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Barnes G-function
Barnes G-function
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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 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:[2]

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

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

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

Functional equation and integer arguments

[edit]

The Barnes G-function satisfies the functional equation

with normalization . Note the similarity between the functional equation of the Barnes G-function and that of the Euler gamma function:

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

In particular, and for , where is the superfactorial.

and thus

where denotes the gamma function and denotes the K-function. In general,for all complex .

The functional equation uniquely defines the Barnes G-function if the convexity condition,

is added.[3] Additionally, the Barnes G-function satisfies the duplication formula,[4]

,

where is the Glaisher–Kinkelin constant.

Characterisation

[edit]

Similar to the Bohr–Mollerup theorem for the gamma function, for a constant we have for [5]

and for

as .

Reflection formula

[edit]

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):

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:[2]

The proof of this result hinges on the following evaluation of the cotangent integral: introducing the notation for the log-cotangent integral, and using the fact that , an integration by parts gives

Performing the integral substitution gives

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

However, within the interval , 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:

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

Using the relation and dividing the reflection formula by a factor of gives the equivalent form:

Adamchik (2003) has given an equivalent form of the reflection formula, but with a different proof.[6]

Replacing with in the previous reflection formula gives, after some simplification, the equivalent formula shown below

(involving Bernoulli polynomials):

Taylor series expansion

[edit]

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

It is valid for . Here, is the Riemann zeta function:

Exponentiating both sides of the Taylor expansion gives:

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

Multiplication formula

[edit]

Like the gamma function, the G-function also has a multiplication formula:[7]

where is a constant given by:

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

Absolute value

[edit]

It holds true that , thus . From this relation and by the above presented Weierstrass product form one can show that

This relation is valid for arbitrary , and . If , then the below formula is valid instead:

for arbitrary real y.

Asymptotic expansion

[edit]

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

Here the are the Bernoulli numbers and is the Glaisher–Kinkelin constant. (Note that somewhat confusingly at the time of Barnes [8] the Bernoulli number would have been written as , but this convention is no longer current.) This expansion is valid for in any sector not containing the negative real axis with large.

Relation to the log-gamma integral

[edit]

The parametric log-gamma can be evaluated in terms of the Barnes G-function:[9]

Taking the logarithm of both sides introduces the analog of the Digamma function ,

where [2][1][10]

with Taylor series

References

[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
The Barnes G-function, denoted G(z)G(z), is an entire function on the complex plane that generalizes the Euler Gamma function Γ(z)\Gamma(z) as the second-order case of the multiple Gamma functions, often referred to as the double Gamma function. It satisfies the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) for (z)>0\Re(z) > 0, with the normalization G(1)=1G(1) = 1, and is uniquely determined by this relation along with its Weierstrass canonical product form:
G(z+1)=(2π)z/2e(1+γ)z2/2z/2k=1(1+zk)kez+z2/(2k),G(z+1) = (2\pi)^{z/2} \, e^{-(1+\gamma)z^2/2 - z/2} \prod_{k=1}^\infty \left(1 + \frac{z}{k}\right)^k e^{-z + z^2/(2k)},
where γ0.57721\gamma \approx 0.57721 is the Euler-Mascheroni constant. This function provides an analytic continuation of the product of factorials, defined for positive integers nn as G(n+1)=k=1n1k!G(n+1) = \prod_{k=1}^{n-1} k!, a close relative of the superfactorial (n)=k=1nk!\sf(n) = \prod_{k=1}^n k!, to the complex domain, and it arises naturally in the evaluation of infinite products and determinants in number theory.
Introduced by the Australian mathematician Ernest William Barnes in his 1899 paper "The theory of the G-function" in the Quarterly Journal of Mathematics, the Barnes G-function built upon earlier work by Glaisher and Kinkelin on multiple factorials and was further developed in Barnes's 1904 paper "On the theory of the multiple Gamma function" in the Transactions of the Cambridge Philosophical Society. Its asymptotic behavior is captured by a Stirling-type approximation:
logG(x+1)x22logx3x24+x2log(2π)+ζ(1)+O(logxx),\log G(x+1) \sim \frac{x^2}{2} \log x - \frac{3x^2}{4} + \frac{x}{2} \log(2\pi) + \zeta'(-1) + O\left(\frac{\log x}{x}\right),
which involves the Riemann zeta function derivative at -1 and connects to the Glaisher-Kinkelin constant A=e1/12ζ(1)1.282427A = e^{1/12 - \zeta'(-1)} \approx 1.282427, a fundamental constant in analytic number theory.
The function has zeros at the non-positive integers and its logarithmic derivative is related to the digamma function and the Hurwitz zeta function. Notable applications include the computation of Barnes multiple zeta functions, regularized determinants of Laplacians on spheres, and evaluations in statistical mechanics, such as the partition function of the Potts model. Further generalizations to higher-order multiple Gamma functions Gn(z)G_n(z) extend its utility in multivariate analysis and special function theory.

