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Reduced-order LL local ODE and shell

1 · Prerequisites

2 · Summary

This page fixes a flat, prescribed-field Landau–Lifshitz reduction and proves local existence, uniqueness, and preservation of the future unit timelike shell for its explicit second-order ODE. It gives a uniform finite-interval residual estimate for LAD families that already satisfy specified small-defect and coefficient bounds, and a separate finite-time stability estimate for two specified Lipschitz second-order vector fields on a common compact phase region with the same initial data. Both results are conditional: neither constructs regular LAD families, compares an unrestricted third-order LAD solution to LL, or establishes global convergence.

The flat Lorentz–Abraham–Dirac equation is a separate adopted effective postulate. Neither equation is derived here from a coupled Maxwell point source, a finite-body limit, or an observation. The page does not evaluate a singular self-field at the particle worldline. Its SI tensor convention is inherited from rpm-external-charge, and the finite-body moment convention is available on rpm-spin-finite-size.

Prerequisite frameworks: rpm-spin-finite-size and rpm-external-charge.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

LemmaStatement: AI-adaptedProof: AI-adaptedverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

Reduced-order Landau–Lifshitz local ODE and mass shell

Physical scope

Mathematical local-existence and shell-preservation result for the explicitly displayed reduced-order vector field on flat affine Minkowski space. It asserts no global existence, physical truth, or approximation accuracy.

Statement

Let (A,V,η,C+) be an oriented, time-oriented affine Minkowski space of dimension four with signature (−,+,+,+), and fix an inertial chart (x0,x1,x2,x3) with x0=ct, c>0. Let O⊆A be open and let F be a C2 alternating covariant two-tensor on O. In this chart write Fab:=ηacFcb and let ∂b denote the coordinate partial derivative. Fix constants α∈R and τe≥0. For every U∈V, define

ΠUab:=δba+UaUbc2,f0a(x,U):=αFab(x)Ub,

Ba(x,U):=α(∂bFac)(x)UbUc+α2Fab(x)Fbc(x)Uc,aLLa(x,U):=f0a(x,U)+τeΠUabBb(x,U).

For the physical interpretation, xa are in metres, τ is in seconds, c is in metres per second, U is in metres per second, α=q/m, and τe is a time. Here a proper-time parameter means that the parameter is measured in seconds and the four-velocity is normalized by η(U,U)=−c2; define the future unit shell by S+:={U∈C+:η(U,U)=−c2}. For each initial datum (x0,U0)∈O×V with U0∈S+, the system

dxadτ=Ua,dUadτ=aLLa(x,U),(x(0),U(0))=(x0,U0)

has a unique local solution on an open proper-time interval about 0. Along that interval η(U,U)=−c2 and U remains future directed. This is a local ODE statement: it makes no claim of global existence for arbitrary F.

Facts & Assumptions

Given: The affine Minkowski and inertial-chart conventions above; O open; F∈C2; c>0; α∈R; τe≥0; and initial future unit timelike data.

[A1]

F is alternating, so Fab=−Fba, and the displayed field is the reduced-order LL vector field. The C2 hypothesis is used so its first derivatives are C1.

[F1]

Oriented time-oriented affine Minkowski space (the spacetime primitives): the affine metric has signature (−,+,+,+) and the time orientation selects a future timelike cone.

[F2]

Time orientation, future and past timelike/null/causal vectors, and the closed cones and Inertial frames and inertial charts of the affine Minkowski model: the future timelike cone is the convex component containing the frame’s future basis vector e0.

[F3]

Directional derivatives and partial derivatives of a map U⊆Rm→Rn: ∂b denotes the coordinate partial derivative in direction xb.

[F5]

Picard-Lindelöf local existence and uniqueness for first-order systems: a continuous locally Lipschitz vector field on an open Euclidean state domain has a unique local solution through each initial state.

Proof

1.1givenA1F3F4F5F6F7algebra

Antisymmetry gives η(U,f0)=αUaFabUb=0. On the unit shell, UaΠUab=Ub+(η(U,U)/c2)Ub=0, so η(U,aLL)=0. The coordinate right-hand side G=(U,aLL(x,U)) is C1 on the open state domain, identified by the inertial chart with an open subset of R8: F is C2, its partials [F3] are C1, and the remaining factors are polynomial in U, using [F4]. In any closed rectangular box in this domain, [F6] bounds all first coordinate partial derivatives of the eight components of G by a common constant D. For two states z,z′ in the box, change their coordinates one at a time; each intervening coordinate segment stays in the box, so [F7] gives ∣Gi(z′)−Gi(z)∣≤D∑j=18∣zj′−zj∣≤8D∥z′−z∥2 for each component i. Therefore ∥G(z′)−G(z)∥2≤8D∥z′−z∥2, proving that G is locally Lipschitz. Thus [F5] gives a unique local full-state solution through (x0,U0).

1.2givenA1F4F5algebra

For arbitrary U, antisymmetry gives η(U,f0)=0 and the projector formula gives η(U,ΠUB)=(1+η(U,U)/c2)η(U,B). Along the full solution put h(τ)=η(U,U)+c2; then h′(τ)=2η(U,aLL)=2τec2η(U,B)h(τ). The coefficient is continuous. The zero function solves this scalar linear IVP with h(0)=0, and the scalar vector field is locally Lipschitz in h because it is linear in that variable, so uniqueness [F5] gives h=0 on the full common interval. Thus the proper-time normalization η(U,U)=−c2 is preserved.

2.1givenF1F2F8step 1.2algebra∎

In the inertial frame of [F2], e0 has coordinates (1,0,0,0). For any future timelike W, convexity of C+ makes (1−s)e0+sW timelike for 0≤s≤1. A timelike vector cannot have zeroth component zero, since then its squared norm would be the nonnegative spatial norm square. If W0≤0, the continuous zeroth component along this segment takes the value zero by [F8], a contradiction; hence every future timelike vector has W0>0. Conversely, if W is timelike and W0>0, then W0>∣W∣ in this frame, and (1−s)e0+sW has time component 1−s+sW0>s∣W∣ for every 0≤s≤1. It is therefore timelike throughout and joins e0 to W, so W belongs to the same timelike component C+. Thus a timelike vector is future exactly when its zeroth component is positive. Along the solution, the preserved shell makes U timelike. Its initial vector is future, so U0(0)>0; if U0 became nonpositive, [F8] on the interval between that time and 0 would force a zero component, again impossible. Hence U remains future directed throughout the local interval. No continuation beyond this interval is asserted.

LemmaStatement: AI-adaptedProof: AI-adaptedverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

Conditional LAD-to-LL residual and finite-interval stability

Physical scope

Conditional finite-interval residual estimate for regular flat LAD families satisfying the stated small-defect and bounded-coefficient hypotheses, together with finite-time stability for two specified Lipschitz second-order vector fields on a common compact phase region with the same initial data. It proves neither existence of such LAD families nor convergence of LAD trajectories or global-in-time accuracy.

Statement

Use the flat definitions f0, B, and ΠU of Reduced-order Landau–Lifshitz local ODE and mass shell. Let I=[τ−,τ+] with τ−<τ+ be a common compact proper-time interval, and suppose each curve below is C3 on an open neighborhood of I. For each 0<ε≤ε∗, let xε:I→A be a curve in affine Minkowski space with Uε=x˙ε, aε=U˙ε, and η(Uε,Uε)=−c2. Let F be a fixed C2 two-form on a neighborhood of the curves, fix a constant αε∈R for each ε, and set f0,ε=αεF(Uε) and δε:=aε−f0,ε. Suppose every curve satisfies the flat LAD equation

aε=f0,ε+ε(a˙ε−η(aε,aε)c2Uε).

Use the Euclidean norm of inertial components and its induced operator norm. In the SI interpretation ε is a time and αε=q/m; all constants and field norms carry the corresponding units. Assume constants A,M,P,C0,C1≥0, independent of ε, satisfy on I

∣αε∣≤A,∥F∥op≤M,∥ΠUε∥op≤P,∥δε∥≤C0ε,∥δ˙ε∥≤C1ε.

Then throughout I,

∥aε−(f0,ε+εΠUεBε)∥≤P(C1+AMC0)ε2.

The estimate is conditional on the displayed common-interval and uniform bounds. It does not establish that regular LAD solutions satisfying them exist, nor does it imply global-in-time convergence.

For a separate finite-interval comparison, let d∈N with d≥1, let Ω⊆Rd×Rd be open in the topology of the usual Euclidean metric d2 on R2d, and let K⊆Ω be compact for that metric. Let T>0 and τe,C,L≥0. Fix positive coordinate scales sj for the 2d phase coordinates and define ∥ξ∥1:=∑j=12d∣ξj∣/sj for ξ∈R2d. In a dimensional application choose the position and velocity scales consistently with one fixed time unit, so the two blocks of the lifted vector fields below have the same rate units. All constants use these fixed scales; in particular L has units of inverse time, LT is dimensionless, and Cτe2 has the units of a phase-space rate. Let Aτe,A~τe:Ω→Rd be specified acceleration maps, and define the corresponding second-order phase vector fields

Xτe(q,v):=(v,Aτe(q,v)),X~τe(q,v):=(v,A~τe(q,v)).

All vector integrals in this comparison are taken componentwise as real Riemann integrals.

Assume that for all z,z′∈K,

∥Xτe(z)−Xτe(z′)∥1≤L∥z−z′∥1,∥X~τe(z)−X~τe(z′)∥1≤L∥z−z′∥1,

and that ∥Xτe(z)−X~τe(z)∥1≤Cτe2 for every z∈K. If z1,z2:[0,T]→K are restrictions of C1 maps on an open interval containing [0,T], solve z˙1=Xτe(z1) and z˙2=X~τe(z2) pointwise on [0,T], and satisfy z1(0)=z2(0), then

sup⁡0≤t≤T∥z1(t)−z2(t)∥1≤Cτe2TeLT.

This stability claim assumes both solutions exist on the full interval and remain in the stated common region. It concerns only the two specified second-order systems; it is not an existence or convergence claim for the third-order LAD equation.

Facts & Assumptions

Given: The flat LL definitions from Reduced-order Landau–Lifshitz local ODE and mass shell, a common compact interval, the stated C3 normalized curves, fixed C2 field, and all five uniform bounds. For the separate comparison, the phase space, common compact region, constants, vector fields, and solutions specified in the Statement.

[A1]

Each curve obeys the displayed LAD equation, with ε>0 serving as its radiation-time parameter.

[A2]

η(Uε,Uε)=−c2 throughout I; all derivatives below are ordinary proper-time derivatives in the flat inertial chart.

[A3]

For the comparison, d∈N, d≥1, Ω⊆Rd×Rd is open in the d2 topology, K⊆Ω is compact for d2, T>0, and τe,C,L≥0; fixed phase-coordinate scales determine the stated ℓ1 norm and the displayed fields Xτe,X~τe.

[A4]

Both fields are Lipschitz on K with constant at most L, and their difference is bounded there by Cτe2.

[A5]

The comparison curves are restrictions of C1 maps on an open interval containing [0,T], take values in K on [0,T], solve their respective displayed ODEs pointwise there, and have the same initial state; hence r(t)=∥z1(t)−z2(t)∥1 is continuous on [0,T].

[F1]

Reduced-order Landau–Lifshitz local ODE and mass shell: f0a=αFabUb, Ba=α(∂bFac)UbUc+α2FabFbcUc, and ΠUab=δba+UaUb/c2.

