The Miller theorem refers to the process of creating equivalent circuits. It asserts that a floating impedance element, supplied by two voltage sources connected in series, may be split into two grounded elements with corresponding impedances. There is also a dual Miller theorem with regards to impedance supplied by two current sources connected in parallel. The two versions are based on the two Kirchhoff's circuit laws. Miller theorems are not only pure mathematical expressions. These arrangements explain important circuit phenomena about modifying impedance (Miller effect, virtual ground, bootstrapping, negative impedance, etc.) and help in designing and understanding various commonplace circuits (feedback amplifiers, resistive and time-dependent converters, negative impedance converters, etc.). The theorems are useful in 'circuit analysis' especially for analyzing circuits with feedback and certain transistor amplifiers at high frequencies. There is a close relationship between Miller theorem and Miller effect: the theorem may be considered as a generalization of the effect and the effect may be thought as of a special case of the theorem.
Miller theorem (for voltages)
Definition The Miller theorem establishes that in a linear circuit, if there exists a branch with impedance Z {\displaystyle Z} , connecting two nodes with nodal voltages V 1 {\displaystyle V_{1}} and V 2 {\displaystyle V_{2}} , we can replace this branch by two branches connecting the corresponding nodes to ground by impedances respectively Z 1 − K {\displaystyle {\frac {Z}{1-K}}} and K Z K − 1 {\displaystyle {\frac {KZ}{K-1}}} , where K = V 2 V 1 {\displaystyle K={\frac {V_{2}}{V_{1}}}} . The Miller theorem may be proved by using the equivalent two-port network technique to replace the two-port to its equivalent and by applying the source absorption theorem. This version of the Miller theorem is based on Kirchhoff's voltage law; for that reason, it is named also Miller theorem for voltages.
Explanation
The Miller theorem implies that an impedance element is supplied by two arbitrary (not necessarily dependent) voltage sources that are connected in series through the common ground. In practice, one of them acts as a main (independent) voltage source with voltage V 1 {\displaystyle V_{1}} and the other – as an additional (linearly dependent) voltage source with voltage V 2 = K V 1 {\displaystyle V_{2}=K{V_{1}}} . The idea of the Miller theorem (modifying circuit impedances seen from the sides of the input and output sources) is revealed below by comparing the two situations – without and with connecting an additional voltage source V 2 {\displaystyle V_{2}} . If V 2 {\displaystyle V_{2}} were zero (there was not a second voltage source or the right end of the element with impedance Z {\displaystyle Z} was just grounded), the input current flowing through the element would be determined, according to Ohm's law, only by V 1 {\displaystyle V_{1}}
I i n 0 = V 1 Z {\displaystyle I_{in0}={\frac {V_{1}}{Z}}}
and the input impedance of the circuit would be
Z i n 0 = V 1 I i n 0 = Z . {\displaystyle Z_{in0}={\frac {V_{1}}{I_{in0}}}=Z.}
As a second voltage source is included, the input current depends on both the voltages. According to its polarity, V 2 {\displaystyle V_{2}} is subtracted from or added to V 1 {\displaystyle V_{1}} ; so, the input current decreases/increases
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