Ordinary Differential Equations/Non Homogenous 1

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Non-Homogeneous EquationsEdit

A non-homogeneous equation of constant coefficients is an equation of the form


where ci are all constants and f(x) is not 0.

Complementary FunctionEdit

Every non-homogeneous equation has a complementary function (CF), which can be found by replacing the f(x) with 0, and solving for the homogeneous solution. For example, the CF of




Superposition PrincipleEdit

The superposition principle makes solving a non-homogeneous equation fairly simple. The final solution is the sum of the solutions to the complementary function, and the solution due to f(x), called the particular integral (PI). In other words,

General Solution = CF + PI

Method of Undetermined CoefficientsEdit

The method of undetermined coefficients is an easy shortcut to find the particular integral for some f(x). The method works only if a finite number of derivatives of f(x) eventually reduces to 0, or if the derivatives eventually fall into a pattern in a finite number of derivatives. If this is true, we then know part of the PI - the sum of all derivatives before we hit 0 (or all the derivatives in the pattern) multiplied by arbitrary constants. This is the trial PI. We can then plug our trial PI into the original equation to solve it fully.

As we will see, we may need to alter this trial PI depending on the CF. If the trial PI contains a term that is also present in the CF, then the PI will be absorbed by the arbitrary constant in the CF, and therefore we will not have a full solution to the problem.

f(x) = ConstantEdit

The simplest case is when f(x) is constant, for example


The solution to the CF is


We now need to find a trial PI. When we differentiate y=3, we get zero. Therefore, our trial PI is the sum of a functions of y before this, that is, 3 multiplied by an arbitrary constant, which gives another arbitrary constant, K.

We now set y equal to the PI and find the derivatives up to the order of the DE (here, the second).


We can now substitute these into the orginal DE:


By summing the CF and the PI, we can get the general solution to the DE:


f(x) = PolynomialEdit

This is the general method which includes the above example. A polynomial of order n reduces to 0 in exactly n+1 derivatives (so 1 for a constant as above, three for a quadratic, and so on). So we know that our PI is


For an example, lets take


First off, we know that our PI is


In order to plug in, we need to calculate the first two derivatives of this:


Plugging in we get:


Solving gives us


So, our PI is


However, we need to get the complementary function as well. To get that, set f(x) to 0 and solve just like we did in the last section. For this equation, the roots are -3 and -2. So that makes our CF


Summing gives us our general solution:


f(x) = Power of eEdit

Powers of e don't ever reduce to 0, but they do become a pattern. In fact it does so in only 1 differentiation, since it's its own derivative. So we know


where K is our constant and p is the power of e givin in the original DE.

For example, consider


We make our trial PI


Which then gives


Plugging in, we get


That's the particular integral. We found the CF earlier. So the general solution is


f(x) = Polynomial × Power of eEdit

Polynomials multiplied by powers of e also form a loop, in n derivatives (where n is the highest power of x in the polynomial). So we know that our trial PI is


where C is a constant and p is the power of e in the equation.

For example, lets try


We can now set our PI to


Plugging in, we get


Thats the particular solution. We found the homogeneous solution earlier. So the total solution is


f(x) = Trigonometric FunctionsEdit

Trig functions don't reduce to 0 either. But they do have a loop of 2 derivatives - the derivative of sin x is cos x, and the derivative of cos x is -sin x. So we put our PI as


where C is a constant and p is the term inside the trig. function in the original DE.

For example, lets try


We set our PI to


Plugging in, we get


Thats the particular solution. We found the homogeneous solution earlier. So the total solution is


f(x) = A MixtureEdit

Not only are any of the above solvable by the method of undetermined coefficients, so is the sum of one or more of the above. This is because the sum of two things whose derivatives either go to 0 or loop must also have a derivative that goes to 0 or loops. The   would be the sum of the individual   functions.

If the Trial PI shares terms with the CFEdit

When dealing with  , or sometimes with polynomials (if the homogeneous equation has roots of 0) as f(x), you may get the same term in both the trial PI and the CF. If this happens, the PI will be absorbed into the arbitrary constants of the CF, which will not result in a full solution. To overcome this, multiply the affected terms by x as many times as needed until it no longer appears in the CF.

As an example, let's take


First, solve the homogeneous equation to get the CF.


The auxiliary polynomial is


Find the roots of the auxiliary polynomial. In this case, they are


The CF is


Now for the particular integral. Since f(x) is a polynomial of degree 1, we would normally use Ax+B. However, since both a term in x and a constant appear in the CF, we need to multiply by x² and use


We solve this as we normally do for A and B.


