Accumulating Under a Curve
The definite integral is the second face of integration: it measures the accumulated area between the curve and the -axis, from to . Where the derivative was about instantaneous rates, the definite integral is about totals — the total distance from a velocity, the total accumulated from a rate.
The definition is a limit of Riemann sums: slice the interval into thin rectangles of width , each with height given by the curve. The sum of rectangle areas approximates the region, and as the slices get thinner () the approximation becomes exact: This is why the integral sign is an elongated "S" for "sum."
Two important features:
- Signed area. Where is below the axis (negative), its contribution is negative. The definite integral gives net signed area, so regions below the axis subtract.
- A number, not a function. Unlike the indefinite integral (a family of functions with ), the definite integral is a single number — there is no constant of integration.
Numerically, Riemann sums (and refinements like the trapezoidal rule and Simpson's rule) are exactly how computers evaluate integrals that have no closed form — a cornerstone of scientific computing.
Common pitfall: treating the definite integral as always giving the geometric (positive) area, and confusing it with the indefinite integral. The definite integral is signed — area below the axis counts as negative, so a symmetric curve can integrate to zero even though it encloses real area. And a definite integral is a single number (no ), unlike the indefinite integral, which is a family of functions.
The area under a curve approximated by rectangles that grow thinner and more numerous, the accent shaded region converging to the exact integral, with a below-axis lobe shaded to subtract.