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  • Literature-sourced: the exact statement appears in a cited source; only wording and notation differ.
  • AI-adapted: a semantically identical restatement of literature-sourced material, modulo indexing, notation, and boundary cases adopted by the library.
  • AI-generated: a genuinely novel statement formulated by AI, with no source for the claim itself.

These labels describe origin, not correctness: citations and verification chips remain separate evidence.

Connections And Free Fall

1 · Prerequisites

2 · Summary

This page supplies the connection, the geodesic theory and the free-fall postulate of the classical framework built on gr-tensors-and-observers. Everything on the page is stated for a time-oriented smooth Lorentzian four-manifold (M,g,N) in the sense of gr-framework-and-geometry; the first eight items are mathematics — complete conditional deductions from that structure — and the last three items are physics: one adopted postulate, one model-conditional theorem and one scope note. No item on this page reports a measurement or asserts that the model describes nature.

Proper time and four-velocity. A future timelike worldline is defined as a C1 or piecewise-C1 curve whose velocity, and whose one-sided tangents at piece endpoints, are future timelike; its proper-time density is −g(γ′,γ′)/c, with c>0 the unit-convention constant, and its four-velocity is the corresponding unit tangent (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold). The proper-time increment is proved to be independent of the admissible partition, additive over subintervals and strictly positive over nondegenerate parameter intervals; it is invariant under orientation-preserving reparametrization, the four-velocity satisfies g(U,U)=−c2 and dγ/dτ=U, and U reparametrizes the worldline by proper time (Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent).

The metric-selected connection. For the symmetric nondegenerate metric g there is exactly one torsion-free g-compatible affine connection: the construction is the Koszul form 2g(∇XY,Z)=K(X,Y,Z) in the three smooth vector fields, from which torsion freedom and metric compatibility are verified from the defining identities and uniqueness is derived; the same theorem extends the derivative to dual and tensor fields so that it commutes with contraction, satisfies the Leibniz rule and annihilates g and g−1 (Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields). Along a curve the covariant derivative satisfies the metric pairing identity; parallel sections exist and are unique, the transport map is a linear bijection preserving g, geodesic speed is constant so the causal character of a nonconstant geodesic cannot change, proper time is an affine parameter of a future timelike geodesic, and a reparametrization of a geodesic with nowhere-zero tangent preserves the geodesic equation exactly when it is affine. Constant geodesics remain constant under every reparametrization (Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed).

Geodesics and exponential coordinates. The geodesic initial-value problem has a unique maximal solution γp,v for every (p,v)∈TM; its flow domain is open with smooth evaluation map, the scaling relation γp,sv(t)=γp,v(st) holds, and the exponential map exp⁡p(v):=γp,v(1) is smooth on a star-shaped open domain with d(exp⁡p)0=id⁡TpM, so it is a local diffeomorphism at the origin (The geodesic initial-value problem and the exponential map of the metric-selected connection). The exponential coordinate chart ψp∘exp⁡p−1 then gives gab(p)=ηab, ∂agbc(p)=0 and Γabc(p)=0 at the point. In the exponential chart, a geodesic through p is the straight radial line while its initial vector remains in the chosen star-shaped domain; no claim is made for a later return to the chart after that vector leaves the domain. The theorem explicitly claims nothing at second order (Point-normal and exponential coordinate charts of the metric-selected connection).

Variational characterization and the radial maximum. For a C2 future timelike curve contained in one smooth chart domain and parametrized by proper time up to origin, consider C2 variations valued in that same chart domain, with fixed endpoints and future timelike fibers. The first variation of the length functional is computed under the integral sign, with Ds-Dt commutation and an integration by parts; using compactly supported bump variation fields one concludes that L′(0)=0 for every such variation if and only if Dtγ′=0, i.e. stationarity is exactly the geodesic equation in the given proper-time parameter (First variation of the length of a timelike curve: stationarity is the geodesic equation). The Lorentzian Gauss lemma gexp⁡pv(d(exp⁡p)vv,d(exp⁡p)vw)=gp(v,w) is proved from the two-parameter family F(s,r)=exp⁡p(sv(r)) and DsJ=DrT, and it yields the radial maximum: every piecewise-C1 future timelike curve from p to q in the exponential domain has length at most −gp(vq,vq), with equality exactly for monotone reparametrizations of the radial geodesic from p to q (The Lorentzian Gauss lemma and the radial maximum of proper time).

Adopted clock, free-fall and light-ray rules. The physical content of the page is one postulate (Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework): ideal clocks measure the proper time of their future timelike worldlines; an ideal freely falling massive test body has as worldline a future timelike geodesic of the metric-selected connection traversed with four-velocity U=dγ/dτ, g(U,U)=−c2; and an ideal light ray is a future null geodesic in the geometric-optics approximation. These clauses are adopted assumptions of the classical smooth model in the test-field regime, explicitly not derived from the geometry and not empirical results; they exclude self-force and radiation back-reaction, finite-size and tidal couplings beyond the test-body idealization, non-geometric-optics propagation, dispersion and dissipation, matter with non-negligible self-field, distributional or lower-dimensional sources, and quantum effects. From the free-fall clause and the uniqueness and maximality of geodesics it follows as a model-conditional theorem that the worldlines of two ideal freely falling massive test bodies released at the same event with the same four-velocity are restrictions of the same unique maximal timelike geodesic, independent of rest mass or other body parameters (The free-fall worldline of an ideal test body is determined by its initial event and four-velocity). The theorem uses no measured input and establishes nothing about bodies in nature; empirical comparisons of free-fall universality are separate source-backed observations with apparatus, calibration and uncertainty qualifications and are not recorded on this page.

Scope of the local-inertial reading. The final item separates the mathematics of normal coordinates from its physical reading (Scope of normal coordinates and of the local-inertial-frame reading): the identities gab(p)=ηab, ∂agbc(p)=0, Γabc(p)=0 are first order at a single event; they assert nothing about second derivatives, curvature or a neighborhood isometric to Minkowski space, they give no global inertial frame and no relation between the exponential charts at different points, and they are not an empirical equivalence-principle statement. The standard sources for the page are Carroll, Lecture Notes on General Relativity (Chs. 1-4), Reall, Part III General Relativity (§§3.1-3.4, 6.4) and Tong, General Relativity (§§1.1, 3.2-3.3); the harvest, locators and dispositions are recorded in the batch coverage file.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

DefinitionDefinition: AI-adaptedProof: Not applicableOpen item page →

Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold

Definition

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model) and let c>0 be a fixed real constant. All curves below take values in M; the physical reading of c, of a worldline as the history of a clock or body, and of the parameter values as times is not part of this definition and is adopted separately in the postulates of the framework.

(a) Regularity classes. Let I⊆R be an interval with nonempty interior (Intervals of R: the nine order-convex forms, nondegeneracy, and length) and let γ:I→M be a map. A chart representative of γ is the map x∘γ for a smooth chart (U,x) of M (Smooth manifolds and their smooth charts).

  • For k∈N0∪{∞} and an interior point t0∈I, the map γ is Ck at t0 when there is a chart representative x∘γ defined near t0 that is Ck there in the componentwise Euclidean sense. This condition is independent of the chart: on the overlap of two chart representatives the transition map is smooth and the chain rule applies (The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a), Cr and smooth maps between smooth manifolds). If t0∈I is an included endpoint of I, the coordinate representative and its derivatives through order k are continuous up to t0 on the relative interval I∩(t0−δ,t0+δ) for some δ>0, with derivatives at t0 taken one-sided. For k=∞ this holds at every finite order. Merely possessing a one-sided secant tangent, as defined next, does not by itself make a curve C1 at the endpoint. The map γ is Ck on I when it is Ck at every point of I.

  • Let b∈R and ε>0. A curve γ:(b−ε,b]→M has left tangent v∈Tγ(b)M at b when for one — equivalently every — chart (U,x) around γ(b), writing v=∑a=03va∂a∣γ(b) (Coordinate derivations form a basis of the tangent space), the difference quotients satisfy (xa(γ(t))−xa(γ(b)))/(t−b)→va as t↑b for a=0,1,2,3. A right tangent at the left end of a curve is defined analogously with t↓b. Chart independence is the one-sided chain-rule computation for the smooth transition maps (The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a)).

  • A curve γ:[a,b]→M with a<b is piecewise C1 when there is a finite partition a=s0<s1<⋯<sm=b such that for every i the restriction of γ to [si−1,si] is C1 up to its included endpoints in the one-sided sense above: in every endpoint chart its component derivatives on the open piece have continuous one-sided limits, agreeing with its endpoint derivatives. Equivalently each piece has a C1 extension to its closed parameter piece. In particular its right tangent at si−1 and left tangent at si exist. Such a partition is called admissible for γ. The piece extensions give continuity at the corners; no agreement of the two one-sided tangents at a corner is required.

(b) Velocity. If γ is C1 at an interior point t, its velocity γ′(t)∈Tγ(t)M is the derivation [f]↦(f∘γ)′(t) on smooth germs at γ(t), extending The velocity derivation of a smooth curve from smooth to C1 curves. Equal germ representatives agree along the curve near t, and the one-variable product rule proves the derivation identity. In a chart around γ(t) the velocity has the component expression

γ′(t)=∑a=03ddt(xa∘γ)(t) ∂a∣γ(t),

the coordinate expression of the derivation (Coordinate derivations form a basis of the tangent space). At an included endpoint of the domain, γ′ means the corresponding one-sided tangent of clause (a).

(c) Timelike worldlines. For k∈{1,2,3,…}∪{∞}, a Ck future timelike worldline is a Ck curve γ:I→M whose velocity γ′(t) is future timelike at every t∈I, in the sense of Timelike, null, spacelike and causal vectors of a Lorentz vector space and Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model: gγ(t)(γ′(t),γ′(t))<0 and gγ(t)(γ′(t),Nγ(t))<0. A piecewise-C1 future timelike worldline is a piecewise-C1 curve γ:[a,b]→M whose velocity at every point of each open piece and whose one-sided tangents at the two ends of each piece are future timelike; the definition is applied to a map on an arbitrary interval I with nonempty interior by requiring it on every compact subinterval of I. A future timelike velocity is in particular nonzero, so every future timelike worldline is regular.

(d) Proper time and length. Let γ:[a,b]→M be a piecewise-C1 future timelike worldline and let a=s0<s1<⋯<sm=b be an admissible partition. On each open piece (si−1,si) the function

hi(s):=−gγ(s)(γ′(s),γ′(s))

is continuous and strictly positive: it is a finite sum of products of continuous real functions in any chart around a point of the piece, as gab∘γ and the components of γ′ are continuous (A vector-valued function has a limit, or is continuous, if and only if each of its components does; with the algebra of continuous vector-valued functions, Sums, scalar multiples, products, absolute values, maxima, minima and quotients with nonvanishing denominator of continuous functions are continuous, as are constants, the identity and every polynomial function, Continuity of f:A→R at a point of A and on A: the ε-δ condition, its agreement with lim⁡x→cf(x)=f(c) at a limit point, and continuity at an isolated point), and the square root is continuous on (0,∞) (Rational powers ar of a positive base, Continuity and derivatives of positive-base real powers). The continuous one-sided limits of the component derivatives, required by the C1 extension of each piece, and continuity of g imply that hi tends to the norm of the corresponding endpoint tangent. The future timelike hypothesis on those tangents makes these limits strictly positive, and hi extends to a continuous function on [si−1,si]; hence it is Darboux integrable there (The lower and upper Darboux integrals of a bounded f on [a,b] as sup⁡PL(f,P) and inf⁡PU(f,P), Darboux integrability as their equality, and the notation ∫abf, A continuous function on [a,b] is Riemann integrable, by Heine-Cantor and Riemann's criterion). The proper-time increment of γ over [a,b] is

τ(b)−τ(a):=1c∑i=1m∫si−1sihi(s) ds,

and the Lorentzian length of γ over [a,b] is Lg(γ):=c (τ(b)−τ(a)). For a base point s0∈I the proper-time function τ:I→R of a future timelike worldline is the function with τ(s0)=0 and τ(s) equal to the increment from s0 to s when s>s0, and minus the increment from s to s0 when s<s0. That the increment is independent of the admissible partition, so that τ is well defined, and that it is invariant under increasing C1 reparametrization with strictly positive derivative (including one-sided endpoint derivatives), comparing the increment over the actual image interval, are proved in Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent ↗; the display is the value for any admissible partition.

(e) Four-velocity. Let γ be a piecewise-C1 future timelike worldline and let t be a parameter value at which γ is differentiable (interior point of a piece, or an included endpoint with its one-sided tangent). The four-velocity of γ at t is

U(t):=c γ′(t)−gγ(t)(γ′(t),γ′(t))∈Tγ(t)M.

By construction gγ(t)(U(t),U(t))=−c2, and γ′(t)=(−g(γ′,γ′)/c)U(t) with a strictly positive scalar factor. If U is written as the derivative of γ with respect to proper time, U=dγ/dτ, this is a statement proved in Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent ↗, not part of the present definition.

