2.3.31 · D1Modern Physics

Foundations — Relativistic momentum p = γmv

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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.


1. Speed , and the number

Look at the number line below.

What to notice in the figure: the horizontal axis is speed . Three dots (snail, half light-speed, fast electron) all sit to the left of the magenta wall at . No matter how hard you push (the violet arrow "speeding up"), a dot can slide toward but never land on it. Extract this: real speeds fill the open interval ; itself is forbidden.

Why the topic needs it: the whole story of relativistic momentum is what happens as creeps toward that wall — so you must first see that the wall exists and is never reached.


2. Direction and sign — is really a vector

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.

Why the topic needs it: is a pure number that only depends on how fast (never which way), while the direction rides on the that multiplies it. Keeping these separate stops sign errors later.


3. The ratio

Why the topic needs it: every relativistic formula is cleaner written with than with .


4. The square-root piece

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 on the left (the violet dot, "at rest") and dives toward on the right as (the magenta dot). Extract this: in the next step we divide 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 . Understand its downward shape and 's explosion becomes obvious.


5. The Lorentz factor

What to notice in the figure: the magenta curve hugs the dotted line for small (so everyday speeds are "ordinary, Newtonian"), passes through the orange dot at , then rears up into a near-vertical cliff as . Extract this: below relativity barely matters; near the wall it dominates completely.

Why the topic needs it: is the entire relativistic correction. Momentum .

The very same 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.


6. Rest mass

Why the topic needs it: is the unchanging anchor. All the speed-dependence lives in , never in .


7. Momentum (the Newtonian starting point)


8. Proper time vs lab time — and why they differ by

This is the one genuinely new idea the derivation needs, so we justify it rather than assert it.

Plain reading: for each tick of the travelling clock, the lab sees times as much time pass. The moving clock runs slow.


9. Why swapping for rescues conservation

Here is the logical bridge to the parent formula — no hand-waving.


10. Reading the assembled formula

Now every symbol is earned, so the parent formula reads as plain English:


Prerequisite map

Node labels use full names (matching the sections above).

divide by

divide by

carries a

feeds

reciprocal is

combine with mass

combine with speed

gives sign to

Pythagoras light clock

Pythagoras light clock

supplies ratio

invariant enables

guarantees

injects gamma into

multiplies

gets boosted into

Speed v metres per second

Light speed c the wall

Direction sign of velocity

Beta equals v over c

Shrink factor root of 1 minus beta squared

Lorentz factor gamma

Rest mass m invariant

Newton momentum p equals m v

Proper time tau moving clock invariant

Lab time t

Time dilation dt equals gamma d-tau

Covariance clean transform

Relativistic momentum gamma m v


Equipment checklist

Cover the right side and test yourself.

What is and how many m/s roughly?
The universal speed limit, 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 and its range.
; it lies in .
What does do as goes from to ?
It slides from down to .
Write the Lorentz factor .
, always .
Value of at rest, and as ?
at rest; near light-speed.
Is ?
No — that is the shrinking factor; is its reciprocal.
What is rest mass — 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.
; how hard a moving object is to stop.
Why is proper time 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 in one sentence.
Pythagoras on the slanted light-pulse path gives .
Why does dividing by instead of rescue conservation?
is invariant, so transforms as one clean object — a conservation law true in one frame stays true in all.
In , what carries the speed dependence?
(on the motion), not the mass .

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