Definition and Basic Properties

Functional Equation and Normalization

The Barnes G-function G(z)G(z) is defined as an entire function of the complex variable zz satisfying the functional equation G(z+1)=Γ(z)G(z),G(z+1) = \Gamma(z) G(z), where Γ(z)\Gamma(z) denotes the Euler gamma function. This equation, introduced by Barnes in his study of multiple gamma functions, generalizes the defining recurrence of the gamma function itself, which obeys Γ(z+1)=zΓ(z)\Gamma(z+1) = z \Gamma(z) with the normalization Γ(1)=1\Gamma(1) = 1. To ensure uniqueness among entire functions satisfying the recurrence, the Barnes G-function is normalized by the condition G(1)=1G(1) = 1. For positive integers, the functional equation yields an iterative relation G(n+1)=Γ(n)G(n)G(n+1) = \Gamma(n) G(n). Starting from G(1)=1G(1) = 1 and using Γ(n)=(n1)!\Gamma(n) = (n-1)! for positive integers nn, repeated application produces the finite product form G(n+1)=k=1n1(k!),G(n+1) = \prod_{k=1}^{n-1} (k!), which aligns with the superfactorial interpretation of the G-function at integer arguments.

Values at Integers and Special Points

The Barnes G-function G(z)G(z) has zeros at all non-positive integers, that is, G(n)=0G(n) = 0 for every integer n0n \leq 0. This property arises from the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) combined with the poles of the gamma function Γ(z)\Gamma(z) at non-positive integers and the normalization G(1)=1G(1) = 1. For positive integers, the values are given explicitly by G(1)=1G(1) = 1 and, for n2n \geq 2, G(n)=k=1n2k!.G(n) = \prod_{k=1}^{n-2} k!. This finite product of factorials provides a direct computational method for integer arguments. Representative small values include:
  • G(2)=1G(2) = 1 (empty product),
  • G(3)=1!=1G(3) = 1! = 1,
  • G(4)=1!2!=2G(4) = 1! \cdot 2! = 2,
  • G(5)=1!2!3!=12G(5) = 1! \cdot 2! \cdot 3! = 12,
  • G(6)=1!2!3!4!=288G(6) = 1! \cdot 2! \cdot 3! \cdot 4! = 288.
These integer values connect the Barnes G-function to the superfactorial (n)\sf(n), defined as the product of the first nn factorials (n)=k=1nk!\sf(n) = \prod_{k=1}^n k!. The relation is (n)=n!G(n+1)/G(2)\sf(n) = n! \, G(n+1) / G(2); since G(2)=1G(2) = 1, this simplifies to (n)=n!G(n+1)\sf(n) = n! \, G(n+1). At the special half-integer point z=1/2z = 1/2, the value is G(12)=A3/2π1/4e1/821/24,G\left( \frac{1}{2} \right) = A^{-3/2} \, \pi^{-1/4} \, e^{1/8} \, 2^{1/24}, where AA is the Glaisher–Kinkelin constant, defined as A=exp(112ζ(1))1.2824271291A = \exp\left( \frac{1}{12} - \zeta'(-1) \right) \approx 1.2824271291 with ζ(s)\zeta(s) the Riemann zeta function; this constant emerges in asymptotic analyses involving products of factorials and multiple gamma functions.

