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LEDs & Diode Sources — Abridged Guide

Quick-reference guide to LEDs and diode sources — band gap physics, material systems, spectral width, efficiency, thermal management, SLEDs, and photonics applications. For full derivations and worked examples, see the Comprehensive Guide.

Comprehensive LEDs & Diode Sources Guide

1.Introduction

LEDs are semiconductor devices that convert electrical energy directly to light via electroluminescence in forward-biased p-n junctions. They offer quasi-monochromatic emission (20–70 nm FWHM), nanosecond switching, and lifetimes exceeding 50,000 hours.
LEDs fill the niche between broadband lamps (too wide, too much heat) and lasers (too narrow, too coherent). Choose LEDs when you need spectral selectivity without coherent speckle.

2.Types & Classification

Wavelength from Band Gap
λ (nm)=1240Eg (eV)\lambda \text{ (nm)} = \frac{1240}{E_g \text{ (eV)}}
Surface-emitting LEDs produce Lambertian beams (120° FWHM). Edge-emitting LEDs produce higher-radiance asymmetric beams (~30° × 120°) better suited to fiber coupling. SLEDs provide amplified spontaneous emission with laser-like beam quality.
TypeBeam FWHMTypical BWBest For
Surface-emitting~120°15–50 MHzIllumination, displays
Edge-emitting~30° × 120°~200 MHzFiber coupling, comms
SLED~10° × 30°~200 MHzOCT, fiber sensing, FOG
White LEDs use phosphor conversion (blue LED + yellow phosphor), not a single white-emitting junction. For color-critical applications, check the CRI and spectral power distribution — not just “white.”
LED Spectral Calculator

3.Semiconductor Physics

Photon Energy
E=hν=hcλE = h\nu = \frac{hc}{\lambda}
Only direct band gap semiconductors (GaAs, GaN, InGaN, AlGaInP) emit light efficiently. Indirect materials (Si, Ge) require phonon-assisted recombination and are extremely poor emitters. This is why LEDs use III-V compound semiconductors.
The forward voltage of an LED approximately equals the band gap voltage E_g/e: ~1.8 V for red, ~3.0 V for blue, ~3.5 V for UV. If you know V_f, you can estimate the wavelength.

4.Material Systems

Three material families cover UV through SWIR: III-nitrides (AlGaN/InGaN) for 200–530 nm, phosphides (AlGaInP) for 540–650 nm, and arsenides (GaAs/InGaAs) for 700–1700+ nm. The “green gap” at 530–580 nm is where neither system performs well.
MaterialRange (nm)ColorV_f (V)
AlGaN200–365UV4–6
InGaN365–530Violet–Green2.8–3.5
AlGaInP540–650Yellow–Red1.8–2.2
GaAs/AlGaAs630–870Red–NIR1.4–1.8
InGaAs/InP920–1700NIR–SWIR0.7–1.0
AlGaInP red LEDs are significantly more temperature-sensitive than InGaN blue LEDs. Budget extra thermal headroom for red sources in hot environments.

5.Spectral Characteristics

Theoretical FWHM
Δν1.8kBTh;Δλ=λ2cΔν\Delta\nu \approx \frac{1.8\, k_B T}{h} \quad;\quad \Delta\lambda = \frac{\lambda^2}{c}\,\Delta\nu
LED FWHM ranges from ~15 nm (UV) to ~100 nm (SWIR). The spectral width broadens with wavelength because Δλ ∝ λ². Temperature increases both red-shift the peak (~0.1 nm/°C for red LEDs) and broaden the spectrum.
For pump or excitation applications, check what fraction of the LED’s broad emission actually overlaps the target absorption band. A 40 nm FWHM LED may put only 5–10% of its power into a narrow (~3 nm) absorption line — a laser diode is far more efficient in that case.

