Intuition The ONE core idea
"Amount of motion" — how hard a moving thing is to stop — grows faster than ordinary physics predicts when you push toward the speed of light. All of that extra growth is captured by a single number, the Lorentz factor γ , and this page builds every symbol from scratch until that one sentence becomes an equation.
This page assumes nothing . Before you touch the parent formula, every letter in it — and every hidden idea behind it — must have a plain meaning and a picture. We build them one at a time, each resting on the one before.
v
v is how far something travels in one second — metres per second (m/s). A snail: tiny v . A bullet: bigger v . Light: the biggest v anything can have.
Definition The speed of light
c
c ≈ 3 × 1 0 8 m/s is the top speed of the universe — a wall no object with mass can reach. It is the same for every observer, no matter how they move. That last sentence is the strange fact all of relativity is built on.
Look at the number line below.
What to notice in the figure: the horizontal axis is speed v . Three dots (snail, half light-speed, fast electron) all sit to the left of the magenta wall at c . No matter how hard you push (the violet arrow "speeding up"), a dot can slide toward c but never land on it. Extract this: real speeds fill the open interval 0 ≤ v < c ; c itself is forbidden.
Why the topic needs it: the whole story of relativistic momentum is what happens as v creeps toward that wall c — so you must first see that the wall exists and is never reached.
Speed alone is not enough for momentum. A ball thrown left and one thrown right at the same speed have opposite momenta, and in a collision they can cancel.
Definition Velocity as a signed quantity
Along one line, pick a positive direction (say, "to the right"). Then velocity carries a sign : v > 0 means moving right, v < 0 means moving left. Its size (always ≥ 0 ) is the speed . In full 3-D we write it as a vector v with an arrow showing direction.
Intuition Why sign matters for momentum
Momentum p inherits the sign of v : rightward motion gives p > 0 , leftward gives p < 0 . This is exactly why total momentum can stay the same in a collision — a positive p and a negative p can add to zero. If you dropped the sign you could never explain a head-on crash. Everything on this page uses the magnitude ∣ v ∣ inside γ (because γ depends on v 2 , so its sign does not matter), but the direction travels along with v in p = γ m v .
Why the topic needs it: γ is a pure number that only depends on how fast (never which way), while the direction rides on the v that multiplies it. Keeping these separate stops sign errors later.
Definition Beta — speed as a fraction of light
β = c ∣ v ∣
β (Greek letter "beta") measures your speed in units of light-speed , ignoring direction. If ∣ v ∣ = c , then β = 1 . If you move at half of light-speed, β = 0.5 .
Intuition Why bother with
β ?
Writing v / c everywhere is clumsy. Since only the fraction of light-speed matters for the relativistic effects, we give that fraction its own short name. β always lives between 0 and 1 (never quite 1 ), exactly like a percentage of the way to the wall.
Why the topic needs it: every relativistic formula is cleaner written with β than with v / c .
Before the star of the show, meet the small quantity underneath it.
What to notice in the figure: the orange curve starts pinned at height 1 on the left (the violet dot, "at rest") and dives toward 0 on the right as β → 1 (the magenta dot). Extract this: in the next step we divide 1 by this curve ; dividing by a number heading to zero makes the result blow up — that is the seed of every dramatic effect.
Why the topic needs it: it is the raw material of γ . Understand its downward shape and γ 's explosion becomes obvious.
Definition Gamma — the "relativistic stubbornness" number
γ = 1 − β 2 1 = 1 − v 2 / c 2 1
γ (Greek "gamma") is one divided by the shrinking factor from Step 4. Because we divide 1 by something between 1 and 0 , the answer is always ≥ 1 , and it shoots up to infinity as β → 1 .
γ is NOT 1 − β 2
The shrinking factor goes down to 0 . γ is its reciprocal , so it goes up to ∞ . If your γ ever comes out less than 1 , you flipped the fraction.
What to notice in the figure: the magenta curve hugs the dotted line γ = 1 for small β (so everyday speeds are "ordinary, Newtonian"), passes through the orange dot at β = 0.8 , γ = 1.667 , then rears up into a near-vertical cliff as β → 1 . Extract this: below β ≈ 0.1 relativity barely matters; near the wall it dominates completely.
Why the topic needs it: γ is the entire relativistic correction. Momentum = γ × ( Newton’s m v ) .
The very same γ also governs how much a moving clock lags — that is developed in Lorentz factor and time dilation , and we borrow one result from it in Step 8.
Definition Rest mass (invariant mass)
m is the amount of "stuff" in a particle — its permanent, built-in inertia. Crucially, m is the same number for every observer , no matter how fast the particle moves. It is a fixed label, like a serial number.
Common mistake "Mass grows with speed"
Old books wrote γ m and called it "relativistic mass". Modern convention keeps m fixed and puts γ on the motion instead. The particle does not get more stuff; it gets harder to accelerate because γ multiplies its momentum.