Representations

Infinite Product Form

The Barnes G-function possesses a Weierstrass canonical product representation, which serves as its explicit form and enables analytic continuation throughout the complex plane. This representation is given by G(1+z)=(2π)z/2exp[12(z+(1+γ)z2)]k=1(1+zk)kexp(z+z22k),G(1 + z) = (2\pi)^{z/2} \exp\left[-\frac{1}{2}\left(z + (1 + \gamma)z^{2}\right)\right] \prod_{k=1}^{\infty} \left(1 + \frac{z}{k}\right)^{k} \exp\left(-z + \frac{z^{2}}{2k}\right), where γ\gamma denotes the Euler-Mascheroni constant. The infinite product converges uniformly on compact subsets of the complex plane, confirming that G(z)G(z) is an entire function of order 2. This product form arises from the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) through techniques such as Hadamard canonical factorization or regularization via multiple Hurwitz zeta functions, which handle the divergent aspects of the naive product over gamma functions. For positive integers nn, the values of the G-function connect to the hyperfactorial H(n)=k=1nkkH(n) = \prod_{k=1}^{n} k^{k} via the exact relation G(n+1)=(n!)nH(n)G(n+1) = \frac{(n!)^n}{H(n)}.

Logarithmic Representations

The logarithmic representations of the Barnes G-function provide expressions for lnG(z)\ln G(z), which are essential for numerical computations, asymptotic approximations, and analytic continuations in the complex plane, as the function itself grows rapidly. A key logarithmic form arises from the infinite product representation of G(z+1)G(z+1), yielding lnG(z+1)=z2ln(2π)12z(z+1)γ2z2+k=1[kln(1+zk)z+z22k],\ln G(z+1) = \frac{z}{2} \ln (2\pi) - \frac{1}{2} z (z+1) - \frac{\gamma}{2} z^2 + \sum_{k=1}^\infty \left[ k \ln \left(1 + \frac{z}{k}\right) - z + \frac{z^2}{2 k} \right], where γ\gamma is the Euler-Mascheroni constant. This series converges for complex zz avoiding the branch cut along the negative real axis and is regularized by the γz2/2\gamma z^2 / 2 term to handle divergent contributions from the harmonic series in the expansion. For practical evaluation, the sum is truncated at a large kk where terms become negligible, making it suitable for moderate-sized z|z|. An alternative integral representation connects lnG(z+1)\ln G(z+1) directly to the logarithm of the gamma function: lnG(z+1)=zlnΓ(z+1)0zlnΓ(t+1)dt+12zln(2π)12z(z+1).\ln G(z+1) = z \ln \Gamma(z+1) - \int_0^z \ln \Gamma(t+1) \, dt + \frac{1}{2} z \ln (2\pi) - \frac{1}{2} z (z+1). Here, the principal branches of the logarithms are taken along the positive real axis and analytically continued elsewhere; the integral can be computed numerically using quadrature methods, particularly when zz is real and positive. This form highlights the cumulative nature of the G-function as a "double gamma" and aids in deriving further properties. The logarithmic derivative, ddzlnG(z)=G(z)G(z)\frac{d}{dz} \ln G(z) = \frac{G'(z)}{G(z)}, admits a closed form involving the digamma function ψ(z)\psi(z): G(z)G(z)=12ln(2π)+12z+(z1)ψ(z).\frac{G'(z)}{G(z)} = \frac{1}{2} \ln (2\pi) + \frac{1}{2} - z + (z-1) \psi(z). This relation follows from differentiating the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) and integrating the resulting recurrence for the derivative, providing an efficient way to compute derivatives without evaluating G(z)G(z) separately. It also satisfies the recurrence G(z+1)G(z+1)=G(z)G(z)+ψ(z)\frac{G'(z+1)}{G(z+1)} = \frac{G'(z)}{G(z)} + \psi(z). These logarithmic forms enable accurate computation of lnG(z)\ln G(z) for complex zz. For Re(z)3/2\operatorname{Re}(z) \geq 3/2, high-precision approximations use Padé approximants to auxiliary functions in the integral representation, achieving relative errors below 103010^{-30}; extension to the full complex plane employs the reflection formula to map points outside this region. Such methods are implemented in numerical libraries for applications in special function evaluations and random matrix theory.

