Polarization

Light from the Sun, a bulb, or a candle is a transverse wave, and a transverse wave's displacement can point anywhere perpendicular to its direction of travel. Polarization is simply the bookkeeping of which direction it points, and how that direction changes with time. Two perpendicular oscillations of the same frequency, added together with some fixed phase lag between them, can trace out a straight line, a circle, or an ellipse — and that shape is the polarization state. This matters practically the moment you put a polarizing filter (sunglasses, an LCD screen, a camera filter) in the beam: the filter passes only the component of the electric field along its own axis, and Malus's law tells you exactly how much intensity survives. This article builds linear, circular, and elliptical polarization from two perpendicular SHMs with a phase difference δ\delta, then works Malus's law through a multi-polarizer problem.

The core insight

Two perpendicular SHM components with a fixed phase difference δ\delta trace a line, circle, or ellipse — the shape is the polarization state — and a polarizer transmits intensity I=I0cos⁡2θI=I_0\cos^2\theta of whatever linearly polarized light hits it (Malus's law).

The core idea

A transverse wave travelling along zz has its displacement confined to the xyxy-plane, perpendicular to the propagation direction. Write the two perpendicular components as SHMs of the same frequency and amplitude parameters E0x,E0yE_{0x}, E_{0y}, differing only by a phase δ\delta:

Ex(z,t)=E0xcos⁡(kz−ωt),Ey(z,t)=E0ycos⁡(kz−ωt+δ).E_x(z,t) = E_{0x}\cos(kz-\omega t), \qquad E_y(z,t) = E_{0y}\cos(kz-\omega t+\delta).

where: E0x,E0yE_{0x}, E_{0y} are the component amplitudes, kk is the wavenumber, ω\omega is the angular frequency, and δ\delta is the phase difference between the two components. As tt advances, the resultant vector E⃗=Exx^+Eyy^\vec E = E_x\hat x + E_y\hat y sweeps out a curve in the xyxy-plane, and the shape of that curve names the polarization state.

  • Linear polarization (δ=0\delta = 0 or π\pi): the two components rise and fall in lockstep (or exactly opposed), so E⃗\vec E never leaves a single fixed line, at angle θ=arctan⁡(±E0y/E0x)\theta = \arctan(\pm E_{0y}/E_{0x}) to the xx-axis. Nothing rotates; only the magnitude oscillates.
  • Circular polarization (E0x=E0y=E0E_{0x}=E_{0y}=E_0, δ=±π/2\delta = \pm\pi/2): then Ex=E0cos⁡(kz−ωt)E_x = E_0\cos(kz-\omega t) and Ey=∓E0sin⁡(kz−ωt)E_y = \mp E_0\sin(kz-\omega t), so Ex2+Ey2=E02E_x^2+E_y^2=E_0^2 at every instant — a circle of constant radius. The tip of E⃗\vec E rotates at the steady rate ω\omega, and the sign of δ\delta fixes whether that rotation is right- or left-handed.
  • Elliptical polarization is the general case: any E0x,E0y,δE_{0x}, E_{0y}, \delta outside the two special conditions above traces an ellipse. Linear and circular polarization are its degenerate limits — collapse the ellipse to a line at δ=0,π\delta=0,\pi, or inflate it to a circle when E0x=E0yE_{0x}=E_{0y} and δ=π/2\delta=\pi/2.

Unpolarized light (an ordinary bulb, the Sun) has no fixed δ\delta at all — it is an incoherent jumble of many independent polarization states, so E⃗\vec E's direction wanders randomly and rapidly with no traceable pattern.

