2.3.4 · D2Modern Physics

Visual walkthrough — Compton scattering — wavelength shift derivation

2,248 words10 min readBack to topic

Before line one we agree on the cast of characters — the only objects in this whole story:

Everything below builds on these. Let us watch the collision.


Step 1 — The picture of the collision itself

WHAT: We draw the "before" and "after" of one photon hitting one resting electron.

WHY: You cannot conserve anything until you know what is moving where. Every later arrow lives on this diagram, so we pin down directions first.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

Read the figure left to right:

  • Before: a photon flies in along the horizontal () axis. The electron (magenta dot) sits at rest at the collision point.
  • After: the photon leaves at angle above the axis with a new, longer wavelength (drawn as a fatter ripple). The electron recoils below the axis at angle .

Each moving object carries two quantities we track:


Step 2 — Conserve energy (the height of the bank account)

WHAT: We say the total energy before equals the total energy after.

WHY: Conservation of energy — nothing creates or destroys energy in a collision. Whatever the photon loses, the electron gains.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

Think of energy as the height of two stacked bars. The left stack (before) and the right stack (after) must reach the same total height:

Term by term: the photon's energy shrank from to (because ), and exactly that missing chunk got added to the electron. Solving for the electron's energy:

The bracket is positive (since ), so : the electron ended up with more than its resting energy. Good — it is moving now.


Step 3 — Conserve momentum as arrows

WHAT: We conserve momentum, but momentum is a vector (an arrow), so we split it into horizontal () and vertical () parts.

WHY: Conservation of momentum holds separately in every direction. A single number can't capture "which way" — arrows can. So we draw the arrows and read off their shadows on each axis.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

The incoming photon's arrow points purely along . After the bounce there are two arrows: the scattered photon (up-right) and the electron (down-right). Their combined shadow on each axis must match the "before" shadow.

Horizontal (): before, only the incoming photon; after, the two horizontal shadows.

Vertical (): before, nothing moves vertically, so the two vertical shadows must cancel.

The minus sign is the whole point: the photon goes up, the electron goes down, and they exactly balance to zero.


Step 4 — Isolate the electron, then delete its angle

WHAT: We move the electron terms alone to one side, then square both equations and add them.

WHY: We do not care where the electron went (). The trick (a right-triangle identity) lets vanish completely.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

Rearranging Step 3 to put the electron's two shadows alone:

Now picture and as the two legs of a right triangle whose hypotenuse is . By Pythagoras the legs squared add to the hypotenuse squared — and the 's collapse:

Expand and use on the photon's angle:

Term by term: two "pure" pieces and (from the two photon speeds), and one cross term that carries the angle. That cross term is where hides — remember it.


Step 5 — The relativistic bridge for the electron

WHAT: We connect the electron's energy to its momentum using the relativistic relation, then square equation so both live as squared quantities.

WHY: We now have from momentum (Step 4) and from energy (Step 2). To make them meet we need the one equation linking a particle's energy and momentum — the Relativistic energy-momentum relation. We use it (not ) because the recoil can be near light-speed.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

The relation is itself a right triangle: is the hypotenuse, and are the legs.

Why square now? The bridge above needs (energy squared), but Step 2 only gave us (energy to the first power). So we square purely to match the form the bridge demands — that's the whole reason for this move, nothing more:

Subtract and divide by — the resting-energy piece cancels beautifully:

We now have two expressions for the same — one from arrows , one from energy . Set them equal.


Step 6 — Equate and watch the cancellation

WHAT: Set and cancel every matching term.

WHY: Both are , so they must be identical. What survives after cancellation is the answer.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

First expand the last term of :

Line up the two sides:

The two "pure" pieces vanish from both sides. What remains is only the cross term and the energy term:

Gather the two pieces on the left:

The angle now lives inside a single, tidy . One step to go.


Step 7 — The final squeeze into

WHAT: Clean up the fractions to reveal .

WHY: We want the shift, a single wavelength difference — so we rewrite as one fraction and divide out the clutter.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

Combine the right-hand bracket over a common denominator:

Substitute and divide both sides by (this kills every ):

Divide by and out drops the result. Here we rename the electron mass as (the subscript "e" just says "electron") to match the standard textbook symbol:


Step 8 — Every case, drawn (this is why we covered all angles)

WHAT: We test the formula at the three landmark angles and the degenerate "wrong mass" case.

WHY: The contract says the reader must never meet a scenario we didn't show. ranges over to , so ranges from to . Let's see all of it.

PICTURE:

Figure — Compton scattering — wavelength shift derivation

Because is symmetric (), scattering "up by " or "down by " gives the same shift — the up/down choice only flips which way the electron recoils, never the wavelength. So every physical angle is covered by this one curve.


The one-picture summary

Figure — Compton scattering — wavelength shift derivation

This single figure compresses the whole journey: collision → two conservation laws → two expressions for → set equal → cancel → shift. Trace the arrows and you have re-derived Compton scattering.

Draw collision, photon in and out plus electron

Conserve energy gives E_e

Conserve momentum x and y

Square and add, delete phi

Square E_e, use relativistic relation

Two forms of p_e squared, set equal

Cancel pure terms, one minus cos survives

Divide out, get Compton shift

Recall Feynman retelling of the whole walkthrough

We drew a bouncy ball of light hitting a still marble (electron). Rule one: the total energy on the "before" shelf must match the "after" shelf — so whatever brightness the light loses, the marble gains as motion (Step 2). Rule two: arrows can't appear from nowhere. The light came in flat, so after the hit the sideways push of the light bouncing up must be cancelled by the marble kicking down (Step 3). We didn't care where the marble went, so we squared its two arrow-legs and added them — Pythagoras erased the marble's angle (Step 4). Then we used Einstein's energy-momentum triangle for the fast marble (Step 5). Now we had the marble's momentum written two ways — once from arrows, once from energy — so we set them equal (Step 6). Magic: all the "plain" pieces cancelled, leaving only the angle wrapped up as . A last tidy-up (Step 7) gave . Zero bend = zero shift; straight-back = biggest shift; hit a whole heavy atom = almost no shift. That last one is the unshifted peak in the real experiment. That's the entire story of the derivation — just pool with light.


Connections

  • Parent note (Hinglish) — the algebra this page illustrates.
  • Photon momentum and energy — supplies , the arrows in Step 3.
  • Relativistic energy-momentum relation — the triangle in Step 5.
  • Conservation of energy and Conservation of momentum — the two rules driving Steps 2–3.
  • de Broglie wavelength — the reverse idea: matter also carries a wavelength.
  • Photoelectric effect — its partner proof that light comes in photons.
  • X-ray production and Bremsstrahlung — where the incoming X-rays come from.

Active-recall flashcards

Which two conservation laws drive the whole derivation?
Energy (Step 2) and momentum in both x and y (Step 3).
How is the electron's recoil angle removed?
Isolate the electron terms, square and add, then use .
Why use the relativistic energy relation, not ?
The recoil can be near light-speed; only gives clean cancellation.
Which terms cancel when the two expressions are equated?
The pure and terms on both sides.
Why does no survive in the final shift?
All -only terms cancel; only the angle term and remain.
Shift at , , ?
, pm, pm.
What produces the unshifted peak?
A tightly bound electron; the whole atom (mass ) recoils, so .