MATH 54 − HINTS TO HOMEWORK 13 PEYAM TABRIZIAN Here are a couple of hints to Homework 13. Make sure to attempt the problems before you check out those hints. Enjoy! S ECTION 9.8: T HE MATRIX EXPONENTIAL FUNCTIONS Again, check out the ‘Systems of differential equations’-handout! 9.8.11. The formula is eAt = X(t)X−1 (0). Remember that you only have to find the inverse at 0, not in general! Or use eAt = P eDt P −1 , where D is your matrix of eigenvalues, and P is your matrix of eigenvectors. 9.8.21. The general solution is x(t) = eAt c. Use the initial condition to solve for c. S ECTION 10.2: M ETHOD OF SEPARATION OF VARIABLES 110.2.3, 10.2.5. Just solve your equation the way you would usually do (for 5, use undetermined coefficients) and plug in the initial conditions. You may or may not find a contradiction! If you find 0 = 0, that usually means there are infinitely many solutions, depending on your constant A or B. 10.2.11. You have to split up your analysis into three cases: Case 1: λ > 0. Then let λ = ω 2 , where ω > 0. This helps you get rid of square roots. Case 2: λ = 0. Case 3: λ < 0. Then λ = −ω 2 , where ω < 0. In each case, solve the equation and plug in your initial condition. You may or may not get a contradiction. Also, remember that y has to be Date: Tuesday, April 28th, 2015. 1 2 PEYAM TABRIZIAN nonzero! 10.2.17, 10.2.19. Follow the outline given in the sections ‘Heat equation’ and ‘Wave equation’ in my Partial Differential Equations-Handouts. You don’t need to worry about Fourier series, as you can just compare the coefficients. 10.2.23. At some point, you should get: ∞ X An sin(nπx) = n=1 By ‘comparing,’ you get An = ∞ X 1 sin(nπx) 2 n n=1 1 . n2 10.2.28. Just put all the X on the left-hand-side, and all the T on the right00 hand-side. Then you should get XX is constant, equal to λ, which gives you X 00 = λX, and use this to solve for T . 10.2.33. All they ask you to solve is the differential equation y 00 = 0, with y(0) = y(L) = 50 for (a), and y(0) = 10 and y(L) = 40 for (b). S ECTION 10.3: F OURIER SERIES 10.3.7. Just calculate (f g)(−x) = f (−x)g(−x) 10.3.9, 10.3.16. Use the following formulas: ∞ nπx nπx o a0 X n f (x)^ + an cos + bn sin 2 T T n=1 Z nπx 1 T an = f (x) cos dx T −T T Z nπx 1 T bn = f (x) sin dx T −T T Where T is such that f is defined on (−T, T ) 10.3.17, 10.3.24. The Fourier series converges to f (x) if f is continuous + (x− ) at x, and converges to f (x )+f if f is discontinuous at x. As for the 2 endpoints T and −T , the fourier series converges to the average of f at those endpoints. MATH 54 − HINTS TO HOMEWORK 13 3 10.3.28. For (b), plug in x = 0 in your Fourier series. This is legit because f is continuous at 0, hence the Fourier series converges to f at 0. For (c), plug in x = π, here the Fourier series converges to 12 ((−π + )2 + (π − )2 ) = π2. S ECTION 10.4: F OURIER COSINE AND SINE SERIES IMPORTANT NOTE: The book uses the following trick A LOT: Namely, suppose that when you calculate your coefficients Am or Bm , m+1 you get something like: Am = (−1)πm +1 . Then notice the following: If m is even, then (−1)m+1 + 1 = 0, so −2 Am = 0, and if m is odd, (−1)m+1 + 1 = −2, and Am = πm . So at some point, you would like to say: f (x)“ = ” ∞ X Am cos(mx) m=1,modd The way you do this is as follows: Since m is odd m = 2k − 1, for k = 1, 2, 3 · · · , and so the sum becomes: f (x)“ = ” ∞ X k=1 −2 cos((2k − 1)x) π(2k − 1) 10.4.4. π-periodic extension just means ‘repeat the graph of f ’. The even-2π periodic extension is just the function: fe (x) = f (−x) f (x) if − π < x < 0 if0 < x < π The odd-2π periodic extension is just the function: if − π < x < 0 −f (−x) 0 ifx = 0 fo (x) = f (x) if0 < x < π And repeat all those graphs! 4 PEYAM TABRIZIAN 10.4.7. Use the formulas: f (x)“ = ” ∞ X Am cos πmx T m=0 where: Z 1 T A0 = f (x)dx T 0 Z πmx 2 T f (x) cos dx Am = T 0 T 10.4.12. Use the formulas: f (x)“ = ” ∞ X Bm sin πmx T m=0 where: B0 = 0 2 Bm = T Z T f (x) sin 0 πmx T dx 10.4.17. The best advice I can give you is: Read the PDE handout, specifically the section about the heat equation! It outlines all the important steps you’ll need!
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