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The Rindler chart: causal horizons of a uniformly accelerated observer and the restrictions of radar time and distance

Physical scope

Conditional model statements about a uniformly accelerated ideal observer in flat classical special relativity: the domain of the Rindler chart, the causal past and future boundaries (horizons) of the congruence worldlines, and the radar time and distance assigned to coaxial congruence worldlines by ideal light signals and ideal clocks. Excludes gravitation, media and dispersion, real apparatus, finite resolution, quantum fields and the Unruh effect, and material models of the reflector; no measurement, statistical or empirical claim is made.

Statement

Adopt Adopted inertial covariance of the model equations, Adopted ideal-clock and ideal-vacuum-light interpretation and The causal signal restriction of the model, and the SI conventions of SI units and coordinate conventions of the special-relativity framework (x0=ct). Let x=(x0,x1,x2,x3) be the chart of an inertial frame (Inertial frames and inertial charts of the affine Minkowski model) and let W:={x1>∣x0∣} be the right wedge. Let Φ and n be the Rindler chart and congruence of Fermi-Walker transport preserves the metric, and explicit rigid and non-rigid observer congruences (b): Φ(θ,ρ,y,z)=(ρsinh⁡θ,ρcosh⁡θ,y,z) on R×(0,∞)×R2 with inverse ρ=(x1)2−(x0)2, θ=12log⁡((x1+x0)/(x1−x0)), pullback metric −ρ2dθ2+dρ2+dy2+dz2, and acceleration field acg=∇nn=ρ−1∂ρ. Fix ρ0>0 and real y0,z0, and let O be the congruence worldline ρ=ρ0, y=y0, z=z0, parametrized by its proper time τ with θ=cτ/ρ0; by Proper acceleration of a massive worldline and its agreement with the acceleration of an observer congruence its proper acceleration is c2/ρ0. Write U(q):=q0+q1 and V(q):=q0−q1 for events q, so that U=ρeθ and V=−ρe−θ on W, and write ≤ and J+, J− for the causal reachability relations of Causal reachability, causal futures and pasts, causal diamonds, and reachability by future causal paths in affine Minkowski space. Then, conditionally on the adopted model:

(i) Chart domain and light rays. Φ is a smooth bijection of R×(0,∞)×R2 onto W with the stated smooth inverse, so the chart domain is exactly W and ρ=0 is not part of its coordinate domain. The boundary of W in the affine model is {x1=∣x0∣}, with arbitrary x2,x3: it is the union of the two null half-planes {x1=x0≥0} and {x1=−x0≥0}. These half-planes are portions of the full null planes appearing as causal horizons in (ii); the full planes are not the wedge boundary. Along the worldline ρ=ρ0 one has V=−ρ0e−θ→0− and U→+∞ as θ→+∞, while U=ρ0eθ→0+ and V→−∞ as θ→−∞. The future null straight lines of the model that lie in the plane y=y0, z=z0 and meet O are exactly the lines of constant V (on which dθ=+dρ/ρ) and the lines of constant U (on which dθ=−dρ/ρ).

(ii) Causal horizons. An event q satisfies q≤p for some event p of O if and only if V(q)<0; an event q satisfies p≤q for some event p of O if and only if U(q)>0. Consequently no event with V(q)≥0 can ever influence O; this set contains the null plane {x1=x0}, the left wedge {x1<−∣x0∣} and the future wedge {x0>∣x1∣}; and no event with U(q)≤0 can ever be influenced by O, a set containing the null plane {x1=−x0}, the left wedge and the past wedge {x0<−∣x1∣}. The null plane {x1=x0} is the boundary of the causal past of O (the future horizon: the surface its worldline approaches as θ→+∞), and the null plane {x1=−x0} is the boundary of the causal future of O (the past horizon); every event of the left wedge is causally unrelated to O in both directions. The same criteria with O any other congruence worldline ρ=ρ1, y=y1, z=z1 hold verbatim: the constants ρ0, y0, z0 do not enter.

