Intuition What this page is for
The parent note built the two equations
x ′ = γ ( x − v t ) , t ′ = γ ( t − c 2 v x ) , γ = 1 − v 2 / c 2 1 .
Here we do the opposite of a proof: we stress-test those equations against every kind of situation you could ever be handed — every sign of velocity, an event ahead of you and behind you, the two extreme speeds (v = 0 and v → c ), a real word problem, and an exam twist. If you can drive these examples, no problem in this topic can surprise you.
Before anything, one reminder about units so no example trips you up.
Definition Working in light-seconds and seconds
A light-second is the distance light travels in one second: 1 ls = c × 1 s . If we measure distance in light-seconds and time in seconds , then the number c becomes just 1 (one light-second per second). This is not a trick — it is a choice of ruler that makes v x / c 2 easy: with c = 1 , it is simply v x . We will state each example in whichever units are cleanest and always convert back.
Every Lorentz-transform problem is one cell of this table. The right column names the example that lands on it.
Cell class
What makes it special
Covered by
Zero velocity (v = 0 )
γ = 1 : nothing should change
Ex. 1
Low velocity (v ≪ c )
must reduce to Galileo x ′ = x − v t
Ex. 2
Event ahead (x > 0 ), forward frame (v > 0 )
standard positive case
Ex. 3
Event behind (x < 0 ) or backward frame (v < 0 )
sign of the − v x / c 2 term flips
Ex. 4
Simultaneous pair (Δ t = 0 )
relativity of simultaneity, both signs
Ex. 5
Limiting speed (v → c )
γ → ∞ , degenerate squeeze
Ex. 6
Real-world word problem
muon / spaceship, pick out x , t , v yourself
Ex. 7
Exam twist (inverse + invariant)
go from S ′ back to S , check s 2
Ex. 8
We march through them in order. Keep the Minkowski diagram , Time dilation , Length contraction and Relativity of simultaneity pages in mind — every example quietly touches one of them.
Worked example 1 · Zero-velocity sanity check — cell:
v = 0
Statement. Frame S ′ does not move: v = 0 . An event happens at x = 4 ls , t = 5 s . Find ( x ′ , t ′ ) .
Forecast: Guess before computing — if the frames don't move relative to each other, should any coordinate change?
Compute γ . γ = 1/ 1 − 0 2 / c 2 = 1/ 1 = 1 .
Why this step? Everything scales by γ ; if γ = 1 there is no stretch at all.
Apply x ′ = γ ( x − v t ) . With v = 0 : x ′ = 1 ⋅ ( 4 − 0 ) = 4 ls .
Why this step? The − v t correction vanishes because v = 0 .
Apply t ′ = γ ( t − v x / c 2 ) . With v = 0 : t ′ = 1 ⋅ ( 5 − 0 ) = 5 s .
Why this step? The − v x / c 2 correction vanishes too.
Verify: ( x ′ , t ′ ) = ( 4 , 5 ) = ( x , t ) . Identical frames give identical coordinates — the transform reduces to the identity , exactly as physics demands. ✓
Worked example 2 · Low speed → Galileo — cell:
v ≪ c
Statement. A car frame moves at v = 30 m/s . An event is at x = 300 m , t = 2 s . Show x ′ ≈ x − v t and t ′ ≈ t . (c = 3 × 1 0 8 m/s .)
Forecast: Do you expect to see any relativistic difference at car speeds?
Estimate v 2 / c 2 . v 2 / c 2 = ( 30 ) 2 / ( 3 × 1 0 8 ) 2 = 900/ ( 9 × 1 0 16 ) = 1 0 − 14 .
Why this step? This tiny number is what sits under the square root; if it is negligible, γ ≈ 1 .
So γ ≈ 1 to 14 decimal places.
Why this step? 1 − 1 0 − 14 ≈ 1 , so γ is indistinguishable from 1.
Space: x ′ ≈ x − v t = 300 − 30 ⋅ 2 = 240 m — the plain Galilean answer.
Why this step? With γ = 1 the Lorentz x ′ is the Galilean x ′ .
Time: the correction v x / c 2 = 30 ⋅ 300/ ( 9 × 1 0 16 ) = 1 0 − 13 s — utterly negligible, so t ′ ≈ t = 2 s .
Why this step? v x / c 2 is the term that "breaks" universal time; here it is 1 0 − 13 s , unmeasurable.
Verify: New theory contains the old one as a limit (Galilean transformation recovered). Units: v x / c 2 has units ( m/s ) ( m ) / ( m/s ) 2 = s . ✓
Worked example 3 · Event ahead, forward-moving frame — cell:
x > 0 , v > 0
Statement. S ′ moves at v = 0.6 c . An event is at x = 10 ls , t = 5 s . Find ( x ′ , t ′ ) .
Forecast: The frame chases toward + x . Will the event's primed distance be larger or smaller than 10? Will its primed time be earlier or later than 5?
Compute γ . γ = 1/ 1 − 0. 6 2 = 1/ 1 − 0.36 = 1/ 0.64 = 1/0.8 = 1.25 .
Why this step? γ multiplies both outputs.