(f) Scope. Proper time, length and four-velocity are defined only for future timelike worldlines. A null or spacelike curve receives no proper time and no four-velocity from this definition, and no limiting or distributional extension of the square-root integrand to such curves is asserted. The parametrization of a worldline is part of the data and is arbitrary in this definition: no affine parameter, no geodesic equation, no completeness or extendability of the domain, and no measurement or clock reading is assumed. Null and spacelike regularity classes are not defined here beyond the general Ck and piecewise-C1 notions of clause (a), which make no causal requirement.

Remarks

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

Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent

Statement

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold and let c>0 (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model).

  1. Well-definedness and additivity of proper time. Let γ:[a,b]→M be a piecewise-C1 future timelike worldline (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold). Then the sum defining τ(b)−τ(a) is the same for every admissible partition of [a,b]; it is written 1c∫abh, where h is the piecewise-defined proper-time density. For every u∈(a,b), τ(b)−τ(a)=(τ(u)−τ(a))+(τ(b)−τ(u)). If a<b, the increment is strictly positive.

  2. Reparametrization and orientation, including subintervals. Let a′<b′ and let φ:[a′,b′]→[a,b] be C1 up to its included endpoints with nonzero derivative everywhere, including one-sided endpoint derivatives. Let γ~:=γ∘φ. Its derivative has constant sign and φ is a C1 diffeomorphism onto its actual image interval. If φ′>0, then γ~ is a piecewise-C1 future timelike worldline and τ~(b′)−τ~(a′)=τ(φ(b′))−τ(φ(a′)). This equals τ(b)−τ(a) when φ(a′)=a and φ(b′)=b. If φ′<0, then γ~ is a piecewise-C1 past timelike traversal. Its unsigned density h~=−g(γ~′,γ~′) obeys 1c∫a′b′h~=τ(φ(a′))−τ(φ(b′))>0, whereas the oriented original difference τ(φ(b′))−τ(φ(a′)) is negative. For endpoint-reversing φ(a′)=b, φ(b′)=a, the latter equals −(τ(b)−τ(a)). This negative oriented difference is not elapsed proper time for a future curve; parameter reversal reverses the causal direction. Non-surjective maps compare increments over their actual image interval, not over the whole original interval.

  3. Proper-time function and four-velocity. Let γ:I→M be a C1 future timelike worldline on an interval with nonempty interior and let τ be its proper-time function based at t0∈I (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold). Then τ is C1 on I with τ′(t)=1c−gγ(t)(γ′(t),γ′(t))>0, so τ is strictly increasing, and at every t∈I the velocity, proper-time density and four-velocity satisfy γ′(t)=τ′(t) U(t) and gγ(t)(U(t),U(t))=−c2. If τ is strictly increasing on I with image J, then the reparametrized curve γτ:=γ∘(τ∣I)−1 is a C1 future timelike worldline on J with γτ′(σ)=U(τ−1(σ)),g(γτ′(σ),γτ′(σ))=−c2. The same formulas hold piece by piece for a piecewise-C1 future timelike worldline, on each open piece and at its endpoints one-sided, with the two corner velocities kept distinct.

Facts & Assumptions

Given: A time-oriented smooth Lorentzian four-manifold (M,g,N), a real c>0, and the worldlines and maps named in the three claims.

[L1]

A future timelike worldline is a C1 (or piecewise-C1) curve whose velocity, and whose one-sided tangents at piece endpoints, are future timelike; the density on each open piece is h=−g(γ′,γ′)>0, and h extends continuously to the closed piece with strictly positive one-sided limits (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold).

[L2]

γ′=∑a(xa∘γ)′∂a in a chart; a strictly positive multiple of a future timelike vector is future timelike (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold, Timelike, null, spacelike and causal vectors of a Lorentz vector space, Coordinate derivations form a basis of the tangent space).

[L4]

If h is continuous on a closed subinterval [u,v] with u<v, then its integral function is differentiable there with derivative h (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 integral function F(x):=∫axf of an integrable f). If G is differentiable on [u,v] with integrable derivative G′, then ∫uvG′=G(v)−G(u) (The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a)).

[L5]

For a monotone C1 surjection φ with integrable derivative, ∫f(φ(t))∣φ′(t)∣dt=∫f(x)dx (Monotone change of variable for Riemann-integrable functions).

[L7]

Proof

technique · direct
1.1L1given

(Common refinement.) Let P={si} and P′={sj′} be admissible partitions of [a,b] for γ, and let Q be the partition whose nodes are the union of the two node sets, ordered increasingly. Then Q is an admissible partition: each interval of Q lies in an interval of P and in one of P′, hence inside one open piece of each of the two parametrizations, and γ is C1 there.

1.2L1L3construct

(The density is independent of the partition.) Define, for each interval [u,v] contained in the closure of one open piece of γ, the number H(u,v):=∫uvh, where h is the continuous positive extension of the density to [u,v] from [L1]; this is the Darboux integral of a continuous function (A continuous function on [a,b] is Riemann integrable, by Heine-Cantor and Riemann's criterion). If the nodes of a subpartition are inserted, [L3] gives additivity: H(u,v)=H(u,w)+H(w,v).

1.3L1L3algebra

(Strict positivity.) For a<b, choose an open piece (si−1,si) and a closed interval [u,v]⊆(si−1,si) with u<v. Fix the midpoint t∗=(u+v)/2. By continuity and h(t∗)>0, shrink the interval symmetrically about t∗ so that h≥m:=h(t∗)/2>0 on the resulting [u,v]; every lower Darboux sum of h on any partition refining {u,v} is at least m(v−u), since h≥m on [u,v] and h>0 elsewhere. Hence the lower integral, which equals the integral because h is integrable, is at least m(v−u)>0 (For bounded f on [a,b] and a partition P: the infimum mi and supremum Mi of f on the i-th subinterval, and the lower and upper Darboux sums L(f,P)=∑imiΔi and U(f,P)=∑iMiΔi, The lower and upper Darboux integrals of a bounded f on [a,b] as sup⁡PL(f,P) and inf⁡PU(f,P), Darboux integrability as their equality, and the notation ∫abf, If f≤g on [a,b] and both are integrable then ∫abf≤∫abg; and m(b−a)≤∫abf≤M(b−a)). Dividing by c>0 gives τ(b)−τ(a)>0 when a<b.

1.4L2L7construct

(Reparametrization: reduction to pieces.) By [L7], the continuous nowhere-zero derivative of φ has one strict sign; consider first φ′>0. The mean value theorem makes φ strictly increasing, and continuity makes its image exactly [α,β] with α=φ(a′)<β=φ(b′). Strict monotonicity gives continuity of its inverse: at each image value the images of nearby parameter endpoints bound a relative neighbourhood. Restrict γ to [α,β] and let P={si} be an admissible partition of that restriction; the preimages φ−1(si) form an admissible partition for γ~=γ∘φ: on each preimage interval (u,v)=φ−1(si−1,si) the curve γ~ is the composition of C1 maps and hence C1, with γ~′=φ′⋅(γ′∘φ) by [L7], a strictly positive multiple of a future timelike vector and therefore future timelike by [L2].

1.5L1L4L6algebra

(Derivative of the proper-time function.) Let γ:I→M be a C1 future timelike worldline and τ(t)=1c∫t0th its proper-time function, h continuous and positive on I. For each compact [u,v]⊆I, [L4] gives τ(v)−τ(u)=1c∫uvh; since h/c is continuous at every t∈I, the first fundamental theorem in the form τ′(t)=h(t)/c follows at every interior point, and one-sided at the endpoints. This is the displayed formula; it is >0 because h>0 and c>0.

2.1step 1.2L3algebra

(Partition independence.) Write the sum of the definition for P as ∑iH(si−1,si) and similarly for P′ and Q. Refining P to Q and applying additivity of step 1.2 to each interval of P split by the nodes of Q, the sum for P equals the sum over Q; the same holds for P′. Hence both sums equal ∑QH and the increment is independent of the admissible partition.

2.2L5L6step 1.4algebra

(Reparametrization: the integral identity.) On a piece (u,v) as in step 1.4, the density of γ~ equals φ′⋅−g(γ′∘φ,γ′∘φ)=φ′ (h∘φ) by bilinearity of the metric and φ′>0; it is continuous and positive on the closed piece. By [L5], ∫uvφ′ (h∘φ)=∫si−1sih. Summing over the finitely many pieces and dividing by c gives τ~(b′)−τ~(a′)=τ(β)−τ(α). At a piece endpoint the one-sided tangent of γ~ is φ′γ′ with the same one-sided value of φ′>0, hence future timelike, so γ~ is a future timelike worldline.

2.3step 1.5givenalgebra

(Four-velocity relation.) At every t∈I, by the definition of U and step 1.5, τ′(t)U(t)=h(t)c⋅cγ′(t)h(t)=γ′(t) and g(U(t),U(t))=c2 g(γ′,γ′)h(t)2=c2g(γ′,γ′)−g(γ′,γ′)=−c2. The same computation applies on each open piece and, by the continuous one-sided velocity and density extensions, at each included one-sided endpoint of a piecewise-C1 worldline; a corner retains its two separate values.

2.4L4L7step 1.3step 1.5construct

(Reparametrization by proper time.) By step 1.5, τ is C1, and its increments are strictly positive by step 1.3, so it is strictly increasing on I; let J:=τ(I) and ψ:=τ−1:J→I. At each interior σ∈J, [L7] applied to τ at t=ψ(σ) gives a C1 local inverse; injectivity identifies it with ψ. At an included endpoint, monotonicity first gives continuity of the inverse from that side: any relative neighbourhood of t has a strictly separated inner endpoint value under τ. For σ′→σ from that side, put t′=ψ(σ′); then t′→t and (ψ(σ′)−ψ(σ))/(σ′−σ)=(t′−t)/(τ(t′)−τ(t))→1/τ′(t). Continuity of τ′>0 makes the inverse derivative continuous up to that endpoint. Applying the same local inverse and endpoint reciprocal-quotient argument to φ, whose derivative is continuous and nowhere zero, also proves the C1 diffeomorphism-onto-image assertion in claim 2. Thus ψ is C1 on J in the stated one-sided sense and ψ′(σ)=1/τ′(ψ(σ)).

3.1step 1.2step 2.1algebra

(Additivity over a splitting.) Fix any u∈(a,b) and insert u into an admissible partition, giving nodes q0=a<⋯<qj=u<⋯<qn=b. By step 1.2 the total sum is ∑i=1jH(qi−1,qi)+∑i=j+1nH(qi−1,qi); after division by the fixed constant c, step 2.1 identifies these sums with the two subinterval increments. Thus τ(b)−τ(a)=(τ(u)−τ(a))+(τ(b)−τ(u)) for every such u.

3.2L2L5L7step 1.3step 2.2algebra

(Reversing orientation.) For φ′<0, use its image [α,β]=[φ(b′),φ(a′)]; the chain rule gives γ~′=φ′(γ′∘φ), a negative multiple of a future timelike tangent, hence past timelike. The closed-piece C1 extensions compose in the same way, including their distinct corner values. Bilinearity gives h~=∣φ′∣(h∘φ). Apply [L5] to the reversed endpoints on each piece and sum to get ∫a′b′h~=∫αβh>0. Meanwhile the signed original difference is τ(φ(b′))−τ(φ(a′))=τ(α)−τ(β)<0. If the image is the full interval [a,b], this is −(τ(b)−τ(a)). Thus the unsigned integral and oriented difference have different signs, as asserted; no proper-time function for a future curve is assigned a negative elapsed value.

4.1L2L7step 2.3step 2.4∎

(Velocity of the reparametrized curve.) For γτ=γ∘ψ and σ∈J, [L7] applied in a chart around γ(ψ(σ)) gives γτ′(σ)=ψ′(σ) γ′(ψ(σ))=γ′(ψ(σ))/τ′(ψ(σ))=U(ψ(σ)) by step 2.3. In particular g(γτ′,γτ′)=−c2 and γτ′ is future timelike, so γτ is a C1 future timelike worldline on J; for a piecewise C1 worldline the same construction applies on each closed piece using its one-sided inverse derivatives, with separate left and right velocities at a corner.

Remarks

TheoremStatement: AI-adaptedProof: AI-generatedprecheck passOpen item page →

Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields

Statement

Let M be a smooth four-manifold without boundary and let g be a smooth symmetric covariant 2-tensor field on M such that gp is nondegenerate at every p∈M (Smooth covariant 2-tensor fields on a smooth manifold). Assume ACω for the canonical tangent-bundle smooth structure (The Axiom of Countable Choice (ACω), A smooth vector field is a smooth section of the tangent bundle). For this general metric define ♭p(v):=gp(v,⋅), ♯p:=♭p−1, and gp−1(α,β):=gp(♯pα,♯pβ). Nondegeneracy makes ♭p injective and hence invertible between the four-dimensional tangent space and its dual. In a chart, gab are the entries of the inverse matrix of (gab). These definitions agree with The inverse metric, musical isomorphisms and index raising in its Lorentzian scope. Here and below repeated upper/lower indices are summed over 0,1,2,3. This holds in particular when (M,g,N) is a time-oriented smooth Lorentzian four-manifold and g is its metric (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model). For smooth local vector fields X,Y,Z put

K(X,Y,Z):=X(g(Y,Z))+Y(g(Z,X))−Z(g(X,Y))+g([X,Y],Z)+g([Z,X],Y)−g([Y,Z],X),

with brackets as in The Lie bracket of smooth vector fields.

