Virtual laboratory/Physics/Atomic physics/The Compton effect — the photon has momentum

The Compton effect — the photon has momentum

An extension of the wave–particle duality and photon topic. A photon scatters off an electron and gives up part of its momentum, so its wavelength increases: Δλ=(h/m_e·c)(1−cosθ). This is proof of the corpuscular nature of light — the photon has momentum (Compton, Nobel 1927).

The Compton effect — the photon has momentum
Physics · Atomic physics · The Compton effect (FIZ.ATOM.PP.05)
Photon scattering angle θ\theta45 °
After scattering off the electron, the photon’s wavelength…
angle θ
45°
wavelength shift Δλ
0.71 pm
wavelength λ'
71.81 pm
energy E'
17.27 keV
🎯 Challenge: hit the shift Δλ
streak: 0

I’ll give you a target Compton shift — set the angle θ to reach it. Δλ = λ_C(1−cosθ).

What just happened?

An X-ray photon struck a free electron like a billiard ball. It gave up part of its momentum and energy, so it bounced off “weaker” — with lower energy, and therefore a longer wavelength. This is the Compton effect.

The Compton shift:

Δλ=λ′−λ0=hmec (1−cos⁡θ)\Delta\lambda = \lambda' - \lambda_0 = \frac{h}{m_e c}\,(1-\cos\theta)

— the increase in wavelength depends only on the scattering angle θ\theta, not on the incident wavelength. The constant λC=h/(mec)≈2.43 pm\lambda_C = h/(m_e c) \approx 2.43\ \text{pm} is the Compton wavelength of the electron. Since 1−cos⁡θ≥01-\cos\theta \ge 0, always Δλ≥0\Delta\lambda \ge 0 — the photon never gains energy.

Extreme cases:

For θ=0∘\theta = 0^\circ (the photon flies straight on) Δλ=0\Delta\lambda = 0 — no collision. For θ=180∘\theta = 180^\circ (back-scattering) the shift is largest: Δλ=2λC\Delta\lambda = 2\lambda_C, because the electron receives maximum momentum.

Why does this matter?

A wave cannot “collide” and transfer momentum like a particle. The fact that the collision calculation works out proves the photon has momentum p=h/λp = h/\lambda and behaves like a particle. The Compton effect is one of the pillars of wave–particle duality.

Why you need this for the exam:

The formula Δλ=λC(1−cos⁡θ)\Delta\lambda = \lambda_C(1-\cos\theta) plus p=h/λp = h/\lambda and conservation of momentum solve Compton scattering problems. The trick: the angle θ\theta gives Δλ, hence λ′\lambda' and the energy of the scattered photon E′=hc/λ′E' = hc/\lambda'.

Remember: the scattered photon always has a longer wavelength (lower energy) — Δλ = λ_C(1−cosθ) ≥ 0. That is proof that light has momentum and a corpuscular nature.

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Theory & formulas

Scattering off an electron

The photon collides with the electron like a particle, giving up part of its energy and momentum, so its wavelength increases: Δλ=hmec(1−cos⁡θ)\Delta\lambda = \dfrac{h}{m_e c}(1 - \cos\theta)

What it proves

The photon has momentum p=hλp=\dfrac{h}{\lambda} — this is proof of the corpuscular nature of light (Compton, Nobel 1927). The shift is largest for back-scattering (θ=180°\theta=180°).

Symbols: Δλ\Delta\lambda — the Compton shift, hh — the Planck constant, mem_e — the electron mass, cc — the speed of light, θ\theta — the scattering angle, pp — the photon momentum.

Frequently asked questions

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What did the Compton effect prove?

That the photon has momentum (p=h/λ) and behaves like a particle in a collision with an electron.

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Why does the photon's wavelength increase?

Because it gives up part of its energy and momentum to the electron — lower energy means a larger λ.

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What does the Compton shift depend on?

On the scattering angle: Δλ=(h/m_e c)(1−cosθ), largest at 180°.

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