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Polarization

5.1 States of Polarization

For a plane wave propagating in the zz-direction:

E=E0xcos(kzωt)x^+E0ycos(kzωt+δ)y^\mathbf{E} = E_{0x}\cos(kz - \omega t)\,\hat{\mathbf{x}} + E_{0y}\cos(kz - \omega t + \delta)\,\hat{\mathbf{y}}

  • Linear polarization: δ=0\delta = 0 or δ=π\delta = \pi. The E-field oscillates along a fixed line.
  • Circular polarization: E0x=E0yE_{0x} = E_{0y} and δ=±π/2\delta = \pm\pi/2. Right-handed (δ=π/2\delta = -\pi/2) or left-handed (δ=+π/2\delta = +\pi/2).
  • Elliptical polarization: General case. The tip of E\mathbf{E} traces an ellipse.

5.2 Malus”s Law

When linearly polarised light of intensity I0I_0 passes through a polariser at angle θ\theta to the Polarisation direction:

I=I0cos2θI = I_0 \cos^2\theta

Proof. The component of E\mathbf{E} along the polariser axis is EcosθE\cos\theta. Since IE2I \propto E^2: I=I0cos2θI = I_0 \cos^2\theta. \blacksquare

Worked Example: Three polarisers in series

Problem. Unpolarised light of intensity I0I_0 passes through three ideal linear polarisers. The First has its transmission axis vertical. The second is at 45°45° to the vertical. The third is Horizontal. What fraction of I0I_0 is transmitted?

Solution. After the first polariser: I1=I0/2I_1 = I_0/2 (vertical polarisation).

After the second: I2=I1cos245°=(I0/2)(1/2)=I0/4I_2 = I_1\cos^2 45° = (I_0/2)(1/2) = I_0/4 (polarised at 45°).

After the third: I3=I2cos245°=(I0/4)(1/2)=I0/8I_3 = I_2\cos^2 45° = (I_0/4)(1/2) = I_0/8 (horizontal polarisation).

Answer: I0/8=12.5%I_0/8 = 12.5\%. Note that inserting the middle polariser increases the transmitted Intensity compared with just the crossed first and third polarisers (which would transmit zero).

5.3 Birefringence and Wave Plates

Birefringent crystals (e.g., calcite) have two refractive indices: non_o (ordinary ray) and nen_e (extraordinary ray). The two rays have orthogonal polarisations and different phase velocities.

A wave plate of thickness tt introduces a relative phase shift between the two polarisation Components:

Δϕ=2πλ(none)t\Delta\phi = \frac{2\pi}{\lambda}(n_o - n_e)\,t

Quarter-wave plate (QWP): Δϕ=π/2\Delta\phi = \pi/2So tQWP=λ/(4none)t_{\mathrm{QWP} = \lambda/(4|n_o - n_e|)}. Converts linear polarisation at 45°45° to the fast/slow axes into circular polarisation, and vice Versa.

Half-wave plate (HWP): Δϕ=π\Delta\phi = \piSo tHWP=λ/(2none)t_{\mathrm{HWP} = \lambda/(2|n_o - n_e|)}. Rotates the plane of linear polarisation by 2θ2\thetaWhere θ\theta is the angle between the Input polarisation and the fast axis.

:::caution Common Pitfall A quarter-wave plate only produces circular polarisation when the input linear polarisation is at Exactly 45°45° to the fast and slow axes. For other input angles, the output is elliptically Polarised. A half-wave plate rotates linear polarisation by 2θ2\thetaNot θ\theta.

Worked Example: Quarter-wave plate design and application

Problem. (a) Design a quarter-wave plate for λ=589\lambda = 589 nm using calcite (no=1.658n_o = 1.658, ne=1.486n_e = 1.486). (b) If linearly polarised light at 30°30° to the fast axis Enters this QWP, describe the output polarisation.

Solution.

(a) Minimum thickness: t=λ/(4none)=589×109/(4×0.172)=8.56×107t = \lambda/(4|n_o - n_e|) = 589 \times 10^{-9}/(4 \times 0.172) = 8.56 \times 10^{-7} m =856= 856 nm.

(b) The components along the fast and slow axes are: Ef=E0cos30°=0.866E0E_f = E_0\cos 30° = 0.866\,E_0 and Es=E0sin30°=0.500E0E_s = E_0\sin 30° = 0.500\,E_0. After the QWP, these have a π/2\pi/2 phase difference but unequal amplitudes (0.8660.5000.866 \neq 0.500), So the output is elliptically polarised (not circular).

5.4 Optical Activity

Certain materials (sugars, quartz) rotate the plane of linearly polarised light. The specific Rotation is:

[α]=θcl[\alpha] = \frac{\theta}{c \cdot l}

Where θ\theta is the rotation angle, cc is the concentration, and ll is the path length.

Optical activity arises from the helical structure of molecules, which gives different refractive Indices for left- and right-circularly polarised light (circular birefringence). If nLn_L and nRn_R Are the refractive indices for left and right circular polarisation:

θ=πlλ(nLnR)\theta = \frac{\pi l}{\lambda}(n_L - n_R)

Optical activity is reciprocal: if the beam is reflected back through the medium, the rotation Is cancelled.

