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The Rindler chart: causal horizons of a uniformly accelerated observer and the restrictions of radar time and distance
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 (). Let be the chart of an inertial frame (Inertial frames and inertial charts of the affine Minkowski model) and let be the right wedge. Let and be the Rindler chart and congruence of Fermi-Walker transport preserves the metric, and explicit rigid and non-rigid observer congruences (b): on with inverse , , pullback metric , and acceleration field . Fix and real , and let be the congruence worldline , , , parametrized by its proper time with ; by Proper acceleration of a massive worldline and its agreement with the acceleration of an observer congruence its proper acceleration is . Write and for events , so that and on , and write and , 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. is a smooth bijection of onto with the stated smooth inverse, so the chart domain is exactly and is not part of its coordinate domain. The boundary of in the affine model is , with arbitrary : it is the union of the two null half-planes and . 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 one has and as , while and as . The future null straight lines of the model that lie in the plane , and meet are exactly the lines of constant (on which ) and the lines of constant (on which ).
(ii) Causal horizons. An event satisfies for some event of if and only if ; an event satisfies for some event of if and only if . Consequently no event with can ever influence ; this set contains the null plane , the left wedge and the future wedge ; and no event with can ever be influenced by , a set containing the null plane , the left wedge and the past wedge . The null plane is the boundary of the causal past of (the future horizon: the surface its worldline approaches as ), and the null plane is the boundary of the causal future of (the past horizon); every event of the left wedge is causally unrelated to in both directions. The same criteria with any other congruence worldline , , hold verbatim: the constants , , do not enter.
(iii) Radar time and distance to a coaxial congruence reflector. Fix with and let be the congruence worldline , , (a second uniformly accelerated observer, coaxial with , with proper acceleration ). Let be the event of at parameter (so up to the base point of ), let be the event of lying on the future null straight line from in the plane , , and let be the event of lying on the future null straight line from ; the reflection at is idealized as instantaneous and as leaving 's motion unchanged, as in The operational radar protocol of an ideal observer. Then exist uniquely, the Rindler time of is , the return event satisfies and , so the round trip lasts in Rindler time and in 's proper time. The radar protocol therefore assigns to the radar time plus the base constant of and the radar distance ; within this coaxial family the radar-time level sets are the intersections of the Rindler rest slices with , , excluding the observer radius (Simultaneity slices and rest distance relative to a future unit timelike vector). The radar distance is not the rest distance: in the slice the two worldlines are at rest distance , whereas for the radar distance is , because is strictly increasing and implies (The elementary numerical bound , Order, continuity, range, and the product, quotient, and reciprocal laws for the natural logarithm). For every distinct positive reflector radius the notions differ: with , one has when and when . The two distance formulas agree only at , 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 the round-trip proper time and the radar distance grow without bound while the reflector's proper acceleration diverges; as the round-trip proper time and the radar distance also grow without bound while the reflector's proper acceleration tends to .
(iv) Restrictions of the protocol. No event with --- in particular no event of the horizon plane , of the left wedge or of the future wedge --- can be assigned a radar time or radar distance by this protocol from , because by (ii) it cannot causally precede any reception event on : the required reflection-to-reception leg is impossible. Separately, every event with lacks an emission-to-reflection leg from . Thus any event admitting this radar triple must satisfy and , equivalently it must belong to ; the horizon is at infinite radar distance in the limit . For example has . It is causally after at , since the displacement is , future timelike, and it even lies on a future null ray from at , with displacement . Nevertheless it cannot send a causal return to , so it receives no radar assignment from . The protocol therefore does not extend to a global coordinate system of .
(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 with inertial chart , ; ideal clocks and light rays; the causal signal restriction; the Rindler chart and congruence data of the statement; , real ; the worldline with ; , ; and, in (iii), with and the coaxial worldline .
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 ; and an idealized signal transmission from to is admitted only if (Adopted inertial covariance of the model equations, Adopted ideal-clock and ideal-vacuum-light interpretation, The causal signal restriction of the model).
Coordinates and model: in every inertial chart , 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)).
Rindler data: is a smooth bijection of onto the right wedge with smooth inverse , , pullback metric ; is future unit timelike with and ; the rest slices are the intersections with of affine hyperplanes orthogonal to with induced metric (Fermi-Walker transport preserves the metric, and explicit rigid and non-rigid observer congruences (b)).
