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Understanding Recombination in Semiconductors

Oct 27, 2024

Lecture Notes

Overview

  • Recap of the previous lecture:

    • Derived Einstein relation between drift and diffusion mobility and diffusion coefficient.
    • Introduced recombination, traps, electron capture, emission, and recombination rate expression.
  • Importance of Recombination Rate:

    • Influences device operation (LEDs, photodetectors).
    • Leads to recombination current or generation recombination current.

Key Corrections

  • Correction of slide typo:

    • Lifetime (Ï„) defined as (\frac{1}{\sigma \cdot \text{thermal velocity} \cdot \text{total trap density}}).
  • Assumptions:

    • Electron and hole trap cross-section are the same.
    • Thermal velocity is the same.
    • Trap energy level assumed to be at mid-gap (maximizes recombination rate).

Total Recombination Rate Expression

  • Formula: (U = \frac{1}{\tau} \times \frac{Pn - n_i^2}{P + n + 2n_i})

    • (n_i) is the intrinsic carrier concentration.
    • (\tau) is the lifetime: larger Ï„ means slower recombination.
  • **Assumptions: **

    1. Equal cross-section of electron and hole traps.
    2. Equal thermal velocity.
    3. Trap energy level at mid-gap.

Recombination in N-type Semiconductors

  • Excess holes matter more than excess electrons in n-type semiconductors.
  • Ignoring minor components simplifies the equation to (U \approx \frac{1}{\tau} \times \Delta P).
  • Important for calculating excess carrier generation: (\Delta P = U \times \tau).

Shockley-Reed-Hall (SRH) Recombination

  • SRH recombination statistics: Trap-related recombination.
  • Significant in explaining how traps affect carrier recombination.

Light Absorption and Carrier Generation

  • Light energy (h\nu) must be (\geq E_g) (bandgap) for absorption.
  • Wavelength condition: (\lambda \leq \frac{1242}{E_g}).

Continuity Equation

  • Concept: Explains carrier distribution and current flow in semiconductors.
  • Expression: (\frac{dn}{dt} = \frac{1}{q} \frac{dJ_n}{dx} + G_L - \frac{\Delta n}{\tau})
  • For steady state: (0 = D_n \frac{d^2\Delta n}{dx^2} + G_L - \frac{\Delta n}{\tau})

Solving Continuity Equation

  • Without field:

    • Diffusion length (L_n = \sqrt{D_n \cdot \tau}).
    • Solutions:
      • Long semiconductor: Exponential decay.
      • Short semiconductor: Linear decay.
  • Implications: Affects diffusion current, critical in device applications (e.g., P-N junctions).

Conclusion

  • Upcoming focus on continuity equation applications and P-N junction.
  • Understanding these concepts vital for device applications like LEDs, photodetectors, and solar cells.