4 Engineering Example 1

4.1 Charge on a capacitor

In the circuit shown in Figure 19, the switch S is closed at t = 0 with a capacitor charge q ( 0 ) = q 0 = constant and d q d t ( 0 ) = 0 .

Figure 19

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Show that q ( t ) = q 0 ( t ) e α t cos ω t + α w sin ω t where α = R 2 L and ω 2 = 1 L C α 2

Laplace transform properties required

The following properties are needed to solve this problem.

F ( s + a ) = L { e a t f ( t ) } (P1)

L d f ( t ) d t = s { f ( t ) } f ( 0 ) (P2)

L d 2 f ( t ) d t 2 = s 2 L { f ( t ) } d f d t ( 0 ) s f ( 0 ) (P3)

L { sin k t } = k s 2 + k 2 with s > 0 (P4)

L { cos k t } = s s 2 + k 2 with s > 0 (P5)

L 1 { L { f ( t ) } } = f ( t ) (P6)

STEP 1 Establish the differential equation for q ( t ) using, for example, Kirchhoff’s law.

Solution

When the switch S is closed, the inductance L , capacitance C and resistance R give rise to a.c. voltages related by

V A V B = L d i d t , V B V D = R i , V D V F = q C  respectively .

So since V A V F = ( V A V B ) + ( V B V D ) + ( V D V F ) = 0 and i = d q d t we have

L d 2 q d t 2 + R d q d t + q C = 0 (1)

STEP 2 Write the Laplace transform of the differential equation substituting for the initial

conditions:

Solution

Since the Laplace transform is linear, the transform of differential Equation (1) is

L L d 2 q d t 2 + R d q d t + q C = L L d 2 q d t 2 + R L d q d t + L { q C } = 0. (2)

We deal with each derivative term in turn: Using property (P3),

L d 2 q d t 2 = s 2 L { q ( t ) } d q d t ( 0 ) s q ( 0 ) .

So, using the initial conditions q ( 0 ) = q 0 and d q d t ( 0 ) = 0

L d 2 q d t 2 = s 2 L { q ( t ) } s q 0 . (3)

By means of property (2)

L d q d t = s L { q ( t ) } q 0 (4)

STEP 3 Solve for the function L { q ( t ) } by substituting from (3) and (4) into Equation (2):

Solution

L [ s 2 L { q ( t ) } s q 0 ] + R [ s L { q ( t ) } q 0 ] + 1 C L { q ( t ) } = 0

L { q ( t ) } [ L s 2 + R s + 1 C ] = L s q 0 + R q 0

L { q ( t ) } = ( L s + R ) ( L s 2 + R s + 1 C ) q 0 (5)

Using the definitions α = R 2 L and ω 2 = 1 L C α 2 enables the denominator in Equation (5) to be expressed as the sum of two squares,

L s 2 + R s + 1 C = L [ s 2 + R s L + 1 L C ] = L [ s 2 + 2 α s + 1 L C ]

= L [ s 2 + 2 α s + α 2 + ω 2 ] = L [ { s + α } 2 + ω 2 ] .

Consequently, with the new expression for the denominator, Equation (5) becomes

L { q ( t ) } = q 0 s ( s + α ) 2 + ω 2 + R L 1 ( s + α ) 2 + ω 2 . (6)

STEP 4 Use the inverse Laplace transform to obtain q ( t ) :

Solution

The inverse Laplace transform is used to find q ( t ) .

Taking the inverse Laplace transform of Equation (6) and using the linearity properties

L 1 { L { q ( t ) } } = q 0 L 1 s ( s + α ) 2 + ω 2 + R L 1 ( s + α ) 2 + ω 2 .

Using property (P6) this can be written as

q ( t ) = q 0 L 1 s + α ( s + α ) 2 + ω 2 + α ( s + α ) 2 + ω 2 + R L ω ω ( s + α ) 2 + ω 2 .

Using the linearity of the Laplace transform again

q ( t ) = q 0 L 1 s + α ( s + α ) 2 + ω 2 + L 1 α ( s + α ) 2 + ω 2 + L 1 R L ω ω ( s + α ) 2 + ω 2 . (7)

Using properties (P1) and (P5)

L 1 s + α ( s + α ) 2 + ω 2 = e α t cos ω t . (8)

Similarly,

L 1 α ( s + α ) 2 + ω 2 = ( α ω ) { e α t sin ω t } (9)

and

L 1 R L ω ω ( s + a ) 2 + ω 2 = ( R L ω ) e α t sin ω t . (10)

Substituting (8), (9) and (10) in (7) gives

q ( t ) = q 0 e α t cos ω t + α ω + R L ω e α t sin ω t . (11)

STEP 5 Finally, show that for t > 0 the solution is

q ( t ) = q 0 e α t [ cos ω t + ( α ω ) sin ω t ]  where  α = R 2 L and ω 2 = 1 L C α 2 .

Solution

Substituting α = R 2 L in (11) gives

q ( t ) = q 0 e α t cos ω t + [ α ω + 2 α ω ] e α t sin ω t

= q 0 e α t [ cos ω t + α ω sin ω t ]