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Plot of the Barnes G function G(z) in the complex plane from -2-2i to 2+2i with colors created with Mathematica 13.1 function ComplexPlot3D
Plot of the Barnes G aka double gamma function G(z) in the complex plane from -2-2i to 2+2i with colors created with Mathematica 13.1 function ComplexPlot3D
The Barnes G function along part of the real axis

In mathematics, the Barnes G-function G(z) is a function that is an extension of superfactorials to the complex numbers. It is related to the gamma function, the K-function and the Glaisher–Kinkelin constant, and was named after mathematician Ernest William Barnes.[1] It can be written in terms of the double gamma function.

Formally, the Barnes G-function is defined in the following Weierstrass product form:

G(1+z)=(2π)z/2exp(z+z2(1+γ)2)k=1{(1+zk)kexp(z22kz)}

where γ is the Euler–Mascheroni constant, exp(x) = ex is the exponential function, and Π denotes multiplication (capital pi notation).

The integral representation, which may be deduced from the relation to the double gamma function, is

logG(1+z)=z2log(2π)+0dtt[1ezt4sinh2t2+z22etzt]

As an entire function, G is of order two, and of infinite type. This can be deduced from the asymptotic expansion given below.

Functional equation and integer arguments

The Barnes G-function satisfies the functional equation

G(z+1)=Γ(z)G(z)

with normalisation G(1) = 1. Note the similarity between the functional equation of the Barnes G-function and that of the Euler gamma function:

Γ(z+1)=zΓ(z).

The functional equation implies that G takes the following values at integer arguments:

G(n)={0if n=0,1,2,i=0n2i!if n=1,2,

(in particular, G(0)=0,G(1)=1) and thus

G(n)=(Γ(n))n1K(n)

where Γ(x) denotes the gamma function and K denotes the K-function. The functional equation uniquely defines the Barnes G-function if the convexity condition,

(x1)d3dx3log(G(x))0

is added.[2] Additionally, the Barnes G-function satisfies the duplication formula,[3]

G(x)G(x+12)2G(x+1)=e14A322x2+3x1112πx12G(2x),

where A is the Glaisher–Kinkelin constant.

Characterisation

Similar to the Bohr–Mollerup theorem for the gamma function, for a constant c>0, we have for f(x)=cG(x)[4]

f(x+1)=Γ(x)f(x)

and for x>0

f(x+n)Γ(x)nn(x2)f(n)

as n.

Reflection formula

The difference equation for the G-function, in conjunction with the functional equation for the gamma function, can be used to obtain the following reflection formula for the Barnes G-function (originally proved by Hermann Kinkelin):

logG(1z)=logG(1+z)zlog2π+0zπxcotπxdx.

The log-tangent integral on the right-hand side can be evaluated in terms of the Clausen function (of order 2), as is shown below:

2πlog(G(1z)G(1+z))=2πzlog(sinπzπ)+Cl2(2πz)

The proof of this result hinges on the following evaluation of the cotangent integral: introducing the notation Lc(z) for the log-cotangent integral, and using the fact that (d/dx)log(sinπx)=πcotπx, an integration by parts gives

Lc(z)=0zπxcotπxdx=zlog(sinπz)0zlog(sinπx)dx=zlog(sinπz)0z[log(2sinπx)log2]dx=zlog(2sinπz)0zlog(2sinπx)dx.

Performing the integral substitution y=2πxdx=dy/(2π) gives

zlog(2sinπz)12π02πzlog(2siny2)dy.

The Clausen function – of second order – has the integral representation

Cl2(θ)=0θlog|2sinx2|dx.

However, within the interval 0<θ<2π, the absolute value sign within the integrand can be omitted, since within the range the 'half-sine' function in the integral is strictly positive, and strictly non-zero. Comparing this definition with the result above for the logtangent integral, the following relation clearly holds:

Lc(z)=zlog(2sinπz)+12πCl2(2πz).

Thus, after a slight rearrangement of terms, the proof is complete:

2πlog(G(1z)G(1+z))=2πzlog(sinπzπ)+Cl2(2πz).

Using the relation G(1+z)=Γ(z)G(z) and dividing the reflection formula by a factor of 2π gives the equivalent form:

log(G(1z)G(z))=zlog(sinπzπ)+logΓ(z)+12πCl2(2πz)

Adamchik (2003) has given an equivalent form of the reflection formula, but with a different proof.[5]

Replacing z with Template:Sfrac − z in the previous reflection formula gives, after some simplification, the equivalent formula shown below (involving Bernoulli polynomials):

log(G(12+z)G(12z))=logΓ(12z)+B1(z)log2π+12log2+π0zB1(x)tanπxdx

Taylor series expansion

By Taylor's theorem, and considering the logarithmic derivatives of the Barnes function, the following series expansion can be obtained:

logG(1+z)=z2log2π(z+(1+γ)z22)+k=2(1)kζ(k)k+1zk+1.

