Photonica

Direct vs indirect bandgap

The two fundamental classes of semiconductor band structure, distinguished by whether the conduction-band minimum and valence-band maximum occur at the same crystal momentum. Determines whether efficient optical emission is possible.

Semiconductors are classified as "direct-bandgap" or "indirect-bandgap" based on whether the conduction-band minimum (lowest electron energy) and the valence-band maximum (highest hole energy) occur at the same crystal momentum k\mathbf{k}. This single distinction has profound consequences for optoelectronic device performance: direct-bandgap semiconductors emit light efficiently; indirect-bandgap semiconductors do not.

Direct bandgap. The conduction-band minimum and valence-band maximum both occur at k=0\mathbf{k} = 0 (the Γ\Gamma point in Brillouin zone notation). An electron-hole transition requires no change in momentum, so a photon (carrying negligible momentum) can mediate it directly. Radiative recombination is a fast, allowed process.

Direct-bandgap semiconductors include the III-V family used in all commercial semiconductor lasers and LEDs:

MaterialEgE_g (eV, 300 K)λg\lambda_g
GaN3.4365 nm (UV)
GaAs1.42873 nm (NIR)
InP1.35918 nm (NIR)
In₀.₅₃Ga₀.₄₇As (LM to InP)0.741675 nm (SWIR)
InGaAsP (varies)0.74 – 1.35918 – 1675 nm
InAs0.363440 nm (mid-IR)
InSb0.177300 nm (mid-IR)
HgCdTe (varies)0 – 1.5tunable LWIR

These materials have B1010B \sim 10^{-10} cm³/s radiative coefficient and form the basis of nearly all commercial light-emitting devices.

Indirect bandgap. The conduction-band minimum and valence-band maximum occur at different k\mathbf{k} points. Optical transitions between them require simultaneous emission or absorption of a phonon to conserve momentum, making the radiative process slow.

Indirect-bandgap semiconductors:

MaterialEgE_g (eV, 300 K)Conduction band min
Si1.12XX valley (along [100] direction)
Ge0.66LL valley (along [111] direction); Γ\Gamma valley only 140 meV higher
GaP2.26XX valley
AlAs2.15XX valley
AlSb1.61XX valley
SiC2.4 – 3.3 (polytype-dependent)indirect

For these, radiative recombination coefficient is 10151014\sim 10^{-15} - 10^{-14} cm³/s — about 5 orders of magnitude smaller than direct-gap materials.

Why the distinction matters: photon vs phonon momentum. Photon momentum at optical frequencies: kphoton104\hbar k_\text{photon} \sim 10^4 m⁻¹, completely negligible compared to electron crystal-momentum at the Brillouin zone edge: kelectron1010\hbar k_\text{electron} \sim 10^{10} m⁻¹. In an indirect transition, the missing momentum must come from a phonon — a second-order process with much smaller matrix element.

Quantitatively: the radiative recombination rate in indirect-gap Si is suppressed by a factor of 105\sim 10^{-5} relative to direct-gap GaAs, almost entirely because of the phonon-coupling factor in the matrix element.

Absorption coefficients. Direct-gap materials have sharper, larger optical absorption near the band edge:

Materialα\alpha at EgE_g + 50 meVα\alpha at EgE_g + 500 meV
GaAs (direct)104\sim 10^4 cm⁻¹5×104\sim 5 \times 10^4 cm⁻¹
InP (direct)104\sim 10^4 cm⁻¹5×104\sim 5 \times 10^4 cm⁻¹
InGaAs (direct)104\sim 10^4 cm⁻¹5×104\sim 5 \times 10^4 cm⁻¹
Si (indirect)10\sim 10 cm⁻¹103\sim 10^3 cm⁻¹
Ge (indirect)100\sim 100 cm⁻¹104\sim 10^4 cm⁻¹

The shape of the absorption edge near EgE_g also differs:

  • Direct gap: α(hνEg)1/2\alpha \propto (h\nu - E_g)^{1/2} — sharp threshold
  • Indirect gap: α(hνEg±hΩphonon)2\alpha \propto (h\nu - E_g \pm h\Omega_\text{phonon})^2 — softer threshold with phonon-mediated steps

This is why photodetector materials are selected:

  • Si detectors (450 – 1100 nm): use Si's wide-window indirect absorption; require thick absorbing layers (~10 μm)
  • InGaAs detectors (900 – 1700 nm): use InGaAs's direct absorption; thin layers (~1 μm) suffice
  • Ge-on-Si detectors (1310/1550 nm): use Ge's near-direct absorption at Γ\Gamma for tighter integration with Si photonics

Engineering indirect-to-direct conversion.

Several strategies make indirect-gap materials emit light:

  1. Tensile strain in Ge: shifts the Γ\Gamma valley below the LL valley, making Ge effectively direct
  2. Ge-Sn alloys: >7%> 7\% Sn shifts to direct
  3. SiGe quantum wells: confinement modifies energy hierarchy
  4. Si nanocrystals: quantum confinement opens direct transitions
  5. Si:Er (erbium doping): introduces a direct radiative transition at 1.54 μm independent of Si band structure
  6. Heterogeneous integration: bond III-V direct-gap material onto Si chips (the standard silicon photonics approach)

Quantum cascade lasers: indirect-gap-like operation. QCLs operate via intersubband transitions within the conduction band of multi-layer III-V structures. The "vertical" intersubband transition is direct in k\mathbf{k}, but the device design has many similarities to indirect-gap absorption (TM-polarization only, oscillator strength engineering, etc.).

Why direct-gap III-Vs are also good detectors. GaAs, InP, InGaAs — all the materials that make great lasers also make great photodetectors. The same large absorption coefficient that enables efficient emission enables efficient absorption. This explains why InGaAs/InP avalanche photodiodes are the standard for telecom receivers.

Direct-indirect crossovers in alloys. Some alloy systems transition between direct and indirect as composition changes:

  • AlₓGa₁₋ₓAs: direct for x<0.45x < 0.45; indirect (XX-valley) above. Critical for AlGaAs/GaAs LEDs and lasers.
  • InₓGa₁₋ₓP: direct for x>0.55x > 0.55; indirect below
  • AlₓIn₁₋ₓAs: direct throughout (LM to InP at x=0.48x = 0.48, indirect-like at higher xx)

These crossovers are exploited to make heterostructures where the cladding is indirect (low-loss) and the active region is direct (efficient emission).

References: Saleh & Teich, Fundamentals of Photonics (3rd ed., 2019), Ch. 16 (semiconductor materials); Yu & Cardona, Fundamentals of Semiconductors (4th ed., 2010) for the canonical band-structure treatment; Coldren, Corzine & Mašanović, Diode Lasers and PICs (2nd ed., 2012), Ch. 2.