First-Order Linear Equations

A first‐order differential equation is said to be linear if it can be expressed in the form

   

where P and Q are functions of x. The method for solving such equations is similar to the one used to solve nonexact equations. There, the nonexact equation was multiplied by an integrating factor, which then made it easy to solve (because the equation became exact).

To solve a first‐order linear equation, first rewrite it (if necessary) in the standard form above; then multiply both sides by the integrating factor

The resulting equation, 

 

is then easy to solve, not because it's exact, but because the left‐hand side collapses:

Therefore, equation (*) becomes

   

making it susceptible to an integration, which gives the solution:

Do not memorize this equation for the solution; memorize the steps needed to get there.

Example 1: Solve the differential equation

 

The equation is already expressed in standard form, with P(x) = 2 x and Q(x) = x. Multiplying both sides by

   

transforms the given differential equation into 

Notice how the left‐hand side collapses into ( μy)′; as shown above, this will always happen. Integrating both sides gives the solution:

 

Example 2: Solve the IVP

Note that the differential equation is already in standard form. Since P(x) = 1/ x, the integrating factor is

 

Multiplying both sides of the standard‐form differential equation by μ = x gives

 

Note how the left‐hand side automatically collapses into ( μy)′. Integrating both sides yields the general solution:

 

Applying the initial condition y(π) = 1 determines the constant c:

 

Thus the desired particular solution is

   

or, since x cannot equal zero (note the coefficient P(x) = 1/ x in the given differential equation),

Example 3: Solve the linear differential equation

   

First, rewrite the equation in standard form:

Since the integrating factor here is

   

multiply both sides of the standard‐form equation (*) by μ = e −2/ x ,

 

collapse the left‐hand side,

 

and integrate:

Thus the general solution of the differential equation can be expressed explicitly as

Example 4: Find the general solution of each of the following equations:

a. 

b. 

Both equations are linear equations in standard form, with P(x) = –4/ x. Since 

 

the integrating factor will be 

 

for both equations. Multiplying through by μ = x −4 yields

Integrating each of these resulting equations gives the general solutions:

 

Example 5: Sketch the integral curve of

   

which passes through the origin.

The first step is to rewrite the differential equation in standard form:

   

Since

 

the integrating factor is

Multiplying both sides of the standard‐form equation (*) by μ = (1 + x 2) 1/2 gives 

As usual, the left‐hand side collapses into (μ y)

   

and an integration gives the general solution:

To find the particular curve of this family that passes through the origin, substitute ( x,y) = (0,0) and evaluate the constant c:

 

Therefore, the desired integral curve is

   

which is sketched in Figure 1.


Figure 1

Example 6: An object moves along the x axis in such a way that its position at time t > 0 is governed by the linear differential equation

 

If the object was at position x = 2 at time t = 1, where will it be at time t = 3?

Rather than having x as the independent variable and y as the dependent one, in this problem t is the independent variable and x is the dependent one. Thus, the solution will not be of the form “ y = some function of x” but will instead be “ x = some function of t.”

The equation is in the standard form for a first‐order linear equation, with P = tt −1 and Q = t 2. Since

   

the integrating factor is

Multiplying both sides of the differential equation by this integrating factor transforms it into

 

As usual, the left‐hand side automatically collapses,

   

and an integration yields the general solution:

Now, since the condition “ x = 2 at t = 1” is given, this is actually an IVP, and the constant c can be evaluated:

 

Thus, the position x of the object as a function of time t is given by the equation

   

and therefore, the position at time t = 3 is

 

which is approximately 3.055.

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