Identities

Reflection Formula

The reflection formula for the Barnes G-function relates its values at complementary points in a manner analogous to the reflection formula for the gamma function. It is given by logG(1z)=logG(z+1)zlog(2π)+0zπxcot(πx)dx,\log G(1 - z) = \log G(z + 1) - z \log (2\pi) + \int_{0}^{z} \pi x \cot(\pi x) \, dx, where the integral represents the log-tangent integral and the equation holds in the complex plane away from the branch cut along the negative real axis. This identity is derived from the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) combined with the reflection formula for the digamma function, ψ(1z)=ψ(z)+πcot(πz)\psi(1 - z) = \psi(z) + \pi \cot(\pi z). The logarithmic derivative of the G-function admits an expression as G(z)/G(z)=k=0[ψ(z+k+1)ψ(k+1)]G'(z)/G(z) = \sum_{k=0}^{\infty} [\psi(z + k + 1) - \psi(k + 1)], allowing the reflection property of the digamma terms to be applied term by term to obtain the integral form after integration. The formula facilitates the evaluation of G(z)G(z) at non-integer points, particularly those with negative or small real part, by reflecting them to the right half-plane where the infinite product representation converges more rapidly or asymptotic approximations are applicable, often in conjunction with the functional equation to shift arguments iteratively. In the special case z=1/2z = 1/2, the reflection formula simplifies and yields G(1/2)=21/24e1/8A3/2π1/4G(1/2) = 2^{1/24} e^{1/8} A^{-3/2} \pi^{-1/4}, where AA is the Glaisher–Kinkelin constant defined by the limit A=limn(2π)n/2nn2/2+n/2+1/12e3n2/4G(n+1),A = \lim_{n \to \infty} \frac{(2\pi)^{n/2} n^{n^2/2 + n/2 + 1/12} e^{-3n^2/4}}{G(n+1)}, linking the value to this fundamental constant in number theory and special functions.

Multiplication Formula

The multiplication theorem for the Barnes G-function generalizes the Gauss multiplication formula for the Gamma function to this higher-order analog, providing a relation for G at multiples of the argument in terms of products of G at shifted arguments. For a positive integer nn, the formula follows from repeated application of the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) combined with the Gauss multiplication theorem for the Gamma function Γ(nz)=(2π)(n1)/2nnz1/2Γ(z)k=1n1Γ(z+kn)\Gamma(n z) = (2\pi)^{(n-1)/2} n^{n z - 1/2} \Gamma(z) \prod_{k=1}^{n-1} \Gamma\left(z + \frac{k}{n}\right). This case is particularly useful for computations and can be derived directly via the Hurwitz zeta function representation of the logarithmic derivative. The multiplication formula facilitates relating values of the G-function at rational multiples of the argument, enabling evaluations at fractional points from known integer values and aiding in the analytic continuation across the complex plane. For instance, it allows expressing G at points like z/3z/3 or z/4z/4 in terms of products involving G(z) and shifted terms, which is valuable in number theory applications such as Barnes multiple zeta functions.

