Limits of integration

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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 limz→a+∫zbf(x)dx and limz→b−∫azf(x)dx again being a and b. For an improper integral ∫a∞f(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