This page lists a variety of integrals that are highly useful in mathematical physics, along with their derivations. The latter are revealed by clicking the appropriate button.
using
in the fourth step. The function in the result is the Gauss hypergeometric function. The result is a finite polynomial if r is a positive integer.
Change the variable of integration and use the previous result:
Factor out the first term inside the binomial and use the previous result:
Given the general binomial expansion
the evaluation of the integral is
using
in the third step. The function in the result is the n-dimensional Lauricella hypergeometric function of n variables. The exponent m must be the same in all binomials in order to factor it out from the other parameters in the second step.
This is a special case of the previous result with summation over one index. Begin as above but stop at the second step:
For
this result is identical to setting
in the previous result.
This is a special case of the previous result. It is the Euler-type integral representation of a Lauricella triple hypergeometric function.
This is a special case of the previous result. It is the Euler-type integral representation of an Appell double hypergeometric function.
This is a special case of the previous result. It is the Euler-type integral representation of the Gauss hypergeometric function. Since this function is symmetric in its first two parameters, they can be interchanged on both sides of the relation.
Trigonometric Integrals
Change variable to
and use a binomial integral:
Change variable to
and proceed as before: sine is replaced with cosine, exponents are interchanged and the result has an additonal overall minus sign.
Given the relationship of the beta function to the gamma function and the former’s trigonometric representation,
the integral is trivial. Alternately given the Gauss summation formula
it can be evaluated from either of the previous two results:
When applied to the equivalence, the second term of this expression is zero on both sides due to the constant lower limit of integration. On the left-hand side of the quivalence, the third term is zero and the first merely removes one instance of integration:
On the right-hand side of the equivalence, the first term is zero because the integrand is zero at the upper limit of integration. The partial differentiation in the third term gives