(a) Existence and formulas. There is exactly one affine connection ∇ on M (Affine connection on a smooth manifold) satisfying

2g(∇XY,Z)=K(X,Y,Z)for all smooth local X,Y,Z.

It is torsion-free and g-compatible, so it is a metric-selected connection for (M,g), meaning torsion-free and satisfying Xg(Y,Z)=g(∇XY,Z)+g(Y,∇XZ) for smooth local fields (the conditions of Metric compatibility, torsion freedom and the metric-selected connection class extended here to nondegenerate g); in every smooth chart its Christoffel symbols are

Γabc=12 gad(∂bgdc+∂cgbd−∂dgbc),

with gad the inverse-metric components defined above (Christoffel symbols of an affine connection).

(b) Uniqueness. If an affine connection ∇′ on M is torsion-free and g-compatible, then ∇′=∇. Consequently the class LC⁡(M,g) of metric-selected connections has exactly one element; it is the Levi–Civita connection of g.

(c) Induced derivative on tensor fields. Let ∇∗ be the dual connection on T∗M and let the product connection of Product connection on tensor and hom bundles act on TsrM:=(TM)⊗r⊗(T∗M)⊗s, for integers r,s≥0, constructed by Finite tensor products of smooth vector bundles. A type (r,s) tensor at p is a multilinear map (Tp∗M)r×(TpM)s→R (A type (r,s) tensor on a finite-dimensional vector space); a smooth tensor field is a section with smooth coefficients in each local product frame. The empty product is the scalar line. Its chart components are Ta1⋯arb1⋯bs=T(dxa1,…,dxar,∂b1,…,∂bs), where dxa is dual to ∂a. This agrees with Tensor fields of type (r,s) on a Lorentzian four-manifold and their components in the Lorentzian case. Put Ta1⋯arb1⋯bs;c:=(∇∂cT)a1⋯arb1⋯bs. Then, in every smooth chart, for every smooth tensor field T of type (r,s),

Ta1⋯arb1⋯bs;c=∂cTa1⋯arb1⋯bs+∑i=1rΓaidc Ta1⋯d⋯arb1⋯bs−∑j=1sΓdbjc Ta1⋯arb1⋯d⋯bs,

where the slot marked d replaces the named index; this derivative commutes with every contraction in the sense of The contraction of a mixed tensor, and it annihilates the metric and the inverse metric:

gab;c=0,gab;c=0.

Facts & Assumptions

Given: A smooth four-manifold M without boundary, a smooth symmetric nondegenerate covariant 2-tensor field g, and smooth vector fields X,Y,Z.

[L1]

An affine connection assigns ∇XY to smooth vector fields and is real-bilinear, function-linear in X, and satisfies ∇X(fY)=X(f)Y+f∇XY (Affine connection on a smooth manifold). Torsion is T(X,Y)=∇XY−∇YX−[X,Y] and g-compatibility is X(g(Y,Z))=g(∇XY,Z)+g(Y,∇XZ) (Torsion tensor of an affine connection and the Statement).

[L2]

Smooth vector fields act as derivations of C∞(M); the bracket satisfies [X,fY]=f[X,Y]+X(f)Y and [fX,gY]=fg[X,Y]+f(Xg)Y−g(Yf)X, and is itself a smooth vector field with coordinate formula [X,Y]j=∑i(Xi∂iYj−Yi∂iXj) (A vector field acts as a derivation of smooth functions, Leibniz rules for the Lie bracket with function multiples, The Lie bracket of smooth vector fields, Coordinate formula for the Lie bracket, Smoothness of a vector field is equivalent to smooth coordinate components).

[L3]

The pairing g(V,W) of smooth local fields is smooth because in a chart it is a finite sum of products of smooth components. Symmetry and nondegeneracy are those of Smooth covariant 2-tensor fields on a smooth manifold; the flat isomorphism defined in the Statement identifies each linear functional with gp(v,⋅) for a unique v.

[L4]

In a chart, the coordinate derivations ∂a form a basis of TpM at every p of the chart, and smooth vector fields are exactly those with smooth coordinate components; the Christoffel symbols are the smooth functions with ∇∂b∂c=∑aΓabc∂a (Coordinate derivations form a basis of the tangent space, Smoothness of a vector field is equivalent to smooth coordinate components, Christoffel symbols of an affine connection).

[L5]

In a chart the inverse matrix satisfies gacgcb=δab. Its entries are Cm for every finite m≥1 by Matrix inversion preserves Ck regularity where the determinant is nonzero, applied to the smooth coordinate representative with nonzero determinant; thus they are smooth. Evaluating the compatibility identity of [L1] on coordinate fields gives ∂agbc=∑d(Γdabgdc+Γdacgbd) whenever compatibility holds. In the time-oriented Lorentzian specialization, Torsion freedom and metric compatibility in chart components supplies the equivalence with this chart identity; its narrower interface is used only for that specialization.

[L6]

The dual connection is characterized by (∇X∗ω)(Y)=X(ω(Y))−ω(∇XY), and the product connection on tensor bundles extends the connections on the factors by the Leibniz rule and is uniquely determined by it (Dual connection, Product connection on tensor and hom bundles).

[L7]

The general tensor bundles and their smooth product frames are those of the Statement and Finite tensor products of smooth vector bundles. Contraction is the sum of evaluations against a basis and its dual (The contraction of a mixed tensor). Under a basis change ei′=∑jBjiej, e′i=∑k(B−1)ikek, the summed coefficient is ∑iBji(B−1)ik=δjk, proving basis independence. In product frames the contracted coefficients are finite sums of smooth coefficients, so contraction is smooth.

Proof

technique · direct
1.1L2L3algebra

The functional K is additive in each of its three arguments, and expanding its six terms with [L2] gives the three scalar rules K(fX,Y,Z)=fK(X,Y,Z),K(X,Y,fZ)=fK(X,Y,Z), K(X,fY,Z)=fK(X,Y,Z)+2X(f)g(Y,Z) for every smooth function f: in the first, the terms containing Y(f) and Z(f) produced by [fX,Y] and [fZ,X] cancel against the derivative-of-f terms in Y(g(Z,fX)) and −Z(g(fX,Y)); in the second, the derivative terms cancel in pairs by symmetry of g; in the third, the terms X(f)g(Y,Z) occur twice and all other derivative terms cancel.

2.1step 1.1L3L4algebra

Work with smooth local fields on each open chart domain and its overlaps. For fixed smooth X,Y, the rule of step 1.1 and bilinearity of g show that the equation 2g(V,Z)=K(X,Y,Z) for all smooth Z is equivalent, in a chart, to the single set of identities 2g(V,∂c)=K(X,Y,∂c) for c=0,1,2,3: writing Z=∑cZc∂c on the chart gives K(X,Y,Z)=∑cZcK(X,Y,∂c).

3.1step 2.1L3L4L5algebra

In each smooth chart (U,x) put VU:=12∑a,bgabK(X,Y,∂b) ∂a, a smooth field on U; by step 2.1 and gacgab=δcb it satisfies 2g(VU,∂c)=2∑bgacgab12K(X,Y,∂b)=K(X,Y,∂c) for every c, hence 2g(VU,Z)=K(X,Y,Z) for every smooth Z on U. If (U,x) and (U′,x′) overlap, then g(VU−VU′,Z)=0 for every smooth Z there, so VU=VU′ pointwise by nondegeneracy; the local fields therefore patch to one smooth vector field ∇XY on M with 2g(∇XY,Z)=K(X,Y,Z) for all Z.

4.1step 3.1L1L3algebra

∇ is an affine connection. Additivity and real homogeneity in X and in Y hold termwise for K; scalar linearity in X is K(fX,Y,Z)=fK(X,Y,Z); and 2g(∇X(fY),Z)=K(X,fY,Z)=fK(X,Y,Z)+2X(f)g(Y,Z)=2g(X(f)Y+f∇XY,Z) for all Z, so ∇X(fY)=X(f)Y+f∇XY by nondegeneracy.

4.2step 3.1L1L2L3algebra

Torsion vanishes. Subtracting the definitions of K(X,Y,Z) and K(Y,X,Z) and using symmetry of g and skew-symmetry of the bracket cancels the X,Y,Z-derivative terms and the four bracket terms except g([X,Y],Z)−g([Y,X],Z)=2g([X,Y],Z); hence 2g(∇XY−∇YX−[X,Y],Z)=K(X,Y,Z)−K(Y,X,Z)−2g([X,Y],Z)=0 for all Z, and T(X,Y)=∇XY−∇YX−[X,Y]=0 by nondegeneracy.

4.3step 3.1L1L2L3algebra

Metric compatibility holds. Adding K(X,Y,Z) and K(X,Z,Y) cancels the Y- and Z-derivative terms by symmetry of g and cancels the bracket terms by skew-symmetry, leaving K(X,Y,Z)+K(X,Z,Y)=2X(g(Y,Z)); dividing by two and using the defining property of ∇ gives X(g(Y,Z))=g(∇XY,Z)+g(Y,∇XZ).

4.4step 3.1L1L3algebra

Any torsion-free g-compatible connection ∇′ satisfies 2g(∇X′Y,Z)=K(X,Y,Z). Indeed, compatibility applied to the three pairings and torsion freedom written as [X,Y]=∇X′Y−∇Y′X, [Z,X]=∇Z′X−∇X′Z, [Y,Z]=∇Y′Z−∇Z′Y turn the six terms of K(X,Y,Z) into ∇′-terms in which g(∇X′Y,Z) occurs twice and every other term cancels in pairs. Hence ∇′=∇ by the displayed defining property and nondegeneracy, proving claim (b) and the uniqueness assertion of (a).

4.5step 3.1L2L4L5algebra

In a chart, the brackets of coordinate fields vanish by [L2], so evaluating K on coordinate fields with [L2] and [L4] gives K(∂b,∂c,∂a)=∂bgca+∂cgba−∂agbc; substituting ∇∂b∂c=∑eΓebc∂e into step 3.1 gives ∑egeaΓebc=12(∂bgca+∂cgba−∂agbc) and multiplying by gad gives the displayed Christoffel formula, whose right side is smooth by [L5].

5.1step 4.5L4L6algebra

(Dual and tensor components.) The dual connection of [L6] is a connection on T∗M, and its components are (∇a∗ω)b=∂aωb−∑dΓdabωd: with ω=∑bωbdxb, the characterizing identity gives (∇∂a∗ω)(∂b)=∂aωb−ω(∇∂a∂b)=∂aωb−∑dΓdabωd.

6.1step 4.5step 5.1L4L6L7algebra

The product connection of [L6] extends ∇ and ∇∗ to all tensor bundles and satisfies the Leibniz rule on tensor products. Its two elementary values are ∇∂c∂b=∑dΓdbc∂d and ∇∂cdxa=−∑dΓadcdxd: the second follows from step 5.1 and dxa(∂b)=δab. Expanding a smooth tensor field T in the coordinate product frame as T=∑Ta1⋯arb1⋯bs ∂a1⊗⋯⊗dxb1⊗⋯ and applying the Leibniz rule, exactly one +Γ term appears for each upper slot and one −Γ term for each lower slot, and the coefficient derivative ∂cT⋯ appears once; this yields the displayed component formula, the sum over d replacing the slot index.

7.1step 6.1L7algebra

The induced derivative commutes with contraction. Let T be of type (r,s) with r,s≥1, contract one upper slot ai with one lower slot bj, and contract the derivative in the same slots. The +Γ term for the upper slot contributes ∑dΓdecT⋯e⋯⋯d⋯ and the −Γ term for the lower slot contributes −∑dΓedcT⋯d⋯⋯e⋯; relabelling the dummy indices (d,e)↦(e,d) in the second sum makes the two contributions equal and opposite, while the remaining terms are exactly the derivative of the contracted components by step 6.1. Summing over d is a finite index sum, so both orders give the same smooth function.

8.1step 6.1L5algebra∎

The metric and inverse metric are annihilated. By step 6.1 with T=g, writing the two lower slots explicitly, gab;c=∂cgab−∑dΓdacgdb−∑dΓdbcgad=0 by the compatibility identity of [L5]. Differentiating gadgdb=δab in the direction ∂c and substituting the compatibility identity gives ∂cgaf+∑dΓfdcgad+∑dΓadcgdf=0, which is gaf;c=0 by step 6.1. This proves claim (c) and completes the proof.

Remarks

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

Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed

Statement

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold and let ∇ be its metric-selected connection; its existence and uniqueness are supplied by Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields. Fix c>0. All intervals I,J below have nonempty interior. For a smooth curve γ:I→M write Dt for the covariant derivative along γ of Covariant derivative along a curve with respect to ∇ (equivalently, the pullback of the Levi–Civita connection).

