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Example of a Laplace system

Rlc circuit

RLC circuit
y 0 - -1
t 1 y 0 - 2
t 2 y 0 - -4

Find the step response for the system above, when u t is the input and y t is the output (i.e. find y t for u t step t ).

Y s Admittance U s
Admittance 1 Impedance 1 1 s 1 s 1 1 2 s 2 s 3 3 s 2 4 s 2 s 3 2 s 2 s 2
Y s 2 s 3 3 s 2 4 s 2 s 3 2 s 2 s 2 U s

With our previous definition of q d t y t p d t u t we can define the Laplace domain equivalents of q and p as:

q s s 3 2 s 2 s 2
p s 2 s 3 3 s 2 4 s 2

When we multiply q s times Y s , we have to remember to include terms relating to the initial conditions of y t . We normally think of the Laplace transform of t y t as s Y s . However, in reality, the general transform is as follows:

t n y t s n Y s s n 1 y 0 - s n 2 t 1 y 0 - s t n 2 y 0 - t n 1 y 0 -

Therefore, using the initial conditions stated above, we can find the Laplace transforms of the first three derivatives of y t .

t 3 y t s 3 Y s s 2 2 s 4
t 2 y t s 2 Y s s 2
t 1 y t s Y s 1

We can now get a complete s -domain equation relating the output to the input by taking the Laplace transform of q d t y t p d t u t . The transform of the right-hand side of this equation is simple as the initial conditions of y t do not come into play here. The result is just the product of p s and the transform of the step function 1 s .

The left-hand side is somewhat more complicated because we have to make certain that the initial conditions are accounted for. To accomplish this, we take a linear combination of Laplace transform of the third derivative of y(t) , Laplace transform of the second derivative of y(t) , and Laplace transform of the first derivative of y(t) according to the polynomial q s . That is to say, we use the coefficients of the s terms in q s to determine how to combine these three equations. We take 1 of Laplace transform of the third derivative of y(t) plus 2 of Laplace transform of the second derivative of y(t) plus 1 of Laplace transform of the first derivative of y(t) plus 2.

When we sum these components, collect the Y s terms, and set it equal to the right-hand side, we have:

s 3 2 s 2 s 2 Y s s 2 1 2 s 3 3 s 2 4 s 2 1 s

Rearranging, we can find the solution to Y s :

Y s 2 s 3 3 s 2 4 s 2 s 3 2 s 2 s 2 1 s s 2 1 s 3 2 s 2 s 2

This solution can be looked at in two parts. The first term on the right-hand side is the particular (or forced) solution. You can see how it depends on p s and u s . The second term is the homogeneous (or natural) solution. The numerator of this term describes how the initial conditions of the system affect the solution (recall that s 2 1 was the part of the result of the linear combination of Laplace transform of the third derivative of y(t) , Laplace transform of the second derivative of y(t) , Laplace transform of the first derivative of y(t) ). The denominator of the second term is the q s polynomial; it serves to describe the system in general.

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Source:  OpenStax, State space systems. OpenStax CNX. Jan 22, 2004 Download for free at http://cnx.org/content/col10143/1.3
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