It is valid for 0<z<1. Here, ζ(x) is the Riemann zeta function:

ζ(s)=n=11ns.

Exponentiating both sides of the Taylor expansion gives:

G(1+z)=exp[z2log2π(z+(1+γ)z22)+k=2(1)kζ(k)k+1zk+1]=(2π)z/2exp[z+(1+γ)z22]exp[k=2(1)kζ(k)k+1zk+1].

Comparing this with the Weierstrass product form of the Barnes function gives the following relation:

exp[k=2(1)kζ(k)k+1zk+1]=k=1{(1+zk)kexp(z22kz)}

Multiplication formula

Like the gamma function, the G-function also has a multiplication formula:[6]

G(nz)=K(n)nn2z2/2nz(2π)n2n2zi=0n1j=0n1G(z+i+jn)

where K(n) is a constant given by:

K(n)=e(n21)ζ(1)n512(2π)(n1)/2=(Ae112)n21n512(2π)(n1)/2.

Here ζ is the derivative of the Riemann zeta function and A is the Glaisher–Kinkelin constant.

Absolute value

It holds true that G(z)=G(z), thus |G(z)|2=G(z)G(z). From this relation and by the above presented Weierstrass product form one can show that

|G(x+iy)|=|G(x)|exp(y21+γ2)1+y2x2k=1(1+y2(x+k)2)k+1exp(y2k).

This relation is valid for arbitrary x{0,1,2,}, and y. If x=0, then the below formula is valid instead:

|G(iy)|=yexp(y21+γ2)k=1(1+y2k2)k+1exp(y2k)

for arbitrary real y.

Asymptotic expansion

The logarithm of G(z + 1) has the following asymptotic expansion, as established by Barnes:

logG(z+1)=z22logz3z24+z2log2π112logz+(112logA)+k=1NB2k+24k(k+1)z2k+O(1z2N+2).

Here the Bk are the Bernoulli numbers and A is the Glaisher–Kinkelin constant. (Note that somewhat confusingly at the time of Barnes [7] the Bernoulli number B2k would have been written as (1)k+1Bk, but this convention is no longer current.) This expansion is valid for z in any sector not containing the negative real axis with |z| large.

Relation to the log-gamma integral

The parametric log-gamma can be evaluated in terms of the Barnes G-function:[5]

0zlogΓ(x)dx=z(1z)2+z2log2π+zlogΓ(z)logG(1+z)

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The proof is somewhat indirect, and involves first considering the logarithmic difference of the gamma function and Barnes G-function:

zlogΓ(z)logG(1+z)

where

1Γ(z)=zeγzk=1{(1+zk)ez/k}

and γ is the Euler–Mascheroni constant.

Taking the logarithm of the Weierstrass product forms of the Barnes G-function and gamma function gives:

zlogΓ(z)logG(1+z)=zlog(1Γ(z))logG(1+z)=z[logz+γz+k=1{log(1+zk)zk}][z2log2πz2z22z2γ2+k=1{klog(1+zk)+z22kz}]

A little simplification and re-ordering of terms gives the series expansion:

k=1{(k+z)log(1+zk)z22kz}=zlogzz2log2π+z2+z22z2γ2zlogΓ(z)+logG(1+z)

Finally, take the logarithm of the Weierstrass product form of the gamma function, and integrate over the interval [0,z] to obtain:

0zlogΓ(x)dx=0zlog(1Γ(x))dx=(zlogzz)z2γ2k=1{(k+z)log(1+zk)z22kz}

Equating the two evaluations completes the proof:

0zlogΓ(x)dx=z(1z)2+z2log2π+zlogΓ(z)logG(1+z)

And since G(1+z)=Γ(z)G(z) then,

0zlogΓ(x)dx=z(1z)2+z2log2π(1z)logΓ(z)logG(z).

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References

  1. E. W. Barnes, "The theory of the G-function", Quarterly Journ. Pure and Appl. Math. 31 (1900), 264–314.
  2. M. F. Vignéras, L'équation fonctionelle de la fonction zêta de Selberg du groupe mudulaire SL(2,), Astérisque 61, 235–249 (1979).
  3. Template:Cite journal
  4. Template:Cite book
  5. 5.0 5.1 Template:Cite arXiv
  6. I. Vardi, Determinants of Laplacians and multiple gamma functions, SIAM J. Math. Anal. 19, 493–507 (1988).
  7. E. T. Whittaker and G. N. Watson, "A Course of Modern Analysis", CUP.