How to convert Integral Equations into Differential Equations?

We’ve covered the basics of integral equations and learned how to derive them from ordinary differential equations. We even solved a linear integral equation using the trial method. Now comes the interesting part—going in reverse.

Before we dive deeper into solving integral equations, you need to master the reverse conversion: turning integral equations back into differential equations. Trust me, this skill becomes essential when you’re working through complex problems.

If you’re just joining this series, here’s what we’ve covered so far:

Converting Integral Equations to Differential Equations

This process is the exact opposite of what we did in Part III. Remember how we converted boundary value differential equations into integral equations? Now we’re reversing that operation.

Here’s the pattern I’ve observed after working through dozens of these conversions:

  • Volterra Integral Equations → Initial Value Problems (IVPs)
  • Fredholm Integral Equations → Boundary Value Problems (BVPs)

The technique is straightforward once you understand the core principle. In the forward conversion, we continuously integrated the differentials within given boundary values. For the reverse process, we continuously differentiate the integral equation and extract conditions by substituting the constant integration limits.

Let me walk you through two worked examples that demonstrate both cases.

Problem 1: Volterra Integral Equation → Initial Value Problem

Problem: Convert the following Volterra integral equation into an initial value problem:

$$y(x) = – \int_{0}^x (x-t) y(t) \, dt$$

Quick context: This is the same integral equation we obtained when converting the initial value problem \( y” + y = 0 \) with conditions \( y(0) = 0 \) and \( y'(0) = 0 \). See Problem 1 of Part III for the forward conversion.

Solution

We start with our integral equation:

$$y(x) = – \int_{0}^x (x-t) y(t) \, dt \quad \ldots (1)$$

Step 1: First differentiation. Differentiate equation (1) with respect to \( x \) using the Leibniz rule:

$$y'(x) = -\frac{d}{dx} \int_{0}^x (x-t) y(t) \, dt$$

When we differentiate under the integral sign, the term \( (x-t) \) differentiates to \( 1 \) with respect to \( x \), while the upper limit contribution vanishes since \( (x-x) = 0 \). This gives us:

$$y'(x) = -\int_{0}^x y(t) \, dt \quad \ldots (2)$$

Step 2: Second differentiation. Differentiate equation (2) with respect to \( x \):

$$y”(x) = -\frac{d}{dx} \int_{0}^x y(t) \, dt$$

By the Fundamental Theorem of Calculus, differentiating an integral with respect to its upper limit yields the integrand evaluated at that limit:

$$y”(x) = -y(x) \quad \ldots (3′)$$

Rearranging gives us our differential equation:

$$y”(x) + y(x) = 0 \quad \ldots (3)$$

Step 3: Extract initial conditions. Substitute the lower limit \( x = 0 \) into equations (1) and (2):

From equation (1):

$$y(0) = – \int_{0}^0 (0-t) y(t) \, dt = 0 \quad \ldots (4)$$

From equation (2):

$$y'(0) = -\int_{0}^0 y(t) \, dt = 0 \quad \ldots (5)$$

Final Result: The differential equation (3) with initial conditions (4) and (5) form the complete initial value problem:

$$y” + y = 0, \quad y(0) = 0, \quad y'(0) = 0 \quad \Box$$

Problem 2: Fredholm Integral Equation → Boundary Value Problem

Problem: Convert the following Fredholm integral equation into a boundary value problem:

$$y(x) = \lambda \int_{0}^{l} K(x,t) y(t) \, dt$$

where the kernel \( K(x,t) \) is defined piecewise as:

$$K(x,t) = \frac{t(l-x)}{l} \quad \text{for } 0 < t < x$$

$$K(x,t) = \frac{x(l-t)}{l} \quad \text{for } x < t < l$$

Reference: This kernel appeared in Example 2 of Part III, where we derived this integral equation from a boundary value problem.

Solution

The given integral equation is:

$$y(x) = \lambda \int_{0}^{l} K(x,t) y(t) \, dt \quad \ldots (1)$$

Since the kernel is piecewise-defined, we split the integral at \( x \):

$$y(x) = \lambda \left( \int_{0}^{x} \frac{(l-x)t}{l} y(t) \, dt + \int_{x}^{l} \frac{x(l-t)}{l} y(t) \, dt \right) \quad \ldots (2)$$

Step 1: First differentiation. Differentiate equation (2) with respect to \( x \). This requires careful application of the Leibniz rule since \( x \) appears both in the limits and inside the integrands:

$$y'(x) = -\frac{\lambda}{l} \int_{0}^x t \, y(t) \, dt + \frac{\lambda}{l} \int_{x}^l (l-t) y(t) \, dt \quad \ldots (3)$$

The boundary terms from Leibniz cancel due to the kernel’s continuity at \( x = t \).

