)); the setting of Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder: charge q, constant C, prescribed uniformly subluminal C3 worldline z, retarded fields E,B and S=E×B/μ0; an emission event s0 with β0=z′(s0)/c, γ0, a=z′′(s0), and the emission spheres xr=z(s0)+rn, tr=s0+r/c, κ0(n)=1−n⋅β0.

[F1]

Emitted-power branch: for a general emission event the κ0-weighted far-zone flux has the limit Pem(s0)=C2μ0c5∫S2∣n×((n−β0)×a)∣2κ0−5dσ (the uniform pointwise convergence and the interchange of limit and integral being established in its proof), and this equals γ06(∣a∣2−∣β0×a∣2)q2/(6πε0c3); for ∣β0∣≤δ<1 it satisfies PL≤Pem≤(1−δ2)−3PL and ∣Pem−PL∣≤3δ2(1−δ2)−3PL with PL=q2∣a∣2/(6πε0c3), and at β0=0 it reduces to the exact rest-event Larmor power. (Instantaneous-rest Larmor power and uniform low-speed comparison for a prescribed point charge (a)-(d),(f))

[F2]

Point fields and remainder: on Ω∖Γ, E=Evel+Eacc, B=n×E/c, with the velocity part O(r−2) bounded by ∣C∣(1+v∗/c)(1−v∗/c)−3r−2 and the acceleration part the leading term; at (xr,tr) the retarded data are those of the emission event and s(xr,tr)=s0. (Retarded point fields off the worldline: Lienard-Wiechert potentials, the velocity/acceleration split and the uniform far-zone remainder (b),(c), Complete retarded point fields: unique retarded root, the delta substitution with denominator 1−n⋅β, Liénard–Wiechert potentials and fields, and a uniform far-zone remainder (c),(d))

[F3]

Four-acceleration identity: for a C2 chart worldline t↦(ct,r(t)) with coordinate velocity w(t)=r′(t) and acceleration a(t)=w′(t), the four-acceleration satisfies η(A,A)=γw4∣a∣2+γw6(w⋅a)2/c2≥0, vanishing exactly when a=0. (Norms of four-velocity and four-acceleration, and the observer rest-space decomposition (e))

[F4]

Retarded root: ∂ts=1/κ off the worldline, and κ0(n)=1−n⋅β0∈[1−v∗/c,1+v∗/c]. (Uniformly subluminal prescribed worldline, retarded root and retarded geometric data off the worldline (a),(b))

[F5]

Conventions: ∣u×v∣2=∣u∣2∣v∣2−(u⋅v)2 with the Euclidean inner product; the polar measure equals the chart surface measure; ε0μ0c2=1 and C=q/(4πε0). (The cross product in R3, The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn, Agreement with the existing polar sphere measure, Framework-local SI units, the vacuum constants and the exact/measured status of their values)

[F6]

Flux reading and integral rules: S is the Poynting energy-flux density; ∣∫f∣≤∫∣f∣, monotonicity holds, and dominated convergence applies on the finite-measure sphere. (Vacuum electromagnetic energy density and energy flux (the Poynting vector), Local and fixed-volume electromagnetic energy balance, The modulus of an integral is bounded by the integral of the modulus, Monotonicity and nonnegative homogeneity of the nonnegative integral, Dominated convergence)

Proof

technique · direct translation of the emitted-power branch already proved on this page, together with the four-acceleration identity and the scope reading of the weighted definition
1.1F1F2F4F6algebra

Weighted flux limit (a). The definition of Pem(s0) in the Statement is the limit of the κ0-weighted far-zone fluxes, and the corresponding limit and its value C2μ0c5∫S2∣n×((n−β0)×a)∣2κ0−5dσ are exactly clause (f) of [F1], whose proof establishes the uniform pointwise convergence of κ0r2n⋅S to the displayed integrand and the domination needed to pass the limit through the sphere integral [F6]; the same clause uses κ0=1−n⋅β0 and r=c(tr−s0) on the emitted spheres [F2]. The interpretation of the weight as the emission-time/observation-time factor is ∂ts=1/κ of [F4], evaluated at the emission event, and the boundary-corrected reading of S⋅n−(z′⋅n)u is the leading-order form of that factor. This is (a).