Expansions

Taylor Series Expansion

The Taylor series expansion for the logarithm of the Barnes G-function provides a useful representation for computations near the origin. Specifically, the power series for lnG(z+1)\ln G(z+1) around z=0z = 0 is given by lnG(z+1)=12[ln(2π)1]z1+γ2z2+n=3(1)n1ζ(n1)nzn,\ln G(z+1) = \frac{1}{2} \left[ \ln(2\pi) - 1 \right] z - \frac{1 + \gamma}{2} z^2 + \sum_{n=3}^{\infty} (-1)^{n-1} \frac{\zeta(n-1)}{n} z^n, where γ\gamma is the Euler-Mascheroni constant and ζ(s)\zeta(s) is the Riemann zeta function. This expansion arises from the infinite product representation of the G-function through regularization of divergent sums involving the zeta function. The coefficients in the series are expressed in terms of values of the Riemann zeta function at positive integers: for instance, ζ(2)=π2/6\zeta(2) = \pi^2/6, ζ(3)1.20206\zeta(3) \approx 1.20206, and higher even values ζ(2k)=(1)k+1B2k(2π)2k/(2(2k)!)\zeta(2k) = (-1)^{k+1} B_{2k} (2\pi)^{2k} / (2 (2k)!), where B2kB_{2k} are Bernoulli numbers. The linear term 12[ln(2π)1]z\frac{1}{2} [\ln(2\pi) - 1] z incorporates the normalization from the product form, while the quadratic term separates the regularized contribution from ζ(1)\zeta(1), effectively capturing the Euler-Mascheroni constant γ0.57721\gamma \approx 0.57721. Expanding to low orders yields explicit terms up to z3z^3: lnG(z+1)=12[ln(2π)1]z1+γ2z2+π218z3+O(z4).\ln G(z+1) = \frac{1}{2} \left[ \ln(2\pi) - 1 \right] z - \frac{1 + \gamma}{2} z^2 + \frac{\pi^2}{18} z^3 + O(z^4). The radius of convergence of this power series is z<1|z| < 1, limited by the nearest pole of lnG(z+1)\ln G(z+1) at z=1z = -1. Beyond this disk, analytic continuation can be achieved using the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) or other representations, allowing evaluation in larger regions of the complex plane. This series facilitates numerical approximations and theoretical analysis near z=0z = 0, with the zeta coefficients enabling connections to number-theoretic properties.

Asymptotic Expansion

The asymptotic expansion of the Barnes G-function provides a Stirling-like approximation for its logarithm as z|z| \to \infty in the complex plane, enabling accurate evaluation and analysis for large arguments. This expansion incorporates the asymptotic behavior of the gamma function while adding higher-order terms specific to the multiple gamma structure of the G-function. The series is divergent but yields optimal approximations when truncated appropriately. The precise form of the expansion is given by lnG(z+1)z24+zlnΓ(z+1)(z(z+1)2+112)lnzlnA+k=1B2k+22k(2k+1)(2k+2)z2k,\ln G(z+1) \sim \frac{z^2}{4} + z \ln \Gamma(z+1) - \left( \frac{z(z+1)}{2} + \frac{1}{12} \right) \ln z - \ln A + \sum_{k=1}^\infty \frac{B_{2k+2}}{2k(2k+1)(2k+2) z^{2k}}, valid for phz<πδ|\mathrm{ph}\, z| < \pi - \delta with δ>0\delta > 0. Here, B2k+2B_{2k+2} denote the Bernoulli numbers, which appear in the infinite sum as coefficients for the even-powered inverse terms in zz, mirroring their role in the classical Stirling series but extended to capture the "double" nature of the approximation. This expansion holds particularly in the right half-plane Re(z)>0\mathrm{Re}(z) > 0, where the principal branch of the logarithms is well-defined, and the remainder after NN terms satisfies error bounds of the form O(z2N)O(|z|^{-2N}) for fixed NN as z|z| \to \infty. More refined estimates, including exponentially improved asymptotics with error terms exponentially small along certain rays (such as the positive real axis), have been established to enhance precision in numerical applications. The structure of the series connects directly to Stirling's asymptotic for lnΓ(z+1)\ln \Gamma(z+1), augmented by quadratic and logarithmic adjustments that reflect the iterative functional relation of the G-function, effectively providing a double-layered approximation.