So the total solution is


Variation of ParametersEdit

Variation of parameters is a method for finding a particular solution to the equation   if the general solution for the corresponding homogeneous equation   is known. We will now derive this general method.

We already know the general solution of the homogenous equation: it is of the form  . We will look for a particular solution of the non-homogenous equation of the form  , with u and v functions of the independent variable x. Differentiating this we get


Now notice that there is currently only one condition on  , namely that  . We now impose another condition, that


This means that   will have no second derivatives of   and  . Thus, these new parameters (hence the name "variation of parameters") will be the solutions to some first order differential equation, which can be solved. Let us finish the problem:







where the last step follows from the fact that   and   are solutions of the homogeneous equation.

Therefore, we have   and  . Multiplying the first equation by   and the second by   and adding gives



A similar procedure gives


Now it is only necessary to evaluate these expressions and integrate them with respect to   to get the functions   and  , and then we have our particular solution  . The general solution to the differential equation   is therefore  .

Note that the main difficulty with this method is that the integrals involved are often extremely complicated. If the integral does not work out well, it is best to use the method of undetermined coefficients instead.

The quantity that appears in the denominator of the expressions for   and   is called the Wronskian of   and  .

Laplace TransformsEdit

The Laplace transform is a very useful tool for solving nonhomogenous initial-value problems. It allows us to reduce the problem of solving the differential equation to that of solving an algebraic equation. We begin with some setup.

Definition of the Laplace TransformEdit

The Laplace transform of   is defined as


This can also be written as  . When writing this on paper, you may write a cursive capital "L" and it will be generally understood. There is also an inverse Laplace transform  , but calculating it requires an integration with respect to a complex variable. Luckily, it is frequently possible to find   without resorting to this integration, using a variety of tricks which will be described later. However, it is first necessary to prove some facts about the Laplace transform.

Two Properties of the Laplace TransformEdit

Property 1. The Laplace transform is a linear operator; that is,  .

The proof of this property follows immediately from the definition of the Laplace transform and is left to the reader.

Property 2. If  , then  

  (integrating by parts)

It is property 2 that makes the Laplace transform a useful tool for solving differential equations. As a corollary of property 2, note that  .

Laplace Transforms of Simple FunctionsEdit





The last two can be easily calculated using Euler's formula  .

In order to find more Laplace transforms, in particular the transform of  , we will derive two more properties of the transform.

Two More Properties of the Laplace TransformEdit

Property 3. If  , then  .

Property 4. If  , then  .

The proofs are straightforward and are left to the reader.

Now we can easily see that   . Applying Property 3 multiple times, we can find that  . At last we are ready to solve a differential equation using Laplace transforms.

Using Laplace Transforms to Solve Non-Homogeneous Initial-Value ProblemsEdit

In general, we solve a second-order linear non-homogeneous initial-value problem as follows: First, we take the Laplace transform of both sides. This immediately reduces the differential equation to an algebraic one. We then solve for  . Finally, we take the inverse transform of both sides to find  .

Let's begin by using this technique to solve the problem


We begin by taking the Laplace transform of both sides and using property 1 (linearity):

  (using the initial conditions)

Now we isolate  :


Here we have factored   in preparation for the next step. We now attempt to take the inverse transform of both sides; in order to do this, we will have to break down the right hand side into partial fractions.


The first two fractions imply that  . Setting   gives  , while setting   gives  . The other three fractions similarly give   and  . Therefore:


And finally we can take the inverse transform (by inspection, of course) to get


The ConvolutionEdit

The convolution is a method of combining two functions to yield a third function. The convolution has applications in probability, statistics, and many other fields because it represents the "overlap" between the functions. We are not concerned with this property here; for us the convolution is useful as a quick method for calculating inverse Laplace transforms.

Definition. The convolution   is defined as  .

The convolution has several useful properties, which are stated below:

Property 1.   (Associativity)

Property 2.   (Commutativity)

Property 3.   (Distribution over addition)

We now prove the result that makes the convolution useful for calculating inverse Laplace transforms.


  (changing order of integration)
Now let  .

Let's solve another differential equation:


Taking Laplace transforms of both sides gives


We now have to find  . To do this, we notice that  , so   by the Theorem above. Thus, the solution to our differential equation is the convolution of sine with itself. We proceed to calculate this:


Therefore, the solution to the original equation is