  1. Metric pairing. For smooth sections V,W of the pullback bundle γ∗TM, ddt gγ(t)(V(t),W(t))=gγ(t)(DtV(t),W(t))+gγ(t)(V(t),DtW(t)). In particular, if DtV=DtW=0 on I, then g(V,W) is constant on I.

  2. Parallel transport. Let γ:[a,b]→M be a piecewise smooth curve with a<b. For every v∈Tγ(a)M there is exactly one continuous piecewise smooth section V of γ∗TM with DtV=0 on each smooth piece and V(a)=v; the parallel-transport map Pγ:Tγ(a)M→Tγ(b)M, v↦V(b), is linear, bijective, and satisfies gγ(b)(Pγv,Pγw)=gγ(a)(v,w) for all v,w. For a=b, the unique section is its prescribed fibre vector and Pγ is the identity; no Dt condition is imposed on a singleton.

  3. Geodesic speed and proper time. Along a geodesic γ:I→M (Geodesic of an affine connection) the function t↦gγ(t)(γ′(t),γ′(t)) is constant. If γ is nonconstant, its tangent is nowhere zero and its causal character (timelike, null or spacelike) is constant; a constant geodesic has zero tangent and is assigned none of those causal characters. If γ is a future-directed timelike geodesic and g(γ′,γ′)=−λ2 with λ>0, then for t0<t1 its proper-time increment over [t0,t1] is λ(t1−t0)/c (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold), so proper time is an affine parameter. In this parameter its four-velocity is U=(c/λ)γ′ and is parallel: DτU=0. Proper time is not assigned to a past-directed curve by that definition; reversing the parameter gives a future-directed timelike geodesic with the same (positive) proper-time magnitude. A nonconstant null geodesic has null tangent and admits no proper-time parametrization.

  4. Affine reparametrizations. Let γ:I→M be a geodesic whose tangent is nowhere zero, and let h:J→I be a C2 diffeomorphism onto its open image with h′≠0. Then γ∘h is a geodesic if and only if h(s)=as+b with constants a≠0, b; in that case a is the constant h′, and every affine parameter of this nonconstant geodesic arises in this way from a fixed one. If γ is constant, then γ∘h is constant and hence geodesic for every such h; no affine restriction on h follows.

Facts & Assumptions

Given: A time-oriented smooth Lorentzian four-manifold (M,g,N) with its metric-selected connection ∇, a smooth curve γ:I→M, and the sections and maps named in the claims.

[L1]

The covariant derivative along a smooth curve is defined by the pullback connection, satisfies Dt(fV)=f′V+fDtV for functions f of the parameter, and if V=s∘γ for a local ambient section s then DtV=(∇s)γ(t)(γ′(t)) (Covariant derivative along a curve, Covariant derivative along a curve is independent of frame and extension).

[L2]

In a chart, ∇∂b∂c=∑aΓabc∂a, ∇ is torsion-free and g-compatible, and ∂agbc=∑d(Γdabgdc+Γdacgbd) (Christoffel symbols of an affine connection, Metric compatibility, torsion freedom and the metric-selected connection class, Torsion freedom and metric compatibility in chart components).

[L3]

A geodesic is a curve with Dtγ′=0 in its parameter; such a parameter is called affine; constant curves are geodesics (Geodesic of an affine connection).

[L4]

For a piecewise smooth curve there is exactly one continuous piecewise parallel section through every initial vector; its value at the terminal parameter is the parallel transport of Parallel transport along a piecewise smooth curve, and the construction is independent of frames and subdivisions (Parallel section along a curve, Existence and uniqueness of parallel sections, Covariant derivative along a curve).

[L5]

Along a future timelike worldline, proper time has density −g(γ′,γ′)/c, and the four-velocity satisfies U=cγ′/−g(γ′,γ′), γ′=τ′U, g(U,U)=−c2 (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold, Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent).

[L6]

A nonzero causal vector is future-directed exactly when its pairing with the time-orientation field N is negative, and that pairing is nonzero (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model, Timelike, null, spacelike and causal vectors of a Lorentz vector space). Along a continuous nonzero timelike tangent on the connected interval I, this pairing is continuous and cannot change sign, so being future-directed at one parameter value makes it future-directed throughout. The zero vector has no causal character; a nonzero vector of zero norm is null (Timelike, null, spacelike and causal vectors of a Lorentz vector space).

[L7]

A differentiable real function on an interval with zero derivative is constant (A function continuous on an interval I whose derivative vanishes at every interior point of I is constant on I; consequently two such functions with the same derivative differ by a constant), applied on compact subintervals and extended to included endpoints by continuity. Applied to chart components, this also makes a curve with zero velocity locally constant and hence constant on its connected interval.

Proof

technique · direct
1.1L1L2algebra

(Component form of Dt.) On a chart domain around a parameter value, let ea:=∂a∘γ be the pulled-back coordinate frame and write γ′=∑bγ˙beb, V=∑aVaea, with coefficient functions Va on the parameter interval. By [L1], Dtec=(∇∂c)γ(t)(γ′(t))=∑a,bΓabcγ˙bea. The pullback product rule therefore gives DtV=∑a(∂tVa+∑b,cΓabcγ˙bVc)ea. This uses ambient extensions only for the coordinate frame, not for the arbitrary coefficient functions along the curve, and hence also applies to repeated points and constant base curves. The same formula and pairing calculation hold for C1 fields along a C1 curve, with the derivatives interpreted at included endpoints one-sided.

2.1step 1.1L2L7algebra

(Metric pairing.) With the notation of step 1.1, g(V,W)=∑a,bgabVaWb, so ddtg(V,W)=∑a,b(∂cgabγ˙cVaWb+gab∂tVaWb+gabVa∂tWb). Substituting the compatibility identity of [L2] for ∂cgab and the component formula of step 1.1 for DtV and DtW, the terms in which Γ multiplies V or W match, using symmetry gab=gba and the relabelling of the summed indices b,c,d; the remaining terms are exactly the two derivatives ∂tVaWbgab and Va∂tWbgab. Hence the displayed pairing identity holds; if DtV=DtW=0, the derivative of the smooth function g(V,W) vanishes on each chart, hence on I; [L7] gives constancy.

3.1step 2.1L4L7algebra

(Parallel transport.) On a singleton, [L4] and the transport definition give the unique prescribed vector and identity map, which preserves the metric. For a<b, let γ:[a,b]→M be piecewise smooth and v∈Tγ(a)M. The existence and uniqueness of a continuous piecewise parallel section through v is [L4]; the map Pγ is therefore well defined, and it is linear because the difference of two parallel sections with initial values v,w is a parallel section (linearity of Dt from step 1.1) with initial value v−w. It is bijective with inverse given by the same construction for the reversed curve. For v,w apply claim 1 to their parallel sections V,W on each smooth piece: g(V,W) has zero derivative there and is continuous across corners, hence constant on [a,b] by [L7], so g(Pγv,Pγw)=g(v,w).

3.2step 2.1L3L4L6L7algebra

(Constant speed and causal character.) Let γ be a geodesic, so Dsγ′=0 by [L3]. Applying the pairing identity of step 2.1 with V=W=γ′ gives ddsg(γ′,γ′)=2g(Dsγ′,γ′)=0 on every chart of the domain; hence g(γ′,γ′) is a constant by [L7]. By [L4], the tangent γ′ is the parallel section with its value prescribed at any one parameter, and parallel transport is bijective. Thus if γ′ vanishes once it vanishes everywhere, so γ is constant; otherwise it is nowhere zero. In the latter case its constant squared norm fixes its timelike, null or spacelike character on all of I. If it is causal, [L6] makes its continuous pairing with N nowhere zero, so its time orientation is also constant, including the null case.

4.1step 3.2L5L6algebra

(Timelike geodesics and proper time.) Let γ be a future-directed timelike geodesic with g(γ′,γ′)=−λ2, λ>0. Its proper-time density is λ2/c=λ/c, constant, so for t0<t1 the increment over [t0,t1] is λ(t1−t0)/c by [L5]; hence proper time is an affine function of the parameter and an affine parameter of γ. The four-velocity is U=dγ/dτ=(c/λ)γ′; since Dtγ′=0 and dτ/dt=λ/c is constant, DτU=(c/λ)Dt((c/λ)γ′)=0. A nonconstant null geodesic has nonzero null tangent by step 3.2, so the integrand in [L5] is zero and the curve is not a future timelike worldline; it admits no proper-time parametrization.

5.1step 3.2L3L7algebra∎

(Affine reparametrizations.) Let γ:I→M have nowhere-zero tangent and be a geodesic; let h:J→I be a C2 diffeomorphism onto its open image with h′≠0, and put γ~=γ∘h. In a chart and on each parameter interval where h and γ are taken on a fixed chart, γ~′=h′ (γ′∘h), so by step 1.1 Dsγ~′=h′′ (γ′∘h)+(h′)2 (Dtγ′)∘h=h′′ (γ′∘h), where the last equality is the geodesic equation for γ and the two terms arise exactly as in the product rule Ds(h′ (γ′∘h))=h′′(γ′∘h)+h′ Ds(γ′∘h) with Ds(γ′∘h)=h′ (Dtγ′)∘h. Since γ′∘h is nowhere zero, γ~ is a geodesic if and only if h′′≡0 on J, that is h(s)=as+b with constants a=h′≠0 and b. If γ is constant, then γ~ is constant and geodesic for every h by [L3]. Conversely, every C2 diffeomorphism with h′′=0 has this affine form, and for a nonconstant geodesic starting from a fixed affine parameter t, every other affine parameter s is related by s=at+b with a≠0 by applying the criterion to h=s∘t−1.

Remarks

TheoremStatement: AI-adaptedProof: AI-generatedprecheck passOpen item page →

The geodesic initial-value problem and the exponential map of the metric-selected connection

Statement

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold and let ∇ be its metric-selected connection, whose existence and uniqueness are supplied by Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields; its Christoffel symbols are the smooth chart functions of Christoffel symbols of an affine connection. Recall that a geodesic is a curve with Dtγ′=0 in its parameter (Geodesic of an affine connection, Covariant derivative along a curve).

(a) Local existence, uniqueness and maximality. For every (p,v)∈TM there is a unique maximal geodesic γp,v:Ip,v→M with γp,v(0)=p and γp,v′(0)=v; its domain Ip,v is an open interval containing 0 and is not asserted to be all of R.

(b) Smooth dependence. The set G:={(t,p,v):t∈Ip,v}⊆R×TM is open, and the evaluation map (t,p,v)↦γp,v(t) is smooth on G.

(c) Scaling. For every s∈R and every t∈R, t∈Ip,sv if and only if st∈Ip,v, and then γp,sv(t)=γp,v(st).

(d) The exponential map. Define Ep:={v∈TpM:1∈Ip,v} and exp⁡p:Ep→M, exp⁡p(v):=γp,v(1), and let ψp:TpM→R4 be the coordinate isomorphism of a basis e0,…,e3 of TpM. Then Ep is open and star-shaped about 0 (if v∈Ep and 0≤s≤1, then sv∈Ep), exp⁡p is smooth, exp⁡p(0)=p, and, under the canonical identification T0(TpM)≅TpM induced by the chart ψp on TpM, d(exp⁡p)0=id⁡TpM. Consequently there is a star-shaped open neighborhood Wp⊆Ep of 0 such that exp⁡p∣Wp is a diffeomorphism onto an open subset of M.

Facts & Assumptions

Given: A time-oriented smooth Lorentzian four-manifold (M,g,N) with its metric-selected connection ∇, a point p0∈M and a vector v0∈Tp0M.

[L1]

In a chart (U,x), a smooth curve γ with y=x∘γ and position--velocity lift z=(y,y˙) taking values in x(U)×R4 is a geodesic if and only if x¨k+∑i,jΓkij(x)x˙ix˙j=0 for k=0,1,2,3, equivalently z˙=F(z) for the smooth field F(x,w)=(w,−Γ(x)[w,w]) on x(U)×R4 (Coordinate geodesic equation, Christoffel symbols of an affine connection).

[L2]

For a smooth autonomous field F on an open subset of R8 and a base state z0 there are h>0 and a neighborhood Z of z0 such that every y∈Z has a unique solution Φ(⋅,y) on [−h,h] with Φ(0,y)=y, and Φ:(−h,h)×Z→R8 is smooth in y and C1 in t with ∂tΦ=F∘Φ (The fundamental theorem for autonomous smooth ODEs).

[L3]

For a jointly smooth ODE field on an open time-state-parameter domain, nearby initial states and parameters have solutions on a common compact interval around the initial time; at each fixed time the solution value is smooth in the initial-state/parameter pair (Smooth dependence of ODE solutions on parameters; its proof 2.1 supplies a nondegenerate symmetric interval). The Picard–Lindelöf theorem gives local existence and uniqueness through every admissible initial datum (Picard-Lindelöf local existence and uniqueness for first-order systems). The inherited tangent-bundle convention assumes ACω (The Axiom of Countable Choice (ACω)); the parameter theorem itself requires no additional Choice assumption.

