QNT-11
Compton wavelength shift
Δλ = λc (1 − cos θ), λc = h /(me c).
Governing equation
where
- \theta
- Scatter angle (°)
- \lambda
- Incident wavelength (pm)
- \Delta\lambda
- Shift (pm)
- \lambda'
- Scattered wavelength (pm)
The figure, part by part
Each numbered marker wears the color of its card. Hover a card to light the marker. Tap a marker to jump to that card. The slider walks a red point along the curve; Animate drawing traces it like a pen.
Governing law — red
Domain of the variable — blue
Response curve — green
Rate of change — amber
Lecture brief
Historical brief
Planck (1900), Einstein’s photoelectric law, Bohr, de Broglie, Heisenberg and Schrödinger’s 1926 equation rebuilt matter as amplitude. These sheets are the first solvable models: wells, spin, tunneling, uncertainty. This sheet (QNT-11 — Compton wavelength shift) is the form associated with Compton 1923. Working symbols: , , . Treating the photon as a particle of energy hf and momentum h/λ colliding elastically with a free electron yields Compton's shift.
Purpose
Live realistic example
In symbols
Calculator
Inputs
Outputs
- Shift \Delta\lambda2.4263 pm
- Scattered wavelength \lambda'12.4263 pm
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Free library
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- SI Brochure (BIPM)BIPM · Free PDF / open book
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Narration of this film
Free electron at rest, unpolarised photon.
Treating the photon as a particle of energy hf and momentum h/λ colliding elastically with a free electron yields Compton's shift.
Watch on YouTube