Riemann Sum Calculator

Approximate definite integrals using left, right, midpoint, and trapezoidal rules. Visualize rectangles and see exact integral with error analysis.

Riemann Sum:ab f(x) dx ≈ Σ f(xk*) Δx ,   Δx = (b-a)/n

Choose method: left, right, midpoint, or trapezoid.

Enter a function of x. Use ^ for exponent, * for multiplication, sin(), cos(), exp(), log(), sqrt().
sin(x)
e⁻ˣ
4 - x²
√(4-x²)
1/(1+x²)
1 to 200
Calculating...

Understanding Riemann Sums

Riemann sums are a family of methods to approximate the definite integral ∫ab f(x) dx. The interval [a, b] is divided into n subintervals of equal width Δx = (b−a)/n. On each subinterval [xk−1, xk], we choose a sample point xk* and form a rectangle (or trapezoid) with height f(xk*). The sum of the areas approximates the integral.

General formula:

ab f(x) dx ≈ Δx · [f(x1*) + f(x2*) + … + f(xn*)]

where xk* lies in the k‑th subinterval.

Common Rules (Sample Point Choices)

MethodSample point xk*Formula (Δx = (b−a)/n)Geometric interpretation
Left Riemann sumLeft endpoint: a + (k−1)ΔxΔx·[f(a) + f(a+Δx) + … + f(b−Δx)]Height of each rectangle is the left‑side value; underestimates increasing functions, overestimates decreasing functions.
Right Riemann sumRight endpoint: a + kΔxΔx·[f(a+Δx) + f(a+2Δx) + … + f(b)]Height is right‑side value; overestimates increasing functions, underestimates decreasing functions.
Midpoint ruleMidpoint: a + (k−½)ΔxΔx·[f(a+½Δx) + f(a+1½Δx) + … + f(b−½Δx)]Height at subinterval midpoints; often more accurate (error O(Δx²)).
Trapezoidal rule(Δx/2)·[f(a) + 2f(a+Δx) + 2f(a+2Δx) + … + f(b)]Uses trapezoids instead of rectangles; averages left and right sums, also O(Δx²) error.

Error Analysis & Convergence

For a continuous function, as n → ∞ (Δx → 0), all Riemann sums converge to the true integral. The speed of convergence depends on the method:

  • Left/Right sums: error ≈ O(Δx) (first‑order). Doubling n roughly halves the error.
  • Midpoint & Trapezoidal rules: error ≈ O(Δx²) (second‑order). Doubling n reduces error by a factor of about 4.

More precisely, if f is twice continuously differentiable, the midpoint rule error is about −(b−a)Δx² f''(ξ)/24, and trapezoidal error is about −(b−a)Δx² f''(ξ)/12 for some ξ in (a,b). Hence midpoint is often slightly better.

Why Use Riemann Sums?

  • Numerical integration when an antiderivative is difficult or impossible (e.g., f(x) = e−x²).
  • Foundation of the definite integral – the limit of Riemann sums defines the integral.
  • Applications in physics (work, distance, center of mass), probability (expected values), economics (consumer surplus), and engineering (average values).

Calculator features:

  • Symbolic parsing via nerdamer, safe evaluation with math.js
  • Exact integral computed when possible using symbolic integration (fallback to high‑precision adaptive Simpson)
  • Interactive graph with rectangles/trapezoids drawn dynamically
  • Adjustable precision and up to 200 subintervals for smooth visualization
  • Supports mathematical constants like π and e in limits and functions

Frequently Asked Questions

For smooth functions, the midpoint and trapezoidal rules are generally more accurate (error ~ 1/n²) than left/right (error ~ 1/n). The trapezoidal rule often performs well, but midpoint can be slightly better for some functions. The calculator shows the exact error to help you compare.

The calculator evaluates only at the sample points. If a sample point lies outside the domain (e.g., sqrt(x) with x negative), you'll get an error. Ensure your interval is within the domain.

First we try symbolic integration with nerdamer. If that fails (or the result is not elementary), we compute a highly accurate approximation using adaptive Simpson quadrature (error ~ 1e‑10) to serve as the "exact" reference.

This calculator is designed for proper integrals on finite intervals. For improper integrals, you would need to truncate the interval appropriately.