Malus's law. A linear polarizer transmits only the component of E⃗\vec E along its transmission axis. If linearly polarized light of amplitude E0E_0 (intensity I0I_0) meets a polarizer with its axis at angle θ\theta to E⃗\vec E, the transmitted amplitude is E0cos⁡θE_0\cos\theta, so intensity — proportional to amplitude squared — obeys

I=I0cos⁡2θ.I = I_0\cos^2\theta.

where: I0I_0 is the intensity of the already linearly polarized light striking the polarizer, and θ\theta is the angle between the incoming polarization direction and the polarizer's transmission axis. When unpolarized light hits the first polarizer, there is no single θ\theta to plug in — averaging cos⁡2θ\cos^2\theta over all directions gives ⟨cos⁡2θ⟩=1/2\langle\cos^2\theta\rangle = 1/2, so exactly half the intensity survives, and the transmitted beam emerges fully linearly polarized along that polarizer's axis. Any polarizer placed after that one then obeys Malus's law directly, since its input is now linearly polarized.

Figure
Two perpendicular oscillations with a quarter turn phase lag combine into a circle traced by the tip of the field vector
Two perpendicular SHMs with delta equal to pi over 2 trace a circle Ex Ey tip of E at t = 0 rotates at rate omega Ex(t) = E0 cos(omega t) Ey(t) = E0 sin(omega t), quarter cycle ahead
Derivation ATransmitted intensity through a linear polarizer

The goal is to show why the intensity transmitted by an ideal linear polarizer, when the incoming light is already linearly polarized at angle θ\theta to the polarizer's transmission axis, must fall off as cos⁡2θ\cos^2\theta rather than as a simple linear factor of θ\theta — the difference between amplitude and intensity is the whole content of the derivation, and it is exactly the step students skip.

Step 1. Resolve the incoming field. Let the incoming linearly polarized light have amplitude E0E_0, oscillating along a fixed direction that makes angle θ\theta with the polarizer's transmission axis. Decompose E0E_0 into a component along the axis, E0cos⁡θE_0\cos\theta, and a component perpendicular to it, E0sin⁡θE_0\sin\theta.

Step 2. Apply what an ideal polarizer does. An ideal polarizer transmits the full component along its axis and blocks the perpendicular component entirely — it does not attenuate the parallel piece at all. So the transmitted amplitude is simply Eout=E0cos⁡θE_{\text{out}} = E_0\cos\theta; nothing more subtle happens at this stage.

Step 3. Convert amplitude to intensity. Intensity is proportional to the square of amplitude, I∝E2I \propto E^2, because energy flux in a wave goes as the square of the field. So Iout∝(E0cos⁡θ)2=E02cos⁡2θI_{\text{out}} \propto (E_0\cos\theta)^2 = E_0^2\cos^2\theta, while the incoming intensity is I0∝E02I_0 \propto E_0^2. Dividing the two removes the unknown proportionality constant.

Step 4. Read off Malus's law. Taking the ratio gives Iout/I0=cos⁡2θI_{\text{out}}/I_0 = \cos^2\theta, so I=I0cos⁡2θI = I_0\cos^2\theta. The squaring is the entire reason the falloff is gentler near θ=0\theta=0 and steeper near θ=90∘\theta=90^\circ than a plain cos⁡θ\cos\theta would give — a common point of confusion, since it is amplitude, not intensity, that goes as cos⁡θ\cos\theta.

Worked example

Unpolarized light of intensity I0=100 W/m2I_0 = 100\ \text{W/m}^2 passes through two ideal polarizers in sequence: the first has a vertical axis, the second (the analyzer) is set at 30∘30^\circ to the first. A third question asks what angle would instead reduce the final intensity to exactly I0/8I_0/8.

Step 1. Unpolarized light striking the first polarizer transmits half its intensity, emerging linearly polarized along the vertical: I1=I0/2=100/2=50 W/m2I_1 = I_0/2 = 100/2 = 50\ \text{W/m}^2.

Step 2. Apply Malus's law at the second polarizer with θ=30∘\theta=30^\circ between the now-polarized beam and the analyzer's axis: I2=I1cos⁡2(30∘)=50×(3/2)2=50×(3/4)=37.5 W/m2I_2 = I_1\cos^2(30^\circ) = 50\times(\sqrt3/2)^2 = 50\times(3/4) = 37.5\ \text{W/m}^2.