6.Efficiency Metrics

Wall-Plug Efficiency
ηWPE=PopticalIF×VF=ηEQE×hνeVF\eta_{\text{WPE}} = \frac{P_{\text{optical}}}{I_F \times V_F} = \eta_{\text{EQE}} \times \frac{h\nu}{e V_F}
EQE = IQE × extraction efficiency. WPE accounts for the additional loss of voltage efficiency (V_f > E_g/e). State-of-the-art blue LEDs reach 60–70% WPE; red ~30–40%; green ~20–30%.
TypeEQE (%)WPE (%)Efficacy (lm/W)
Blue InGaN60–8050–70
Green InGaN25–4020–3080–120
Red AlGaInP30–5025–4040–70
PC White35–55150–220
Efficiency droop at high current means two LEDs at half-current produce more light per watt than one LED at full current. For maximum efficiency, underdriving is always beneficial.
LED Thermal & Efficiency Calculator

7.Thermal Management & Output Stability

Junction Temperature
Tj=Ta+(IFVF)(1ηWPE)×Rθ(j-a)T_j = T_a + (I_F V_F)(1 - \eta_{\text{WPE}}) \times R_{\theta(j\text{-}a)}
Output power drops ~5% per 10°C for blue LEDs and ~10–15% per 10°C for red LEDs. Wavelength shifts ~0.1–0.2 nm/°C (red) or ~0.03–0.05 nm/°C (blue). Lifetime halves for every ~10–15°C above rated T_j.
For spectroscopy and fluorescence work, always use a TEC-stabilized LED source with monitor photodiode feedback. Without active stabilization, output can drift 5–10% over a 20°C ambient temperature swing.

8.Packaging & Mounting

Through-hole and TO-cans for low power; SMD/COB for lighting; butterfly (14-pin) for precision photonics. Butterfly packages integrate TEC, thermistor, monitor PD, and fiber pigtail — the gold standard for stable, fiber-coupled output.
PackagePowerThermalStabilityCost
Through-hole< 100 mWPoorNone$
SMD0.1–5 WModerateNone$
COB10–200 WGoodNone$$
TO-can< 500 mWModerateOptional PD$$
Butterfly 14-pin< 100 mW (fiber)Excellent (TEC)TEC + PD$$$
FC/APC connectors on fiber-pigtailed SLEDs are essential — FC/PC connectors produce ~4% back-reflection that degrades SLED performance and can cause parasitic lasing.

9.Superluminescent Diodes

SLEDs generate amplified spontaneous emission — higher power and spatial coherence than LEDs, broader spectrum than laser diodes. Bandwidths: 5–100+ nm. Key applications: OCT (coherence length = resolution), fiber gyroscopes (reduces coherent backscatter error), and component testing.
SLEDs are fragile regarding back-reflections. Always use an optical isolator or FC/APC termination. Even 0.1% feedback can produce spectral ripple.

10.Driving & Modulation

Series Resistor
R=VsupplyVfIfR = \frac{V_{\text{supply}} - V_f}{I_f}
Always drive LEDs with a constant-current source, not a voltage source. LED dynamic resistance is very low (~1 Ω), so small voltage changes cause large current swings. PWM dimming preserves spectral shape; analog dimming shifts wavelength.
Modulation Bandwidth
f3dB=12πτcf_{\text{3dB}} = \frac{1}{2\pi \tau_c}
For time-resolved fluorescence, LED pulse drivers can produce optical pulses as short as 1–2 ns. Surface-emitting LEDs support ~50 MHz modulation; edge-emitting LEDs reach ~200 MHz.

11.Selection Guide

1
Wavelength
Match to absorption band, fluorophore, or detector range.
2
Spectral width
< 5 nm → laser/SLED. > 20 nm → LED is simpler and speckle-free.
3
Optical power
Estimate required irradiance accounting for coupling losses.
4
Beam pattern
Lambertian for area illumination; edge-emitting for fiber.
5
Package
Butterfly for precision; SMD for PCB integration; free-space for microscopy.
6
Thermal budget
Calculate T_j. Ensure heatsink keeps T_j below rated maximum.
Follow the selection sequence: wavelength → spectral width → power → beam pattern → package → thermal budget. The LED vs. laser vs. lamp choice comes down to spectral width (lamp > LED > laser), coherence (laser > LED ≈ lamp), and switching speed (laser > LED >> lamp).
If the application needs < 5 nm spectral width, choose a laser diode or SLED with a filter. If it tolerates > 20 nm, an LED is simpler, cheaper, and speckle-free.
Continue Learning

The Comprehensive Guide includes 7 worked examples, 6 SVG diagrams, 3 data tables, and 10 references.

All information, equations, and calculations have been compiled and verified to the best of our ability. For mission-critical applications, we recommend independent verification of all values. If you find an error, please let us know.