(iii) Radar time and distance to a coaxial congruence reflector. Fix ρm>0 with ρm≠ρ0 and let Rm be the congruence worldline ρ=ρm, y=y0, z=z0 (a second uniformly accelerated observer, coaxial with O, with proper acceleration c2/ρm). Let e− be the event of O at parameter θe (so τ(e−)=ρ0θe/c up to the base point of τ), let qm be the event of Rm lying on the future null straight line from e− in the plane y=y0, z=z0, and let e+ be the event of O lying on the future null straight line from qm; the reflection at qm is idealized as instantaneous and as leaving Rm's motion unchanged, as in The operational radar protocol of an ideal observer. Then e−,qm,e+ exist uniquely, the Rindler time of qm is θm=θe+∣log⁡(ρm/ρ0)∣, the return event satisfies θ(e+)=θe+2∣log⁡(ρm/ρ0)∣ and (θe+θ(e+))/2=θm, so the round trip lasts 2∣log⁡(ρm/ρ0)∣ in Rindler time and (2ρ0/c)∣log⁡(ρm/ρ0)∣ in O's proper time. The radar protocol therefore assigns to qm the radar time τrad(qm)=(ρ0/c)θm plus the base constant of τ and the radar distance ρrad(qm)=ρ0∣log⁡(ρm/ρ0)∣; within this coaxial family the radar-time level sets are the intersections of the Rindler rest slices θ=const with y=y0, z=z0, excluding the observer radius ρ0 (Simultaneity slices and rest distance relative to a future unit timelike vector). The radar distance is not the rest distance: in the slice θ=θm the two worldlines are at rest distance ∣ρm−ρ0∣, whereas for ρm=2ρ0 the radar distance is ρ0log⁡2<ρ0, because log⁡ is strictly increasing and e>2 implies log⁡2<log⁡e=1 (The elementary numerical bound 2<e<3, Order, continuity, range, and the product, quotient, and reciprocal laws for the natural logarithm). For every distinct positive reflector radius the notions differ: with r=ρm/ρ0, one has log⁡r<r−1 when r>1 and −log⁡r>1−r when 0<r<1. The two distance formulas agree only at r=1, where both have the continuous degenerate value zero. The coincident case is not a nonzero emission-reflection-reception triple of the protocol, whose distinct-reflector hypothesis remains in force. As ρm→0+ the round-trip proper time and the radar distance grow without bound while the reflector's proper acceleration c2/ρm diverges; as ρm→+∞ the round-trip proper time and the radar distance also grow without bound while the reflector's proper acceleration tends to 0.

(iv) Restrictions of the protocol. No event with V≥0 --- in particular no event of the horizon plane {x1=x0}, of the left wedge or of the future wedge --- can be assigned a radar time or radar distance by this protocol from O, because by (ii) it cannot causally precede any reception event on O: the required reflection-to-reception leg is impossible. Separately, every event with U≤0 lacks an emission-to-reflection leg from O. Thus any event admitting this radar triple must satisfy U>0 and V<0, equivalently it must belong to W; the horizon is at infinite radar distance in the limit ρm→0+. For example q=x−1(2ρ0,0,y0,z0) has U(q)=V(q)=2ρ0>0. It is causally after O at θ=0, since the displacement is (2ρ0,−ρ0,0,0), future timelike, and it even lies on a future null ray from O at θ=log⁡2, with displacement (5ρ0/4,−5ρ0/4,0,0). Nevertheless it cannot send a causal return to O, so it receives no radar assignment from O. The protocol therefore does not extend to a global coordinate system of A.

(v) Scope. All clauses are conditional computations and readings in flat classical spacetime with ideal clocks, ideal light rays and ideal reflectors, for the specified congruence worldlines. They are not empirical claims and contain no measurement, apparatus, source, detector or statistical content; gravitation, media, dispersion, finite resolution, quantum effects and material models of the reflector are excluded. No choice principle is used.

