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

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

For example, the function is defined on the interval

with the limits of integration being and .[1]

Integration by Substitution (U-Substitution) edit

In Integration by substitution, the limits of integration will change due to the new function being integrated. With the function that is being derived,   and   are solved for  . In general,

 
where   and  . Thus,   and   will be solved in terms of  ; the lower bound is   and the upper bound is  .

For example,

 

where   and  . Thus,   and  . Hence, the new limits of integration are   and  .[2]

The same applies for other substitutions.

Improper integrals edit

Limits of integration can also be defined for improper integrals, with the limits of integration of both

 
and
 
again being a and b. For an improper integral
 
or
 
the limits of integration are a and ∞, or −∞ and b, respectively.[3]

Definite Integrals edit

If  , then[4]

 

See also edit

References edit

  1. ^ "31.5 Setting up Correct Limits of Integration". math.mit.edu. Retrieved 2019-12-02.
  2. ^ "𝘶-substitution". Khan Academy. Retrieved 2019-12-02.
  3. ^ "Calculus II - Improper Integrals". tutorial.math.lamar.edu. Retrieved 2019-12-02.
  4. ^ Weisstein, Eric W. "Definite Integral". mathworld.wolfram.com. Retrieved 2019-12-02.