This circuit has the same steady-state behavior as the circuit from the previous problem , but with some transient behavior prior to that.
A D C voltage source V S and a D C current source I S feed a circuit with resistors R 1 and R 2 , inductor L , and capacitor C as shown. At time t = 0 , the inductor and capacitor are de-energized. Currents I R 1 ( t ) and I R 2 ( t ) flow in resistors R 1 and R 2 , respectively.
Determine the value of the quantity Q .
Q = ∫ 0 ∞ ( I R 1 ( t ) − I 0 ) d t + ∫ 0 ∞ ( 4 I 0 − I R 2 ( t ) ) d t
Details and Assumptions:
1)
V
S
=
1
0
volts
2)
I
S
=
5
amps
3)
R
1
=
2
Ω
4)
R
2
=
3
Ω
5)
L
=
5
0
H
6)
C
=
1
F
7)
I
0
=
1
amp
8)
Source and current polarities are as indicated in the diagram
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Luckily revisited my solution only to see a more interesting one. Thank you for sharing
You're welcome! Hope there were no other prerequisites for the "Final Value Theorem" - guess I'll have to double-check.
Edit: Seems there are no further prerequisites.
Let I 1 = I R 1 and I 2 = I R 2 . Let the charge on the capacitor be Q c and the current through it be I c at a general time t . Applying Kirchoff's laws gives the circuit equations:
− 1 0 − 2 I 1 + 3 I 2 + 5 0 I ˙ 2 = 0 5 0 I ˙ 2 + 3 I 2 = Q c I S = 5 = I 1 + I 2 + Q ˙ c
Simplifying the equations a bit more leads to the system of ODEs:
2 Q ˙ c + 5 0 I ˙ 2 = − 5 I 2 + 2 0 5 0 I ˙ 2 = − 3 I 2 + Q c
I 2 ( 0 ) = Q c ( 0 ) = 0
Taking Laplace transform on both sides and solving for I 2 ( s ) and I c ( s ) knowing that I c ( s ) = s Q c ( s ) :
I 2 ( s ) = s ( 1 0 0 s 2 + 5 6 s + 5 ) 2 0 I c ( s ) = ( 1 0 0 s 2 + 5 6 s + 5 ) 2 0 ( 5 0 s + 3 ) ∵ 5 = I 1 + I 2 + Q ˙ c
Now computing the inverse Laplace transform using Wolfram leads to the following. Let:
a = − 2 5 7 − 5 0 7 1 b = − 2 5 7 + 5 0 7 1
I 2 ( t ) = 7 1 2 ( ( − 7 1 + 1 4 7 1 ) e a t − ( 7 1 + 1 4 7 1 ) e b t + 1 4 2 ) I c ( t ) = 7 1 5 ( ( 1 1 + 7 1 ) e a t + ( 7 1 − 1 1 ) e b t ) ∵ 5 = I 1 + I 2 + Q ˙ c ∴ I 1 ( t ) = 5 − I 2 ( t ) − I c ( t )
After having obtained these closed form expressions, the next step is to evaluate the required integrals which also have a closed form:
∫ 0 ∞ ( 4 − I 2 ( t ) ) d t = ∫ 0 ∞ ( 4 − 7 1 2 ( ( − 7 1 + 1 4 7 1 ) e a t − ( 7 1 + 1 4 7 1 ) e b t + 1 4 2 ) ) d t ∫ 0 ∞ ( I 1 ( t ) − 1 ) d t = ∫ 0 ∞ ( 5 − 7 1 2 ( ( − 7 1 + 1 4 7 1 ) e a t − ( 7 1 + 1 4 7 1 ) e b t + 1 4 2 ) − 7 1 5 ( ( 1 1 + 7 1 ) e a t + ( 7 1 − 1 1 ) e b t ) − 1 ) d t
I did not even consider touching these manageable but very tedious monsters. Numerically evaluating leads to:
Q = ∫ 0 ∞ ( I 1 ( t ) − 1 ) d t + ∫ 0 ∞ ( 4 − I 2 ( t ) ) d t ≈ 7 7 . 6
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You can use the final limit theorem to avoid inverse Laplace-Transforms and integration at the same time! Before we begin, we normalize all currents, voltages, time and elements by the values given below: voltages: 1 V , currents: 1 A , time: 1 s ⇒ R : 1 Ω , C : 1 F , L : 1 H , Q : 1 C The network equations remain the same in the process, but now all currents, voltages, time and elements represent their normalized dimensionless counterparts.
After switching ( t ≥ 0 )
The network was de-energized at t = 0 − , so all initial conditions at t = 0 − vanish and i R 1 , 2 ( t ) only depend on the input sources v s ( t ) , i s ( t ) . To calculate the two currents efficiently with Laplace-Transforms, we define the voltage u C ( t ) over C from top to bottom. With KVL, we get V s ( s ) = s 1 0 , I s ( s ) = s 5 ⇒ I R 1 ( s ) = R 1 U C ( s ) − V s ( s ) = 2 U C ( s ) − s 5 , I R 2 ( s ) = s L + R 2 U C ( s ) = 5 0 s + 3 U C ( s ) To calculate U C ( s ) , we combine R 1 , V s ( s ) into an equivalent current source and use superposition afterwards: U C ( s ) = ( ( s L + R 2 ) ∥ R 1 ∥ s C 1 ) ⋅ ( I s ( s ) + R 1 V s ( s ) ) = s + 2 1 + 5 0 s + 3 1 1 ⋅ ( s 5 + s 5 ) = s 2 + 0 . 5 6 s + 0 . 0 5 s + 0 . 0 6 ⋅ s 1 0 We calculate the Laplace-Transforms of both integrands. The poles at s = 0 cancel out, i.e. I 0 , 4 I 0 are the steady-state currents i R 1 , 2 ( t ) will converge to: I R 1 ( s ) − s I 0 s 4 I 0 − I R 2 ( s ) = 2 U C ( s ) − s 6 = ( s 2 + 0 . 5 6 s + 0 . 0 5 ) s − 6 s 2 + 1 . 6 4 s = s 2 + 0 . 5 6 s + 0 . 0 5 − 6 s + 1 . 6 4 = s 4 − 5 0 s + 3 U C ( s ) = ( s 2 + 0 . 5 6 s + 0 . 0 5 ) s 4 s 2 + 2 . 2 4 s = s 2 + 0 . 5 6 s + 0 . 0 5 4 s + 2 . 2 4 ∣ ∣ ∣ ∣ ∣ ∣ ∣ ∣ ∣ s 1 , 2 = − 2 5 7 ± 6 2 5 4 9 − 2 0 1 = − 2 5 7 ± 5 0 7 1 < 0 Both remaining poles s 1 , 2 lie in the open left plane, so we may use the Final Value Theorem to calculate both parts of Q together: Q = s → 0 lim s ⋅ s 1 ( I R 1 ( s ) − s I 0 + s 4 I 0 − I R 2 ( s ) ) = s → 0 lim s 2 + 0 . 5 6 s + 0 . 0 5 − 2 s + 3 . 8 8 = 0 . 0 5 3 . 8 8 = 7 7 . 6
Rem.: This way is efficient if you're only interested in the value of Q , but not the transients i R 1 , 2 ( t ) For the transients, there is no way around partial fraction decomposition (PFD) and inverse Lapace-Transform :(