Facts & Assumptions

Given: The adopted model: affine Minkowski space (A,V,η,C+) with inertial chart x, x0=ct; ideal clocks and light rays; the causal signal restriction; the Rindler chart and congruence data of the statement; ρ0>0, real y0,z0; the worldline O with θ=cτ/ρ0; U(q)=q0+q1, V(q)=q0−q1; and, in (iii), ρm>0 with ρm≠ρ0 and the coaxial worldline Rm.

[L1]

Adopted framework assumptions: the affine Minkowski model is the framework's spacetime; ideal clocks read the proper time of their worldline; ideal vacuum light rays are the future null straight lines with coordinate speed c; and an idealized signal transmission from p to q is admitted only if q∈J+(p) (Adopted inertial covariance of the model equations, Adopted ideal-clock and ideal-vacuum-light interpretation, The causal signal restriction of the model).

[L2]

Coordinates and model: in every inertial chart x0=ct, η=diag⁡(−1,1,1,1) in the orthonormal frame, and points are determined by their coordinates (SI units and coordinate conventions of the special-relativity framework, Inertial frames and inertial charts of the affine Minkowski model, Oriented time-oriented affine Minkowski space (the spacetime primitives)).

[L3]

Rindler data: Φ(θ,ρ,y,z)=(ρsinh⁡θ,ρcosh⁡θ,y,z) is a smooth bijection of R×(0,∞)×R2 onto the right wedge W={x1>∣x0∣} with smooth inverse ρ=(x1)2−(x0)2, θ=12log⁡x1+x0x1−x0, pullback metric −ρ2dθ2+dρ2+dy2+dz2; n=ρ−1∂θ is future unit timelike with acg=∇nn=ρ−1∂ρ and η(acg,acg)=ρ−2; the rest slices θ=const are the intersections with W of affine hyperplanes orthogonal to n with induced metric dρ2+dy2+dz2 (Fermi-Walker transport preserves the metric, and explicit rigid and non-rigid observer congruences (b)).

[L5]

Causal structure: a vector is timelike iff η(v,v)<0 and null iff nonzero with η(v,v)=0, and each nonzero causal vector is future or past; C+={v:v0>∣vs∣}, Cˉ+={v:v0≥∣vs∣} in every inertial chart; for q≠p, q∈J+(p) iff the straight segment from p to q is a future causal path; and the causal reachability relations are those of Causal reachability, causal futures and pasts, causal diamonds, and reachability by future causal paths in affine Minkowski space (Timelike, null, spacelike and causal vectors of a Lorentz vector space, Time orientation, future and past timelike/null/causal vectors, and the closed cones, The closed future cone in inertial coordinates: description, finite sums, and the coordinate criterion for causal reachability (a),(c), Future causal reachability, absence of causal loops, time monotonicity and the straight-worldline proper-time maximum (b), Curves, regular causal curves and future timelike worldlines in affine Minkowski space (a),(b)).

[L6]

Radar protocol: the radar time of a reflected event q with emission e− and reception e+ on the observer's worldline is the midpoint proper time τrad(q)=(τ(s−)+τ(s+))/2 and the radar distance is c(τ(s+)−τ(s−))/2; the protocol is conditional on the existence of the three events and uses the symmetric half-split convention (The operational radar protocol of an ideal observer).

[L7]

Rest distance: in a simultaneity slice of a future unit timelike n, the rest distance of two events is η(q−p,q−p) (Simultaneity slices and rest distance relative to a future unit timelike vector (a),(d)).

[L8]

Logarithm: log⁡:(0,∞)→R is continuous and strictly increasing with log⁡1=0, log⁡(xy)=log⁡x+log⁡y and log⁡(1/x)=−log⁡x; log⁡ is differentiable with log⁡′x=1/x, and the mean value theorem applies to it on closed intervals with the endpoint continuity supplied by differentiability (The natural logarithm as the inverse of the exponential function, Order, continuity, range, and the product, quotient, and reciprocal laws for the natural logarithm, The natural logarithm has derivative 1/x and equals the integral from 1 to x of 1/t, The mean value theorem, as the case g(x)=x of Cauchy's: for f continuous on [a,b] with a<b and differentiable on (a,b) there is c∈(a,b) with f(b)−f(a)=f′(c)(b−a), A function differentiable at c is continuous at c).