Space. Using c = 1 so distances are in ls, times in s: x ′ = γ ( x − v t ) = 1.25 ( 10 − 0.6 ⋅ 5 ) = 1.25 ( 10 − 3 ) = 1.25 ⋅ 7 = 8.75 ls .
Why this step? v t = 0.6 ⋅ 5 = 3 ls is how far S ′ has slid forward; the event is now only 7 ls ahead before the γ stretch.
Time. t ′ = γ ( t − v x / c 2 ) = 1.25 ( 5 − 0.6 ⋅ 10 ) = 1.25 ( 5 − 6 ) = 1.25 ⋅ ( − 1 ) = − 1.25 s .
Why this step? With c = 1 , v x / c 2 = 0.6 ⋅ 10 = 6 ; because x is large and positive, this correction is big enough to push t ′ negative — in S ′ the event already happened.
Verify: Sign check with the Minkowski diagram below: a far-ahead event, seen by a forward observer, is dragged to an earlier primed time. Positive x , positive v ⇒ subtract ⇒ time can go negative. ✓
Worked example 4 · Event behind / backward frame — cell:
x < 0 or v < 0
Statement. Same speed magnitude but now S ′ moves the other way, v = − 0.6 c , and the event is behind the origin at x = − 10 ls , t = 5 s . Find ( x ′ , t ′ ) .
Forecast: Two sign flips (v and x ). Do they cancel or double up in the time equation?
γ is unchanged. γ = 1/ 1 − ( − 0.6 ) 2 = 1/ 0.64 = 1.25 .
Why this step? γ depends on v 2 , so the sign of v never affects it — a moving clock slows the same whichever way it moves.
Space. x ′ = γ ( x − v t ) = 1.25 ( − 10 − ( − 0.6 ) ( 5 )) = 1.25 ( − 10 + 3 ) = 1.25 ( − 7 ) = − 8.75 ls .
Why this step? − v t = + 3 now (double negative); the event stays behind, at − 8.75 ls.
Time. t ′ = γ ( t − v x / c 2 ) = 1.25 ( 5 − ( − 0.6 ) ( − 10 )) = 1.25 ( 5 − 6 ) = − 1.25 s .
Why this step? ( − 0.6 ) ( − 10 ) = + 6 : the two minus signs multiply to a plus , so the correction is identical to Ex. 3. This is the key lesson — it is the product v x , not either sign alone, that sets the time shift.
Verify: By pure mirror symmetry the answer is ( − 8.75 ls , − 1.25 s ) : the whole picture of Ex. 3 flipped left-to-right. Sign discipline confirmed. ✓
Worked example 5 · Simultaneous in
S , not in S ′ — cell: Δ t = 0 , both signs of x
Statement. In S , two flashes happen at the same time t = 0 : flash A at x A = + 8 ls , flash B at x B = − 8 ls . Frame S ′ moves at v = 0.6 c . Which flash does S ′ see first?
Forecast: They are simultaneous in S . Guess: does S ′ still call them simultaneous? If not, which comes first — the one ahead or the one behind?
γ = 1.25 as before.
Why this step? Same speed, same factor.
Flash A (x = + 8 ): t A ′ = γ ( 0 − v x A / c 2 ) = 1.25 ( 0 − 0.6 ⋅ 8 ) = 1.25 ( − 4.8 ) = − 6 s .
Why this step? Only the − v x / c 2 term survives (t = 0 ); a positive x gives a negative primed time.
Flash B (x = − 8 ): t B ′ = γ ( 0 − v x B / c 2 ) = 1.25 ( 0 − 0.6 ⋅ ( − 8 )) = 1.25 ( + 4.8 ) = + 6 s .
Why this step? Negative x flips the sign, giving a positive primed time.
Compare. t A ′ = − 6 < t B ′ = + 6 , so in S ′ flash A (ahead) happens first , a full 12 s before B.
Why this step? The observer moving toward + x meets the event on that side "earlier" in her time coordinate.
Verify: Δ t = 0 in S but Δ t ′ = t B ′ − t A ′ = 12 s = 0 in S ′ . This is exactly Relativity of simultaneity — simultaneity is not absolute, and the ordering is set by the sign of x . ✓
Worked example 6 · The limit
v → c — cell: degenerate / limiting speed
Statement. Track γ and the transform as v climbs: v = 0.8 c , 0.99 c , 0.9999 c . What happens to γ , and to an event at x = 1 ls , t = 0 ?
Forecast: As v approaches c , does γ approach some finite ceiling or blow up?
v = 0.8 c : γ = 1/ 1 − 0.64 = 1/ 0.36 = 1/0.6 = 1.6 6 .
Why this step? Establish the baseline before pushing higher.
v = 0.99 c : γ = 1/ 1 − 0.9801 = 1/ 0.0199 ≈ 7.089 .
Why this step? The number under the root is shrinking toward 0, so γ shoots up.
v = 0.9999 c : γ = 1/ 1 − 0.99980001 = 1/ 0.00019999 ≈ 70.71 .
Why this step? Each step closer to c makes 1 − v 2 / c 2 ten-fold smaller, γ ten-fold... no, ≈ 10 -fold bigger. It diverges : γ → ∞ as v → c .