Other Properties

Absolute Value

As |t| → ∞, the modulus |G(1 + it)| exhibits exponential decay with leading behavior involving terms from the asymptotic expansion of log G(z + 1) specialized to the line Re(z) = 1. This decay reflects the cumulative structure from the functional equation, being slower than that of the Gamma function. Two-sided inequalities for |G(z)| in the complex plane can be derived using the reflection formula G(z) G(1 − z) = exp[(1/2 − z) log(2π) + (z − 1/2)(γ + log(2π)) − ζ′(−1)] / [√(2π) Γ(z)], which relates the modulus in the left and right half-planes. For regions with Re(z) > 0, extensions of Batir's inequalities for the positive real line provide bounds in terms of the Gamma and digamma functions. These inequalities facilitate growth estimates, showing sub-Gaussian decay in the imaginary direction while exponential growth occurs for large positive Re(z).

Zeros and Analytic Continuation

The Barnes G-function G(z)G(z) is an entire function of order 2, meaning it is holomorphic everywhere in the complex plane and its growth is controlled by exp(zρ)\exp(|z|^\rho) for any ρ>2\rho > 2 but not for ρ<2\rho < 2. Its zeros are located precisely at the non-positive integers z=0,1,2,z = 0, -1, -2, \dots, with no zeros elsewhere in the complex plane; these locations arise from the factors in its infinite product representation. At z=nz = -n for n=0,1,2,n = 0, 1, 2, \dots, the multiplicity of the zero is n+1n+1. Unlike the gamma function, which has simple poles at the non-positive integers, the Barnes G-function has no poles anywhere in the finite complex plane. This pole-free nature stems directly from its construction via the infinite product, which introduces zeros that precisely cancel the poles encountered when iteratively applying the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z) across the plane. The Barnes G-function is initially defined for positive real arguments via its relation to superfactorials or a finite product, but analytic continuation to the entire complex plane is accomplished using either the infinite Weierstrass-type product representation, G(z+1)=(2π)z/2exp(12z(z+1)γz22)k=1[(1+zk)kexp(z+z22k)],G(z+1) = (2\pi)^{z/2} \exp\left( -\frac{1}{2} z(z+1) - \frac{\gamma z^2}{2} \right) \prod_{k=1}^\infty \left[ \left(1 + \frac{z}{k}\right)^k \exp\left( -z + \frac{z^2}{2k} \right) \right], which converges uniformly on compact sets and defines the function holomorphically everywhere, or by stepping across the plane using the functional equation starting from values on the positive real axis. The functional equation itself facilitates continuation by relating values in adjacent strips, ensuring no singularities are introduced beyond the inherent zeros. As z|z| \to \infty with argzπδ|\arg z| \leq \pi - \delta for fixed δ>0\delta > 0, the growth of the G-function is given asymptotically by G(z)exp(z22(lnz1)),|G(z)| \sim \exp\left( \frac{|z|^2}{2} (\ln |z| - 1) \right), which follows from the leading terms in its full asymptotic expansion for lnG(z+1)\ln G(z+1), lnG(z+1)14z2+zlnΓ(z+1)(12z(z+1)+112)lnzlnA+k=1B2k+2(2k)(2k+1)(2k+2)z2k,\ln G(z+1) \sim \frac{1}{4}z^2 + z \ln \Gamma(z+1) - \left( \frac{1}{2}z(z+1) + \frac{1}{12} \right) \ln z - \ln A + \sum_{k=1}^\infty \frac{B_{2k+2}}{(2k)(2k+1)(2k+2) z^{2k}}, where AA is the Glaisher-Kinkelin constant and BmB_m are Bernoulli numbers; substituting the Stirling approximation for lnΓ(z+1)\ln \Gamma(z+1) yields the dominant behavior. This exponential growth of order 2 underscores the function's classification and distinguishes it from the gamma function, which grows like exp(z(lnz1))\exp(|z| (\ln |z| - 1)).