[F9]

The triangle inequality and the stated ℓ1 norm: applying ∣u+v∣≤∣u∣+∣v∣ to each scaled coordinate and summing gives ∥ξ+ζ∥1≤∥ξ∥1+∥ζ∥1.

Proof

1.1givenA1A2F1F2algebra

Differentiating η(Uε,Uε)=−c2 gives η(Uε,aε)=0. Differentiating this identity once more gives η(Uε,a˙ε)=−η(aε,aε). By [F1], ΠUεa˙ε=a˙ε+Uεη(Uε,a˙ε)/c2=a˙ε−η(aε,aε)Uε/c2. Therefore [A1] is exactly aε=f0,ε+εΠUεa˙ε.

1.2givenA3A4A5F3F4F6F8F9

Use the Euclidean phase-space and compact-region conventions of [F8] for the comparison data [A3]. Put δ:=Cτe2 and r(t):=∥z1(t)−z2(t)∥1. For each coordinate component j, set hj(t):=(z1−z2)j(t)−∫0t[Xτe(z1(s))−X~τe(z2(s))]j ds. The integrand is continuous because it equals z˙1,j−z˙2,j by the pointwise ODEs. By [F3], hj is continuous on [0,T], differentiable in its interior, and has derivative zero there. Equality of the initial data gives hj(0)=0. The mean value theorem [F6] on [0,t] therefore gives hj(t)=0 for each 0<t≤T, while this also holds at t=0. Consequently (z1−z2)(t)=∫0t(Xτe(z1(s))−X~τe(z2(s))) ds. Apply the scalar integral bound of [F4] to each component and add the finitely many inequalities using linearity; then split the integrand as Xτe(z1)−Xτe(z2)+Xτe(z2)−X~τe(z2). The field assumptions and [F9] give r(t)≤∫0t∥Xτe(z1(s))−X~τe(z2(s))∥1 ds≤L∫0tr(s) ds+δt.

2.1givenA2F1F2step 1.1

The product and chain rules [F2], with x˙=U and U˙=a, give f˙0,εa=αε(∂bFac)UbUc+αεFabaεb,Bεa=αε(∂bFac)UbUc+αεFabf0,εb. Subtracting the equalities and using δε=aε−f0,ε gives f˙0,ε−Bε=αεFδε.

2.2step 1.2A4F7

If L=0, step 1.2 gives r(t)≤δt≤δT=δTeLT by [F7].

2.3step 1.2A3A5F3

Suppose L>0 and define G(t):=δt+L∫0tr(s) ds. The function r is continuous, so [F3] applies; step 1.2 gives r≤G, while [F3] gives G′(t)=δ+Lr(t)≤δ+LG(t) for 0<t<T.

3.1givenA1F1step 1.1step 2.1algebra

Subtract f0,ε+εΠUεBε from the reformulated LAD equation in step 1.1. Since a˙−B=δ˙+(f˙0−B), step 2.1 yields aε−(f0,ε+εΠUεBε)=εΠUε(δ˙ε+αεFδε). Taking Euclidean norms and applying the assumed bounds gives at each τ∈I ∥aε−(f0,ε+εΠUεBε)∥≤εP(C1ε+AMC0ε)=P(C1+AMC0)ε2. The constants do not depend on ε or τ, so the estimate is uniform on I.

3.2step 2.3F5F6F7

Define H(t):=e−Lt(G(t)+δ/L). By [F5], [F7], and G′≤δ+LG from step 2.3, H′(t)=e−Lt(G′(t)−LG(t)−δ)≤0 on (0,T). For each 0<t≤T, the mean value theorem [F6] on [0,t] gives H(t)≤H(0)=δ/L, hence r(t)≤G(t)≤δ(eLt−1)/L.

