Klein–Nishina Cross Section
Also known as: Compton Scattering Cross Section
QED correction to Thomson scattering: photon cross-section shrinks at high energy.
Polar plot of the Klein–Nishina cross section: increase photon energy and watch forward scattering dominate.
The first experimentally verified prediction of QED — from Dirac's equation to detector clicks.
Unit systems
Where it holds
Dimensional analysis
Klein and Nishina applied the Dirac equation to photon-electron scattering, producing the first fully relativistic QED cross section.
Why do high-energy gamma rays pass through matter more easily than low-energy ones?
Estimate the total cross-section for 1 MeV photons scattering off free electrons.
- Medical imaging: Compton scattering dominates in CT scans at diagnostic energies
- Gamma-ray telescope design (Compton telescopes)
- Radiation shielding calculations for nuclear reactors
- Inverse Compton scattering in astrophysics (boosting CMB photons to X-ray energies)
- The Klein-Nishina formula is NOT the same as Thomson scattering — Thomson is only the low-energy limit.
- The scattered photon always has lower energy than the incident one (except , not higher.
- The formula assumes a free electron at rest — bound electrons require atomic form factors (incoherent scattering function).
Limiting cases
What if…
The formula reduces to the Thomson cross section , independent of photon energy. The scattering becomes symmetric in forward/backward directions.
The total cross section drops . The photon is extremely penetrating and scattering is sharply forward-peaked.
A relativistic electron boosts low-energy photons to high energies. The cross section in the electron rest frame still follows Klein-Nishina, but Lorentz transformation shifts the result. This process powers astrophysical X-ray and gamma-ray sources.
Differential cross section at 90° for a 1 MeV photon
- ω:
- θ:
- r c:
- 3.8615926e-13
- α:
- 0.00729735
- m e c2:
- 0.511 MeV
- Step 1: Find using Compton formula: .
- Step 2: Compute prefactor: .
- Step 3: Compute bracket: .
- Step 4: .
Forward scattering (θ → 0) for a 0.1 MeV photon
- ω:
- θ:
- 0.01 rad
- r c:
- 3.8615926e-13
- α:
- 0.00729735
- Step 1: : , (negligible shift).
- Step 2: Bracket: .
- Step 3: Prefactor: .
- Step 4: . This matches the Thomson forward scattering value .