Optical Dispersion
Also known as: Cauchy Dispersion Formula · Chromatic Dispersion
A material's electrons resonate at ultraviolet frequencies. Visible light pushes those electrons, and the closer its frequency is to resonance (toward blue), the more strongly the medium responds — raising the index. Shorter wavelength means larger n, so blue bends more.
White light enters a prism and fans into a spectrum whose spread tracks the Cauchy dispersion n(lambda) = A + B/lambda^2.
Equivalent forms
Two fitted constants reproduce the entire visible color-spread of a glass — the math behind every prism and the chromatic flaw in every cheap lens.
Unit systems
- SI:
- lambda in nm (or m), n dimensionless
- CGS:
- lambda in cm
- Imperial:
- n dimensionless
Where it holds
Cauchy fit the measured index of glasses to an empirical inverse-power series in wavelength. Decades later Sellmeier grounded the behavior in resonance physics, but Cauchy's compact A + B/lambda^2 still serves the visible band.
Why does a prism fan white light into a rainbow?
Glass slows blue light more than red, so the refractive index depends on wavelength. Cauchy's formula captures this dispersion — the reason every color bends by a different angle.