NE 345: Photonic Materials and Devices
Estimated study time: 12 minutes
Table of contents
Sources and References
- Saleh and Teich, Fundamentals of Photonics (Wiley)
- Kasap, Optoelectronics and Photonics: Principles and Practices (Pearson)
- Coldren, Corzine, and Mashanovitch, Diode Lasers and Photonic Integrated Circuits (Wiley)
- Yariv and Yeh, Photonics: Optical Electronics in Modern Communications (Oxford)
- Online: RP Photonics Encyclopedia, MIT OCW 6.007 Applied Electromagnetics
Chapter 1: Nature of Light and Material Response
1.1 Plane Waves, Index, and Dispersion
A monochromatic plane wave propagating in a dielectric satisfies
\[ \mathbf{E}(\mathbf{r},t) = \mathbf{E}_0 \exp\!\left[ i(\mathbf{k}\cdot\mathbf{r} - \omega t) \right], \]with wavevector magnitude \( k = n\omega/c \). The refractive index \( n(\omega) \) is frequency dependent because material polarisation lags the driving field. Near a single Lorentz oscillator of resonance \( \omega_0 \) and damping \( \gamma \),
\[ \varepsilon(\omega) = 1 + \frac{\omega_p^{2}}{\omega_0^{2} - \omega^{2} - i\gamma\omega}, \]producing normal dispersion \( dn/d\omega > 0 \) away from resonance and anomalous dispersion near \( \omega_0 \) accompanied by absorption.
1.2 Group Velocity and Irradiance
Optical pulses propagate at the group velocity
\[ v_g = \frac{d\omega}{dk} = \frac{c}{n + \omega\,dn/d\omega}, \]which differs from the phase velocity \( v_p = c/n \) whenever the medium is dispersive. Group-velocity dispersion stretches pulses and limits bit rates in fibre-optic links.
The time-averaged energy flow is the Poynting vector magnitude
\[ I = \tfrac{1}{2}\,n\,c\,\varepsilon_0\,|E_0|^{2}. \]This irradiance is what photodetectors measure.
Chapter 2: Reflection, Refraction, and Coatings
2.1 Snell’s Law and Fresnel Equations
At a planar interface between media of indices \( n_1 \) and \( n_2 \),
\[ n_1 \sin\theta_1 = n_2 \sin\theta_2. \]Fresnel coefficients for the electric-field amplitude are, for s-polarisation,
\[ r_s = \frac{n_1\cos\theta_1 - n_2\cos\theta_2}{n_1\cos\theta_1 + n_2\cos\theta_2}, \]and analogously for p-polarisation. The reflectance is \( R = |r|^2 \).
2.2 Antireflection Coatings
A quarter-wave layer of refractive index \( n_c = \sqrt{n_1 n_s} \) thickness \( \lambda/(4 n_c) \) interferometrically cancels reflection at the design wavelength. For a silicon solar cell, a silicon-nitride AR coating with \( n \approx 2 \) and thickness \( \approx 75 \) nm eliminates reflection near 600 nm, lifting short-circuit current by tens of percent. Multilayer dielectric stacks achieve broadband or high-reflectance mirrors by stacking alternating high- and low-index quarter-wave films.
Chapter 3: Absorption, Emission, and Coherence
3.1 Absorption in Semiconductors
In a direct-gap semiconductor, the absorption coefficient above the gap grows as
\[ \alpha(h\nu) = A\,(h\nu - E_g)^{1/2}, \]reflecting the joint density of states. Indirect-gap materials like silicon require phonon assistance, giving weaker absorption
\[ \alpha(h\nu) \propto (h\nu - E_g \mp \hbar\Omega)^{2}. \]This is why silicon photodetectors need tens of micrometres of active material while GaAs detectors need only a micron or two.
3.2 Coherence
Lasers exhibit near-ideal spatial coherence and very narrow spectra; incoherent sources such as LEDs have coherence times of femtoseconds.