Relations to Other Functions

Relation to the Gamma Function

The Barnes G-function satisfies the functional equation G(z+1)=Γ(z)G(z),G(z+1) = \Gamma(z) \, G(z), with the normalization condition G(1)=1G(1) = 1. This recurrence relation directly links the G-function to the Gamma function, allowing iterative computation and highlighting its role as a generalization. By iteratively applying this relation, the G-function can be expressed for positive integers n2n \geq 2 as G(n)=k=1n2k!G(n) = \prod_{k=1}^{n-2} k!, a finite product of factorials equivalent to shifted Gamma function values at positive integers. This structure positions the G-function as a "higher-order" analog of the Gamma function, extending its multiplicative properties to a broader class of special functions. Unlike the Gamma function, which exhibits simple poles at the non-positive integers z=0,1,2,z = 0, -1, -2, \dots, the G-function is an entire function of order two with simple zeros precisely at these points, avoiding poles through the accumulation of zeros that balance the recurrence. The G-function was introduced by Ernest William Barnes in 1904 as a key component of his theory of multiple gamma functions, generalizing the classical Gamma function to higher dimensions via successive applications of such recurrences.

Relation to the Log-Gamma Integral

The Barnes G-function admits an integral characterization in terms of the logarithm of the gamma function, providing an alternative definition to its product form. Specifically, lnG(z+1)=zlnΓ(z+1)0zlnΓ(t+1)dt+12zln(2π)12z(z+1),\ln G(z+1) = z \ln \Gamma(z+1) - \int_0^z \ln \Gamma(t+1) \, dt + \frac{1}{2} z \ln (2\pi) - \frac{1}{2} z (z+1), where the logarithms take their principal values on the positive real axis and are analytically continued via continuity. This expression holds for complex zz in suitable domains, reflecting the entire nature of G(z)G(z). This relation derives from the functional equation G(z+1)=Γ(z)G(z)G(z+1) = \Gamma(z) G(z), which upon taking logarithms yields lnG(z+1)lnG(z)=lnΓ(z)\ln G(z+1) - \ln G(z) = \ln \Gamma(z). Integrating both sides from 1 to z+1z+1 and incorporating the digamma function ψ(w)=ddwlnΓ(w)\psi(w) = \frac{d}{dw} \ln \Gamma(w), whose integral representation is ψ(z+1)=0(ette(z+1)t1et)dt\psi(z+1) = \int_0^\infty \left( \frac{e^{-t}}{t} - \frac{e^{-(z+1)t}}{1 - e^{-t}} \right) dt, leads to the log-gamma integral form after accounting for boundary terms and normalization G(1)=1G(1) = 1. The focus remains on the cumulative effect of the log-gamma, avoiding direct use of the digamma integral for the derivation. Combined with the normalization condition G(1)=1G(1) = 1, this integral representation uniquely determines the Barnes G-function as an entire function of order 2, equivalently to its Weierstrass product form 1G(z+1)=eAz2+Bzn=1(1+zn)nez+z2/(2n)\frac{1}{G(z+1)} = e^{A z^2 + B z} \prod_{n=1}^\infty \left(1 + \frac{z}{n}\right)^n e^{-z + z^2/(2n)}, where AA and BB are constants related to the Riemann zeta function. Numerically, this form facilitates computation of G(z)G(z) in vertical strips of the complex plane, such as Rezk<1/2|\operatorname{Re} z - k| < 1/2 for integer kk, by leveraging efficient algorithms for lnΓ(w)\ln \Gamma(w) and quadrature for the integral, which converges rapidly due to the smoothness of lnΓ(t+1)\ln \Gamma(t+1).[https://www.sciencedirect.com/science/article/pii/S0010465503004983) This approach is particularly advantageous for high-precision evaluations where the product form may suffer from overflow or underflow.