5.5 Brewster’s Angle

At the Brewster angle θB\theta_BThe reflected beam for p-polarised light vanishes (rp=0r_p = 0):

tanθB=n2n1\tan\theta_B = \frac{n_2}{n_1}

Proof. Setting rp=0r_p = 0 requires n2cosθi=n1cosθtn_2\cos\theta_i = n_1\cos\theta_t. Using Snell’s law n1sinθi=n2sinθtn_1\sin\theta_i = n_2\sin\theta_t:

cosθisinθi=cosθtsinθt    cotθi=cotθt    θi=θt\frac{\cos\theta_i}{\sin\theta_i} = \frac{\cos\theta_t}{\sin\theta_t} \implies \cot\theta_i = \cot\theta_t \implies \theta_i = \theta_t'

Where θt=90°θt\theta_t' = 90° - \theta_t. This gives θi+θt=90°\theta_i + \theta_t = 90°So:

tanθi=n2n1\tan\theta_i = \frac{n_2}{n_1} \quad \blacksquare

At Brewster’s angle, the reflected beam is purely s-polarised, and the reflected and refracted beams Are perpendicular (θB+θt=90°\theta_B + \theta_t = 90°). This principle is used in Brewster windows and Polarisation by reflection.

For an air-glass interface (n1=1n_1 = 1, n2=1.5n_2 = 1.5): θB=arctan(1.5)=56.3°\theta_B = \arctan(1.5) = 56.3°.

Worked Example: Brewster's angle and reflected intensity

Problem. Unpolarised light is incident on a glass surface (n=1.50n = 1.50) at Brewster’s angle. What fraction of the incident intensity is reflected, and what is the polarisation state of the Reflected light?

Solution. θB=arctan(1.50)=56.3°\theta_B = \arctan(1.50) = 56.3°.

The reflected light is purely s-polarised. The reflectance for s-polarisation at θB\theta_B: θt=90°56.3°=33.7°\theta_t = 90° - 56.3° = 33.7°. rs=n1cosθBn2cosθtn1cosθB+n2cosθt=cos56.3°1.50cos33.7°cos56.3°+1.50cos33.7°=0.5551.50×0.8320.555+1.50×0.832=0.5551.2480.555+1.248=0.6931.803=0.384r_s = \frac{n_1\cos\theta_B - n_2\cos\theta_t}{n_1\cos\theta_B + n_2\cos\theta_t} = \frac{\cos 56.3° - 1.50\cos 33.7°}{\cos 56.3° + 1.50\cos 33.7°} = \frac{0.555 - 1.50 \times 0.832}{0.555 + 1.50 \times 0.832} = \frac{0.555 - 1.248}{0.555 + 1.248} = \frac{-0.693}{1.803} = -0.384

Rs=(0.384)2=0.148R_s = (-0.384)^2 = 0.148.

The incident unpolarised light has equal s and p components (Is=Ip=I0/2I_s = I_p = I_0/2). Only the s Component is reflected: Ireflected=Rs×I0/2=0.148×I0/2=0.074I0I_{\mathrm{reflected} = R_s \times I_0/2 = 0.148 \times I_0/2 = 0.074\,I_0}.

The reflected light is 100% s-polarised with intensity 0.074I00.074\,I_0 (about 7.4% of the incident).

5.6 Faraday Rotation

In a magneto-optical material with a magnetic field B\mathbf{B} applied along the propagation Direction, the plane of polarisation rotates by:

θF=VBl\theta_F = V B l

Where VV is the Verdet constant (rad/(T\cdotM)), BB is the magnetic field strength, and ll is the path length through the material.

Mechanism. The magnetic field induces circular birefringence: left and right circular polarisations Experience different refractive indices (nLnRn_L \neq n_R). Unlike natural optical activity, Faraday Rotation is non-reciprocal: if the beam is reflected back through the medium, the rotation Doubles rather than cancelling.

Applications. Optical isolators (one-way light valves), optical circulators, and magneto-optical Sensors. An optical isolator consists of a polariser, a Faraday rotator set to rotate by 45°45°And An analyser at 45°45° to the polariser. Forward-propagating light is transmitted; backward light Is rotated by another 45°45° (total 90°90°) and blocked by the analyser.

Worked Example: Faraday rotation in flint glass

Problem. A Faraday rotator uses heavy flint glass with Verdet constant V=32V = 32 rad/(T\cdotM). (a) What magnetic field over a 10 cm length produces a 45°45° rotation? (b) If linearly polarised Light makes a round trip through the rotator, what is the total rotation?

Solution.

(a) θF=VBl    B=θF/(Vl)=(π/4)/(32×0.10)=0.785/3.2=0.245\theta_F = VBl \implies B = \theta_F/(Vl) = (\pi/4)/(32 \times 0.10) = 0.785/3.2 = 0.245 T.

(b) Because Faraday rotation is non-reciprocal, the return trip adds another 45°45°: Total rotation =90°= 90°. The polarisation is rotated by 90°90° after the round trip, which is the Basis of optical isolation.

5.7 Polarization by Scattering

When light is scattered by particles much smaller than the wavelength (Rayleigh scattering), the Scattered light is partially polarised. Light scattered at 90°90° to the incident direction is completely linearly polarised in the plane perpendicular to the scattering plane.

Proof. Consider an incident unpolarised beam propagating along z^\hat{\mathbf{z}}. The E\mathbf{E}-field oscillates in the xyxy-plane. An observer along x^\hat{\mathbf{x}} (scattering Angle 90°90°) receives radiation from the accelerating electrons. The dipole radiation pattern of an Oscillator along y^\hat{\mathbf{y}} has zero intensity along y^\hat{\mathbf{y}} but maximum along x^\hat{\mathbf{x}}. The oscillator along x^\hat{\mathbf{x}} radiates zero along its own axis. Thus The observer along x^\hat{\mathbf{x}} sees only the yy-component: the scattered light is Polarised along y^\hat{\mathbf{y}}. \blacksquare

This explains why the sky is polarised at 90°90° from the sun and why polarising sunglasses reduce Glare from horizontal surfaces (Brewster’s angle reflection from road/water).

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