4.1step 2.2step 3.2A4F6∎

For L,t>0, the mean value theorem and monotonicity of the exponential [F6] give eLt−1≤LteLt. Therefore step 3.2 yields r(t)≤δteLt≤δTeLT; the same bound holds at t=0 by r(0)=0. This proves the estimate in the L>0 case; together with step 2.2, it covers all L≥0. Substituting δ=Cτe2 gives the asserted uniform stability bound.

PostulateStatement: AI-adaptedProof: Not applicable‡ sources checked 2026-10-15Open item page →

Flat Lorentz–Abraham–Dirac effective equation

Physical scope

Adopted flat-space point-particle effective equation in a prescribed external field. It is a model postulate, not a derivation from a coupled Maxwell point source, finite-body limit, or observation; it asserts no solution existence or global accuracy.

Postulate

Restrict Charged and spinning test-body quantities to its flat affine Minkowski branch, with signature (−,+,+,+), proper time τ in seconds, future four-velocity U=dx/dτ satisfying η(U,U)=−c2, constant primitive m>0 in kilograms and nonzero charge q∈R in coulombs. Let the prescribed external electromagnetic two-form F be C2 on an open neighborhood of the worldline; use the component convention F0i=−Ei/c, Fij=ϵijkBk of The electromagnetic two-form, its observer decomposition and the four-current. Let a:=dU/dτ and

α:=q/m,τe:=q26πϵ0mc3>0,f0a:=αFabUb,

where ϵ0=(μ0c2)−1 follows Framework-local SI units, the vacuum constants and the exact/measured status of their values. Adopt the flat LAD effective equation

aa=f0a+τe(daadτ−ηbcabacc2Ua).

The derivative is the ordinary derivative in an inertial affine chart. Its dimensions are consistent: a and f0 are accelerations, the parenthesized term has acceleration per second, and τe is a time. This is an adopted effective model equation for sufficiently regular curves (at least C3); it is not asserted to be an exact law of nature, a point-source Maxwell construction, or a globally well-posed dynamics. In particular, no existence, uniqueness, stability, or empirical claim is part of this postulate.

At each proper-time value τ, define the particle's instantaneous rest frame to be the tuple (x(τ);e0,e1,e2,e3), where e0=U(τ)/c and (e1,e2,e3) is a positively oriented η-orthonormal basis of U(τ)⊥. This is a pointwise basis at the event x(τ), not one inertial chart along an accelerated curve; the rest-space norm is ∥v∥rest:=η(v,v) for v∈U(τ)⊥. Use of the equation as a reduced physical approximation carries the source's qualitative validity qualification that radiation reaction be small relative to the applied Lorentz force in this instantaneous rest frame. This postulate neither asserts that condition for arbitrary F nor supplies a numerical threshold; the qualification is not used to deduce the local ODE results or the force-free counterexample.

Facts & Assumptions

Given: The flat charged-body quantities and proper-time convention of Charged and spinning test-body quantities, the flat electromagnetic tensor sign convention of The electromagnetic two-form, its observer decomposition and the four-current, the SI definition of ϵ0 in Framework-local SI units, the vacuum constants and the exact/measured status of their values, and the additional smoothness and nonzero-charge restrictions explicitly stated above.

[A1]

Adopt the displayed third-order equation as a separate flat effective model postulate. Its validity as a physical approximation is not concluded here.

[F1]

Charged and spinning test-body quantities: the flat branch uses a prescribed two-form, constant primitive m,q, proper-time parameter, and η(U,U)=−c2.

[F2]

The electromagnetic two-form, its observer decomposition and the four-current: in the stated SI inertial chart F0i=−Ei/c and Fij=ϵijkBk.

[F3]

Framework-local SI units, the vacuum constants and the exact/measured status of their values: ϵ0=(μ0c2)−1; no numerical value or precision is assumed.

Adopted status

The equation is taken as a modeling premise. The source discussion motivates radiation-reaction modeling and order reduction but does not turn this postulate into an experimentally proved universal law. No self-field is evaluated at the worldline here.

