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The solutions to the sample second test of math 2214, focusing on differential equations with complex roots and the application of variation of parameters. Finding the general solution, initial value problems, and the behavior of solutions as t approaches negative and positive infinities.
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Math 2214 Monday, October 13
16 − 52 )/2, that is 2 ± 3 i. Therefore the general solution to the differential equation is y = e^2 t^ (C 1 cos 3t + C 2 sin 3t), where C 1 ,C 2 are arbitrary con- stants. We now plug in the initial conditions: first t = 0, y = 0 yields 0 = C 1 , so y = C 2 e^2 t^ sin 3t. Now we differentiate by product rule to obtain y′^ = 2 C 2 e^2 t^ sin 3t + 3 C 2 e^2 t^ cos 3t. Plugging in t = 0, y′^ = 3, we obtain 3 = 3 C 2. Therefore C + 2 = 1 and we conclude that the solution to the initial value problem is y(t) = e^2 t^ sin 3t. As t → −∞, y(t) → 0, while as t → ∞, y(t) oscillates with ever increasing amplitude, and this increasing amplitude tends to infinity.
A( 4 t^2 + 8 t + 2 )e^2 t^ − 4 A( 2 t^2 + 2 t)e^2 t^ + 4 At^2 e^2 t^ = 2 e^2 t^.
The terms in t^2 e^2 t^ and te^2 t^ cancel and we are left with A 2 e^2 t^ = 2 e^2 t^. Therefore A = 1 and we conclude that the solution to the differential equation is y = yC + yP = C 1 e^2 t^ + C 2 te^2 t^ + t^2 e^2 t^.
y′^ = u′t + u + v′t^3 + 3 t^2 v = u + 3 t^2 v y′′^ = u′^ + 6 tv + 3 t^2 v′.
Plugging back into t^2 y′′^ − 3 ty′^ + 3 y = 2 t^3 , we obtain
t^2 (u′^ + 6 tv + 3 t^2 v′) − 3 t(u + 3 t^2 v) + 3 (ut + t^3 v) = 2 t^3.
As always happens at this point, the terms in u, v cancel and we are left only with terms in u′, v′, that is t^2 u′^ + 3 t^4 v′^ = 2 t^3 , which simplifies to u′^ + 3 t^2 v′^ = 2 t. If multiply the equation u′^ + v′t^2 = 0 from above by 3 and subtract, we obtain − 2 u′^ = 2 t. Therefore
u′^ = −t and we deduce that u = −t^2 /2. Also we get v′^ = 1 /t and we deduce that v = lnt (we don’t need a “C” here because we only need a particular solution). Therefore yP = ut + vt^3 = −t^3 / 2 + t^3 lnt and we conclude that the general solution is y = yC + yP = C 1 t +C 2 t^3 −t^3 / 2 +t^3 lnt. We can tidy this up a little, because the C 2 t^3 and −t^3 / 2 can be combined (replace C 2 with C 2 + 1 /2) to obtain y = C 1 t +C 2 t^3 + t^3 lnt.
2 g + 3 cos 3t − 2 sin 3t − y′^ − 3 (e + y) = 2 y′′.
When the system is at rest and there is no force, y′′^ = y′^ = y = 0 and we obtain the equation 2g − 3 e = 0. The equation then becomes 2y′′^ + y′^ + 3 y = 3 cos 3t − 2 sin 3t.
Test on Friday, October 17. Material section 3.1 to section 3.10 on the assignment sheet. Review session on Thursday October 16 at 5 p.m. in McBryde 226.