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Lecture Notes in Differential Equations - Bruce E. Shapiro

Lecture Notes in Differential Equations - Bruce E. Shapiro

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28 LESSON 4. LINEAR EQUATIONS<br />

Exponentiat<strong>in</strong>g both sides of the equation<br />

∫<br />

∫<br />

∫<br />

pdt + C pdt<br />

µ = e = e e C = C 1 e<br />

pdt<br />

(4.27)<br />

where C 1 = e C and C is any constant. S<strong>in</strong>ce we want any function µ that<br />

will work, we are free to choose our constant arbitrarily, e.g., pick C = 0<br />

hence C 1 = 1, and we f<strong>in</strong>d that<br />

µ(t) = e<br />

∫<br />

p(t)dt<br />

(4.28)<br />

has the properties we desire. We say the equation 4.28 is an <strong>in</strong>tegrat<strong>in</strong>g<br />

factor for the differential equation 4.10. S<strong>in</strong>ce we have already chosen<br />

the constant of <strong>in</strong>tegrate, we can safely ignore the constant of <strong>in</strong>tegration<br />

when <strong>in</strong>tegrat<strong>in</strong>g p. To recap, the general solution of y ′ + py = q is given by<br />

equation 4.18 whenever µ is given by 4.28. The particular solution of a given<br />

<strong>in</strong>itial value problem <strong>in</strong>volv<strong>in</strong>g a l<strong>in</strong>ear ODE is then solved by substitut<strong>in</strong>g<br />

the <strong>in</strong>itial condition <strong>in</strong>to the general solution obta<strong>in</strong>ed <strong>in</strong> this manner.<br />

It is usually easier to memorize the procedure rather than the formula for<br />

the solution (equation 4.18):<br />

Method to Solve y ′ + p(t)y = q(t)<br />

1. Computer µ = e ∫ p(t)dt and observe that µ ′ (t) = p(t)µ(t).<br />

2. Multiply the ODE through by µ(t) giv<strong>in</strong>g<br />

µ(t)y ′ + µ ′ (t)y = µ(t)q(t)<br />

3. Observe that the left-hand side is precisely (d/dt)(µ(t)y).<br />

4. Integrate both sides of the equation over t, remember<strong>in</strong>g that<br />

∫<br />

(d/dt)(µy)dt = µ(t)y,<br />

∫<br />

µ(t)y =<br />

q(t)ydt + C<br />

5. Solve for y by divid<strong>in</strong>g through by µ. Don’t forget the constant<br />

on the right-hand side of the equation.<br />

6. Use the <strong>in</strong>itial condition to f<strong>in</strong>d the value of the constant, if this<br />

is an <strong>in</strong>itial value problem.

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