2026-09-05
The common-emitter (CE) amplifier is the workhorse voltage gain stage of discrete BJT design. Signal enters the base, exits (inverted and amplified) at the collector, and the emitter is the "common" terminal shared between input and output. It delivers the highest voltage gain of the three BJT topologies (CE, CB, CC) — often 100× or more — which is why it dominated audio preamps, IF strips, and countless op-amp input stages before ICs took over.
How it works: A small AC voltage at the base modulates the base-emitter junction, which exponentially controls collector current. That current flows through a collector resistor RC, developing a voltage swing that's the amplified (and inverted) copy of the input.
Core design equations (assuming voltage-divider bias and a bypassed emitter resistor):
Worked example — audio preamp: You want a gain of 50 from a 2N3904 running at IC = 1 mA on a 12 V rail. Then re = 26 Ω, so RC = 50 × 26 Ω = 1.3 kΩ (use 1.3 kΩ or 1.5 kΩ). Set the collector quiescent voltage at 6 V for maximum symmetric swing: VC = 12 − (1 mA)(1.3 kΩ) = 10.7 V — too high. Drop IC to 2 mA and recalculate: re = 13 Ω, RC = 650 Ω, VC = 12 − 1.3 = 10.7 V. Still high — pick RC = 3 kΩ and accept a gain closer to 230, or add a partially-bypassed emitter resistor to stabilize gain.
The bypass capacitor trap: The unbypassed version (emitter degeneration) gives Av ≈ −RC/RE — predictable, linear, temperature-stable, but low gain. Fully bypassing RE with a large capacitor restores the high gm-based gain but reintroduces temperature drift and BJT-to-BJT variation. Split the emitter resistor (small unbypassed RE1 in series with bypassed RE2) for the best of both worlds — modest, controlled gain with reasonable linearity.
Watch out for: Miller effect on Cbc multiplies collector-base capacitance by (1 + |Av|), crushing high-frequency response. That's exactly why cascode topologies exist.