[L9]

Exponential and hyperbolic data: eu→+∞ as u→+∞, eu→0 as u→−∞, 2<e<3 with log⁡e=1; sinh⁡u=(eu−e−u)/2, cosh⁡u=(eu+e−u)/2, cosh⁡2u−sinh⁡2u=1, and cosh⁡u±sinh⁡u=e±u (The exponential tends to +∞ at +∞ and to 0 at −∞, The elementary numerical bound 2<e<3, The six hyperbolic functions and their natural domains, Addition formulas, identities, parity, and derivatives of the hyperbolic functions, The exponential addition formula exp⁡(x+y)=exp⁡(x)exp⁡(y)).

Proof

technique · direct
1.1L2L3algebra

(Chart domain, wedge and boundary.) From [L3], Φ is a smooth bijection onto W with the stated smooth inverse defined for x1>∣x0∣, so the coordinate domain is exactly W and ρ=0 is excluded; on W the coordinates satisfy U=ρeθ>0 and V=−ρe−θ<0, and conversely U>0 and V<0 define W, since x1=(U−V)/2>∣x0∣=∣U+V∣/2 is equivalent to U>0,V<0. The boundary is x1=∣x0∣, split into the two half-planes x1=x0≥0 (where V=0, U≥0) and x1=−x0≥0 (where U=0, V≤0); these are the parts of the full null planes V=0 and U=0 that bound W, while the full planes extend beyond.

1.2L3L4algebra

(The worldline O and its parametrization.) By [L3] the curve θ↦Φ(θ,ρ0,y0,z0) is a flow line of n=ρ−1∂θ restricted to ρ=ρ0; its tangent with respect to θ is ∂θ=ρ0n, so by [L4] its four-velocity is cn, its proper time satisfies dτ=ρ0 dθ/c, i.e. θ=cτ/ρ0 up to an additive constant, and its proper acceleration is c2/ρ0. Along it, U=ρ0eθ and V=−ρ0e−θ.

1.3L3L5algebra

(The future null lines of the plane through O.) Let p,q be events in the plane y=y0, z=z0 and w:=q−p. Since w2=w3=0, one has ΔU:=U(q)−U(p)=w0+w1, ΔV:=V(q)−V(p)=w0−w1, and ΔUΔV=(w0)2−(w1)2; hence w∈Cˉ+ iff ΔU≥0, ΔV≥0 and ΔUΔV≥0, and w is future null iff in addition ΔUΔV=(w2)2+(w3)2=0, i.e. iff either ΔV=0<ΔU or ΔU=0<ΔV. Differentiating U=ρeθ and V=−ρe−θ along a curve in W gives dU=eθ(dρ+ρ dθ) and dV=−e−θ(dρ−ρ dθ), so the future null lines through a point of O in the plane are exactly the constant-U lines (dθ=−dρ/ρ) and the constant-V lines (dθ=+dρ/ρ).

1.4L8L9algebra

(The logarithmic inequality.) For r>0 with r≠1, the mean value theorem applied to log⁡ on the interval between 1 and r gives log⁡r−log⁡1=1ζ(r−1) for some ζ strictly between 1 and r; since ζ>1 when r>1 this gives log⁡r<r−1, and since 0<ζ<1 when 0<r<1 it gives −log⁡r>1−r; equality holds only at r=1. In particular log⁡2<2−1=1, and also e>2 gives log⁡2<log⁡e=1 by strict increase of log⁡.

