Compton Shift Calculator
Find the Compton wavelength shift.
Result
How it is calculated
The shift depends only on the scattering angle, not on the incoming photon's wavelength: Δλ = λc × (1 − cos θ). Here θ is the angle in degrees between the incoming and scattered photon directions, and λc = h/(mₑc) = 2.42631023867×10⁻¹² m is the electron Compton wavelength. The tool converts the angle to radians, evaluates the cosine and reports the shift both in picometres (4 decimals) and in metres (scientific notation). It accepts angles from 0° to 180° only; anything outside that range returns no result. The shift is zero at 0° (no deflection) and largest at 180° (backscatter), where it equals 2λc.
Worked example
Take a scattering angle of 60°. Then cos 60° = 0.5, so 1 − cos θ = 0.5. Multiply by the Compton wavelength: 2.4263 pm × 0.5 ≈ 1.2132 pm. The result is 1.2132 pm, or 1.2132e-12 m. The scattered photon's wavelength is therefore longer than the incident one by about 1.2 picometres.
Common mistakes
- Entering the angle in radians: the field expects degrees, so π/2 typed as 1.5708 is read as about 1.57°, giving a tiny shift.
- Confusing the scattering angle θ with the angle of the recoiling electron; the formula uses the photon's deflection angle.
- Expecting the shift to depend on the incident wavelength. It does not, which is why it is only noticeable for X-rays and gamma rays whose wavelength is comparable to a few picometres.
- Entering an angle above 180° (for example 270°) to mean a reflex angle; the tool returns nothing because the valid range is 0–180°.
- Treating the result as the new wavelength rather than the increase in wavelength.
About this calculator
This calculator finds the Compton wavelength shift, Δλ = λ_c(1 − cos θ), that occurs when a photon scatters off a free electron and loses energy — where λ_c is the electron's Compton wavelength (h/mₑc ≈ 2.426 pm) and θ is the scattering angle. Discovered experimentally by Arthur Compton in 1923, this shift is measurable only in high-energy photons like X-rays and gamma rays, and it was decisive proof that light behaves as discrete particles (photons) carrying momentum, not just waves.
The Compton effect is central to X-ray physics and medical imaging (it accounts for a major source of image scatter and dose in radiography and CT), astrophysics (Compton scattering shapes the spectra of X-ray sources and the early universe's photon-baryon interactions), and radiation detector design in particle physics.
Physics students studying quantum mechanics and wave-particle duality, medical physicists modeling radiation dose and scatter, and researchers working with X-ray or gamma-ray spectroscopy all use this calculation, entering the scattering angle to find the wavelength shift.
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