Step 3. For the third part, require I2=I0/8=12.5 W/m2I_2 = I_0/8 = 12.5\ \text{W/m}^2 using I2=(I0/2)cos⁡2θI_2 = (I_0/2)\cos^2\theta: I0/8=(I0/2)cos⁡2θ  ⟹  cos⁡2θ=1/4  ⟹  cos⁡θ=1/2  ⟹  θ=60∘I_0/8 = (I_0/2)\cos^2\theta \implies \cos^2\theta = 1/4 \implies \cos\theta = 1/2 \implies \theta = 60^\circ.

The intensity after the first polarizer is 50 W/m², after the second (at 30°) is 37.5 W/m², and an analyzer angle of 60° would instead give exactly I0/8=12.5 W/m2I_0/8 = 12.5\ \text{W/m}^2.

Competitive stretch

A wave has Ex=3cos⁡(kz−ωt)E_x=3\cos(kz-\omega t) and Ey=3cos⁡(kz−ωt+π/2)E_y=3\cos(kz-\omega t+\pi/2) (SI units, V/m). Equal amplitudes with δ=π/2\delta=\pi/2 is exactly the circular-polarization condition, so this beam is circularly polarized, and its tip sweeps through every orientation over one cycle — a linear polarizer placed in this beam transmits exactly half the intensity, independent of the polarizer's orientation, unlike the strongly angle-dependent linear case above.

Common traps

  • Treating "polarized" and "coherent" as the same idea. Polarization is about the direction E⃗\vec E oscillates in; coherence is about phase stability over time between different waves — logically separate properties.
  • Applying Malus's law to unpolarized input directly. I=I0cos⁡2θI=I_0\cos^2\theta needs I0I_0 to already be linearly polarized. For unpolarized light on the first polarizer, halve the intensity first, then apply Malus's law only from the second polarizer onward.
  • Confusing amplitude falloff with intensity falloff. The field component drops as cos⁡θ\cos\theta, but intensity — the measurable quantity — drops as cos⁡2θ\cos^2\theta, the square, as the derivation above makes explicit.
  • Assuming sound can be polarized. Polarization needs a transverse wave with two independent perpendicular oscillation directions; sound is longitudinal and has none, so the concept simply does not apply to it.

Ask the tutor: want to work through three polarizers in sequence, or convert an amplitude-and-phase description into the resulting ellipse shape — ask the AI tutor to walk it with you.

Why does unpolarized light lose exactly half its intensity at the first polarizer, not some other fraction?

Because unpolarized light has no preferred direction — E⃗\vec E points every which way with equal likelihood over time, so the transmitted fraction cos⁡2θ\cos^2\theta needs to be averaged over all θ\theta from 00 to 2π2\pi. That average, ⟨cos⁡2θ⟩\langle\cos^2\theta\rangle, works out to exactly 1/21/2 regardless of the polarizer's orientation, since there is nothing in unpolarized light to prefer one axis over another. Once past that first polarizer, though, the light is fully linear, so any later polarizer follows Malus's law with a definite θ\theta, not an average.

How is circular polarization different from unpolarized light — both seem to have no fixed direction?

The key difference is coherence and predictability. In circularly polarized light, ExE_x and EyE_y are locked together by a fixed phase difference δ=±π/2\delta=\pm\pi/2 and equal amplitude, so the tip of E⃗\vec E traces a perfectly repeatable circle at a steady rate ω\omega — you can predict exactly where it points at any future instant. Unpolarized light has no such fixed relationship at all; its direction wanders randomly and unpredictably, with no traceable curve. Circular polarization is a definite, orderly state; unpolarized light is the absence of any such order.

If I stack three polarizers, can the final intensity ever exceed what two polarizers alone would give?

Yes, surprisingly — inserting a polarizer at an intermediate angle between two crossed polarizers (at 90∘90^\circ to each other, which alone transmit nothing) can let some light through, because each stage re-polarizes the beam along its own axis before the next cos⁡2θ\cos^2\theta factor is applied. With just two crossed polarizers you get zero; add a third at, say, 45∘45^\circ between them, and each stage's Malus factor is no longer zero, so light gets through where two alone blocked it completely. Work each stage in sequence, feeding each output intensity in as the next stage's I0I_0.

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Where this leads