Limits of integration

From HandWiki
Short description: Upper and lower limits applied in definite integration

In calculus and mathematical analysis the limits of integration (or bounds of integration) of the integral abf(x)dx

of a Riemann integrable function f defined on a closed and bounded interval are the real numbers a and b, in which a is called the lower limit and b the upper limit. The region that is bounded can be seen as the area inside a and b.

For example, the function f(x)=x3 is defined on the interval [2,4] 24x3dx with the limits of integration being 2 and 4.[1]

Integration by Substitution (U-Substitution)

In Integration by substitution, the limits of integration will change due to the new function being integrated. With the function that is being derived, a and b are solved for f(u). In general, abf(g(x))g(x) dx where u=g(x) and du=g(x) dx. Thus, a and b will be solved in terms of u; the lower bound is g(a) and the upper bound is g(b).

For example, 022xcos(x2)dx=04cos(u)du

where u=x2 and du=2xdx. Thus, f(0)=02=0 and f(2)=22=4. Hence, the new limits of integration are 0 and 4.[2]

The same applies for other substitutions.

Improper integrals

Limits of integration can also be defined for improper integrals, with the limits of integration of both limza+zbf(x)dx and limzbazf(x)dx again being a and b. For an improper integral af(x)dx or bf(x)dx the limits of integration are a and ∞, or −∞ and b, respectively.[3]

Definite Integrals

If c(a,b), then[4] abf(x) dx=acf(x) dx +cbf(x) dx.

See also

  • Integral
  • Riemann integration
  • Definite integral

References