finFET Noise

Noise Aspect FinFET vs Planar Better or Worse? Why (Physical Reason)
1/f (Flicker) Noise at Moderate/High Vgs Lower Better Volume inversion keeps carriers away from interface → less trap interaction.
1/f Noise Variation (Device-to-Device) Larger spread Worse Each fin has its own sidewall roughness, trap density, and geometry → statistical variation.
RTS (Random Telegraph Signal) Noise More prominent in minimum fins Worse One trap can strongly modulate current because channel width is tiny (a few nm).
Thermal Channel Noise (γ-factor) Slightly different; often slightly lower Slightly Better Improved gate control and reduced channel length modulation reduce excess thermal noise.
Gate-Induced Noise (Gatenoise / Induced Gate Noise) Bias-dependent; correlation (α) improves slightly Better for RF 3D geometry and better electrostatics reduce channel–gate capacitive coupling.
Shot Noise from Source/Drain Tunneling Minimal at 14–22 nm; increases <10 nm Worse at very small nodes Shorter channels & high fields → more tunneling → shot-like behavior.
Subthreshold Noise Often lower Better Stronger electrostatic control → reduced drain-induced barrier lowering → lower leakage/noise.
Mismatch-Induced Noise Variation Higher Worse Fin width/height LER, quantized number of fins → mismatch → noise spread.
Low-Frequency Noise in Analog Bias Region (Vgs just above Vth) Often lower but more unpredictable Mixed Volume inversion helps, but trap sensitivity is highest near threshold.
Channel Mobility Fluctuation Noise Reduced influence Better Carriers distributed in bulk rather than entirely at interface.
Carrier Number Fluctuation Noise Strong at low Vgs; weaker at high Vgs Better at high Vgs Better gate control and volume inversion reduce ΔN sensitivity.
Noise in Wide Devices Highly dependent on number of fins Mixed More fins → noise averages out; few fins → noisy and inconsistent.
RTS Noise Averaging in Multi-Fin Devices Improved Better Many fins statistically de-correlate RTS bursts, lowering impact.
Noise Figure in LNAs/Current Mirrors Generally slightly improved Better Lower flicker + improved electrostatics → cleaner gm for same current.
High-Frequency Noise (mmWave) Slightly better Better Improved gate control and reduced Cgd → better NFmin and Gmax.


  • Flicker noise improves because carriers move into the fin volume, away from surface traps.

  • RTS noise worsens because extremely narrow fins amplify single-trap effects.

  • Thermal noise slightly improves due to better electrostatic control.

  • Gate noise improves because channel–gate coupling is weaker in multi-gate geometry.

  • Noise variation worsens because fin geometry variations dominate mismatch.

  • Subthreshold noise improves thanks to lower DIBL and steeper subthreshold slope.

  • mmWave/high-freq noise improves due to better channel charge control and reduced Cgd.

✔ Better for:

  • Precision analog at moderate–high overdrive

  • LNAs and RF front-ends

  • Low-noise current mirrors (with multiple fins)

  • gm/Id-based design (FinFETs have stronger electrostatics → better gm)

✘ Worse for:

  • Very small devices with 1–2 fins

  • Circuits biased near threshold

  • Small-signal circuits sensitive to RTS and noise bursts

  • Ultra-low-power circuits where stochastic variation dominates

Comments

Popular posts from this blog

Why Whittling Down Precision Could be Your Best Finishing Touch (Chris Mangelsdorf)