Congruence flow lines and proper acceleration: a flow line of with tangent has four-velocity and proper time ; its proper acceleration is (Kinematics of an observer congruence: acceleration, expansion, shear, vorticity and Born rigidity (b), Four-velocity and four-acceleration of a future timelike worldline (a),(c), Proper time along a future timelike worldline, The proper-time function is a strictly increasing C^1 parametrization with C^1 inverse, Norms of four-velocity and four-acceleration, and the observer rest-space decomposition (a), Proper acceleration of a massive worldline and its agreement with the acceleration of an observer congruence (b)).
Causal structure: a vector is timelike iff and null iff nonzero with , and each nonzero causal vector is future or past; , in every inertial chart; for , iff the straight segment from to 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)).
Radar protocol: the radar time of a reflected event with emission and reception on the observer's worldline is the midpoint proper time and the radar distance is ; 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).
Rest distance: in a simultaneity slice of a future unit timelike , the rest distance of two events is (Simultaneity slices and rest distance relative to a future unit timelike vector (a),(d)).
Logarithm: is continuous and strictly increasing with , and ; is differentiable with , 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 of Cauchy's: for continuous on with and differentiable on there is with , A function differentiable at is continuous at ).
Exponential and hyperbolic data: as , as , with ; , , , and (The exponential tends to at and to at , The elementary numerical bound , The six hyperbolic functions and their natural domains, Addition formulas, identities, parity, and derivatives of the hyperbolic functions, The exponential addition formula ).
Proof
(Chart domain, wedge and boundary.) From [L3], is a smooth bijection onto with the stated smooth inverse defined for , so the coordinate domain is exactly and is excluded; on the coordinates satisfy and , and conversely and define , since is equivalent to . The boundary is , split into the two half-planes (where , ) and (where , ); these are the parts of the full null planes and that bound , while the full planes extend beyond.
(The worldline and its parametrization.) By [L3] the curve is a flow line of restricted to ; its tangent with respect to is , so by [L4] its four-velocity is , its proper time satisfies , i.e. up to an additive constant, and its proper acceleration is . Along it, and .
(The future null lines of the plane through .) Let be events in the plane , and . Since , one has , , and ; hence iff , and , and is future null iff in addition , i.e. iff either or . Differentiating and along a curve in gives and , so the future null lines through a point of in the plane are exactly the constant- lines () and the constant- lines ().
(The logarithmic inequality.) For with , the mean value theorem applied to on the interval between and gives for some strictly between and ; since when this gives , and since when it gives ; equality holds only at . In particular , and also gives by strict increase of .
(Causal criteria for the worldline .) For an arbitrary displacement , is equivalent to , and : this follows from and and the inertial cone criterion [L5]. (Forward.) Let with on , so ; then and , so . Similarly with gives nothing yet, but the same argument with the roles of and reversed and the sign of shows ; to obtain from one uses : then and , so ; and gives no upper bound. (Reverse.) Suppose ; choose with , i.e. , which is possible because as ; then , and and tend to as while the transverse displacement is fixed, so for all sufficiently large the three general inequalities just established hold and . Similarly, if , choose very negative so that and , while ; then and for all sufficiently negative . Hence the criteria, and since the construction used only the positivity of and the fixed transverse coordinates of the worldline, the same criteria hold for every congruence worldline , , . The remaining consequences in (ii) follow by evaluating the signs of and on the horizon plane, the left wedge () and the future and past wedges.
(Limits along and along the reflector family.) By [L9], and as , while and as ; hence along , and as , and with as .
(Clause (iii): the radar geometry.) Suppose first . The constant- future null line from has , and its intersection with is at the unique with , i.e. since ; the return leg must be the constant- line through (the constant- line leaves increasing), and it meets at the unique with , i.e. . If instead , the same computation with the roles of and exchanged, using the two formulas and , gives and , i.e. in both cases and with midpoint . Uniqueness of and holds because each constant- or constant- line meets each of the lines exactly once, and and are future null by step 1.3.
(Clause (i).) Step 1.1 gives the bijection, its domain, the boundary description and the identification of the horizon planes with and on the wedge closure; step 1.3 identifies the two families of future null lines in the plane through with the constant- and constant- lines and their differential equations; step 2.2 gives the asymptotic limits of and along .
(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 and there, using that gives and , gives , and gives ; the horizon interpretations as boundary of the causal past and future of follow from the two criteria together with the limits of step 2.2, and the invariance in is the last sentence of step 2.1.
(Clause (iii): the radar assignments and the distance comparison.) By [L6] and step 2.3, the radar time is , since along by step 1.2, and the radar distance is ; the radar-time level sets in the coaxial family are the sets , which are precisely the restrictions of the Rindler rest slices to , , ; indeed every such has emission parameter , and [L3] identifies the unrestricted -level slices as rest slices. The rest distance in the slice is by [L7] and the induced metric of [L3]. With , the radar distance is and the rest distance is , so by step 1.4 the radar distance is strictly smaller than the rest distance for and strictly larger for , with equality only in the degenerate case in which both are zero; in particular at , .
