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Fresnel Equations | Physics - Wyatt's Notes

When light strikes a planar interface between media with refractive indices n1n_1 and n2n_2The Amplitudes of the reflected and transmitted waves depend on the polarisation.

For an incident wave with amplitude EiE_iThe reflection and transmission coefficients are:

s-polarisation (perpendicular to the plane of incidence):

rs=n1cosθin2cosθtn1cosθi+n2cosθt,ts=2n1cosθin1cosθi+n2cosθtr_s = \frac{n_1\cos\theta_i - n_2\cos\theta_t}{n_1\cos\theta_i + n_2\cos\theta_t}, \quad t_s = \frac{2n_1\cos\theta_i}{n_1\cos\theta_i + n_2\cos\theta_t}

p-polarisation (parallel to the plane of incidence):

rp=n2cosθin1cosθtn2cosθi+n1cosθt,tp=2n1cosθin2cosθi+n1cosθtr_p = \frac{n_2\cos\theta_i - n_1\cos\theta_t}{n_2\cos\theta_i + n_1\cos\theta_t}, \quad t_p = \frac{2n_1\cos\theta_i}{n_2\cos\theta_i + n_1\cos\theta_t}

Reflectance and transmittance (energy fractions):

R=r2,T=n2cosθtn1cosθit2R = |r|^2, \quad T = \frac{n_2\cos\theta_t}{n_1\cos\theta_i}|t|^2

With R+T=1R + T = 1 (energy conservation).

At the Brewster angle θB\theta_BThe reflected beam for p-polarised light has zero amplitude: rp=0r_p = 0:

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

Proof. Setting rp=0r_p = 0: 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\frac{\cos\theta_i}{\sin\theta_i} = \frac{\cos\theta_t}{\sin\theta_t}

cotθi=cotθt    θi+θt=90\cot\theta_i = \cot\theta_t \implies \theta_i + \theta_t = 90^\circ

So tanθi=tanθB=n2/n1\tan\theta_i = \tan\theta_B = n_2/n_1. \blacksquare

At Brewster’s angle, the reflected and refracted beams are perpendicular. This is why polarising Filters work at specific angles for reflected glare.

10.3 Total Internal Reflection and the Evanescent Wave

Section titled “10.3 Total Internal Reflection and the Evanescent Wave”

When n1>n2n_1 \gt n_2 and θi>θc=arcsin(n2/n1)\theta_i \gt \theta_c = \arcsin(n_2/n_1), sinθt>1\sin\theta_t \gt 1So cosθt=isin2θt1\cos\theta_t = i\sqrt{\sin^2\theta_t - 1} becomes imaginary.

The transmitted field becomes an evanescent wave:

Eteκxei(kzzωt)E_t \propto e^{-\kappa x}\, e^{i(k_z z - \omega t)}

Where κ=k0n12sin2θin22\kappa = k_0\sqrt{n_1^2\sin^2\theta_i - n_2^2} and kz=k0n1sinθik_z = k_0 n_1\sin\theta_i.

The field decays exponentially with penetration depth δ=1/κ\delta = 1/\kappa but propagates along the Interface. No energy is transported into the second medium: R=1R = 1.

Frustrated total internal reflection. If a third medium is brought within a few wavelengths of The interface, energy can tunnel across the gap (analogous to quantum tunnelling).

The Fresnel coefficients are real for θi<θc\theta_i < \theta_c (normal incidence/transmission) and may be positive or negative, indicating phase shifts:

  • External reflection (n1<n2n_1 < n_2): rs<0r_s < 0 for all θi\theta_i (phase shift of π\pi for s-polarisation). rpr_p changes sign at Brewster’s angle.
  • Internal reflection (n1>n2n_1 > n_2): For θi<θc\theta_i < \theta_c, both rsr_s and rpr_p are positive at normal incidence. rpr_p changes sign at Brewster’s angle.

At normal incidence (θi=0\theta_i = 0):

rs=rp=n1n2n1+n2r_s = r_p = \frac{n_1 - n_2}{n_1 + n_2}

The reflection coefficient is negative when n1<n2n_1 < n_2, corresponding to a π\pi phase shift. For n1>n2n_1 > n_2, the reflection coefficient is positive (no phase shift).

The reflectance RR varies with angle of incidence:

  • For s-polarisation, RsR_s increases monotonically from ((n1n2)/(n1+n2))2((n_1 - n_2)/(n_1 + n_2))^2 at normal incidence to 11 at grazing incidence.
  • For p-polarisation, RpR_p drops to 00 at Brewster’s angle, then increases to 11 at grazing incidence.

