Pole splitting is a phenomenon exploited in some forms of frequency compensation used in an electronic amplifier. When a capacitor is introduced between the input and output sides of the amplifier with the intention of moving the pole lowest in frequency (usually an input pole) to lower frequencies, pole splitting causes the pole next in frequency (usually an output pole) to move to a higher frequency. This pole movement increases the stability of the amplifier and improves its step response at the cost of decreased speed.
Example of pole splitting
This example shows that introducing capacitor CC in the amplifier of Figure 1 has two results: firstly, it causes the lowest frequency pole of the amplifier to move still lower in frequency and secondly, it causes the higher pole to move higher in frequency. This amplifier has a low frequency pole due to the added input resistance Ri and capacitance Ci, with the time constant Ci ( RA || Ri ). This pole is lowered in frequency by the Miller effect. The amplifier is given a high frequency output pole by addition of the load resistance RL and capacitance CL, with the time constant CL ( Ro || RL ). The upward movement of the high-frequency pole occurs because the Miller-amplified compensation capacitor CC alters the frequency dependence of the output voltage divider. The first objective, to show the lowest pole decreases in frequency, is established using the same approach as the Miller's theorem article. Following the procedure there, Figure 1 is transformed to the electrically equivalent circuit of Figure 2. Application of Kirchhoff's current law to the input side of Figure 2 determines the input voltage v i {\displaystyle \ v_{i}} to the ideal op amp as a function of the applied signal voltage v a {\displaystyle \ v_{a}} , namely,
v i v a = R i R i + R A 1 1 + j ω ( C M + C i ) ( R A ‖ R i ) , {\displaystyle {\frac {v_{i}}{v_{a}}}={\frac {R_{i}}{R_{i}+R_{A}}}{\frac {1}{1+j\omega (C_{M}+C_{i})(R_{A}\|R_{i})}}\ ,}
which exhibits a roll-off with frequency beginning at f1 where
f 1 = 1 2 π ( C M + C i ) ( R A ‖ R i ) = 1 2 π τ 1 , {\displaystyle {\begin{aligned}f_{1}&={\frac {1}{2\pi (C_{M}+C_{i})(R_{A}\|R_{i})}}\\&={\frac {1}{2\pi \tau _{1}}}\ ,\\\end{aligned}}}
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