Step 2: Second differentiation. Differentiate equation (3) with respect to \( x \):

$$y”(x) = -\frac{\lambda}{l} \cdot x \cdot y(x) – \frac{\lambda}{l} \cdot (l-x) \cdot y(x)$$

$$y”(x) = -\frac{\lambda}{l} y(x) \left[ x + (l-x) \right] = -\frac{\lambda}{l} y(x) \cdot l$$

$$y”(x) = -\lambda y(x)$$

Rearranging gives us the differential equation:

$$y”(x) + \lambda y(x) = 0 \quad \ldots (4)$$

Step 3: Extract boundary conditions. Substitute both integration limits into equation (2):

At \( x = 0 \): The first integral vanishes (limits 0 to 0), and in the second integral, the factor \( x = 0 \) makes the integrand zero:

$$y(0) = 0 \quad \ldots (5)$$

At \( x = l \): The second integral vanishes (limits \( l \) to \( l \)), and in the first integral, the factor \( (l-x) = 0 \) makes the integrand zero:

$$y(l) = 0 \quad \ldots (6)$$

Final Result: The ODE (4) with boundary conditions (5) and (6) constitutes the boundary value problem:

$$y” + \lambda y = 0, \quad y(0) = 0, \quad y(l) = 0 \quad \Box$$

Key Takeaways

After working through these conversions, here’s what you should remember:

  1. Differentiation is the reverse of integration—repeatedly differentiate the integral equation until the integral disappears.
  2. Volterra → IVP: Use the lower limit to extract initial conditions.
  3. Fredholm → BVP: Use both limits to extract boundary conditions.
  4. The Leibniz rule is essential when the variable appears both in the limits and under the integral sign.
  5. Piecewise kernels require splitting the integral and careful bookkeeping during differentiation.

Frequently Asked Questions

Why convert integral equations back to differential equations?

Sometimes differential equations are easier to solve using established methods like characteristic equations or variation of parameters. Converting back also helps verify that your original transformation was correct—if you can recover the starting ODE and its conditions, you’ve validated your work.

What is the Leibniz rule and why is it important here?

The Leibniz integral rule tells you how to differentiate an integral when the variable of differentiation appears in the limits, inside the integrand, or both. The general form is: d/dx ∫_{a(x)}^{b(x)} f(x,t) dt = f(x,b(x))·b'(x) − f(x,a(x))·a'(x) + ∫_{a(x)}^{b(x)} ∂f/∂x dt. Without this rule, you cannot correctly differentiate Volterra or Fredholm integral equations.

How do I know when to stop differentiating?

Stop when the integral term completely disappears and you’re left with a pure differential equation. For second-order ODEs, this typically requires two differentiations. The number of differentiations needed corresponds to the order of the original differential equation.

What is the difference between Volterra and Fredholm integral equations?

Volterra integral equations have variable upper limits (like ∫₀ˣ), while Fredholm integral equations have fixed limits (like ∫₀ˡ). This distinction determines whether the resulting ODE is an initial value problem or a boundary value problem.

Why do Volterra equations produce initial value problems?

Volterra equations have a variable upper limit and a fixed lower limit. When you substitute the lower limit into the integral equation and its derivatives, all integrals evaluate to zero—giving you conditions at a single point (the initial value). This is characteristic of IVPs.

Why do Fredholm equations produce boundary value problems?

Fredholm equations have fixed limits at both ends. Substituting each limit into the equation gives you conditions at two separate points—the boundaries. This naturally produces a BVP with conditions specified at both endpoints of the interval.

What is a piecewise kernel and how do I handle it?

A piecewise kernel K(x,t) has different formulas depending on whether t x. To handle it, split the integral at x into two parts: one from the lower limit to x, and another from x to the upper limit. Apply the appropriate kernel formula to each part before differentiating.

What role does the parameter λ play in the Fredholm equation?

The parameter λ (lambda) is called the eigenvalue parameter. It appears in eigenvalue problems where non-trivial solutions exist only for specific values of λ. In the boundary value problem y” + λy = 0 with y(0) = y(l) = 0, only certain values of λ produce non-zero solutions (the eigenfunctions).

Can every integral equation be converted to a differential equation?

Not always. The conversion works when the kernel and the integral structure allow differentiation to eliminate the integral entirely. Some integral equations, particularly those with singular kernels or certain non-separable forms, may not convert cleanly to ODEs. In such cases, direct methods for integral equations become necessary.

What is the Fundamental Theorem of Calculus and how is it used here?

The Fundamental Theorem of Calculus states that d/dx ∫_{a}^{x} f(t) dt = f(x). This is a special case of the Leibniz rule where the integrand doesn’t depend on x. It’s used in the final differentiation step to eliminate the remaining integral and obtain the differential equation.