Anti-reflection coatings use destructive interference between reflections from two interfaces. For a single-layer coating of index ncn_c and thickness λ/4\lambda/4 on glass (ngn_g), the reflectance at wavelength λ\lambda is:

R=(nc2ngnc2+ng)2R = \left(\frac{n_c^2 - n_g}{n_c^2 + n_g}\right)^2

The reflectance is zero when nc=ngn_c = \sqrt{n_g}. For crown glass (ng=1.52n_g = 1.52), the optimal coating index is nc1.23n_c \approx 1.23, approximated by magnesium fluoride (n1.38n \approx 1.38), giving R1%R \approx 1\% per surface.

In total internal reflection, the reflected beam is laterally shifted relative to the geometrically predicted path. This Goos-Hanchen shift arises because the evanescent wave penetrates the second medium before being reflected:

D=λπsinθisin2θi(n2/n1)2D = \frac{\lambda}{\pi} \frac{\sin\theta_i}{\sqrt{\sin^2\theta_i - (n_2/n_1)^2}}

The shift is of order one wavelength for angles near the critical angle and decreases as θi\theta_i increases beyond θc\theta_c.

10.7 Worked Example: Reflectance at Normal Incidence

Section titled “10.7 Worked Example: Reflectance at Normal Incidence”

Problem. Calculate the reflectance of uncoated glass (ng=1.52n_g = 1.52) at normal incidence in air.

Solution

At normal incidence, r=(11.52)/(1+1.52)=0.52/2.520.206r = (1 - 1.52)/(1 + 1.52) = -0.52/2.52 \approx -0.206. The reflectance is R=r20.0425R = |r|^2 \approx 0.0425, or about 4.25%4.25\% per surface. For a lens with two surfaces, total transmission through uncoated glass is approximately T=(10.0425)20.917T = (1 - 0.0425)^2 \approx 0.917, meaning about 8.3%8.3\% of incident light is lost to reflections.

\blacksquare

Problem. Find the phase difference between s- and p-polarised components after total internal reflection in glass (n1=1.5n_1 = 1.5) at θi=60\theta_i = 60^\circ with n2=1n_2 = 1.

Solution

From the Fresnel equations with complex cosθt\cos\theta_t:

rs=cosθiisin2θi(n2/n1)2cosθi+isin2θi(n2/n1)2=eiδsr_s = \frac{\cos\theta_i - i\sqrt{\sin^2\theta_i - (n_2/n_1)^2}}{\cos\theta_i + i\sqrt{\sin^2\theta_i - (n_2/n_1)^2}} = e^{i\delta_s}

rp=(n2/n1)2cosθiisin2θi(n2/n1)2(n2/n1)2cosθi+isin2θi(n2/n1)2=eiδpr_p = \frac{(n_2/n_1)^2\cos\theta_i - i\sqrt{\sin^2\theta_i - (n_2/n_1)^2}}{(n_2/n_1)^2\cos\theta_i + i\sqrt{\sin^2\theta_i - (n_2/n_1)^2}} = e^{i\delta_p}

where δs=2arctan(sin2θi(n2/n1)2/cosθi)\delta_s = -2\arctan(\sqrt{\sin^2\theta_i - (n_2/n_1)^2}/\cos\theta_i) and δp=2arctan(sin2θi(n2/n1)2/((n2/n1)2cosθi))\delta_p = -2\arctan(\sqrt{\sin^2\theta_i - (n_2/n_1)^2}/((n_2/n_1)^2\cos\theta_i)).

For n1=1.5n_1 = 1.5, n2=1n_2 = 1, θi=60\theta_i = 60^\circ: (n2/n1)20.444(n_2/n_1)^2 \approx 0.444, sin260=0.75\sin^2 60^\circ = 0.75, so sin2θi(n2/n1)20.750.4440.553\sqrt{\sin^2\theta_i - (n_2/n_1)^2} \approx \sqrt{0.75 - 0.444} \approx 0.553, cos60=0.5\cos 60^\circ = 0.5.

