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19 Elliptic IntegralsSymmetric Integrals

§19.16 Definitions

Contents
  1. §19.16(i) Symmetric Integrals
  2. §19.16(ii) R−a⁡(𝐛;𝐳)
  3. §19.16(iii) Various Cases of R−a⁡(𝐛;𝐳)

§19.16(i) Symmetric Integrals

19.16.1 RF⁡(x,y,z)=12⁢∫0∞dts⁡(t),
19.16.2 RJ⁡(x,y,z,p)=32⁢∫0∞dts⁡(t)⁢(t+p),
19.16.2_5 RG⁡(x,y,z)=14⁢∫0∞1s⁡(t)⁢(xt+x+yt+y+zt+z)⁢t⁢dt.
19.16.3 Moved to (19.23.6_5).

where p (≠0) is a real or complex constant, and

19.16.4 s⁡(t)=t+x⁢t+y⁢t+z.

In (19.16.1)–(19.16.2_5), x,y,z∈ℂ∖(−∞,0] except that one or more of x,y,z may be 0 when the corresponding integral converges. In (19.16.2) the Cauchy principal value is taken when p is real and negative. See also (19.20.14). It should be noted that the integrals (19.16.1)–(19.16.2_5) have been normalized so that RF⁡(1,1,1)=RJ⁡(1,1,1,1)=RG⁡(1,1,1)=1.

A fourth integral that is symmetric in only two variables is defined by

19.16.5 RD⁡(x,y,z)=RJ⁡(x,y,z,z)=32⁢∫0∞dts⁡(t)⁢(t+z),

with the same conditions on x, y, z as for (19.16.1), but now z≠0.

Just as the elementary function RC⁡(x,y) (§19.2(iv)) is the degenerate case

and RD is a degenerate case of RJ, so is RJ a degenerate case of the hyperelliptic integral,

19.16.7 32⁢∫0∞dt∏j=15t+xj.

§19.16(ii) R−a⁡(𝐛;𝐳)

All elliptic integrals of the form (19.2.3) and many multiple integrals, including (19.23.6) and (19.23.6_5), are special cases of a multivariate hypergeometric function

19.16.8 R−a⁡(𝐛;𝐳)=R−a⁡(b1,…,bn;z1,…,zn),

which is homogeneous and of degree −a in the z’s, and unchanged when the same permutation is applied to both sets of subscripts 1,…,n. Thus R−a⁡(𝐛;𝐳) is symmetric in the variables zj and zℓ if the parameters bj and bℓ are equal. The R-function is often used to make a unified statement of a property of several elliptic integrals. Before 1969 R−a⁡(𝐛;𝐳) was denoted by R⁡(a;𝐛;𝐳).

19.16.9 R−a⁡(𝐛;𝐳)=1B⁡(a,a′)⁢∫0∞ta′−1⁢∏j=1n(t+zj)−bj⁢dt=1B⁡(a,a′)⁢∫0∞ta−1⁢∏j=1n(1+t⁢zj)−bj⁢dt,
b1+⋯+bn>a>0, bj∈ℝ, zj∈ℂ∖(−∞,0],

where B⁡(x,y) is the beta function (§5.12) and

19.16.10 a′=−a+∑j=1nbj.
19.16.11 R−a⁡(𝐛;λ⁢𝐳) =λ−a⁢R−a⁡(𝐛;𝐳),
R−a⁡(𝐛;x⁢𝟏) =x−a,
𝟏=(1,…,1).

When n=4 a useful version of (19.16.9) is given by

19.16.12 R−a⁡(b1,…,b4;c−1,c−k2,c,c−α2)=2⁢(sin2⁡ϕ)1−a′B⁡(a,a′)⁢∫0ϕ(sin⁡θ)2⁢a−1⁢(sin2⁡ϕ−sin2⁡θ)a′−1⁢(cos⁡θ)1−2⁢b1×(1−k2⁢sin2⁡θ)−b2⁢(1−α2⁢sin2⁡θ)−b4⁢dθ,

where

19.16.13 c =csc2⁡ϕ;
a,a′ >0;
b3 =a+a′−b1−b2−b4.

For generalizations and further information, especially representation of the R-function as a Dirichlet average, see Carlson (1977b).

§19.16(iii) Various Cases of R−a⁡(𝐛;𝐳)

R−a⁡(𝐛;𝐳) is an elliptic integral iff the z’s are distinct and exactly four of the parameters a,a′,b1,…,bn are half-odd-integers, the rest are integers, and none of a, a′, a+a′ is zero or a negative integer. The only cases that are integrals of the first kind are the four in which each of a and a′ is either 12 or 1 and each bj is 12. The only cases that are integrals of the third kind are those in which at least one bj is a positive integer. All other elliptic cases are integrals of the second kind.

19.16.14 RF⁡(x,y,z) =R−12⁡(12,12,12;x,y,z),
19.16.15 RD⁡(x,y,z) =R−32⁡(12,12,32;x,y,z),
19.16.16 RJ⁡(x,y,z,p) =R−32⁡(12,12,12,1;x,y,z,p),
19.16.17 RG⁡(x,y,z) =R12⁡(12,12,12;x,y,z),
19.16.18 RC⁡(x,y) =R−12⁡(12,1;x,y).

(Note that RC⁡(x,y) is not an elliptic integral.)

When one variable is 0 without destroying convergence, any one of (19.16.14)–(19.16.17) is said to be complete and can be written as an R-function with one less variable:

19.16.19 R−a⁡(b1,…,bn;0,z2,…,zn)=B⁡(a,a′−b1)B⁡(a,a′)⁢R−a⁡(b2,…,bn;z2,…,zn),
a+a′>0, a′>b1.

Thus

19.16.20 RF⁡(0,y,z) =12⁢π⁢R−12⁡(12,12;y,z),
19.16.21 RD⁡(0,y,z) =34⁢π⁢R−32⁡(12,32;y,z),
19.16.22 RJ⁡(0,y,z,p) =34⁢π⁢R−32⁡(12,12,1;y,z,p),
19.16.23 RG⁡(0,y,z) =14⁢π⁢R12⁡(12,12;y,z)=14⁢π⁢z⁢R−12⁡(−12,32;y,z).

The last R-function has a=a′=12.

Each of the four complete integrals (19.16.20)–(19.16.23) can be integrated to recover the incomplete integral:

19.16.24 R−a⁡(𝐛;𝐳)=z1a′−b1B⁡(b1,a′−b1)⁢∫0∞tb1−1⁢(t+z1)−a′⁢R−a⁡(𝐛;0,t+z2,…,t+zn)⁢dt,
a′>b1, a+a′>b1>0.