2.1step 1.1F1F3F5algebra

Closed form and four-acceleration form (b). Clause (f) of [F1] evaluates the integral as γ06(∣a∣2−∣β0×a∣2)q2/(6πε0c3), which is the first displayed equality; at β0=0 the weight is 1 and the formula reduces to the rest-event Larmor statement of [F1]. For the four-acceleration form, apply [F3] to the chart worldline t↦(z(t),t): its coordinate velocity is w=z′(s0)=cβ0, its Lorentz factor is γw=γ0, and its coordinate acceleration is a=z′′(s0), so η(A,A)=γ04∣a∣2+γ06(cβ0⋅a)2/c2=γ04∣a∣2+γ06(β0⋅a)2. By [F5], γ04∣a∣2+γ06(β0⋅a)2=γ06[(1−∣β0∣2)∣a∣2+(β0⋅a)2]=γ06(∣a∣2−∣β0×a∣2), since ∣β0×a∣2=∣β0∣2∣a∣2−(β0⋅a)2. Hence Pem=q2η(A,A)/(6πε0c3). This is (b).

3.1step 2.1F1algebra

Low-speed comparison (c). The eventwise inequalities PL≤Pem≤γ06PL and the uniform bounds PL≤Pem≤(1−δ2)−3PL, ∣Pem−PL∣≤3δ2(1−δ2)−3PL for ∣β0∣≤δ<1 are clause (f) of [F1], transported verbatim to this setting; the case ∣β0∣=0 gives the exact rest formula and is the δ=0 endpoint of the comparison. The statement adds no smallness assertion beyond the explicit hypothesis ∣β0∣≤δ. This is (c).

4.1step 1.1step 3.1F2F4F6algebra∎

Scope (d). The definition is per unit emission time at the single event s0: the weight is the retarded Jacobian of [F4], not a dynamical rate, and no worldline evolution, self-force, radiation reaction or mass is introduced anywhere in steps 1.1-3.1. The near (velocity) part of the fields is O(r−2) with the uniform remainder of [F2], so its product contributions to S are O(r−3) and O(r−4), and after multiplication by r2 and integration over the compact sphere they contribute O(r−1) and O(r−2) respectively, vanishing in the limit; this is why the weighted definition isolates the acceleration-field radiation. The κ0-weighting is declared as part of the definition of emitted power, not inferred as a physical law, and no empirical or measurement content is added. This is (d).

RemarkRemark: AI-adaptedProof: Not applicableOpen item page →

Self-force, runaways and finite-size regularizations are not supplied by this page

Physical scope

Recorded scope limitations of the classical point-charge radiation model of this page: diverging electrostatic self-energy for stationary nonzero point charge, absence of a C1 sourced extension through an interior nonzero pure point-source worldline, undefined self-field/current products, prescribed-source-only emitted power per unit laboratory emission time without a supplied particle mechanical energy-loss law, and deferred finite-size and self-force dynamics. Excluded: any assertion, proof or measurement of radiation reaction, runaways, self-force dynamics or electromagnetic mass.

Remarks

Every cited conditional result retains its stated hypotheses. In particular, the point-source and causal-wave comparisons below assume Countable Choice (ACω, The Axiom of Countable Choice (ACω)) through their source suppliers; this qualification supplies no additional field or self-interaction model.

Record, with no speculative content, the limits of the radiation model built on this page.

(a) [Self-energy] For nonzero charge q≠0, the truncated electrostatic field energy of the stationary idealized point charge diverges as the inner cutoff is removed (Divergence of the point-charge field energy and the limits of mass inference): the point source's own field carries infinite energy in this framework's idealization, and any finite-energy treatment of a point-like charge requires modifying the source or the field near the singularity, or an explicit cutoff, none of which is supplied here. The q=0 branch has zero field energy and no divergence.