δs=2arctan(0.553/0.5)=2arctan(1.106)95.9\delta_s = -2\arctan(0.553/0.5) = -2\arctan(1.106) \approx -95.9^\circ

δp=2arctan(0.553/(0.4440.5))=2arctan(2.491)136.2\delta_p = -2\arctan(0.553/(0.444 \cdot 0.5)) = -2\arctan(2.491) \approx -136.2^\circ

The relative phase difference Δ=δpδs40.3\Delta = \delta_p - \delta_s \approx -40.3^\circ, which is why TIR can convert linear to elliptical polarisation (the basis of Fresnel rhomb quarter-wave plates).

\blacksquare

At θi=θc=arcsin(n2/n1)\theta_i = \theta_c = \arcsin(n_2/n_1), we have θt=90\theta_t = 90^\circ and cosθt=0\cos\theta_t = 0. The Fresnel coefficients become:

rs=n1cosθc0n1cosθc+0=1r_s = \frac{n_1\cos\theta_c - 0}{n_1\cos\theta_c + 0} = 1

rp=n2cosθc0n2cosθc+0=1r_p = \frac{n_2\cos\theta_c - 0}{n_2\cos\theta_c + 0} = 1

Both polarisations have R=1R = 1 at the critical angle, and the transmitted wave propagates exactly along the interface with no energy flow into the second medium.

flowchart TD
A[10_Fresnel Equations] --> B[Key Concepts]
A --> C[Core Principles]
A --> D[Practical Applications]
B --> E[Fundamental definitions]
C --> F[Design patterns]
D --> G[Real-world usage]

The Fresnel equations describe how light splits at an interface between two media. At normal incidence, reflection and transmission depend only on the refractive index mismatch. As the angle increases, the two polarisations behave differently: s-polarised light reflects more strongly, while p-polarised light can reach zero reflection at Brewster’s angle. Total internal reflection occurs beyond the critical angle, where the transmitted wave becomes evanescent, decaying exponentially while carrying no energy across the boundary. This is the optical analogue of quantum tunnelling. The Fresnel coefficients encode both amplitude and phase changes, essential for thin-film coatings and anti-reflection layers.

Mistake 1: Swapping the numerator and denominator terms in rsr_s and rpr_p The s-polarisation coefficient is rs=(n1cosθin2cosθt)/(n1cosθi+n2cosθt)r_s = (n_1\cos\theta_i - n_2\cos\theta_t)/(n_1\cos\theta_i + n_2\cos\theta_t) while rp=(n2cosθin1cosθt)/(n2cosθi+n1cosθt)r_p = (n_2\cos\theta_i - n_1\cos\theta_t)/(n_2\cos\theta_i + n_1\cos\theta_t). The key difference is that rsr_s starts with n1cosθin_1\cos\theta_i in the numerator while rpr_p starts with n2cosθin_2\cos\theta_i. Swapping these gives incorrect reflection coefficients, especially near Brewster’s angle.

Mistake 2: Assuming R+T=1R + T = 1 always implies no absorption Energy conservation R+T=1R + T = 1 holds for lossless dielectric interfaces. In absorbing media, the Fresnel coefficients become complex and R+TR + T may not equal 1 when using the real-valued intensity definitions. Students often apply the simple form to metallic surfaces where the refractive index is complex.

  • Electromagnetic Waves: Derives the boundary conditions for electromagnetic fields at interfaces from which the Fresnel equations follow.
  • Polarization: The s- and p-polarisation decomposition used in the Fresnel equations is the basis for Brewster angle polarisation and wave plate theory.
  • Geometric Optics: Takes the ray limit of Fresnel reflection and refraction, yielding Snell’s law and the thin lens equation.

Mistake 3: Forgetting that the phase shift on reflection depends on the refractive index ordering For external reflection (n1<n2n_1 < n_2), rs<0r_s < 0 at all angles, meaning the reflected wave undergoes a π\pi phase shift. For internal reflection (n1>n2n_1 > n_2), rs>0r_s > 0 at normal incidence with no phase shift. Students frequently apply the wrong phase convention, which matters for thin-film interference calculations.

Fresnel equations describe how light splits at an interface between two media. At normal incidence, reflection and transmission depend only on the refractive index mismatch. As the angle of incidence increases, the two polarisations behave differently: s-polarised light reflects more strongly, while p-polarised light can reach zero reflection at Brewster’s angle. Total internal reflection occurs beyond the critical angle, where the transmitted wave becomes evanescent. The Fresnel coefficients encode both amplitude and phase changes, which is essential for understanding thin-film coatings and anti-reflection layers. The key physical picture is that the boundary conditions for the electric and magnetic fields force the reflected and transmitted amplitudes to adjust continuously with angle.