Chapter 4: Waveguides and Optical Fibres
4.1 Planar Dielectric Waveguides
A symmetric slab of index \( n_1 \) clad by \( n_2 < n_1 \) guides modes whose transverse field satisfies the eigenvalue equation
\[ \tan\!\left(\frac{k_x d}{2} - \frac{m\pi}{2}\right) = \frac{\gamma}{k_x}, \]with \( k_x^{2} + \beta^{2} = n_1^{2} k_0^{2} \) inside and \( \beta^{2} - \gamma^{2} = n_2^{2} k_0^{2} \) outside. Only discrete values of \( \beta \) give bound modes. The number of supported modes scales with the normalised frequency \( V = k_0 d \sqrt{n_1^{2} - n_2^{2}} \); a single-mode waveguide requires \( V < \pi \) for symmetric slabs.
4.2 Optical Fibres
Step-index fibres are cylindrical analogues. Single-mode fibre at 1550 nm typically has a 9 \(\mu\)m core and index contrast near 0.003. Modal, material, and waveguide dispersion contribute to pulse broadening. Chromatic dispersion
\[ D = -\frac{\lambda}{c}\frac{d^{2}n}{d\lambda^{2}} \]crosses zero near 1310 nm in standard silica fibre. Dispersion-shifted fibres move this zero to 1550 nm, aligning with the minimum-loss window.
Chapter 5: Light-Emitting Devices
5.1 The pn Junction Under Forward Bias
Under forward bias \( V \), minority-carrier injection produces excess carriers that recombine. Radiative recombination rate is \( R_{rad} = B n p \), and total recombination also includes Shockley-Read-Hall (non-radiative) and Auger terms. Internal quantum efficiency is
\[ \eta_{i} = \frac{R_{rad}}{R_{rad} + R_{nr}}. \]5.2 LED Materials and Extraction
Visible LEDs use direct-gap III-V alloys: AlGaInP for red-yellow and InGaN for green-blue. White light is typically produced by blue InGaN pumping a YAG:Ce phosphor. External quantum efficiency is limited by extraction: Snell’s law restricts the escape cone from a high-index semiconductor (\( n \approx 3.5 \)) to a half-angle \( \theta_c = \arcsin(1/n) \approx 16° \). Surface texturing, shaped dies, and encapsulants raise extraction efficiency beyond 80% in modern devices.
5.3 Laser Diodes
A semiconductor laser is an LED with optical feedback and gain above threshold. Stimulated emission occurs when population inversion is maintained via strong injection into a narrow active region, often a quantum well. The threshold current density satisfies
\[ g_{th} = \alpha_i + \frac{1}{2L}\ln\!\left(\frac{1}{R_1 R_2}\right), \]balancing modal gain against internal loss and mirror loss. Above threshold, output power grows linearly with current with slope \( \eta_d h\nu/q \).
Chapter 6: Photodetectors and Photovoltaics
6.1 Photodetector Figures of Merit
Responsivity \( \mathcal{R} = I_{ph}/P_{opt} \) measures photocurrent per watt. Ideal quantum efficiency gives \( \mathcal{R} = q/h\nu \) so at 1550 nm the ideal responsivity is 1.25 A/W. Avalanche photodiodes multiply primary photocurrent by an internal gain \( M \) at the cost of excess noise.
6.2 Solar Cells
A solar cell is a large-area photodiode operated in the fourth quadrant under illumination. The diode equation with photogeneration is
\[ I = I_0 \left[ \exp\!\left( \frac{qV}{n k_B T} \right) - 1 \right] - I_{ph}. \]Open-circuit voltage and short-circuit current define the power curve; maximum power is extracted at the knee. The fill factor
\[ FF = \frac{V_{mp} I_{mp}}{V_{oc} I_{sc}} \]captures the squareness of the curve. The Shockley–Queisser limit places single-junction efficiency at about 33% under AM1.5 illumination. Multijunction, tandem, and perovskite-silicon devices push toward higher limits by better matching the solar spectrum.
Across emitters and detectors, the common thread is engineering the interaction of photons with charge carriers: confining modes, matching indices, tuning band gaps, and managing radiative versus non-radiative pathways so that optical energy flows predictably into and out of electronic systems.