Modern PhysicsSpecial Relativity

The Lorentz Transformation

x′ = γ(x − vt) and t′ = γ(t − vx/c²) convert events between frames.

Not started Jump to practice

Time dilation, length contraction and the relativity of simultaneity are three faces of one rule: the Lorentz transformation. It converts the coordinates $(x, t)$ of any event in frame $S$ to its coordinates $(x', t')$ in a frame $S'$ moving at $v$ along $x$, with the origins together at $t = t' = 0$.

Key idea

$$x' = \gamma(x - vt),\qquad t' = \gamma\left(t - \frac{vx}{c^2}\right).$$ To go back, swap the primes and change the sign of $v$: $x = \gamma(x' + vt')$, $t = \gamma\left(t' + \frac{vx'}{c^2}\right)$. With distances in light-years and times in years, $c = 1$ ly/yr and $v$ is just $\beta$.

Why it works

Start from Galileo's $x' = x - vt$ and allow a stretch factor: $x' = \gamma(x - vt)$. By postulate 1, $S$ sees $S'$ move at $-v$ in the same way: $x = \gamma(x' + vt')$. Now use postulate 2. A flash from the shared origin at $t = 0$ moves as $x = ct$ in $S$ and $x' = ct'$ in $S'$. Substituting gives $ct' = \gamma(c - v)t$ and $ct = \gamma(c + v)t'$. Multiply: $c^2tt' = \gamma^2(c^2 - v^2)tt'$, so $\gamma = 1/\sqrt{1 - v^2/c^2}$. Finally, solve the two $x$ equations for $t'$: $$t' = \gamma\left(t - \frac{vx}{c^2}\right).$$ The $-\frac{vx}{c^2}$ term is the new part: clocks spread along $x$ disagree, which is the relativity of simultaneity.
A spacetime diagram with the moving frame's axes drawn in. Each event's $x'$ and $t'$ are read along the tilted axes; the dashed lines of equal $t'$ are tilted, so events level with each other in $S$ are not level in $S'$.

Worked examples

Worked example: Transform an event

In frame $S$ an event happens at $x = 4.0$ ly, $t = 2.0$ yr. Find its coordinates in a frame moving at $0.60c$ along $+x$.
  1. $\gamma = 1.25$, and with $c = 1$ ly/yr, $v = 0.60$ ly/yr.
  2. $x' = 1.25(4.0 - 0.60 \times 2.0) = 1.25 \times 2.8 = 3.5$ ly.
  3. $t' = 1.25(2.0 - 0.60 \times 4.0) = 1.25 \times (-0.40) = -0.50$ yr.

Answer: $x' = 3.5$ ly, $t' = -0.50$ yr: in $S'$ the event happened half a year before the origins met

Worked example: Simultaneity, by formula

Two events happen at $t = 0$ in $S$, at $x = 0$ and at $x = 3.0$ ly. When does each happen in a frame moving at $0.60c$?
  1. First event: $t' = 1.25(0 - 0) = 0$.
  2. Second: $t' = 1.25(0 - 0.60 \times 3.0) = -2.25$ yr.
  3. So in $S'$ the event at $x = 3.0$ ly happened 2.25 years earlier.

Answer: $t' = 0$ and $t' = -2.25$ yr

Worked example: Back again

An event has $x' = 1.0$ ly and $t' = 3.0$ yr in a frame moving at $0.80c$ relative to $S$. Find $x$ and $t$.
  1. $\gamma = 1/0.60 = 1.667$, and the reverse transformation uses $+v$.
  2. $x = 1.667(1.0 + 0.80 \times 3.0) = 1.667 \times 3.4 = 5.67$ ly.
  3. $t = 1.667(3.0 + 0.80 \times 1.0) = 1.667 \times 3.8 = 6.33$ yr.

Answer: $x = 5.67$ ly, $t = 6.33$ yr

Two quick checks for any answer. A light flash moving as $x = ct$ in $S$ must come out as $x' = ct'$ in $S'$: try it, and the $\gamma$'s and $\beta$'s cancel. And at everyday speeds $\gamma \approx 1$ and $\frac{vx}{c^2}$ is tiny, so the transformation becomes Galileo's $x' = x - vt$ and $t' = t$, as it must.

Common mistake

Dropping the $vx/c^2$ term and writing $t' = \gamma t$. That is time dilation for a clock at $x = 0$ only. For events elsewhere, the $-\frac{vx}{c^2}$ term carries the relativity of simultaneity, and leaving it out gives wrong times, even the wrong order of events. Check: two events with the same $t$ but different $x$ must get different $t'$.

Practice

Pass with 3 right answers, the last 2 in a row. Each right answer earns 3 XP.

Loading practice…

Builds on

Leads to

Sources and further reading

  • OpenStax University Physics Volume 3, 5.5 The Lorentz Transformation
  • MIT OpenCourseWare 8.20 Introduction to Special Relativity (January IAP 2005)
@teddyrookbook GitHub