(b) [Undefined self-interaction; nonzero and zero source branches] The framework's source model Distributional Maxwell equations with point and stationary-sheet sources pairs distributions against compact smooth tests and expressly excludes arbitrary products of distributions. An explicit nonzero singular self-field is the stationary Coulomb field of The localized Newtonian potential and the ideal point-charge Coulomb field(d): for a constant trajectory z(t)=x0 and q≠0, ∣Eq(x)∣=∣q∣/(4πε0∣x−x0∣2) for x≠x0, which tends to infinity as x→x0. Its point-source charge distribution is supported on that stationary worldline. For q=0, the point-source pairings of Distributional Maxwell equations with point and stationary-sheet sources(b) give ρpt=Jpt=0 for every admitted trajectory; in the stationary Coulomb source-field branch, Eq=0 off x0 extends smoothly by zero, with B=0. Thus that zero-source branch has no self-field singularity and no nontrivial self-interaction. This states the source-field branch, not uniqueness among fields with an additional free field.

The moving pure point-source branch retains a precise general obstruction: if q≠0, z is an admitted C1 proper trajectory, and locally integrable fields satisfy the distributional Maxwell equations with exactly its point-source pair (Distributional vacuum Maxwell equations for the declared point and stationary-sheet sources, Distributional Maxwell equations with point and stationary-sheet sources(b),(e)), there is no C1 extension of the electric field through any interior worldline event that still satisfies those sourced equations. To see this, suppose such an extension exists near (x0,t0)=(z(t0),t0) and write g=div⁡E. Its distributional divergence is the regular distribution of this continuous g by Distributional differentiation is continuous and commutes, under the stated Countable Choice convention. On a fixed compact box inside that neighbourhood, ∣g∣≤M<∞ by A continuous real-valued function on a nonempty compact metric space is bounded and attains a greatest and a least value. Choose a spatial bump 0≤ϕr≤1, equal to one on Br/2(x0) and supported in Br(x0); continuity of z gives a time interval Jr about t0, inside that fixed box's time interval, with z(Jr)⊂Br/2(x0). Choose a nonzero nonnegative smooth temporal bump ηr supported in Jr, with Ar=∫ηr dt>0 (Compactly supported scaled Euclidean bumps). The compact smooth test ϕr(x)ηr(t) has charge pairing qAr, whereas its pairing with g has modulus at most M(2r)3Ar: the spatial support lies in the side-2r cube, and iterated integration of the continuous compactly supported integrand gives this bound (Riemann--Fubini on product rectangles, with lower and upper section integrals and content-zero exceptional sections, Riemann–Lebesgue comparison for distribution test integrands, If f≤g on [a,b] and both are integrable then ∫abf≤∫abg; and m(b−a)≤∫abf≤M(b−a)). The sourced Gauss identity would therefore give ∣q∣/ε0≤M(2r)3 for every sufficiently small r>0, an impossibility. This is a failure of a C1 sourced extension, not a claim that every moving field norm blows up; the explicit norm blowup above is the stationary Coulomb case.

For nonzero singular self-fields, evaluating the field on its own point-source support or forming its product with the distributional source is not supplied by these postulates. A vanishing component of the current does not remedy the singular charge-field product. More generally the prescribed moving-source framework supplies no arbitrary distribution-product operation, regularization or self-force equation; its emitted-power results below do not introduce one. No moving-source norm blowup is inferred from the stationary example, and no equation of motion is derived in either charge branch.

(c) [What the emitted-power items do and do not give] Instantaneous-rest Larmor power and uniform low-speed comparison for a prescribed point charge and Relativistic emitted power of a prescribed point charge at a general emission event are prescribed-source statements: they compute the emitted power of a stipulated worldline at a stipulated emission event, per unit laboratory emission time, using the retarded-time conversion factor in their weighted far-zone flux definition. At an instantaneous-rest emission event that factor is one, so the power also equals the fixed-sphere flux specified in Instantaneous-rest Larmor power and uniform low-speed comparison for a prescribed point charge(e). These results determine no worldline evolution, no back-reaction and no mechanical energy-loss rate of the particle; identifying the emitted power with such a loss rate requires an additional mechanical balance assumption.

(d) [Deferred, not claimed] Extended-charge or finite-size regularizations of the self-field, the well-posedness of any self-force dynamics, runaway solutions and an electromagnetic derivation of rest mass are outside this page and are neither stated nor proved here. No experiment, measurement, statistical estimate or precision is reported or implied, and nothing in this remark is a refutation of any physical theory.

5 · Examples, experiments and counterexamples

None yet.

Sources