Why the topic needs it: m is the unchanging anchor. All the speed-dependence lives in γ , never in m .
Definition Momentum — amount of motion
p = m v ( Newton )
Momentum measures how hard a moving object is to stop: heavier (m big) or faster (v big) ⇒ more p . It carries the sign of v (Step 2), so it points the way the object moves. Units: kg·m/s.
Intuition Why it deserves a name at all
In collisions the total momentum before equals the total after — it is conserved . That conservation (positives and negatives adding up the same before and after) is what makes p physically precious. The parent topic's whole reason for existing: Newton's p = m v stops being conserved for everyone once speeds get near c , and we must repair it. The repair is multiplying by γ . The everyday p = m v version we are upgrading is catalogued in Newtonian momentum p = mv .
This is the one genuinely new idea the derivation needs, so we justify it rather than assert it.
Definition Two different clocks
t = lab time : time read on a clock sitting still in your laboratory.
τ = proper time (Greek "tau"): time read on a clock riding along with the moving particle .
d τ is the same for everybody (invariance)
Relativity's one rule is that light travels at c for every observer . Build a clock from that rule: a light pulse bouncing between two mirrors — each round trip is one "tick". For the astronaut carrying it, the pulse goes straight up and down. But to the lab, the mirrors are also drifting sideways, so the same pulse must travel a longer, slanted zig-zag. Since light's speed is fixed at c for both, a longer path means more lab-seconds per tick . Both observers are watching the identical pulse, so they agree on how many ticks happened — that shared tick-count is the proper time τ . Because it counts the particle's own light-clock ticks, everyone computes the same τ : it is invariant .
Plain reading: for each tick d τ of the travelling clock, the lab sees γ times as much time d t pass. The moving clock runs slow.
Here is the logical bridge to the parent formula — no hand-waving.
Intuition The covariance argument
A particle's motion through space is a list of positions x at times t . When a second observer moves relative to you, both x and t get scrambled together by the Lorentz transformation — so the ordinary velocity x / t is a mixed-up quantity that changes shape from frame to frame.
Now the key: proper time τ does not scramble — it is the invariant we just built. So if we divide the (scrambling) displacement d x by the (non-scrambling) d τ , the result m d x / d τ transforms as a clean, whole object between frames — the same kind of object in everyone's coordinates. When a rule ("total momentum is unchanged") is written with such objects, and it holds in one frame, the Lorentz transformation carries it unchanged into every other frame. That is exactly what we needed: conservation valid for all observers.
Newton's p = m d x / d t fails this test because d t scrambles. Replacing d t with the invariant d τ is the minimal fix — and via Step 8 it injects the factor γ . (The full machinery is the Energy-momentum four-vector .)
Now every symbol is earned, so the parent formula reads as plain English:
Mnemonic Gamma Mounts the Velocity
p = γ m v — the γ rides on the motion, not the mass. And γ ≥ 1 because it sits on top of the fraction 1/ … .
Node labels use full names (matching the sections above).
Speed v metres per second
Direction sign of velocity
Shrink factor root of 1 minus beta squared
Newton momentum p equals m v
Proper time tau moving clock invariant
Time dilation dt equals gamma d-tau
Covariance clean transform
Relativistic momentum gamma m v
Cover the right side and test yourself.
What is c and how many m/s roughly? The universal speed limit, ≈ 3 × 1 0 8 m/s, same for all observers.
Why does momentum need a sign / direction? So opposite motions can cancel — that is how total momentum is conserved in a head-on collision.
Define β and its range. β = ∣ v ∣/ c ; it lies in 0 ≤ β < 1 .
What does 1 − β 2 do as v goes from 0 to c ? It slides from 1 down to 0 .
Write the Lorentz factor γ . Value of γ at rest, and as v → c ? γ = 1 at rest; γ → ∞ near light-speed.
Is γ = 1 − β 2 ? No — that is the shrinking factor; γ is its reciprocal.
What is rest mass m — does it change with speed? The invariant amount of stuff; it is the same in every frame (does not grow).
Write Newtonian momentum and say what it measures. p = m v ; how hard a moving object is to stop.
Why is proper time τ the same for all observers? It counts the particle's own light-clock ticks, and everyone watches the identical pulse, so they agree on the tick-count.
Derive d t = γ d τ in one sentence. Pythagoras on the slanted light-pulse path
( c d t ) 2 = ( c d τ ) 2 + ( v d t ) 2 gives
d t / d τ = 1/ 1 − β 2 = γ .
Why does dividing by d τ instead of d t rescue conservation? d τ is invariant, so
m d x / d τ transforms as one clean object — a conservation law true in one frame stays true in all.
In p = γ m v , what carries the speed dependence? γ (on the motion), not the mass m .