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Impulse Forcing Functions

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Presentation on theme: "Impulse Forcing Functions"β€” Presentation transcript:

1 Impulse Forcing Functions
MAT 275

2 At right is a function, 𝑦= 1 (2𝛼) , βˆ’π›Ό<𝑑<𝛼 0, π‘‘β‰€βˆ’π›Ό or 𝑑β‰₯𝛼
Sometimes, energy is contributed into a system instantaneously. These are called impulses. At right is a function, 𝑦= 1 (2𝛼) , βˆ’π›Ό<𝑑<𝛼 0, π‘‘β‰€βˆ’π›Ό or 𝑑β‰₯𝛼 The main thing to observe here is that the area under the horizontal bar is 1. The parameter 𝛼 can be allowed to trend to 0 as a limit. However, we require that the area below the horizontal bar remain 1 unit. As 𝛼 β†’0, the height of the bar trends to infinity. The function is non-zero for increasing smaller amounts of time. In this way, the unit impulse function 𝛿 is defined as 𝛿 𝑑 =0 for all 𝑑≠0, and βˆ’βˆž ∞ 𝛿 𝑑 𝑑𝑑 =1. The impulse can occur anywhere. If it occurs at 𝑑=𝑐, we just build in the shift, 𝛿 π‘‘βˆ’π‘ =0 for all 𝑑≠𝑐. The integral expression (governing the area) stays the same. (c) ASU SoMSS - Scott Surgent. If you see an error,

3 The Laplace Transform of 𝛿 π‘‘βˆ’π‘ is 𝐿 𝛿 π‘‘βˆ’π‘ = 𝑒 βˆ’π‘π‘  .
Example: Find the solution of 𝑦 β€²β€² +9𝑦=𝛿 π‘‘βˆ’4 , with 𝑦 0 =0 and 𝑦 β€² 0 =0. Solution: Apply the Laplace Transform operator to both sides: 𝐿 𝑦 β€²β€² +9𝑦 =𝐿 𝛿 π‘‘βˆ’4 𝐿 𝑦 β€²β€² +9𝐿 𝑦 =𝐿 𝛿 π‘‘βˆ’4 𝑠 2 𝐿 𝑦 βˆ’π‘ π‘¦ 0 βˆ’ 𝑦 β€² 0 +9𝐿 𝑦 = 𝑒 βˆ’4𝑠 𝐿 𝑦 𝑠 2 +9 = 𝑒 βˆ’4𝑠 Thus, 𝐿 𝑦 = 𝑒 βˆ’4𝑠 𝑠 2 +9 , so that the solution is 𝑦= 𝐿 βˆ’1 𝑒 βˆ’4𝑠 𝑠 (c) ASU SoMSS - Scott Surgent. If you see an error,

4 The 𝑒 βˆ’4𝑠 inverts back to 𝑒 4 (𝑑) … not back to the impulse function!
From the last slide, we have that the solution is 𝑦= 𝐿 βˆ’1 𝑒 βˆ’4𝑠 𝑠 The 𝑒 βˆ’4𝑠 inverts back to 𝑒 4 (𝑑) … not back to the impulse function! The 1 𝑠 inverts as follows: 𝐿 βˆ’ 𝑠 = 1 3 𝐿 βˆ’ 𝑠 = 1 3 sin (3𝑑) . Thus, the solution is 𝑦= 1 3 𝑒 4 𝑑 sin 3 π‘‘βˆ’4 . This can be interpreted as follows: When 𝑑<4, the factor 𝑒 4 𝑑 =0, so 𝑦=0, so β€œnothing is happening”. Then at 𝑑=4, an impulse of energy is instantaneously applied to the system, setting in motion the solution, 𝑦= 1 3 sin 3π‘‘βˆ’12 , which β€œstarts” at 𝑑=4 and continues forever as 𝑑>4. The graph is: (c) ASU SoMSS - Scott Surgent. If you see an error,

5 Example: Solve 𝑦 β€²β€² +5 𝑦 β€² +6𝑦=𝛿 π‘‘βˆ’3 +𝛿(π‘‘βˆ’6), where 𝑦 0 =0, 𝑦 β€² 0 =0.
Solution: We have: 𝐿{ 𝑦 β€²β€² }+5𝐿{ 𝑦 β€² }+6𝐿{𝑦}=𝐿{𝛿 π‘‘βˆ’3 }+𝐿 𝛿 π‘‘βˆ’6 𝑠 2 𝐿 𝑦 βˆ’π‘ π‘¦ 0 βˆ’ 𝑦 β€² 𝑠𝐿 𝑦 βˆ’π‘¦ 0 +6𝐿 𝑦 = 𝑒 βˆ’3𝑠 + 𝑒 βˆ’6𝑠 𝐿 𝑦 𝑠 2 +5𝑠+6 = 𝑒 βˆ’3𝑠 + 𝑒 βˆ’6𝑠 Thus, 𝐿 𝑦 = 𝑒 βˆ’3𝑠 + 𝑒 βˆ’6𝑠 𝑠 2 +5𝑠+6 , so that 𝑦= 𝐿 βˆ’1 𝑒 βˆ’3𝑠 + 𝑒 βˆ’6𝑠 𝑠 2 +5𝑠+6 . Ignoring the e terms for the moment, we have 1 𝑠 2 +5𝑠+6 = 1 𝑠+2 𝑠+3 = 1 𝑠+2 βˆ’ 1 𝑠+3 . Next slide… (c) ASU SoMSS - Scott Surgent. If you see an error,

6 From the last slide, we have, 𝑦= 𝐿 βˆ’1 𝑒 βˆ’3𝑠 + 𝑒 βˆ’6𝑠 𝑠 2 +5𝑠+6 .
We also have 1 𝑠 2 +5𝑠+6 = 1 𝑠+2 𝑠+3 = 1 𝑠+2 βˆ’ 1 𝑠+3 . Inverting, we have 𝐿 βˆ’1 1 𝑠+2 = 𝑒 βˆ’2𝑑 and 𝐿 βˆ’1 βˆ’ 1 𝑠+3 = βˆ’π‘’ βˆ’3𝑑 . Note that the e terms invert to 𝑒 3 (𝑑) and 𝑒 6 (𝑑). Thus, the solution is 𝑦= 𝑒 3 𝑑 𝑒 βˆ’2 π‘‘βˆ’3 βˆ’ 𝑒 βˆ’3 π‘‘βˆ’3 + 𝑒 6 (𝑑) 𝑒 βˆ’2 π‘‘βˆ’6 βˆ’ 𝑒 βˆ’3 π‘‘βˆ’6 . Simplified, we have 𝑦= 𝑒 3 𝑑 𝑒 6βˆ’2𝑑 βˆ’ 𝑒 9βˆ’3𝑑 + 𝑒 6 (𝑑) 𝑒 12βˆ’2𝑑 βˆ’ 𝑒 18βˆ’3𝑑 . In the graph, there are two β€œimpulses” at t = 3 and t = 6: (c) ASU SoMSS - Scott Surgent. If you see an error,


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