Relation to the Glaisher-Kinkelin Constant

The Glaisher-Kinkelin constant AA, approximately 1.2824271291, is defined as A=e1/12ζ(1)A = e^{1/12 - \zeta'(-1)}, where ζ(s)\zeta'(s) denotes the derivative of the Riemann zeta function evaluated at s=1s = -1. This constant arises in asymptotic analyses of products involving factorials and powers, such as the hyperfactorial function H(n)=k=1nkkH(n) = \prod_{k=1}^n k^k. Introduced by J. W. L. Glaisher in 1894 for the asymptotic behavior of the hyperfactorial and further developed by H. Kinkelin in related contexts, the constant was later connected to the Barnes G-function through E. W. Barnes' work on multiple gamma functions in 1904. Barnes demonstrated that the G-function provides an analytic continuation and generalization that incorporates AA naturally in its properties. The Glaisher-Kinkelin constant appears explicitly in the asymptotic expansion of lnG(z+1)\ln G(z+1) for large z|z| with argz<π|\arg z| < \pi, where the constant term includes lnA-\ln A: lnG(z+1)=z22logz3z24+z2log(2π)+(112lnA)112logz+O(1z).\ln G(z+1) = \frac{z^2}{2} \log z - \frac{3z^2}{4} + \frac{z}{2} \log (2\pi) + \left( \frac{1}{12} - \ln A \right) - \frac{1}{12} \log z + O\left( \frac{1}{z} \right). This Stirling-like series, derived by Barnes, highlights AA's role in the leading behavior of the G-function, analogous to how the Euler-Mascheroni constant appears in the gamma function's expansion. For integer arguments, the relation manifests in the limit limnG(n+1)nn2/21/12(2π)n/2e3n2/4A=e1/12,\lim_{n \to \infty} \frac{G(n+1) \, n^{n^2/2 - 1/12} \, (2\pi)^{n/2} \, e^{-3n^2/4}}{A} = e^{1/12}, which connects the growth of G(n+1)=k=1nk!G(n+1) = \prod_{k=1}^n k! to AA. This expression underscores the constant's significance in evaluating the G-function at positive integers via Barnes' integral representation and product formula.

Extensions to Multiple G-Functions

The multiple G-function provides a higher-dimensional generalization of the Barnes G-function, extending its properties to multi-variable settings in connection with the Barnes multiple gamma function. Defined for z ∈ ℝ^n, the function G_n(z) satisfies the functional equation Gn(z+ej)=Γn(z)Gn(z)G_n(\mathbf{z} + \mathbf{e}_j) = \Gamma_n(\mathbf{z}) G_n(\mathbf{z}) for each standard basis vector \mathbf{e}_j (j = 1, \dots, n), where \Gamma_n(\mathbf{z}) denotes the Barnes multiple gamma function of n variables, with the normalization condition G_n(\mathbf{1}) = 1, where \mathbf{1} is the n-dimensional vector of ones. For n=1, this reduces to the standard Barnes G-function, satisfying G_1(z + 1) = \Gamma_1(z) G_1(z) with G_1(1) = 1, where \Gamma_1(z) = \Gamma(z) is the Euler gamma function. The multi-variable functional equation generalizes this by incorporating shifts along each coordinate axis, enabling product forms over successive applications of the basis shifts. Barnes introduced the underlying multiple gamma function \Gamma_n(\mathbf{z}) in 1904 as part of his development of higher-order generalizations of the gamma function, motivated by analytic continuations and zeta function theory; the multiple G-function emerges as the accompanying "exponential" component fulfilling the shift relations. These functions find applications in the theory of Barnes multiple zeta functions, which regularize infinite products and series to define \Gamma_n(\mathbf{z}) via derivatives at s=0, and in contour integral representations that express properties of \Gamma_n(\mathbf{z}), such as reflection formulas and asymptotic behaviors in multiple variables.
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