The event's time t ′ = γ ( 0 − v x / c 2 ) = − γ v x / c 2 grows without bound in magnitude.
Why this step? Nothing with mass can reach v = c — the transform becomes singular (division-by-zero inside γ ), which is physics saying "c is a wall."
Verify: Sequence γ ∈ { 1.667 , 7.089 , 70.71 } is monotone increasing and unbounded. The v = c case is genuinely undefined (0 in the denominator), the correct degenerate behaviour. ✓
Worked example 7 · Real-world word problem — the muon — cell: word problem
Statement. A muon is created high in the atmosphere and moves straight down at v = 0.98 c . In its own frame it lives τ = 2.2 μ s before decaying. Using the transform, how far does the muon travel in the ground frame before decaying? (c = 3 × 1 0 8 m/s .)
Forecast: In 2.2 μ s at 0.98 c a Newtonian would get ≈ 647 m . Guess: will the ground see it go further or less far?
Identify frames. Let S ′ = muon (it is at rest there), S = ground. Two events: birth ( x ′ = 0 , t ′ = 0 ) and death ( x ′ = 0 , t ′ = τ = 2.2 × 1 0 − 6 s ) — same place in S ′ because the muon sits still in its own frame.
Why this step? Choosing the frame where the muon is at rest makes its lifetime the clean proper time τ .
γ . γ = 1/ 1 − 0.9 8 2 = 1/ 1 − 0.9604 = 1/ 0.0396 ≈ 5.025 .
Why this step? This factor stretches the muon's short life into ground time.
Ground time of death via the inverse t = γ ( t ′ + v x ′ / c 2 ) with x ′ = 0 : t = γ τ = 5.025 × 2.2 × 1 0 − 6 ≈ 1.106 × 1 0 − 5 s = 11.06 μ s .
Why this step? We go from primed → unprimed, so we use the inverse transform; the moving muon's clock ran slow, so the ground clock reads longer (Time dilation ).
Ground distance. In S the muon travels d = v t = 0.98 × ( 3 × 1 0 8 ) × 1.106 × 1 0 − 5 ≈ 3251 m ≈ 3.25 km .
Why this step? Distance is speed × ground time; using the dilated time gives the real experimental range.
Verify: Naive answer 647 m vs relativistic ≈ 3251 m — the factor is γ ≈ 5.03 , and indeed 647 × 5.025 ≈ 3251 . This extra reach is exactly why muons reach the ground and get detected. Units: ( m/s ) ( s ) = m . ✓
Worked example 8 · Exam twist — inverse transform + invariant interval — cell: inverse &
s 2
Statement. You are given the primed coordinates of an event: x ′ = 3 ls , t ′ = 5 s , with v = 0.6 c . (a) Find ( x , t ) in S using the inverse transform. (b) Confirm the Spacetime interval s 2 = c 2 t 2 − x 2 matches in both frames.
Forecast: Two independent checks. Will the interval computed from primed values equal the one from unprimed values?
γ = 1.25 (from v = 0.6 c ).
Why this step? Same speed as our earlier examples; reuse it.
Inverse space x = γ ( x ′ + v t ′ ) = 1.25 ( 3 + 0.6 ⋅ 5 ) = 1.25 ( 3 + 3 ) = 1.25 ⋅ 6 = 7.5 ls .
Why this step? Going from S ′ back to S flips the sign of v , turning the minus into a plus — the inverse transform.
Inverse time t = γ ( t ′ + v x ′ / c 2 ) = 1.25 ( 5 + 0.6 ⋅ 3 ) = 1.25 ( 5 + 1.8 ) = 1.25 ⋅ 6.8 = 8.5 s .
Why this step? Same sign-flip logic for the time equation.
Interval in S (c = 1 ): s 2 = t 2 − x 2 = 8. 5 2 − 7. 5 2 = 72.25 − 56.25 = 16 .
Why this step? Compute the candidate invariant from the unprimed values.
Interval in S ′ : s ′2 = t ′2 − x ′2 = 5 2 − 3 2 = 25 − 9 = 16 .
Why this step? Compute the same quantity from the primed values.
Verify: s 2 = s ′2 = 16 — the spacetime interval is frame-independent , the geometric heart the parent note promised. Both the inverse coordinates and the invariance check out. ✓
Recall Active recall — cover the answers
In Ex. 4, why did two sign flips give the same time shift as Ex. 3? ::: Because the correction depends on the product v x ; ( − ) ( − ) = ( + ) , identical to ( + ) ( + ) .
Ex. 5: which of two S -simultaneous events does a forward-moving observer see first? ::: The one at larger positive x (ahead), because t ′ = − γ v x / c 2 is more negative there.
As v → c , what happens to γ ? ::: It diverges to ∞ ; v = c makes the transform singular — a speed wall for massive objects.
In the muon problem, which time do you use to get ground distance? ::: The dilated ground time t = γ τ , not the proper lifetime τ .
Mnemonic One-line survival kit for any problem
"Find γ , decide which frame you start in, subtract for forward (primed) and add for inverse (unprimed), and the sign of t ′ is ruled by the product v x ."