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Particle spacetime, observers and worldlines — Examples

1 · Prerequisites

2 · Summary

These worked examples verify the page's conditional test-particle framework: flat manifolds can fail chronology or completeness, ideal-clock readings differ for the specified reunion paths, a null ray image does not fix momentum scale, and straight massive free motion has constant momentum and observer energy. They are mathematical constructions and model deductions, not reports of measurements.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

None yet.

5 · Examples, experiments and counterexamples

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

Flat local geometry without completeness

Physical scope

Explicit Lorentzian model manifolds illustrating that local flatness does not imply global causal regularity or geodesic completeness; these are mathematical countermodels, not claims about nature.

Example

Use SI length coordinates: θ,x1,x2,x3, the periods L,ℓ, and the affine parameters s below are measured in metres; the displayed metric has dimensionless components and its line element has units square metres. Thus the tangent dγ/ds is dimensionless with norm −1, while the physical four-velocity is c dγ/ds and the ideal proper-time increment is ds/c, with c in metres per second. For L,ℓ>0, consider the flat Lorentzian cylinder ML=(R/LZ)×R3 and the open slab Sℓ=(0,ℓ)×R3, each with metric −dθ2+∑i=13d(xi)2 and future direction ∂θ, where dθ is induced by the covering coordinate on R/LZ. The cylinder curve γ:R→ML, γ(s)=([s]L,0,0,0), is a closed future timelike geodesic. The slab contains a timelike geodesic defined on a finite affine interval that cannot be extended inside the slab. Thus locally Minkowski metrics need not preclude a closed future timelike geodesic or a finite-affine-interval geodesic that cannot be extended within its manifold.

Facts & Assumptions

Given: L,ℓ>0, the quotient cylinder and open slab with the displayed metric.

[F1]

The definition distinguishes a prescribed smooth Lorentzian background from any claim of completeness or global inertial structure (Particle spacetime, observers and worldlines).

[F2]

A geodesic is an affinely parametrized curve satisfying Dsγ′=0; in a chart with constant metric components, each coordinate line is an affine geodesic of the metric-selected connection (Geodesic of an affine connection, A chart with constant metric components has vanishing metric-selected Christoffel symbols and curvature).

Verification

1.1givenF1F2constructalgebra

The quotient coordinate [s]L has local lifts to real intervals; on every such chart the metric components are constant Minkowski components. The curve γ(s)=([s]L,0,0,0) is locally a coordinate line with tangent ∂θ, norm −1, and future sign. By [F2] it is a future timelike affine geodesic. Since γ(s+L)=γ(s), it is closed.

2.1givenF2constructalgebra∎

In the slab, β(s)=(s,0,0,0) for s∈(0,ℓ) is a vertical coordinate line with unit future timelike tangent; [F2] makes it an affine geodesic on this finite interval. If it extended continuously to s=0 as a curve in Sℓ, its first coordinate would have to equal 0, which is excluded from the slab; the same obstruction holds at s=ℓ. Therefore it cannot be extended within this manifold despite the locally constant metric.

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

Ideal-clock readings for a flat reunion path

Physical scope

Conditional ideal-clock calculation for two specified piecewise-inertial flat worldlines that reunite; it is a model prediction, not an experimental report.

Example

Choose an inertial frame (o;e0,e1,e2,e3) and its inertial chart χ from Inertial frames and inertial charts of the affine Minkowski model, with coordinates (x0,x1,x2,x3)=(ct,x,y,z). Use the flat specialization of the prescribed background: M=A with its affine smooth structure, g the metric induced by η on tangent vectors, and N=e0 the constant future time-axis field. Thus gab=diag⁡(−1,1,1,1) in χ. Let T>0 seconds and 0<v<c. A lab clock has chart path χ∘xL(t)=(ct,0,0,0) for 0≤t≤2T. A traveler has chart path χ∘xR(t)=(ct,vt,0,0) on [0,T] and χ∘xR(t)=(ct,v(2T−t),0,0) on [T,2T]. The traveler reverses direction at t=T and reunites with the lab at t=2T.

Facts & Assumptions

Given: The paths above, T>0, 0<v<c, and the ideal-clock adoption of Ideal clocks on a prescribed Lorentzian background.

[F1]

On a future timelike path, the adopted ideal-clock reading is dτ=c−1−g(T,T) ds (Ideal clocks on a prescribed Lorentzian background).

