Three Polarizers (paradox)
Ideal linear polarizers in series: unpolarized light of unit intensity yields I₁ = 1/2 after the first polarizer. Each subsequent polarizer transmits the component along its transmission axis, so I₂ = I₁ cos²(θ₂ − θ₁) and I₃ = I₂ cos²(θ₃ − θ₂). When θ₁ = 0° and θ₃ = 90°, two polarizers alone give extinction, but a middle polarizer at θ₂ = 45° gives I₃ = (I₁/4) sin²(2θ₂), maximal at 45° — not because light is “created,” but because P₂ rotates the polarization state between the crossed outer sheets.
Who it's for: Follows the Malus-law polarizer page; good for lecture demos of quantum vs classical language (this page stays classical).
Key terms
- Malus law
- linear polarizer
- crossed polarizers
- projection
How it works
Three **linear polarizers** in series: **P₁** prepares polarization, **P₂** is the usual “surprise” insert, **P₃** is often **crossed** with **P₁**. With only **P₁** and **P₃** orthogonal, **Malus** gives **I₃ = 0**. Adding **P₂** at **45°** between them gives **I₃ = (I₁/4) sin²(2θ₂)** when **θ₁ = 0** and **θ₃ = 90°** — **nonzero** at **θ₂ = 45°**. The third sheet **projects** twice; intensities multiply as **cos²** of successive axis differences (after **P₁**, **I₂ = I₁ cos²(θ₂−θ₁)**, **I₃ = I₂ cos²(θ₃−θ₂)**).
Key equations
Frequently asked questions
- Does this violate energy conservation?
- No. The middle sheet absorbs the orthogonal component at each stage; the final intensity is still ≤ the incident intensity. With three ideal sheets the transmitted fraction is at most 1/8 of the incident unpolarized power in the symmetric 0–45–90 configuration.
- Why is the “paradox” not seen with two polarizers only?
- Two crossed polarizers block because the field after the first is orthogonal to the second. A third at 45° creates a component along the last axis in two steps: first projection onto 45°, then onto 90°.
More from Optics & Light
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Airy Disk & Rayleigh Limit
Circular aperture Fraunhofer pattern; first dark ring; two-point resolution.
Optical Bench (sandbox)
Up to 4 elements: thin lenses, vertical mirrors, wedge δ; paraxial ray trace.
Telescope & Microscope (2 lenses)
Kepler / Galileo / microscope presets; paraxial rays, M, f_obj/f_eye hint.
Whispering Gallery (Rays)
Circular mirror: shallow chords refocus acoustic energy opposite the source (geometric optics).
Fiber Bragg Grating
λ_B = 2 n_eff Λ; Lorentzian toy reflectivity vs λ and probe wavelength.
Laser Speckle
Random phased waves: |Σ e^{i(k·r+φ)}|² grain pattern (qualitative).