[L4]

For a geodesic with nowhere-zero tangent, a C2 diffeomorphism h of its parameter makes γ∘h a geodesic exactly when h′′=0, equivalently h(t)=at+b with a≠0. A constant geodesic remains geodesic under every such reparametrization (Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed, clause 4). Constant curves are geodesics, the zero vector gives the constant geodesic, and uniqueness of geodesics with prescribed initial data is part of the maximality statement to be proved (Geodesic of an affine connection).

[L5]

Smooth maps with invertible differential at a point are local diffeomorphisms there; charts are smooth and their inverses are smooth; the differential of a smooth curve computes velocities (The smooth inverse function theorem on manifolds, The differential of a smooth map, Cr and smooth maps between smooth manifolds, The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a)).

[L6]

A closed bounded interval K⊆R with the usual metric d(s,t)=∣s−t∣ is a compact metric space, and every open cover of a compact metric space has a Lebesgue number δ>0 such that every subset of diameter less than δ lies in one cover member (Heine-Borel in Rn: with the Euclidean metric a subset of Rn is compact if and only if it is closed and bounded, and the proof by bisection uses no choice principle; the same holds on the real line, Every open cover of a compact metric space has a Lebesgue number: a δ>0 such that every nonempty subset of diameter less than δ lies inside a single member of the cover).

Proof

technique · direct
1.1L1givenalgebra

(Chart geodesic system.) Fix a chart (U,x); its domain is an open subset x(U)⊆R4, so D:=x(U)×R4 is open in R8, and the field F(x,w)=(w,−Γ(x)[w,w]) is smooth on D because the Christoffel symbols are smooth. By [L1], a smooth curve in U is a geodesic exactly when its coordinate lift solves z˙=F(z). Conversely, every solution z=(y,w) with values in D satisfies y′=w and y′′=−Γ(y)[y′,y′], so x−1∘y is the corresponding geodesic.

1.2L2L3L5constructalgebra

(Local flow and joint smoothness.) By [L2], near any z0∈D there is a local flow Φ:(−h0,h0)×Z0→D solving ∂tΦ=F(Φ) with Φ(0,y)=y. Apply [L3] to the jointly smooth parameter field H(r,z,λ):=λF(z) on R×D×R, at (r,z,λ)=(0,z0,0). There are a>0, an open neighborhood Z⊆Z0 of z0, and b>0 such that its solutions U(r,y,λ) exist on [−a,a] for (y,λ)∈Z×(−b,b); at the fixed time c:=a/2>0, the map (y,λ)↦U(c,y,λ) is smooth. Shrink b so cb<h0. For 0≤r≤c and ∣λ∣<b, the curve r↦Φ(rλ,y) is defined and satisfies dΦ(rλ,y)/dr=λF(Φ(rλ,y)) with initial value y. Uniqueness in [L3] gives U(c,y,λ)=Φ(cλ,y), including λ=0. Consequently Φ(t,y)=U(c,y,t/c) for ∣t∣<cb and y∈Z. The right side is a composition of smooth maps in the pair (t,y), so, with h:=cb, the restriction Φ:(−h,h)×Z→D is jointly smooth and remains the unique local solution through each y∈Z.

2.1step 1.1step 1.2L1L3given

(Agreement of solutions.) Let γ1,γ2 be geodesics whose parameter intervals share a nondegenerate interval J containing a parameter t0 with γ1(t0)=γ2(t0) and γ1′(t0)=γ2′(t0). Consider the set of t∈J at which both their positions and tangent vectors agree. It is closed because the two lifted curves t↦(γi(t),γi′(t)) in the Hausdorff tangent bundle are continuous. It is relatively open because, in a chart about any agreement point, the position--velocity lifts solve the same first-order system and local uniqueness from [L3] makes them agree nearby, including a one-sided neighborhood when that point is an included endpoint. It is nonempty by the data at t0, so connectedness of J makes it all of J. Applying this to each compact subinterval of the common domain proves agreement wherever both are defined. In particular two solutions through (p,v) with the same value and tangent at parameter 0 agree on their common domain.

3.1step 1.2step 2.1L2L3L4construct

(Maximal geodesic.) Fix (p,v)∈TM and let S be the set of all geodesics γ defined on an open interval containing 0 with γ(0)=p and γ′(0)=v; it is nonempty by [L2] applied in a chart around p to the state (x(p),v), and its parameter domains all contain 0. Let Ip,v be the union of those domains and define γp,v(t):=γ(t) for any γ∈S whose domain contains t; by step 2.1 this is independent of the choice of γ. The union of intervals containing 0 is an interval containing 0, and Ip,v is open: if t0∈Ip,v, then t0 lies in the domain of some γ∈S, and [L2] applied at the state of γ at t0 extends a representative solution to a neighbourhood of t0 which, by step 2.1, agrees with γp,v on the overlap. Every geodesic in S is a restriction of this union. To include arbitrary interval domains, let η:J→M be any geodesic with the same initial data, allowing included endpoints as in Geodesic of an affine connection. At each included finite endpoint e of J, smooth one-sided data give a position--velocity state (η(e),η′(e)). Step 1.2 gives a two-sided local solution through that state in a chart about η(e); the one-sided coordinate lift of η solves the same ODE, so uniqueness in [L3] makes them agree on their common one-sided interval. They therefore glue to a smooth geodesic across e. Opening the at most two included endpoints gives an extension η^ on an open interval J^⊇J containing 0, so η^∈S. Hence J⊆Ip,v and η=γp,v∣J. In particular no extension on any strictly larger interval exists, whether open, closed or half-open, and any other maximal geodesic with the data equals this one. This proves (a).

4.1step 3.1step 1.2L5algebra

(Smoothness of one geodesic.) For γ=γp,v and t0∈Ip,v, choose a chart around γ(t0) and apply step 1.2 at the state (γ(t0),γ′(t0)); the coordinate lift of γ agrees near t0 with the smooth local flow of that state, so t↦γp,v(t) is smooth on Ip,v.

4.2step 2.1step 3.1L4algebra

(Scaling.) Let s∈R. For s=0, the constant curve at p is a geodesic with initial data (p,0) and is defined on all of R by [L4], so by step 3.1 it is γp,0, and t∈Ip,0 iff 0=0⋅t∈Ip,v holds for all t, with equal values p=γp,v(0). For s≠0, put Js:={t:st∈Ip,v}. On Js the curve t↦γp,v(st) is a geodesic with initial data (p,sv): if v≠0, its tangent is nowhere zero, since a geodesic whose tangent vanished once would, by uniqueness in step 2.1, be constant; then clause 4 of [L4] applies to the affine reparametrization h(t)=st. If v=0, the curve is constant and clause 4 of [L4] handles that case directly. The interval Js is maximal for these initial data: any geodesic extension on a strictly larger interval would, after the inverse affine change of parameter t↦t/s, extend γp,v beyond Ip,v, contrary to step 3.1. Thus uniqueness of the maximal geodesic in step 3.1 gives Js=Ip,sv and γp,sv(t)=γp,v(st), proving (c).

5.1step 4.1step 1.2step 2.1L3L5L6construct

(Openness and smooth dependence.) Let t0∈Ip0,v0. If t0=0, step 1.2 and the flow identity give smooth dependence near (0,p0,v0). Otherwise let K be the compact interval with endpoints 0,t0 and let z:K→TM be the position--velocity lift of γp0,v0. For every s∈K, step 1.2 supplies an open neighborhood Zs of z(s) in a tangent-bundle chart and a local flow on (−hs,hs)×Zs for some hs>0. Compactness gives finitely many such neighborhoods Z1,…,Zm covering z(K); their inverse images under z form an open cover of K, so [L6] supplies a Lebesgue number δ>0. Choose a partition of K with mesh less than min⁡(δ,h1,…,hm), traversed from 0 toward t0. Each subinterval then lies in some z−1(Zi) and has length less than hi, so its solution map is the corresponding local flow map. Compose these finitely many smooth maps; at each stage continuity lets us shrink the neighborhood of (p0,v0) so the nearby state at the next node remains in the next selected flow neighborhood. Thus the position--velocity state at the last node depends smoothly on (p,v) nearby, and a final local flow around z(t0) gives smoothness jointly in (t,p,v) near (t0,p0,v0). This neighborhood is contained in G, so G is open in R×TM and the evaluation is smooth, proving (b).

6.1step 5.1step 4.2L5algebra

(The exponential domain.) By (c), 1∈Ip,sv iff s∈Ip,v for every s∈R. Hence Ep={v:1∈Ip,v} is the preimage of the open set G under the continuous map v↦(1,p,v), so it is open in TpM; and if v∈Ep and 0≤s≤1, then s∈Ip,v because Ip,v is an interval containing 0 and 1, so 1∈Ip,sv and sv∈Ep: the domain is star-shaped about 0. The map exp⁡p is the restriction of the smooth evaluation of (b) to {1}×{p}×Ep, hence is smooth, and exp⁡p(0)=γp,0(1)=p.

7.1step 4.2step 6.1L5given

(Differential at zero.) Choose a basis e0,…,e3 of TpM with coordinate isomorphism ψp:TpM→R4 and identify T0(TpM) with TpM by the chart ψp. For w∈TpM, the curve t↦exp⁡p(tw) has, by (c), exp⁡p(tw)=γp,tw(1)=γp,w(t), so its velocity at 0 is γp,w′(0)=w; hence d(exp⁡p)0(w)=w for every w, that is d(exp⁡p)0=id⁡TpM.

8.1step 6.1step 7.1L5construct∎

(Local diffeomorphism.) Since d(exp⁡p)0 is the identity, it is an isomorphism, so [L5] gives open neighborhoods V⊆Ep of 0 and U⊆M of p such that exp⁡p∣V:V→U is a diffeomorphism. Choose a Euclidean norm on the finite-dimensional space TpM and let Wp be the open ball of some radius contained in V; it is open, contains 0, is star-shaped, and exp⁡p∣Wp is a diffeomorphism onto its open image. This proves (d) and completes the proof.

Remarks

  • No completeness is asserted. The maximal interval Ip,v may be a proper subset of R; nothing above produces a global geodesic or an exponential map defined on all of TM. The local diffeomorphism of claim (d) is a statement about a sufficiently small star-shaped neighborhood of the origin, not about global injectivity.

  • Choice convention. The tangent bundle and its smooth structure carry the inherited ACω of The Axiom of Countable Choice (ACω). The smooth-dependence theorem of [L3] uses no additional Choice assumption. Step 5.1 uses a finite subcover and finitely many chart flows; each flow is uniquely determined by its initial-value problem. No choice function for an infinite family of flows is needed.

  • Generality. The proof uses only that the Christoffel symbols are smooth and that the geodesic equation is the displayed second-order system; it therefore applies verbatim to any smooth affine connection on a smooth four-manifold, with the metric-selected connection being the case used here. The published Riemannian geodesic-flow theorem is not needed; the route is the chart system with the two elementary ODE suppliers.

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Point-normal and exponential coordinate charts of the metric-selected connection

Statement

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold with metric-selected connection ∇ (Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields), whose geodesics and exponential map are those of The geodesic initial-value problem and the exponential map of the metric-selected connection.

(a) Point-normal charts. For every p∈M there is a smooth chart (U,x) around p with x(p)=0 such that, in the components of this chart,

Γabc(p)=0,∂agbc(p)=0,gab(p)=ηab=diag⁡(−1,1,1,1)ab.

The construction starts from any chart around p and is finite: no frame field on U and no global trivialization of TM is used.

(b) Exponential charts. For every p∈M and every gp-orthonormal basis e0,…,e3 of TpM there is a star-shaped open neighborhood W⊆TpM of 0 on which exp⁡p is a diffeomorphism onto an open Up∋p, and the chart

u:=ψ∘exp⁡p−1:Up⟶R4,

where ψ:TpM→R4 is the coordinate isomorphism of the basis, satisfies u(p)=0 and the same three normal-form identities at p as in (a). Moreover every geodesic through p has, in the chart u, the form u(γ(t))=(t−t0) k for a constant k∈R4 whenever γ(t0)=p, k=ψ(γ′(t0)), and (t−t0)γ′(t0)∈W. Thus the portion represented by its radial initial vector in W is a straight coordinate ray through the origin. This claim is not made for a later portion of a geodesic that may return to Up after its radial initial vector has left W. No assertion is made about the second derivatives of the metric at p: the construction is first order and does not make a neighborhood of p isometric to Minkowski space.

Facts & Assumptions

Given: A time-oriented smooth Lorentzian four-manifold (M,g,N) with metric-selected connection ∇, and a point p∈M.

[L1]

For the metric-selected connection, the Christoffel symbols transform under a coordinate change x↔y by the inhomogeneous law Γ~cab=∂yc∂xk(∂xi∂ya∂xj∂ybΓkij+∂2xk∂ya∂yb) (Christoffel symbol transformation law, Christoffel symbols of an affine connection).

[L2]

Metric compatibility is equivalent in a chart to ∂agbc=∑d(Γdabgdc+Γdacgbd); the metric components in a chart are smooth (Torsion freedom and metric compatibility in chart components, Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model).

