Numerical Integration Calculator

Trapezoidal and Simpson approximations with comparison to exact integrals

Parameters

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Show Trail

Controls

xⓘ

Calculated Values

Trapezoid:
0.34;0.34;
Simpson:
0.33;0.33;
Exact:
0.33;0.33;
Trap error %:
0.50;0.50;%
Simpson error %:
0.00;0.00;%

Examples

∫₀¹ x² dx

Exact value 1/3 ≈ 0.333; n = 10.

  • Exact: 0.330.33
  • Trapezoid: 0.340.34

∫₀^π sin(x) dx

Exact value 2.

  • Exact: 2.002.00
  • Simpson: 2.002.00

Visualization

Numerical Integration in Physics

Many physical quantities are defined as integrals: work W = ∫F·dx, charge Q = ∫I·dt, flux Φ = ∫B·dA, and areas under experimental curves. When f(x) has no elementary antiderivative, numerical methods approximate the definite integral.

The trapezoidal rule replaces the function on each subinterval by a straight line. With n equal panels of width h = (b−a)/n, ∫ₐᵇ f ≈ (h/2)[f₀ + 2f₁ + … + 2fₙ₋₁ + fₙ]. Global error scales as O(h²) for smooth functions.

Simpson’s rule fits a parabola through each pair of panels, giving weights 1, 4, 2, 4, …, 4, 1. It requires an even number of intervals and achieves O(h⁴) error — often far more accurate than trapezoid for the same n.

Increasing n refines the approximation but costs computation. In labs, noisy data may need smoothing before integration; propagate uncertainties with Error Propagation when f(xᵢ) come from measurements.

Numerical integration links to ODE solvers: integrating v(t) gives position — the same idea behind Projectile Motion simulations. Monte Carlo integration is an alternative for high-dimensional integrals.

Key Concepts

  • Panel width h = (b − a) / n
  • Trapezoid: chord approximation, error ~ O(h²)
  • Simpson: parabolic arcs, error ~ O(h⁴)
  • More panels → better accuracy, diminishing returns
  • Compare to exact value to validate code or method

Real-World Applications

  • Work from tabulated force vs displacement
  • Charge from current vs time graph
  • Center of mass from density distribution
  • Probability from Maxwell-Boltzmann distribution

Explore Further

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  • 1D Wave Equation

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  • ODE Solver

    Euler and Runge-Kutta 4 methods for first-order ODEs with comparison to analytic solutions.

  • Monte Carlo Intro

    Estimate π and integrals by random sampling — introduction to stochastic computational physics.

  • Newton-Raphson

    Solve nonlinear equations f(x) = 0 with tangent-line iterations — fast when the guess is good.

Physics Equations

Trapezoid:
∫abf≈h2[f0+2∑i=1n−1fi+fn]\int_a^b f \approx \frac{h}{2}\left[f_0 + 2\sum_{i=1}^{n-1}f_i + f_n\right]
Simpson:
∫abf≈h3[f0+4f1+2f2+⋯+fn]\int_a^b f \approx \frac{h}{3}\left[f_0 + 4f_1 + 2f_2 + \cdots + f_n\right]

Step-by-Step Solution

See how the main results are calculated.

1

Step 1: Define the integral and interval

Identify integrand f(x), limits a and b, and number of subintervals n.

Equation:

∫01x2 dx\int_{0}^{1} x^2 \, dx

Result:

n=10,h=(b−a)/n=0.100000n = 10, h = (b-a)/n = 0.100000

Explanation:

Smaller h improves accuracy but increases computation.

2

Step 2: Analytic value (if known)

Evaluate the definite integral exactly for comparison.

Equation:

[x33]01=13−033\left[\frac{x^3}{3}\right]_{0}^{1} = \frac{1^3 - 0^3}{3}

Result:

Iexact=0.333333I_{\text{exact}} = 0.333333
3

Step 3: Trapezoidal rule setup

Approximate area under f by trapezoids on each subinterval.

Equation:

Itrap≈h2[f0+2∑i=1n−1fi+fn]I_{\text{trap}} \approx \frac{h}{2}\left[f_0 + 2\sum_{i=1}^{n-1} f_i + f_n\right]

Explanation:

Sample f at x_i = a + ih for i = 0, 1, …, 10.

4

Step 4: Evaluate trapezoidal sum

f(a) = 0.0000, f(b) = 1.0000

Calculation:

Itrap≈0.335000I_{\text{trap}} \approx 0.335000

Result:

Trapezoid ≈ 0.335000

Explanation:

Error vs exact: 0.167%

5

Step 5: Simpson’s rule (even n)

Using 10 subintervals with weights 1, 4, 2, 4, …, 1.

Equation:

ISimp≈h3[f0+4f1+2f2+⋯+fn]I_{\text{Simp}} \approx \frac{h}{3}\left[f_0 + 4f_1 + 2f_2 + \cdots + f_n\right]

Calculation:

ISimp≈0.333333I_{\text{Simp}} \approx 0.333333

Result:

Simpson ≈ 0.333333

Explanation:

Error vs exact: 0.000% — usually smaller than trapezoid.

6

Step 6: Compare methods

Assess convergence; double n and see if result changes acceptably.

Result:

Exact=0.333333,Trap=0.335000,Simpson=0.333333Exact = 0.333333, Trap = 0.335000, Simpson = 0.333333

Frequently Asked Questions (FAQ)

Why is Simpson often more accurate?

It fits parabolas through triplets of points, capturing curvature better than straight-line trapezoids.

What if n is odd for Simpson?

This calculator uses the next even n automatically so Simpson’s formula applies.

When does trapezoid fail badly?

Sharp peaks, discontinuities, or very coarse n — increase n or use adaptive methods in research code.

Practice MCQs

  1. Doubling n in the trapezoid rule typically:
  2. Simpson’s rule requires:
  3. ∫₀¹ x² dx equals:
  4. Trapezoid approximates f on each panel by:
  5. For smooth functions, Simpson error order is: