Single-Stage & Differential Amplifiers
CS, CG, CD, cascode stages, and the differential pair — the core building blocks of analog ICs
📑 Table of Contents
1. Common-Source (CS) Amplifier
The CS stage is the workhorse amplifier in analog CMOS — high gain, high input impedance, and moderate bandwidth.
Small-Signal Parameters
With an active PMOS load (current source), the gain becomes:
The dominant pole is at the output node: f-3dB = 1/(2π·Rout·Cout), where Cout includes Cdb, load capacitance, and Miller-multiplied Cgd. The gain-bandwidth product is approximately gm/(2π·Cout).
2. CS with Source Degeneration
Adding a resistor (or un-bypassed current source) in the source path trades gain for linearity and bandwidth.
| Parameter | Without RS | With RS |
|---|---|---|
| Voltage gain | −gmRD | −gmRD/(1+gmRS) |
| Linearity | Poor (depends on gm) | Good (gain set by R ratio) |
| Input impedance | ∞ | ∞ |
| Output impedance | RD | RD |
| Bandwidth | Narrower | Wider (pole shifts up) |
Source degeneration is the MOSFET equivalent of emitter degeneration in BJTs. It implements local negative feedback, linearizing the VGS-to-ID relationship.
3. Common-Gate (CG) Amplifier
The CG stage has the input at the source and output at the drain. Gate is AC-grounded.
Key characteristics: non-inverting, low input impedance (1/gm), excellent high-frequency behavior (no Miller effect on Cgd).
The CG is used as: (1) a cascode device stacked on a CS stage, (2) a wideband input stage for current-mode signals, (3) a transimpedance amplifier input for photodiode receivers. Its low Rin provides 50Ω matching for RF applications.
4. Common-Drain (Source Follower)
The source follower provides voltage buffering — near-unity gain with high input impedance and low output impedance.
In a source follower, the source rides with the signal, so VSB changes → Vth changes → gain drops below unity. The body transconductance gmb acts as negative feedback, reducing gain to gm/(gm+gmb). PMOS followers in an n-well process can eliminate this by tying the body to the source.
5. Cascode Amplifier
The cascode combines a CS input stage (M1) with a CG stage (M2) to achieve very high gain and high output resistance without the Miller effect.
With a cascode PMOS load, the gain becomes:
Telescopic: All transistors in a single stack. Highest speed, lowest noise, but limited output swing (VDD − 4VOV − 2Vth). Folded cascode: Input pair and cascode are in separate current branches. Better swing (VDD − 4VOV), wider input common-mode range, but more current consumption and added noise from folding transistors.
6. The Differential Pair
The MOS differential pair is the input stage of virtually every op-amp, comparator, and data converter.
Differential-Mode Gain
Common-Mode Gain
Linear Input Range
The differential pair steers current linearly for small signals. The linear range is approximately:
Beyond this, one transistor steals all the tail current and the other shuts off.
NMOS pair: higher gm per unit current (faster), but higher 1/f noise. PMOS pair: lower 1/f noise, body effect eliminable, input CM range includes ground. Complementary: rail-to-rail input CM but gain varies across range.
7. Diff Pair with Active Load
Replacing resistor loads with a PMOS current mirror converts the differential signal to single-ended while doubling the gain.
The mirror (M3-M4) folds the signal from the left branch into the right branch, creating a single-ended output. This is the first stage of the classic two-stage op-amp (five-transistor OTA).
The current mirror load introduces a half-circuit delay: the signal through M1→M3→M4 arrives at the output later than the direct path through M2. At high frequencies, this mismatch degrades CMRR and introduces systematic offset.
8. Common-Mode Rejection (CMRR)
The CMRR depends entirely on the tail current source impedance. A simple current mirror tail gives moderate CMRR; a cascode tail provides much higher rejection.
| Tail Source Type | RSS | Typical CMRR |
|---|---|---|
| Resistor | R (fixed) | 20–40 dB |
| Simple mirror | ro | 40–60 dB |
| Cascode mirror | gmro² | 80–100+ dB |
9. Amplifier Comparison Summary
| Topology | Av | Rin | Rout | BW | Best For |
|---|---|---|---|---|---|
| Common-Source | −gmRD | ∞ | RD∥ro | Moderate | General amplification |
| CS + Degeneration | −RD/RS | ∞ | RD | Wide | Linear gain stages |
| Common-Gate | +gmRD | 1/gm | RD∥ro | Wide | Wideband, cascode |
| Source Follower | ≈ 0.8–0.9 | ∞ | 1/gm | Very Wide | Buffering, level shift |
| Telescopic Cascode | (gmro)²/2 | ∞ | gmro² | High | High-gain OTA |
| Diff Pair + Mirror | gm(ro∥ro) | ∞ | ro∥ro | Moderate | Op-amp first stage |
10. Numerical Examples
Example 1: CS Amplifier Gain
Example 2: Differential Pair CMRR
Example 3: Telescopic Cascode Gain
🔁 Blog 3 Recap
- CS amplifier: high gain, inverting, limited by Miller effect on Cgd.
- CG amplifier: non-inverting, low Rin, wideband — ideal as cascode partner.
- Source follower: near-unity gain buffer; body effect limits gain to ~0.85.
- Cascode = CS + CG → gain ≈ (gmro)², with telescopic or folded variants.
- The differential pair rejects common-mode; CMRR depends on tail source impedance.
- Active mirror load converts differential to single-ended with doubled gain.
📚 Next up — Blog 4: Op-Amp & OTA Architectures — two-stage, folded-cascode, gain-boosted, and class-AB output stages.
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