(Clause (iv): the restrictions, and the example.) Let admit a radar triple from ; by the ideal-light and signal assumptions of [L1], the emission and reflection legs give and with on , so by step 2.1's criteria and , i.e. ; conversely every event with fails for all and every event with fails , so those events receive no radar assignment. For the example : , and its displacement from the event of at is , with and positive time component, hence future timelike, so is causally after that event by [L5]; the displacement from the event of at , namely by [L9], is , future null, so lies on a future null ray from ; but , so by the criterion cannot reach any event of and receives no radar assignment, showing that the protocol does not extend even to events causally after .
(Clause (iii): the limiting cases.) As we have by strict increase and unboundedness of (equivalently ), so the round-trip proper time and the radar distance grow without bound, while the reflector's proper acceleration by [L4]; as the same divergence of holds while .
(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 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.
Depends on
Proper acceleration of a massive worldline and its agreement with the acceleration of an observer congruence
The uniformly accelerated worldline: hyperbolic motion, constant four-acceleration magnitude, and identification as a Rindler flow line
Fermi-Walker transport preserves the metric, and explicit rigid and non-rigid observer congruences
Kinematics of an observer congruence: acceleration, expansion, shear, vorticity and Born rigidity
Causal reachability, causal futures and pasts, causal diamonds, and reachability by future causal paths in affine Minkowski space
The closed future cone in inertial coordinates: description, finite sums, and the coordinate criterion for causal reachability
Future causal reachability, absence of causal loops, time monotonicity and the straight-worldline proper-time maximum
The causal signal restriction of the model
Adopted ideal-clock and ideal-vacuum-light interpretation
Adopted inertial covariance of the model equations
The operational radar protocol of an ideal observer
Simultaneity slices and rest distance relative to a future unit timelike vector
Four-velocity and four-acceleration of a future timelike worldline
Proper time along a future timelike worldline
The proper-time function is a strictly increasing C^1 parametrization with C^1 inverse
Norms of four-velocity and four-acceleration, and the observer rest-space decomposition
Curves, regular causal curves and future timelike worldlines in affine Minkowski space
Inertial frames and inertial charts of the affine Minkowski model
Oriented time-oriented affine Minkowski space (the spacetime primitives)
SI units and coordinate conventions of the special-relativity framework
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 natural logarithm as the inverse of the exponential function
Order, continuity, range, and the product, quotient, and reciprocal laws for the natural logarithm
The six hyperbolic functions and their natural domains
Addition formulas, identities, parity, and derivatives of the hyperbolic functions
The exponential addition formula
The exponential tends to at and to at
The elementary numerical bound
The derivative of at a point that is a limit point of , and differentiability on a set
Sums, scalar multiples, products and quotients: , , , and when
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 of Cauchy's: for continuous on with and differentiable on there is with
A function differentiable at is continuous at
Dependency tree · 2 levels
Sources
- M. Blau, Lecture Notes on General Relativity (University of Bern, last update October 5, 2026, 1052 PDF pages): Section 1.3 pp. 36-40 (Rindler metric, lines of constant rho and eta, the boundary eta = +-infinity, the lightcone equation d eta = +- rho^{-1} d rho, and item 6: the past lightcone of the accelerated observer covers asymptotically only the region xi^0 < xi^1, so every event above xi^0 = xi^1 is forever invisible) and Section 3.4 pp. 90-93 (Rindler coordinates, their ranges and the right Rindler wedge)
- Wikipedia, 'Rindler coordinates' (encyclopedia article consulted as a secondary treatment): section 'The Rindler horizon' (no observer of the congruence can receive signals from events with T >= X nor send signals to events with T <= -X) and section 'Notions of distance' (the null geodesic equation t - t_0 = log(x/x_0), the radar distance x_0 log(1 + h/x_0) between observers at x_0 and x_0 + h, the comparison with the ruler distance, and the caution that radar distance need not be symmetric under interchange)
- B. Crowell, Special Relativity, revision 2020-12-10 (author-published undergraduate textbook, 246 PDF pages): Section 3.5.2 p. 62 (the lightlike asymptote of hyperbolic motion and the resulting event horizon: provided that the rocket never stops accelerating, the region of spacetime to the left of the dashed line is forever hidden from its passengers) and Section 7.1 p. 148 (the diagonals are event horizons); signature (+---) converted to (-+++), c = 1 formulas restored to x^0 = c t