Special relativity Created 2026-09-24 Updated 2026-10-13
Special relativity describes physics in Minkowski spacetime, where inertial frames assign different space and time coordinates to the same spacetime events. Its two postulates are Einstein's principle of relativity and the same vacuum speed of light in every inertial frame, independent of the source's motion. Together they replace the Galilean transformation with the Lorentz transformation, coupling space and time rather than providing a universal clock. Einstein's 1905 paper developed this account through measuring rods, clocks, and light signals. [ref].
A spacetime event is an occurrence at a definite place and time: a pulse reaching a detector, for example. An inertial frame supplies a Cartesian coordinate system and clocks at rest throughout it. Einstein synchronisation sets a distant clock's reflection reading to the midpoint between a light signal's departure and return readings at the sending clock. The resulting coordinate time records the local synchronized clock at each spacetime event; it differs from the time when a distant observer receives its image. This distinction makes time dilation, length contraction, and the relativity of simultaneity precise measurements. [ref].
The beauty of special relativity is that these different measurements fit one geometry: all inertial frames agree on the Minkowski interval. It lets us translate an experiment between a laboratory and a moving apparatus while preserving the light-signal relations between spacetime events.
During either inertial leg, the traveller can correctly say that the moving home clock runs slowly. The missing step is deciding which distant home-clock reading is simultaneous with turnaround. By the Lorentz transformation, the outward inertial frame's constant-time line through obeys . At it meets the home world line at
For the return inertial frame, use through the same spacetime event ; its home-clock assignment is
The dashed lines in the spacetime diagram illustrate this relativity of simultaneity. For and , they assign and to the home clock. The difference of is a change in the traveller's distant-time assignment, not a sudden physical advance of the home clock.
On each leg, the traveller's of proper time corresponds to of home-clock advance according to that leg's inertial frame. Including the twin paradox simultaneity change gives , exactly the reading at reunion. Actual received light signals remain continuous across a physical turnaround; their arrival times are distinct from the distant spacetime events assigned as simultaneous by Einstein synchronisation.
Velocity-addition formula 2026-10-14
The velocity-addition formula translates a particle's velocity between two specified inertial frames. Let move at signed velocity along the -axis of , with parallel axes and , where is the speed of light. Define and for the same particle's world line, using position and time measured within the corresponding inertial frame. With Lorentz factor , the forward Lorentz boost gives
For collinear motion, write and . The inverse velocity-addition formula is
This is the composition of the particle's velocity in and that frame's velocity relative to . The velocities must belong to this same chain of reference frames, with directions specified. Two arbitrary quoted speeds cannot be inserted blindly. Each velocity measurement uses distances and clocks in a single inertial frame, with Einstein synchronisation for separated clocks.
For example, let and let the particle travel at in . Its velocity in is
The Galilean transformation would instead give , which fails here. For light moving along the positive axis, gives ; similarly gives . Negative directions also work for massive particles: at , gives , while gives . Thus “addition” means composition of signed velocities, rather than addition of their magnitudes.
Figure 1.
Relativistic and Galilean velocity composition for a frame moving at 0.6 times the speed of light
. The horizontal coordinate is the particle's velocity in , and the vertical coordinate is its velocity in . The velocity-addition formula maps into ; the endpoint values describe light. The marked example is , giving . Details.
A short derivation differentiates the Lorentz transformation: and . Dividing these differentials gives the longitudinal velocity-addition formula. The transverse formulas use and , but the same transformed time denominator; omitting it would ignore the relativity of simultaneity. Replacing by gives the inverse. When both relative and particle velocities are small compared with the speed of light, the denominator is close to one and the nonrelativistic limit recovers the Galilean transformation.
The formula lets us compare particle motion in a moving apparatus and a laboratory without losing the invariant speed of light. Einstein's 1905 paper derives the coordinate change in §3 and the composition of velocities in §5, including the collinear formula, its light-speed case, and composition of parallel transformations. [ref]. The rapidity parametrization makes the collinear composition particularly simple.