[L3]

A C1 map between Euclidean open sets with invertible derivative at a point is a local C1 diffeomorphism there, and the inverse function relation x(y(x))=x permits differentiation (Choice-free smooth inverse function theorem in Euclidean space, Christoffel symbol transformation law).

[L4]

A Lorentz form on a real vector space has an orthonormal basis e0,…,e3 with gp(eA,eB)=ηAB, and gp(eA,eB) is the matrix of gp in that basis (Every Lorentz form admits an ordered basis with matrix diag(-1,1,1,1), Lorentz forms of inertia (3,1,0) on a 4-dimensional real vector space).

[L5]

In the chart domain of the exponential map, the radial curves t↦exp⁡p(tv) are geodesics with exp⁡p(tv)=γp,v(t), the differential of exp⁡p at 0 is the identity under the canonical identification T0(TpM)≅TpM, and exp⁡p restricts to a diffeomorphism on a star-shaped neighborhood of 0 (The geodesic initial-value problem and the exponential map of the metric-selected connection).

[L6]

In coordinates, a curve is a geodesic if and only if x¨k+∑i,jΓkij(x)x˙ix˙j=0; the coordinate derivations ∂a form a basis of each tangent space of the chart (Coordinate geodesic equation, Geodesic of an affine connection, Coordinate derivations form a basis of the tangent space).

Proof

technique · direct
1.1L1L3givenconstruct

(Point-normal chart.) Fix a smooth chart (V,y) around p with y(p)=0, and on a Euclidean ball around 0 in y(V) define xa:=ya+12∑b,cΓabc(p) ybyc. Its derivative at 0 is the identity matrix, so by [L3] x restricts to a diffeomorphism from a neighborhood of 0 onto an open set: it is a chart around p with x(p)=0.

1.2L5construct

(Exponential chart.) Fix a gp-orthonormal basis e0,…,e3, let ψ be its coordinate isomorphism, and let W be a star-shaped neighborhood of 0 on which exp⁡p is a diffeomorphism onto an open set Up, as supplied by [L5]. Then exp⁡p(0)=p, so u:=ψ∘exp⁡p−1 is a smooth chart on Up with u(p)=0; it is the composition of the smooth maps exp⁡p−1 and the linear isomorphism ψ.

2.1step 1.1L1L3algebra

(Christoffel symbols vanish at p.) Differentiating the inverse relation x(y(x))=x twice at x=0 where the first derivatives are the identity gives ∂2ya/∂xb∂xc(0)=−∂2xa/∂yb∂yc(0)=−Γabc(p). Substituting this and the identity Jacobians into the transformation law of [L1], with y as the old and x as the new coordinates, gives Γxabc(0)=Γabc(p)−Γabc(p)=0.

2.2step 1.2L5L6algebra

(Straight coordinate lines.) Let k∈R4 and put v:=ψ−1(k)∈TpM; for t in a neighborhood of 0 with tv∈W, [L5] gives u−1(tk)=exp⁡p(tv)=γp,v(t), which is a geodesic. Substituting x(t)=tk into the coordinate geodesic equation of [L6] gives ∑b,cΓabc(tk)kbkc=0 for all a and all t in an interval, hence at t=0: ∑b,cΓabc(0)kbkc=0 for every k∈R4. First take k=eb for each b to obtain Γabb(0)=0. Given a and two indices b≠c, apply this with k=eb+ec and with k=eb−ec and subtract to get 2(Γabc(0)+Γacb(0))=0, that is Γa(bc)(0)=0; torsion freedom gives Γabc(0)=Γa(bc)(0)=0.

2.3step 1.2L5algebra

(The radial portion of every geodesic through p is a straight line.) Let γ be a geodesic with γ(t0)=p and put v0:=γ′(t0). Translate the parameter so that t0=0, and write the translated parameter again as t. For any t in the domain of γ with tv0∈W, the scaling law of The geodesic initial-value problem and the exponential map of the metric-selected connection makes t an allowed parameter of γp,v0 and gives γp,v0(t)=exp⁡p(tv0). By geodesic uniqueness in [L5], γ(t)=γp,v0(t) there, so the inverse exponential chart returns exactly tv0∈W and u(γ(t))=tψ(v0). Because W is star-shaped, its intersection with the line Rv0 is an interval containing 0; this proves the assertion on the connected radial passage through p and makes no claim about a later return to Up after that radial vector leaves W.

3.1step 2.1L2L4algebra

(Metric first derivatives vanish, normal form.) Applying the compatibility identity of [L2] in the chart x at the point p gives ∂agxbc(p)=∑d(Γxdab(p)gxdc(p)+Γxdac(p)gxbd(p))=0 by step 2.1. Let A be the matrix whose columns are the components in the chart x of an orthonormal basis of (TpM,gp), supplied by [L4], and set z:=A−1x near p. Under this constant linear coordinate change the transformation law of [L1] has no second-derivative term and gives Γzbc(0)=0; the metric components satisfy gzab(0)=gxcd(0)AcaAdb=ηab by the choice of A; and ∂gz(0)=0 because a constant linear change composes the derivative array with the fixed invertible Jacobians. This proves (a).

3.2step 2.2L2L5L4algebra

(Metric normal form in the exponential chart.) With Γu(0)=0 from step 2.2, the compatibility identity of [L2] gives ∂agubc(0)=0. The coordinate basis at p is ∂ua∣p=d(exp⁡p)0(ea)⋅ in the identification of [L5], which equals ea; hence guab(0)=gp(ea,eb)=ηab.

4.1step 3.1step 3.2step 2.3∎

Claims (a) and (b) are steps 3.1 and 1.2-3.2 respectively; the final assertion about second derivatives is a scope statement, and the proof above never differentiates the metric twice, so it asserts nothing at second order.

Remarks

  • No flatness and no global inertial frame. The identities of this theorem hold at the single point p. A chart in which Γ(p)=0 and ∂g(p)=0 is not an isometry and does not make U a piece of Minkowski space; the higher derivatives of the metric are not controlled by the construction. The physical reading of such a chart as a local inertial frame, and its limitations, are recorded in Scope of normal coordinates and of the local-inertial-frame reading and are not part of this mathematical statement.

  • Finite choices. Part (a) selects one initial chart, one quadratic correction and one constant matrix from a supplied orthonormal basis; part (b) selects one supplied orthonormal basis and one star-shaped domain. All are finite data, and no additional choice principle is used beyond the inherited ACω of the ambient smooth structure.

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First variation of the length of a timelike curve: stationarity is the geodesic equation

Statement

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold with metric-selected connection ∇ (Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields), let a<b, and let γ:[a,b]→M be a C2 future timelike curve whose image is contained in the domain U of one smooth chart (U,x) (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold). Suppose γ is parametrized so that

gγ(t)(γ′(t),γ′(t))=−c2(t∈[a,b]),

that is, by proper time up to a choice of origin (Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent). Let H:(−ε,ε)×[a,b]→U be a map that is C2 in both variables, with H(0,t)=γ(t) for all t, with H(s,a)=γ(a) and H(s,b)=γ(b) for all s, and such that each curve t↦H(s,t) is future timelike; write T(s,t):=∂tH(s,t), J(t):=∂sH(s,t)∣s=0, so that J(a)=J(b)=0, and

L(s):=∫ab−gH(s,t)(T(s,t),T(s,t)) dt.

Then:

  1. L is differentiable at 0 and L′(0)=−∫abgγ(t)(DtJ(t),γ′(t))−gγ(t)(γ′(t),γ′(t)) dt=−1c∫abgγ(t)(DtJ(t),γ′(t)) dt.
  2. Equivalently, L′(0)=1c∫abgγ(t)(J(t),Dtγ′(t)) dt.
  3. L′(0)=0 for every such variation H if and only if Dtγ′=0 on [a,b]. Consequently, within this class, stationarity of the length functional is exactly the geodesic equation in the given proper-time parameter.

The chart hypothesis is used to realize variations of prescribed compactly supported variation fields by coordinate displacement; the formula of claim 1 and the implication "geodesic ⇒ stationary" are local and do not require it beyond the smooth parametrization.

Facts & Assumptions

Given: A time-oriented smooth Lorentzian four-manifold (M,g,N) with metric-selected connection ∇, an interval [a,b] with a<b, a C2 future timelike curve γ in a chart domain U with g(γ′,γ′)=−c2, and a C2 variation H as in the statement.

[L1]

The metric pairing identity along a curve holds: ddtg(V,W)=g(DtV,W)+g(V,DtW) for smooth sections along a smooth curve (Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed, clause 1).

[L2]

In a chart, DtVa=∂tVa+∑b,cΓabcγ˙bVc for a field V along γ with tangent γ˙, and Γabc=Γacb (Covariant derivative along a curve, Christoffel symbols of an affine connection, Metric compatibility, torsion freedom and the metric-selected connection class, Torsion freedom and metric compatibility in chart components).

[L3]

For a C2 two-parameter family the mixed derivatives commute as ordinary partial derivatives in a chart, so DsT=DtJ (Clairaut--Schwarz theorem for continuous second partial derivatives, Covariant derivative along a curve).

[L4]

If F and H are continuous on [−ε0,ε0]×[a,b] and ∂sF(s,t)=H(s,t) for ∣s∣<ε0, then the compact-rectangle differentiation theorem applies to the Darboux/Riemann integrals of the continuous slices and gives that s↦∫abF(s,t) dt is differentiable at 0 with derivative ∫abH(0,t) dt (Leibniz's rule on a compact rectangle: an interior parameter derivative with a continuous extension may be passed through a Riemann integral, The lower and upper Darboux integrals of a bounded f on [a,b] as sup⁡PL(f,P) and inf⁡PU(f,P), Darboux integrability as their equality, and the notation ∫abf).

[L6]

For 0<r<R in R there is a smooth ρ:R→[0,1] with ρ=1 on [t0−r,t0+r] and support in (t0−R,t0+R) (A smooth bump between concentric Euclidean balls).

[L7]

In a chart, a nondegenerate metric identifies every nonzero tangent vector A with a nonzero covector g(A,⋅) (The inverse metric, musical isomorphisms and index raising). Since the chart coordinate vectors form a basis, at least one coordinate vector ∂j has g(∂j,A)≠0; choosing its sign makes this pairing positive. The coordinate vector field ∂j has constant components in that chart and hence gives a smooth section along γ (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model).

Proof

technique · direct
1.1L4algebra

(Differentiability of L.) The integrand ρ(s,t):=−gH(s,t)(T(s,t),T(s,t)) is strictly positive and continuous on (−ε,ε)×[a,b] (indeed C1): H and T=∂tH are C1 in both variables, the metric components are smooth, and the square root is smooth on (0,∞). Hence [L4] applies and L′(0)=∫ab∂sρ(0,t) dt.

2.1step 1.1L1algebra

(Derivative of the integrand.) By [L1] applied to V=W=T with the derivative in the s-direction (the pairing identity holds for the two-parameter family by the same component computation as for one parameter), ∂sρ(0,t)=−g(DsT,T)−g(T,T)∣s=0.

2.2step 1.1L2L3algebra

(Commutator.) On the chart U, writing Ha=Ha(s,t) and using [L2], DsTa−DtJa=∑b,cΓabc(JbTc−TbJc)=0 since ∂s∂tHa=∂t∂sHa by [L3] and Γ is symmetric in its lower indices. Hence DsT=DtJ at s=0, where J=∂sH, and T=γ′.

3.1step 2.1step 2.2algebra

(First variation formula.) Substituting steps 2.1 and 2.2 into step 1.1, and using g(γ′,γ′)=−c2, gives the formula of claim 1.

4.1step 3.1L1L5algebra

(Integration by parts.) By [L1], ddtg(J,γ′)=g(DtJ,γ′)+g(J,Dtγ′) and both terms are continuous, so the derivative of the C1 function t↦g(J,γ′) is integrable; [L5] gives ∫ab(g(DtJ,γ′)+g(J,Dtγ′))dt=g(J,γ′)∣ab=0 because J(a)=J(b)=0. Multiplying the first variation formula by c and using this identity gives claim 2, L′(0)=1c∫abg(J,Dtγ′)dt.

5.1step 4.1algebra

(⇒ direction of claim 3.) If Dtγ′=0 on [a,b], the integrand of claim 2 vanishes identically for the variation at hand, so L′(0)=0; since H was arbitrary, every such variation is stationary.

6.1step 5.1L6L7construct

(Converse.) If Dtγ′ is nonzero at an endpoint, continuity makes it nonzero at an interior point as well; hence, if Dtγ′ is not identically zero on [a,b], choose t0∈(a,b) with A(t0):=Dtγ′(t0)≠0. The field A is continuous because γ is C2 and the Christoffel symbols are smooth. By [L7], choose a chart coordinate vector field with sign Z=±∂j along γ so g(Z(t0),A(t0))>0; by continuity, this pairing is positive on a neighborhood of t0. Choose a closed interval [u,v]⊆(a,b) with t0 in its interior on which the pairing stays positive. Then choose 0<r<R with [t0−r,t0+r]⊆[u,v] and (t0−R,t0+R)⊆(u,v), and let φ≥0 be the bump of [L6] equal to 1 on [t0−r,t0+r] with support in (t0−R,t0+R). Put J(t):=φ(t)Z(t); its chart components are smooth and it vanishes at a,b. Define H(s,t):=x−1(x(γ(t))+s Jch(t)) on a sufficiently small ∣s∣, where Jch denotes the chart components of J. This is a C2 variation, and [L7] ensures g(J,Dtγ′)>0 wherever φ>0.

