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Benefits of Widlar source and output resistance
Short answer
The Widlar source provides small currents (µA range) with practical resistor values, saving chip area. It offers higher output resistance Ro ≈ ro(1+gmRE) ≈ ro(1+ln(IREF/IO)), lower sensitivity to supply voltage, and reduced dependence on β and temperature.
What are the benefits of Widlar current source as compared to a simple current mirror (current source)? Derive an expression for an output resistance of Widlar Current Source.
Benefits of the Widlar source over a simple mirror
In a simple mirror IO ≈ IREF = (VCC − VBE)/R, so a small current needs a huge resistor. The Widlar source adds RE in the emitter of Q2, giving IO·RE = VT ln(IREF/IO).
| Point | Simple mirror | Widlar source |
|---|---|---|
| Output current | IO ≈ IREF | IO << IREF (µA range) |
| Resistor for 10 µA (VCC = 15 V) | R ≈ 1.4 MΩ | R ≈ 14 kΩ and RE ≈ 12 kΩ |
| Chip area | very large (big R) | small |
| Output resistance | ro | ≈ ro(1 + gm RE), several times higher |
| Sensitivity of IO to VCC | IO ∝ VCC | much less (logarithmic) |
| Sensitivity to β, temperature | higher | lower (emitter feedback) |
So the Widlar source gives small, stable bias currents with practical resistor values, a higher output resistance (better current source) and lower dependence on supply voltage. It is used in the input-stage biasing of the 741.
Output resistance of the Widlar current source
+VCC IO (from load)
| |
R |
| IREF |
+------+ |
| | |
C1 | C2
Q1 B----+-------------B Q2
E1 E2
| |
| RE
| |
GND GND
Small-signal model: Q1 is diode-connected, so its resistance is only about 1/gm1 and the base of Q2 is close to ac ground. Apply a test voltage vx at the collector of Q2 and let ix flow into it.
Emitter node: ix flows into RE ‖ rπ (rπ goes to the
grounded base), so
ve = ix (RE ‖ rπ) = ix R'E
Base is grounded:
vbe = 0 - ve = -ix R'E
Current into collector:
ix = gm vbe + (vx - ve)/ro
= -gm ix R'E + (vx - ix R'E)/ro
Multiply by ro and collect terms:
vx = ix ro + ix R'E (1 + gm ro)
Ro = vx/ix = ro + R'E (1 + gm ro)
Since gm ro >> 1:
Ro ≈ ro (1 + gm R'E), R'E = RE ‖ rπ
If RE << rπ, then Ro ≈ ro(1 + gm RE), where gm = IO/VT and ro = VA/IO. A simple mirror has Ro = ro only, so the Widlar source has an output resistance larger by the factor (1 + gm RE). Since gm·RE = IO·RE/VT = ln(IREF/IO), this factor is typically about 4 to 6 (for example, 5.6 when IREF/IO = 100). This is the result of the current-series negative feedback provided by the unbypassed RE: any rise in IO raises the drop across RE, lowers VBE2 and pulls IO back down.
✓ Answer checked by Claude Opus 5.5 (high effort)
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