Consider the common source amplifier in Fig. 19.14(a). Transistor Q_{1} is biased in saturation by dc source V_{bias} and v_{s} is a noiseless small-signal sinusoid of amplitude \left|V_{s}\right| . Estimate the phase noise at the output including thermal noise of the resistor and transistor as well as flicker noise.
The small-signal equivalent circuit is shown in Fig. 19.14(b). The voltage noise source v_{n1} models the flicker noise of the transistor Q_{1} and has a noise spectral density,
V^{2}_{n1}(f) = \frac{K}{WLC_{ox}f}
The current noise source i_{n} includes the thermal noise of both the transistor and resistor,
i^{2}_{n}(f) = 4kT\left\lgroup\frac{2}{3} \right\rgroup g_{m}+\frac{4kT}{R_{d}}
The resulting voltage at v_{0} takes on the form of (19.55)—a sinusoidal voltage in additive noise.
v _{t} = A\sin (\omega _{0}t) + n(t) (19.55)
The sinusoidal component has amplitude \left|V_{s}\right| g_{m1}(R_{d}\left|\right|r_{o1} ) . The voltage noise spectral density at v_{0} is obtained by a routine noise circuit analysis of Fig. 19.14(b).
Assuming that the zero-crossings of the sinusoidal waveform at v_{0} are disturbed only a small amount by the noise, the approximation in (19.56)
τ _{k} \cong \frac{n_{k}}{A\omega _{0}} (19.56)
may be applied. In terms of phase,
\phi _{k} \cong \frac{n_{k}}{\left|V_{s}\right| }
Where n_{k} is the sampled noise voltage v_{o,n} . Therefore, the phase noise is,
S_{\phi }(f) = \frac{(R_{d}\left|\right|r_{o~1})^{2}}{\left|V_{s}\right|^{2} } \left[\frac{K}{WLC_{ox}f} g^{2}_{m~1} +4kT \left\lgroup\frac{2}{3} \right\rgroup g_{m} + \frac{4kT}{R_{d}} \right]
Note that it has a 1/f component and a white component. ^{14}
14. Strictly speaking, \phi _{k} is a discrete-time random process; hence, there may be some aliasing of the white noise in v _{o,n} causing the phase noise to be larger than this. Naturally, the white noise is assumed to be eventually bandlimited by some capacitance a v _{o} ensuring it has finite power.