2.1L5step 1.1step 1.3algebra

(Causal criteria for the worldline O.) For an arbitrary displacement w, w∈Cˉ+ is equivalent to ΔU≥0, ΔV≥0 and ΔUΔV≥(w2)2+(w3)2: this follows from w0=(ΔU+ΔV)/2 and η(w,w)=−ΔUΔV+(w2)2+(w3)2 and the inertial cone criterion [L5]. (Forward.) Let q≤p with p on O, so w=p−q∈Cˉ+; then ΔV=V(p)−V(q)≥0 and V(p)=−ρ0e−θp<0, so V(q)≤V(p)<0. Similarly ΔU≥0 with U(p)>0 gives nothing yet, but the same argument with the roles of U and V reversed and the sign of ρ0eθp shows U(q)≤U(p); to obtain U(q)>0 from p≤q one uses w=q−p∈Cˉ+: then U(q)−U(p)≥0 and U(p)=ρ0eθp>0, so U(q)≥U(p)>0; and V(q)≥V(p) gives no upper bound. (Reverse.) Suppose V(q)<0; choose θp with −ρ0e−θp>V(q), i.e. V(p)>V(q), which is possible because −ρ0e−θp→0− as θp→+∞; then ΔV>0, and ΔU=ρ0eθp−U(q) and ΔUΔV tend to +∞ as θp→+∞ while the transverse displacement (y0−q2,z0−q3) is fixed, so for all sufficiently large θp the three general inequalities just established hold and q≤p. Similarly, if U(q)>0, choose θp very negative so that U(p)=ρ0eθp<U(q) and ΔU>0, while ΔV=V(q)+ρ0e−θp→+∞; then ΔUΔV→+∞ and p≤q for all sufficiently negative θp. Hence the criteria, and since the construction used only the positivity of ρ0 and the fixed transverse coordinates of the worldline, the same criteria hold for every congruence worldline ρ=ρ1, y=y1, z=z1. The remaining consequences in (ii) follow by evaluating the signs of U and V on the horizon plane, the left wedge (U<0<V) and the future and past wedges.

2.2L9step 1.2algebra

(Limits along O and along the reflector family.) By [L9], ρ0e−θ→0 and ρ0eθ→+∞ as θ→+∞, while ρ0eθ→0 and ρ0e−θ→+∞ as θ→−∞; hence along O, V=−ρ0e−θ→0− and U→+∞ as θ→+∞, and U→0+ with V→−∞ as θ→−∞.

2.3step 1.2step 1.3algebra

(Clause (iii): the radar geometry.) Suppose first ρm>ρ0. The constant-V future null line from e−=(θe,ρ0) has V=−ρ0e−θe, and its intersection with ρ=ρm is at the unique θm with −ρme−θm=−ρ0e−θe, i.e. θm=θe+log⁡(ρm/ρ0)=θe+∣log⁡(ρm/ρ0)∣ since ρm>ρ0; the return leg must be the constant-U line through qm=(θm,ρm) (the constant-V line leaves ρ increasing), and it meets ρ=ρ0 at the unique θ(e+) with ρ0eθ(e+)=ρmeθm, i.e. θ(e+)=θm+log⁡(ρm/ρ0)=θe+2log⁡(ρm/ρ0). If instead 0<ρm<ρ0, the same computation with the roles of U and V exchanged, using the two formulas U=ρeθ and V=−ρe−θ, gives θm=θe+log⁡(ρ0/ρm) and θ(e+)=θm+log⁡(ρ0/ρm), i.e. in both cases θm=θe+∣log⁡(ρm/ρ0)∣ and θ(e+)=θe+2∣log⁡(ρm/ρ0)∣ with midpoint θm. Uniqueness of qm and e+ holds because each constant-U or constant-V line meets each of the lines ρ=const>0 exactly once, and e−≤qm and qm≤e+ are future null by step 1.3.

3.1step 1.1step 1.3step 2.2

(Clause (i).) Step 1.1 gives the bijection, its domain, the boundary description and the identification of the horizon planes with V=0 and U=0 on the wedge closure; step 1.3 identifies the two families of future null lines in the plane through O with the constant-V and constant-U lines and their differential equations; step 2.2 gives the asymptotic limits of U and V along O.