[F2]

For a piecewise-C1 future timelike worldline, proper-time increments are defined as the sum of the integrals over its pieces (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold).

Verification

1.1givenF1algebra

For the lab, dx0/dt=c and dx/dt=0, so −g(dx/dt,dx/dt)=c2 and the clock density is 1. Its elapsed reading is therefore ΔτL=2T.

2.1givenF1F2algebra∎

On either traveler leg, dx0/dt=c and ∣dx/dt∣=v, so −g(dx/dt,dx/dt)=c2−v2>0. The density is the constant 1−v2/c2 on both legs. Additivity across the single corner follows from the piecewise definition [F2], giving ΔτR=2T1−v2/c2<2T=ΔτL. This is a deduction from the ideal-clock model and specified paths, not a measured result.

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

One null ray with distinct momentum scales

Physical scope

Algebraic illustration of affine-parameter and momentum-scale freedom for a null test-particle ray; no scale is inferred from the unparameterized image.

Example

In a prescribed background, let I⊆R be a nonempty open interval and let x:I→M be an affinely parametrized nonzero future-null free geodesic with momentum P=dx/dλ. For any constant a>0, on the rescaled open interval I/a:={λ/a:λ∈I} the same ray image admits momentum Pa=aP using the affine parameter λa=λ/a.

Facts & Assumptions

Given: A null free trajectory from Free massive and null particle geodesics, a positive constant a, and, at any chosen λ0∈I, an observer n at the event x(λ0).

[F1]

A null free particle has dx/dλ=P and nonzero future-null momentum (Free massive and null particle geodesics).

[F2]

Observer energy is En(P)=−c g(P,n) (Mechanical momentum and observer energy).

Verification

1.1givenF1constructalgebra

Define xa(λa)=x(aλa). Then dxa/dλa=aP=:Pa, which remains nonzero future null. Since DλP=0, the constant rescaling also gives DλaPa=0; the image of xa equals the image of x. Thus both parameterizations satisfy the free null equations of [F1].

2.1step 1.1F2algebra∎

For any λ0∈I, the rescaled curve satisfies xa(λ0/a)=x(λ0) and Pa(λ0/a)=aP(λ0). For an observer n at this common event, [F2] gives En(Pa)=aEn(P). Hence the same unparameterized ray supports distinct positive momentum and energy scales; the path image alone does not select one.

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

Straight timelike free particle

Physical scope

Direct flat-space solution of the adopted free massive test-particle equation; the displayed trajectory and conserved quantities are model deductions, not reported observations.

Example

In the affine Minkowski model (A,V,η,C+), let p∈A, let U0∈V be future timelike with η(U0,U0)=−c2, and let m>0. The curve x:R→A, x(τ)=p+τU0, is a straight free massive trajectory.

Facts & Assumptions

Given: The flat affine model with background metric g=η, U0 and m as above. Choose an inertial frame (o;e0,e1,e2,e3) and its inertial chart; at each event of the curve let n=e0 under the canonical identification TqA≅V.

[F1]

The free massive equation is DτU=0 and its solutions are affine timelike geodesics (Free massive and null particle geodesics).

[F2]

The momentum and observer energy are P=mU and En(P)=−c g(P,n) (Mechanical momentum and observer energy).

[F3]

An inertial frame supplies an inertial chart and a future unit time-axis vector e0; the affine tangent-space identification makes this the same observer along the curve (Inertial frames and inertial charts of the affine Minkowski model, The tangent space of the affine Minkowski model at any event is canonically V).

[F4]

In the flat relativistic-particle model, the background metric used in the momentum and observer-energy definitions is g=η (Particle spacetime, observers and worldlines).

Verification

1.1givenF1algebra

Differentiating x(τ)=p+τU0 gives U=U0, which is constant in the flat affine connection. It is future timelike by assumption, and DτU=0, so it solves the free massive equation of [F1]. The mechanical momentum P=mU0 is also constant.

2.1step 1.1F2F3F4algebra∎

In the inertial chart of [F3], write U0=(U0,U). Since χ(x(τ))=χ(p)+τ(U0,U) and t=x0/c, the coordinate velocity is v=cU/U0. The norm gives (U0)2=c2+∣U∣2, while future direction gives U0>0, so ∣v∣<c. The observer n=e0 is fixed under the affine tangent identification; [F2] and [F4] therefore make En(P)=−cη(P,e0) constant because P is constant.

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