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Y-Δ transform

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The Y-Δ transform (also written Y-delta or Wye-delta), Kennelly's delta-star transformation, star-mesh transformation or T-Π (or T-pi) transform is a mathematical technique to simplify analysis of an electrical network. The name derives from the shapes of the circuit diagrams, which look respectively like the letter Y and the Greek capital letter Δ. In the UK the wye diagram is known as a star.

(A Δ-Y transformer, on the other hand, is a transformer that converts three-phase electric power without a neutral wire into 3-phase power with a neutral wire. )

Basic Y-Δ transformation

The transformation is used to establish equivalence for networks with 3 terminals. Where three elements terminate at one point (node) and none is a source, the node is eliminated by transforming the impedances.

File:Delta wye circ.PNG

For equivalence, the impedance between any pair of terminals must be the same for both networks.

Delta-to-Star transformation equations

General Idea:


Balanced System:

Star-to-Delta transformation equations

General Idea:

Note: that the equations are equally valid for impedances expressed in complex form.

In graph theory

In graph theory, the Y-Δ transform is used in contexts where there are no resistances labeling the edges, so it simply means replacing a wye subgraph of a graph with the delta subgraph. A Y-Δ transform preserves the number of edges in a graph, but not the number of vertices or the number of cycles. Two graphs are said to be Y-Δ equivalent if one can be obtained from the other by a series of Y-Δ transforms and their inverses, Δ-Y transforms.

The Petersen graph family is an example of a Y-Δ equivalence class.

Demonstration

Delta-to-Star transformation equations

Let us know the values of Rb, Rc and Ra from the delta configuration in the figure above; we want to obtain the values of R1, R2 and R3 of the equivalent wye configuration. In order to do that, we will calculate the equivalent impedance of both configurations between the points N1-N2, N1-N3 and N2-N3 leaving the other node as if it was unconnected, and we will equal both expressions since the resistance must be the same.

The resistance between N1 and N2 when N3 is not connected in the delta configuration is


On the other hand, the resistance between N1 and N2 in the wye configuration is R(N1,N2)= R1+R2; hence,



Calculating the equivalent resistance between the two other nodes in the same way we obtain the expressions




The equations for the delta-to-star transform can be derived from equations (1), (2) and (3) in the following way:

  1. R1: Adding equations (1) and (3) and subtracting equation (2)
  2. R2: Adding equations (1) and (2) and subtracting equation (3)
  3. R3: Adding equations (2) and (3) and subtracting equation (1)

We will develop the first case as an example:








Which is the expression for R1 for the delta-to-star transform.


Star-to-delta transformation equations

Let


We can rewrite the delta-to-star transfomation equations as



Multiplying the expressions in pairs:




Adding the expressions (4), (5) and (6) we have


Now we will divide each side of expression (7) by R1, leaving


From expression (1) we now that


If we use this in the right side of expression (8) we have


But we defined



Which will simplify the right side of expression (9), leading


which is the expression of Rc for the star-to-delta transform. The expressions for Ra and Rb can be obtained in a similar way dividing expression (7) by R2 and R3, respectively.

See also

References

  • William Stevenson, "Elements of Power System Analysis 3rd ed.", McGraw Hill, New York, 1975, ISBN 0070612854