RemarkRemark: Literature-sourcedProof: Not applicableverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

Self-force status and point-particle limits

Physical scope

Scope remark separating prescribed-field LL/LAD effective equations, finite-body moments and literature results for a specific shrinking-body family. It supplies no point-charge self-field, universal fixed-charge point limit, or quantitative global accuracy claim.

Remark

The present pair prescribes an external field and adopts the flat LAD equation as a separate effective model. It does not construct a coupled Maxwell field sourced by a point charge or evaluate a self-field on the worldline. Body moments and transport convention defines moments for a smooth finite body (and a local curved moment convention); its definitions do not assert a point limit or a self-force law.

Poisson, Pound, and Vega's §22.1 records the formal point-charge equations and the singularity of the field on the worldline; §§22.2–22.6 develop the electromagnetic field near the worldline, singular/regular field split, tail, and equation of motion, particularly §22.6. A self-force calculation therefore requires a specified regularization or extended-body limiting argument. Gralla, Harte, and Wald's conclusions are conditional on assuming a one-parameter family (Fμν(λ),Jμ(λ),TμνM(λ)) of exact solutions to Maxwell's equations, current conservation, and total stress-energy conservation, with the support/scaling hypothesis (i) of their §II and a field decomposition satisfying hypothesis (ii): a retarded self-field plus an external homogeneous Maxwell solution jointly smooth in λ and spacetime. In that scaling limit the body size, charge, and mass tend to zero while the charge-to-mass ratio has a finite limit; the paper does not construct such a family or a constitutive matter model. Under those assumptions, the leading motion is Lorentz-force motion and §IV derives the first-order correction, including self-force, electromagnetic-dipole, and spin terms. In §§V–VI the authors discuss and qualify a self-consistent reduction-of-order formulation; the reduced-order ALD case is tied to negligible spin and electromagnetic-dipole contributions. These conditional results do not establish an unrestricted fixed-charge point construction, arbitrary-duration global accuracy, or the physical truth of the separately adopted postulate Flat Lorentz–Abraham–Dirac effective equation.

Facts & Assumptions

Given: The finite-body moment definitions of Body moments and transport convention, the adopted-model status of Flat Lorentz–Abraham–Dirac effective equation, and the cited literature statements with the restrictions just summarized.

[F1]

Body moments and transport convention: the flat moments are defined by integrals of a smooth stress-energy tensor with spatially compact support; the local curved moments are also definitions, and the supplier explicitly asserts no slice independence or MPD equation.

[F2]

Flat Lorentz–Abraham–Dirac effective equation: LAD is adopted here as a prescribed-field effective equation, not derived by evaluating a Maxwell self-field on the worldline.

[L1]

Poisson, Pound, and Vega, §22.1 and §§22.2–22.6, review the formal point-charge equations, singular field, regular-field decomposition, and tail term, particularly in §22.6. Gralla, Harte, and Wald, §II, assumptions (i)–(ii), state the assumed family and support/field hypotheses; §IV gives the first-order correction, and §§V–VI discuss the qualified reduction-of-order formulation.

Proof

1.1F1

The flat moments and local curved moments in [F1] are definitions for smooth finite-body stress-energy data; the supplier explicitly says no slice-independence theorem or equation of motion is asserted. Thus these moment definitions alone do not specify a point-particle limit or a value of the self-field on the representative worldline.

2.1F2L1step 1.1∎

The LAD equation in [F2] is adopted for a prescribed external field and makes no source construction. Together with the restricted literature results [L1], this establishes the scope of this remark: those specific shrinking-body results do not convert the adopted postulate into an unrestricted fixed-charge point construction or arbitrary-duration global accuracy theorem. The historical source claims remain reports with their own hypotheses, not proofs supplied by this item.

5 · Examples, experiments and counterexamples

None yet.

Sources