7.1step 6.1L1algebra

(Admissibility of the constructed variation.) H fixes the endpoints because J(a)=J(b)=0; it is C2; and for all sufficiently small ∣s∣ its fibers are future timelike and lie in U: the perturbation sJch vanishes outside [u,v], so on the compact set [u,v] the image stays in a fixed compact subset of the chart domain for small ∣s∣, and the family of velocities T(s,t) depends continuously on (s,t) with T(0,t)=γ′(t) future timelike, so by compactness of [a,b] the timelike condition persists for small ∣s∣.

8.1step 7.1step 4.1L5algebra∎

(Nonstationarity.) For this variation, claim 2 and the choice of J give L′(0)=1c∫abφ(t) gγ(t)(Z(t),Dtγ′(t)) dt>0: the pairing is positive wherever φ>0, while φ is nonnegative and is 1 on the nondegenerate interval [t0−r,t0+r], so the integrand is continuous, nonnegative and strictly positive on that interval; hence the integral is strictly positive by [L5]. Therefore a curve with Dtγ′≠0 admits a variation with L′(0)≠0, and stationarity for every variation forces Dtγ′=0, proving claim 3.

Remarks

  • Scope. The variation class is restricted to curves and variations contained in one chart domain with fixed endpoints and timelike fibers; the result asserts nothing about null curves, about maximality (which is the content of The Lorentzian Gauss lemma and the radial maximum of proper time), or about second variations. The chart hypothesis only serves the realization of variations in steps 6.1-7.1; the formula of claim 1 is local and holds for any C2 variation of a timelike curve.

  • Physical reading. The lemma is mathematics: it identifies the stationary curves of the length functional with geodesics. The physical statement that ideal clocks measure proper time and that freely falling bodies follow geodesics is adopted separately in Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework and is not asserted here.

TheoremStatement: AI-adaptedProof: AI-generatedprecheck passOpen item page →

The Lorentzian Gauss lemma and the radial maximum of proper time

Statement

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold with metric-selected connection ∇ (Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields), and let p∈M. Let Wp⊆TpM be a star-shaped open neighborhood of 0 on which exp⁡p is a diffeomorphism onto an open set Up:=exp⁡p(Wp), as supplied by The geodesic initial-value problem and the exponential map of the metric-selected connection and Point-normal and exponential coordinate charts of the metric-selected connection; identify Tv(TpM) with TpM for every v.

(a) Gauss lemma. For every v∈Wp and every w∈TpM,

gexp⁡pv(d(exp⁡p)v(v), d(exp⁡p)v(w))=gp(v,w).

(b) Radial maximum. Let α:[0,1]→Up be a piecewise-C1 future timelike curve with α(0)=p, with nonzero future timelike one-sided tangents, set q:=α(1) and vq:=exp⁡p−1(q). Then

Lg(α)≤−gp(vq,vq),

and equality holds if and only if there are v0∈Wp and a piecewise-C1 strictly increasing surjection ρ:[0,1]→[0,ρ(1)] with vq=ρ(1)v0 and α(t)=exp⁡p(ρ(t)v0) for all t; that is, α is a monotone reparametrization of the radial geodesic segment from p to q. Dividing by c, the proper-time increment of α is at most 1c−gp(vq,vq), which is the proper-time increment of that radial geodesic.

Facts & Assumptions

Given: A time-oriented smooth Lorentzian four-manifold (M,g,N) with metric-selected connection ∇, a point p, a star-shaped domain Wp on which exp⁡p is a diffeomorphism, and the curves and vectors named in the claims.

[L1]

For v∈Wp the curve t↦exp⁡p(tv) is the geodesic γp,v on some open interval containing [0,1], and its tangent has constant norm gp(v,v); radial geodesics are defined by the initial-value problem of The geodesic initial-value problem and the exponential map of the metric-selected connection (The geodesic initial-value problem and the exponential map of the metric-selected connection, Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed, clauses 1 and 3).

[L2]

If V,W are smooth sections of γ∗TM along a smooth curve, then ddtg(V,W)=g(DtV,W)+g(V,DtW); and for a C2 two-parameter family Φ(s,r) one has Ds∂rΦ=Dr∂sΦ, because in a chart both sides equal ∂s∂rΦa plus the same symmetric Γ-contraction (Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed, clause 1, Covariant derivative along a curve, Christoffel symbols of an affine connection, Metric compatibility, torsion freedom and the metric-selected connection class, Clairaut--Schwarz theorem for continuous second partial derivatives).

[L3]

If n is an observer and w is nonzero future causal at the same point, then −g(n,w)>0. If w is future unit timelike, then −g(n,w)≥1, with equality exactly when w=n. Consequently, for any future timelike X, putting s:=−g(X,X) and O:=X/s gives an observer O and −g(n,X)=s[−g(n,O)]≥s, with equality exactly when O=n (Pairing of an observer with future causal vectors, claims 1 and 2, Observers, rest spaces and the spatial projection at an event).

[L4]

The timelike set at a point has exactly two connected components, so a continuous curve of timelike vectors that starts future-directed and never becomes null stays future-directed; the closure of the future timelike component is the future causal cone, and a nonzero limit of future timelike vectors is future causal (The timelike set has exactly two convex components, described in orthonormal coordinates, Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model, Timelike, null, spacelike and causal vectors of a Lorentz vector space).

[L5]

R(t)=−gp(v(t),v(t)) has derivative R′=−gp(v,v′)/R on intervals where R>0, since the square root is differentiable on (0,∞); the fundamental theorem of calculus applies to C1 functions on closed intervals (Rational powers ar of a positive base, Continuity and derivatives of positive-base real powers, The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a)).

[L6]

A C1 curve in Up lifted by exp⁡p−1 is piecewise C1, α=exp⁡p∘v, and α′=d(exp⁡p)v(v′); for the inverse map d(exp⁡p−1)p=id⁡ under the canonical identification, so for the lift of a curve starting at p one has v(t)=tα′(0)+o(t) as t↓0 (The geodesic initial-value problem and the exponential map of the metric-selected connection, The differential of a smooth map, Point-normal and exponential coordinate charts of the metric-selected connection).

Proof

technique · direct
1.1L1L2given

(Two-parameter family.) Let r↦v(r) be a smooth curve in Wp and put F(s,r):=exp⁡p(sv(r)) for s∈[0,1], so that F(0,r)=p and F(1,r)=exp⁡p(v(r)). Set T:=∂sF, J:=∂rF. For each fixed r, s↦F(s,r) is the radial geodesic with tangent v(r) at s=0; hence DsT=0 and g(T,T)=gp(v(r),v(r)) for all s by [L1]. By [L2], DsJ=DrT.

1.2L5L6construct

(The lift of a curve.) Let α be as in (b) and define v(t):=exp⁡p−1(α(t)) for t∈(0,1], v(0):=0; by [L6], v is piecewise C1 with α=exp⁡p∘v and α′=d(exp⁡p)v(v′), and v(t)=tα′(0)+o(t). Write Q(t):=gp(v(t),v(t)) and R(t):=−Q(t) on {Q<0}.

1.3L4L6algebra

(First possible exit from the future timelike cone.) Let T∗:=sup⁡{t∈[0,1]:v(s) is future timelike for every s∈(0,t]}; this is positive by [L6] and continuity, because v(t)=tα′(0)+o(t) and α′(0) is future timelike. The vector v(t) is future timelike for every 0<t<T∗. If T∗<1, openness of the future timelike cone rules out v(T∗) being timelike, since that would extend the defining interval past T∗. If T∗=1 and v(1) is future timelike, the desired cone assertion already holds at the endpoint. In every remaining case, continuity and closure of the future timelike cone imply that v(T∗) is either a nonzero future causal vector or zero; after excluding the timelike case it is either future null (case A) or zero (case B). With signature (−,+,+,+), Q(T∗)=gp(v(T∗),v(T∗))≤0, with equality in case A; the case B value is also 0.

2.1step 1.1L2algebra

(Gauss computation.) By [L2] and step 1.1, ∂sg(T,J)=g(DsT,J)+g(T,DsJ)=g(T,DrT)=12∂rg(T,T)=gp(v(r),v′(r)), using symmetry of g in the middle term and step 1.1 in the last. Since J(0,r)=∂rexp⁡p(0)=0, integrating the constant-in-s right-hand side from s=0 to s=1 gives gexp⁡p(v(r))(d(exp⁡p)v(r)(v(r)),d(exp⁡p)v(r)(v′(r)))=gp(v(r),v′(r)). Every pair (v,w) with v∈Wp is of the form (v(0),v′(0)) for the smooth family r↦v+rw, so the identity holds for all such pairs; this proves (a).

3.1step 1.3step 2.1L1L3L4algebra

(Case A is impossible.) In case A, Q<0 on (0,T∗) and Q(T∗)=0, so its one-sided left derivative satisfies Q′(T∗−)≥0; if T∗ is a corner of the piecewise curve, use the left tangent and left derivative. On the smooth pieces the Gauss lemma of step 2.1 gives Q′(t)=2gp(v,v′)=2gα(t)(T(t),α′(t)), where T(t)=d(exp⁡p)v(t)(v(t)) is the radial tangent. For each t<T∗, the radial geodesic s↦exp⁡p(sv(t)) has constant timelike speed by [L1]; its tangent begins in the future timelike component and stays there by continuity and the two-component classification [L4]. Thus T(t) is future timelike. Since v(T∗) is a nonzero future null vector, d(exp⁡p)v(T∗) is invertible and T(T∗)=lim⁡t↑T∗T(t) is nonzero, null by [L1], and future-directed by [L4]. Let s:=−g(α′(T∗−),α′(T∗−))>0 and O:=α′(T∗−)/s; then O is an observer. By [L3] applied to observer O and future null vector T(T∗), −g(O,T(T∗))>0. Therefore Q′(T∗−)=2g(T(T∗),α′(T∗−))=2s g(T(T∗),O)<0, contradicting Q′(T∗−)≥0. The argument also applies when T∗=1, using the left endpoint tangent of the final piece.

3.2step 1.3step 2.1L1L3L5algebra

(Case B is impossible.) In case B, v(t) is future timelike for t<T∗ and v(T∗)=0, so R>0 on (0,T∗) and R(t)→0 as t↑T∗. On each smooth piece, by [L5] and the Gauss lemma, R′=−gp(v,v′)/R=−gα(T^,α′), where T^:=T/R is future unit timelike by [L1] and the future-directedness of v. Put s:=−g(α′,α′)>0 and O:=α′/s, a future unit timelike observer. Applying claim 2 of [L3] to observers T^,O gives −g(T^,O)≥1, hence R′=−g(T^,α′)≥s>0. Thus R is strictly increasing on each smooth piece of (0,T∗) and, by continuity across the finitely many corners, R(t)>R(δ) whenever 0<δ<t<T∗. Taking t↑T∗ yields R(T∗)≥R(δ)>0, contradicting R(T∗)=0. This argument also applies when T∗=1.

4.1step 3.2L3L5algebra

(Length inequality.) By steps 1.2, 1.3, 3.1 and 3.2, v(t) is future timelike for every t∈(0,1], so R>0 on (0,1]. On each smooth piece put s:=−g(α′,α′)>0, O:=α′/s, and T^:=T/R; both O and T^ are observers. Claim 2 of [L3] gives −g(T^,O)≥1, hence R′=−g(T^,α′)≥s. Integrating over the smooth pieces from δ to 1 and adding gives R(1)−R(δ)≥∫δ1s(t) dt. Letting δ↓0, continuity of v gives R(δ)→0, and the integral over (0,δ) tends to 0 because s is bounded on the finitely many pieces with finite one-sided limits. Therefore Lg(α)≤R(1)=−gp(vq,vq). Dividing by c and using Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent gives the proper-time statement.

5.1step 4.1L3L5L6algebra∎

(Equality case.) If equality holds in step 4.1, the continuous nonnegative function R′−s on each smooth open piece has zero integral over (0,1), so it vanishes identically there. By the equality case of claim 2 in [L3], applied to the observers T^=T/R and O=α′/s, one has O=T^ and hence α′=sT^ on every smooth piece. Since d(exp⁡p)v is invertible for v∈Wp, α′=d(exp⁡p)v(v′) and T=d(exp⁡p)v(v) imply v′=(s/R)v. Also R′=s on each piece, so (v/R)′=v′/R−vR′/R2=0 there; continuity across the finitely many corners makes v/R the same constant throughout (0,1]. Put v0:=v(1)=vq∈Wp and ρ(t):=R(t)/R(1) for t>0, with ρ(0):=0. Then ρ(1)=1, v(t)=ρ(t)v0, and ρ is piecewise C1 and strictly increasing because R′=s>0 on every smooth piece. At t=0, put a:=α′(0). Since exp⁡p−1 is smooth with d(exp⁡p−1)p=id⁡ and the first piece of α is C1 up to 0, v′(t)→a from the right; also v(t)=ta+o(t) by [L6]. Thus R(t)/t→−gp(a,a)>0 and R′(t)=−gp(v,v′)/R→−gp(a,a), so ρ and its derivative extend continuously from the right to 0. Consequently α(t)=exp⁡p(ρ(t)v0), which is the equality form in (b). Conversely, for any equality-form curve from the Statement, α′=ρ′ d(exp⁡p)ρv0(v0) has norm ∣ρ′∣−gp(v0,v0); its length is ρ(1)−gp(v0,v0)=−gp(vq,vq), so equality holds. This proves (b) and completes the proof.

Remarks

  • Scope. The maximum is asserted only for curves remaining in the star-shaped exponential domain Up and does not assert global maximality after leaving it, maximality before every conjugate or cut point, or any statement about null curves. The equality analysis uses that d(exp⁡p)v is invertible along the radial segment; for v∈Wp this holds by the choice of Wp.

  • Auxiliary metric but Lorentzian claims. The proof uses only the nondegenerate Lorentzian metric and the metric-selected connection; no positive-definite Riemannian Gauss lemma or index lemma is consumed. The final comparison is between two proper times of the same future timelike type, and makes no comparison assertion for spacelike or null curves.

PostulateStatement: AI-adaptedProof: Not applicableOpen item page →

Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework

Physical scope

Adopted coupling assumptions of the classical smooth gravitational model: ideal clocks measure the proper time of their future timelike worldlines; ideal freely falling massive test bodies follow future timelike geodesics of the metric-selected connection; ideal light rays are future null geodesics in the geometric-optics approximation. The assumptions are stated in the test-field regime of the smooth four-dimensional model and exclude self-force and radiation back-reaction, finite-size and tidal couplings beyond the test-body idealization, non-geometric-optics propagation, dispersion and dissipation, matter with non-negligible gravitational self-field, distributional or lower-dimensional sources, and quantum effects. They are adopted assumptions of the framework, not derived or empirical results; empirical comparison belongs to fully specified models and reported observations.

Postulate

Adopt as physical assumptions of the classical gravitational framework, in addition to Adopted spacetime model and classical domain of the gravitational framework and the matter-content assumptions of the framework, the following rules by which ideal clocks, test bodies and light couple to the metric g of Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model.

(i) Ideal clocks. An ideal clock is an idealized physical device carried along a future timelike worldline (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold) whose readings are assumed to reproduce the proper time of that worldline: the difference of two readings taken at two events of the worldline is the proper-time increment between those events as defined by the metric, and it is independent of the construction of the clock. Two ideal clocks moving along the same worldline differ only by an additive constant (their choice of zero); different worldlines generally accrue different proper times between the same pair of events. The physical constant c and the unit of duration are those of SI unit and coordinate conventions of the classical gravitational framework.

(ii) Free fall of massive test bodies. A test body is an uncharged idealized body whose internal structure is small compared with the scale over which the geometry of the model varies and whose gravitational self-field is negligible within the model. An ideal freely falling massive test body is assumed to have a worldline that is a future timelike geodesic of the metric-selected connection (Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields, Geodesic of an affine connection), traversed with physical four-velocity U=dγ/dτ satisfying gγ(τ)(U,U)=−c2; proper time is an affine parameter of the worldline (Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent). The worldline is determined by the event at which the body is released together with its four-velocity there, by the uniqueness of the geodesic initial-value problem (The geodesic initial-value problem and the exponential map of the metric-selected connection); no force, charge, or rest mass of the body enters this rule.

(iii) Light rays. In the geometric-optics approximation an ideal light ray propagating in the model is assumed to be a future null geodesic of the metric-selected connection (Timelike, null, spacelike and causal vectors of a Lorentz vector space, Geodesic of an affine connection). A null worldline carries no proper time and no four-velocity in the sense of Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold; within the approximation the propagation of an ideal ray is independent of its frequency, and only the ray's direction in the tangent space is fixed, not a scale along it.

(iv) Scope and exclusions. The three rules are adopted in the test-field regime of the smooth classical model: the clocks, bodies and rays do not back-react on the geometry, and the geometry varies smoothly on the scales relevant to them. Configurations requiring the body's own gravitational field, radiation reaction, an electromagnetic or other self-force, finite-size or tidal couplings beyond the test-body idealization, non-geometric-optics propagation, dispersion or dissipation of light, or quantum effects are outside these assumptions and require additional model content. The assumptions do not assert that any real clock, body or light ray is exactly ideal, nor do they attach measured readings to any model.

Status, scope and limitations

  • Adopted, not derived. Clauses (i)-(iii) are physical assumptions of the framework. Nothing in the mathematical items on this page or its prerequisites produces them: the geodesic initial-value theorem and the first-variation lemma identify geodesics as the stationary curves of the length functional (First variation of the length of a timelike curve: stationarity is the geodesic equation) and construct the exponential map, but they do not assert that any physical body, clock or light ray follows those curves. The equivalence principle and the structure of the nonrelativistic limit motivate these rules; neither proves them.

  • Empirical content is downstream. The framework's empirical significance lies in predictions of fully specified models — a geometry, a matter content and a field law — compared with reported observations under their apparatus, calibration and uncertainty qualifications. Agreement of such a comparison is evidence about the combined model and apparatus assumptions, not a proof of clauses (i)-(iv), and a disagreement can expose an auxiliary assumption, an apparatus effect or an analysis error rather than a foundational postulate.

  • Relation to the flat model. The corresponding assumptions of flat special relativity are separate physical postulates with Minkowski scope; they are not used here as suppliers of curved-spacetime content. The flat model appears on this track only as a comparison and limiting case.

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The free-fall worldline of an ideal test body is determined by its initial event and four-velocity

Physical scope

Model-conditional statement within the classical smooth gravitational framework with its adopted clock, free-fall and light-ray assumptions: under the test-body idealization, two ideal freely falling massive test bodies released at the same event with the same physical four-velocity have the same worldline. It excludes bodies with non-negligible self-field, finite-size or tidal couplings beyond the idealization, self-force and radiation back-reaction, and quantum effects; it makes no empirical claim that all bodies in nature fall alike, and it does not establish the equivalence principle as a law of nature.

Statement

Let a model of the classical gravitational framework be specified by a time-oriented smooth Lorentzian four-manifold (M,g,N) with its metric-selected connection (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model, Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields), and assume the clock, free-fall and light-ray assumptions of Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework. Let p∈M and let U0∈TpM be a future timelike unit vector, gp(U0,U0)=−c2 (Timelike, null, spacelike and causal vectors of a Lorentz vector space).

Suppose B1 and B2 are two ideal freely falling massive test bodies of the model that are released at the event p with physical four-velocity U0: their worldlines γi:Ii→M pass through p and their four-vectors there equal U0. Let τi be their proper times, with origins chosen so that 0∈Ii and γi(0)=p. Let γp,U0:Ip,U0→M be the unique maximal geodesic through (p,U0). Then each physical worldline is a restriction of that maximal geodesic:

Ii⊆Ip,U0,γi(τ)=γp,U0(τ)(τ∈Ii),i=1,2.

In particular, γ1 and γ2 coincide wherever both are defined. The theorem does not assume that either physical worldline has the entire maximal geodesic's domain. The unique geodesic continuation is determined by the release event and the initial four-velocity alone; parameters that distinguish the two bodies, such as their rest masses, do not enter.

Facts & Assumptions

Given: A smooth model as in the statement, an event p, a future timelike unit vector U0∈TpM, and two ideal freely falling massive test bodies B1,B2 released at p with four-velocity U0.

[A1]

Clause (ii) of Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework is the adopted physical assumption that an ideal freely falling massive test body has as worldline a future timelike geodesic of the metric-selected connection, traversed with physical four-velocity U=dγ/dτ satisfying g(U,U)=−c2; clause (i) is the adopted assumption that an ideal clock measures the proper time of its worldline.

[L1]

For the metric-selected connection there is, for every (p,v)∈TM, a unique maximal geodesic with γ(0)=p and γ′(0)=v, and every geodesic with those data is its restriction. Proper time is an affine parameter of a future timelike geodesic, and along it the four-velocity is dγ/dτ, with Dτ(dγ/dτ)=0 (The geodesic initial-value problem and the exponential map of the metric-selected connection, Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent, Geodesic of an affine connection).

[L2]

A worldline with four-velocity U satisfies g(U,U)=−c2 and is future-directed; proper time is strictly increasing along it, so the proper-time parametrization is a bijection from its parameter interval onto its image (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold, Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent).

Proof

technique · direct
1.1A1L2given

For i=1,2, [A1] makes the worldline of Bi a future timelike geodesic traversed with four-velocity Ui=dγi/dτi satisfying g(Ui,Ui)=−c2, and the four-vector of Bi at p is its tangent with respect to its own proper time at the parameter value where it passes through p. Choosing the proper-time origins so that this value is 0, we have γi(0)=p and, by the hypothesis, Ui(0)=U0.

2.1step 1.1L1algebra

By [L1], there is a unique maximal geodesic γp,U0 with γp,U0(0)=p and γp,U0′(0)=U0, and every geodesic with these data is its restriction. Applying this to γ1 and γ2 from step 1.1 gives Ii⊆Ip,U0 and γi=γp,U0∣Ii for each i. They therefore agree at every common proper-time value, while their own domains need not be maximal.

3.1step 2.1A1L1algebra∎

The initial data of the geodesic initial-value problem are the event p and tangent vector U0; the geodesic equation Dτ(dγ/dτ)=0 and its maximal solution contain no rest mass, charge, or other parameter of the body, and clause (ii) of [A1] requires each physical worldline only to be a future timelike geodesic. Therefore the unique geodesic continuation, and the values of each physical worldline wherever defined, are determined by (p,U0) alone; the rest masses or other distinguishing parameters of B1 and B2 do not affect them.

Remarks

  • Model statement, not an empirical law. The theorem is a conditional consequence of the adopted free-fall rule and the mathematical initial-value theory. It does not assert that bodies in nature fall alike, does not test the equivalence principle, and carries the test-body exclusions of Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework: negligible self-field, no self-force or radiation back-reaction, internal structure small compared with the variation scale of the geometry, and no quantum effects. Empirical comparisons of free-fall universality are separate reported observations with their own apparatus, calibration and uncertainty qualifications; none is recorded here.

  • No new empirical premises. The proof uses no measured input and no experiment as a premise, so no empirical_premises entries are attached; the conclusion inherits the model and idealization qualifications of the postulate.

RemarkRemark: AI-adaptedProof: Not applicableOpen item page →

Scope of normal coordinates and of the local-inertial-frame reading

Physical scope

Scope note on the physical reading of point-normal and exponential coordinate charts: what the construction does and does not assert about local inertial frames, freely falling observers and the equivalence principle in the classical smooth model. Excludes global frames, neighborhood flatness, curvature claims, and any empirical equivalence-principle statement.

Scope note

This remark separates the mathematics of Point-normal and exponential coordinate charts of the metric-selected connection and The geodesic initial-value problem and the exponential map of the metric-selected connection from the physical reading usually attached to them, and is bookkeeping: it establishes no mathematical result and no physical law.

  • What the construction gives. For every event p there is a chart with gab(p)=ηab, Γabc(p)=0 and ∂agbc(p)=0. In the exponential chart from an orthonormal basis, each geodesic through p is the straight radial coordinate line while its initial vector remains in the chosen star-shaped exponential domain (Point-normal and exponential coordinate charts of the metric-selected connection). The identities are first order at the single point p.

  • What it does not give. The construction asserts nothing about the second and higher derivatives of the metric, and therefore nothing about the curvature of the model; a chart of this kind is not an isometry and does not make any neighborhood of p identical with a region of Minkowski space. The remark makes no curvature claim here; the second-order behavior is the subject of the curvature material of this track, which is a later page of the same category.

  • No global inertial frame, no congruence. A chart with the normal-form identities at one event is not a global label of events by inertial coordinates, and the exponential charts at different points are not compatible frames. An "observer" in this library is a single future unit timelike vector at a point, and a "congruence" is a field of such vectors on an open set (Observers, rest spaces and the spatial projection at an event, Observer congruences, their observer curves and adapted charts); a freely falling observer is one timelike geodesic, not a global reference frame. Charts adapted to a congruence are a different construction from the normal coordinates of a geodesic through a point.

  • The physical reading is adopted, not derived. The statement that an ideal freely falling test body or observer, using normal coordinates around an event of its own worldline, finds the local form of the metric to be that of Minkowski space at first order — and the associated local inertial-frame reading of the equivalence principle — depends on the adopted clock and free-fall assumptions of Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework. It is a statement about the model in the test-body idealization, not a derivation from the geometry alone and not an empirical claim that real experiments cannot detect a gravitational field locally. The limitations recorded in the postulate — finite-size and tidal couplings of extended bodies, self-force, and nonlocal measurements — are precisely what the first-order identities cannot exclude.

5 · Examples, experiments and counterexamples

None yet.

Sources