Given a bounded function f(x) on a closed interval [a,b], partition [a,b] into n subintervals [x0,x1],[x1,x2],…,[xn−1,xn] with a=x0<x1<⋯<xn=b. In each subinterval [xi−1,xi] pick any point ξi (with xi−1≤ξi≤xi) and form the Riemann sum
∑i=1nf(ξi)(xi−xi−1).
As n→∞ in such a way that the width of the widest subinterval max(xi−xi−1)→0, this sum tends to a single finite number A (when f is continuous, or piecewise continuous). That limit A is the definite integral (or Riemann integral) of f on [a,b], written ∫abf(x)dx. When a=b, ∫aaf(x)dx=0.
Three standard choices of ξi, all giving the same limit for a continuous f:
- Left-end rule: ξi=xi−1, so ∫abf(x)dx=limn→∞∑i=1nf(xi−1)(xi−xi−1).
- Right-end rule: ξi=xi, so ∫abf(x)dx=limn→∞∑i=1nf(xi)(xi−xi−1).
- Mid-point rule: ξi=21(xi−1+xi), so ∫abf(x)dx=limn→∞∑i=1nf(2xi−1+xi)(xi−xi−1).
On a finite partition (before the limit is taken), each rule only gives an approximate value of the integral — this is exactly how Exercise 9.1's five-point partitions are used.
Closed-form limit formula. Dividing [a,b] into n equal subintervals of width h=nb−a, so xi=a+ih, and using the right-end rule gives the standard working formula
∫abf(x)dx=limn→∞nb−a∑r=1nf(a+n(b−a)r). …