3.2step 2.1step 2.2algebra

(Clause (ii).) The two criteria are step 2.1; the stated consequences for the horizon planes, the left wedge and the future and past wedges follow by computing U and V there, using that x1<−∣x0∣ gives U<0 and V>0, x0>∣x1∣ gives U>0,V>0, and x0<−∣x1∣ gives U<0,V<0; the horizon interpretations as boundary of the causal past and future of O follow from the two criteria together with the limits of step 2.2, and the invariance in ρ1,y1,z1 is the last sentence of step 2.1.

3.3L3L6L7step 1.2step 1.4step 2.3algebra

(Clause (iii): the radar assignments and the distance comparison.) By [L6] and step 2.3, the radar time is τrad(qm)=(τ(e−)+τ(e+))/2=(ρ0/c)θm+τ0, since θ=cτ/ρ0+const along O by step 1.2, and the radar distance is ρrad(qm)=c(τ(e+)−τ(e−))/2=ρ0∣log⁡(ρm/ρ0)∣; the radar-time level sets in the coaxial family are the sets θm=const, which are precisely the restrictions of the Rindler rest slices to y=y0, z=z0, ρ≠ρ0; indeed every such qm has emission parameter θe=θm−∣log⁡(ρm/ρ0)∣, and [L3] identifies the unrestricted θ-level slices as rest slices. The rest distance in the slice θ=θm is ∣ρm−ρ0∣ by [L7] and the induced metric dρ2+dy2+dz2 of [L3]. With r=ρm/ρ0≠1, the radar distance is ρ0∣log⁡r∣ and the rest distance is ρ0∣r−1∣, so by step 1.4 the radar distance is strictly smaller than the rest distance for r>1 and strictly larger for 0<r<1, with equality only in the degenerate case r=1 in which both are zero; in particular at ρm=2ρ0, ρ0log⁡2<ρ0.

3.4L1L5L9step 2.1algebra

(Clause (iv): the restrictions, and the example.) Let q admit a radar triple e−,q,e+ from O; by the ideal-light and signal assumptions of [L1], the emission and reflection legs give e−≤q and q≤e+ with e−,e+ on O, so by step 2.1's criteria U(q)>0 and V(q)<0, i.e. q∈W; conversely every event with V≥0 fails q≤p for all p∈O and every event with U≤0 fails p≤q, so those events receive no radar assignment. For the example q=x−1(2ρ0,0,y0,z0): U(q)=V(q)=2ρ0, and its displacement from the event of O at θ=0 is (2ρ0,−ρ0,0,0), with η=−4ρ02+ρ02=−3ρ02<0 and positive time component, hence future timelike, so q is causally after that event by [L5]; the displacement from the event of O at θ=log⁡2, namely (ρ0sinh⁡log⁡2,ρ0cosh⁡log⁡2,0,0)=(34ρ0,54ρ0,0,0) by [L9], is (5ρ0/4,−5ρ0/4,0,0), future null, so q lies on a future null ray from O; but V(q)=2ρ0≥0, so by the criterion q cannot reach any event of O and receives no radar assignment, showing that the protocol does not extend even to events causally after O.

4.1L4L8step 3.3algebra

(Clause (iii): the limiting cases.) As ρm→0+ we have ∣log⁡(ρm/ρ0)∣→+∞ by strict increase and unboundedness of log⁡ (equivalently log⁡(ρ0/ρm)→+∞), so the round-trip proper time (2ρ0/c)∣log⁡(ρm/ρ0)∣ and the radar distance ρ0∣log⁡(ρm/ρ0)∣ grow without bound, while the reflector's proper acceleration c2/ρm→+∞ by [L4]; as ρm→+∞ the same divergence of ∣log⁡(ρm/ρ0)∣ holds while c2/ρm→0+.

5.1step 3.1step 3.2step 3.3step 4.1step 3.4∎

(Clause (v): scope.) Every clause was computed from the adopted model and the cited mathematical suppliers; the several limiting cases (equal radii excluded, the degenerate r=1 value, the two null half-planes versus the full horizon planes, the two limiting reflector radii) were treated explicitly. No apparatus, measurement, statistical or empirical input enters, no choice principle was used, and the statements are conditional model computations.

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