Dirichlet eta function

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Color representation of the Dirichlet eta function. It is generated as a Matplotlib plot using a version of the Domain coloring method.[1]

In mathematics, in the area of analytic number theory, the Dirichlet eta function is defined by the following Dirichlet series, which converges for any complex number having real part greater than zero: η(s)=∑n=1∞(−1)n−1ns=11s−12s+13s−14s+⋯.

This Dirichlet series is the alternating sum corresponding to the Dirichlet series expansion of the Riemann zeta function, ζ(s) — and for this reason the Dirichlet eta function is also known as the alternating zeta function, also denoted Template:Itco*(s). The following relation holds: η(s)=(1−21−s)ζ(s)

Both the Dirichlet eta function and the Riemann zeta function are special cases of polylogarithms.

While the Dirichlet series expansion for the eta function is convergent only for any complex number s with real part > 0, it is Abel summable for any complex number. This serves to define the eta function as an entire function.

Equivalently, we may begin by defining η(s)=1Γ(s)∫0∞xs−1ex+1dx which is also defined in the region of positive real part (Γ(s) represents the gamma function). This gives the eta function as a Mellin transform.

Hardy gave a simple proof of the functional equation for the eta function,[2] which is η(−s)=21−2−s−11−2−sπ−s−1ssin⁡(πs2)Γ(s)η(s+1).

From this, one immediately has the functional equation of the zeta function also, as well as another means to extend the definition of eta to the entire complex plane.

Zeros

The zeros of the eta function include all the zeros of the zeta function: the negative even integers (real equidistant simple zeros); the zeros along the critical line, none of which are known to be multiple and over 40% of which have been proven to be simple, and the hypothetical zeros in the critical strip but not on the critical line, which if they do exist must occur at the vertices of rectangles symmetrical around the x-axis and the critical line and whose multiplicity is unknown.Template:Citation needed In addition, the factor 1−21−s adds an infinite number of complex simple zeros, located at equidistant points on the line Template:Tmath, at sn=1+2nπi/ln⁡(2) where n is any nonzero integer.

The zeros of the eta function are located symmetrically with respect to the real axis and under the Riemann hypothesis would be on two parallel lines ℜ(s)=1/2,ℜ(s)=1, and on the perpendicular half line formed by the negative real axis.

Landau's problem

In the equation Template:Math, "the pole of Template:Math at Template:Math is cancelled by the zero of the other factor" (Titchmarsh, 1986, p. 17), and as a result Template:Math is neither infinite nor zero (see Template:Section link). However, in the equation ζ(s)=η(s)1−21−s, η must be zero at all the points Template:Tmath, where the denominator is zero, if the Riemann zeta function is analytic and finite there. The problem of proving this without defining the zeta function first was signaled and left open by E. Landau in his 1909 treatise on number theory: "Whether the eta series is different from zero or not at the points sn≠1, i.e., whether these are poles of zeta or not, is not readily apparent here."

A first solution for Landau's problem was published almost 40 years later by D. V. Widder in his book The Laplace Transform. It uses the next prime 3 instead of 2 to define a Dirichlet series similar to the eta function, which we will call the λ function, defined for ℜ(s)>0 and with some zeros also on Template:Tmath, but not equal to those of eta. Template:Math proof

An elementary direct and ζ-independent proof of the vanishing of the eta function at sn≠1 was published by J. Sondow in 2003. It expresses the value of the eta function as the limit of special Riemann sums associated to an integral known to be zero, using a relation between the partial sums of the Dirichlet series defining the eta and zeta functions for ℜ(s)>1.

Template:Math proof

Assuming η(sn)=0, for each point sn≠1 where 2sn=2, we can now define ζ(sn) by continuity as follows, ζ(sn)=lims→snη(s)1−22s=lims→snη(s)−η(sn)22sn−22s=lims→snη(s)−η(sn)s−sns−sn22sn−22s=η′(sn)log⁡(2).

The apparent singularity of zeta at sn≠1 is now removed, and the zeta function is proven to be analytic everywhere in ℜs>0, except at s=1 where lims→1(s−1)ζ(s)=lims→1η(s)1−21−ss−1=η(1)log⁡2=1.

Integral representations

A number of integral formulas involving the eta function can be listed. The first one follows from a change of variable of the integral representation of the Gamma function (Abel, 1823), giving a Mellin transform which can be expressed in different ways as a double integral (Sondow, 2005). This is valid for ℜs>0. Γ(s)η(s)=∫0∞xs−1ex+1dx=∫0∞∫0xxs−2ex+1dydx=∫0∞∫0∞(t+r)s−2et+r+1drdt=∫01∫01(−log⁡(xy))s−21+xydxdy.

The Cauchy–Schlömilch transformation (Amdeberhan, Moll et al., 2010) can be used to prove this other representation, valid for Template:Tmath. Integration by parts of the first integral above in this section yields another derivation.

21−sΓ(s+1)η(s)=2∫0∞x2s+1cosh2(x2)dx=∫0∞tscosh2(t)dt.

The next formula, due to Lindelöf (1905), is valid over the whole complex plane, when the principal value is taken for the logarithm implicit in the exponential. η(s)=∫−∞∞(1/2+it)−seπt+e−πtdt. This corresponds to a Jensen (1895) formula for the entire function (s−1)ζ(s), valid over the whole complex plane and also proven by Lindelöf. (s−1)ζ(s)=2π∫−∞∞(1/2+it)1−s(eπt+e−πt)2dt. "This formula, remarquable by its simplicity, can be proven easily with the help of Cauchy's theorem, so important for the summation of series" wrote Jensen (1895). Similarly by converting the integration paths to contour integrals one can obtain other formulas for the eta function, such as this generalisation (Milgram, 2013) valid for 0<c<1 and all s: η(s)=12∫−∞∞(c+it)−ssin⁡(π(c+it))dt. The zeros on the negative real axis are factored out cleanly by making c→0+ (Milgram, 2013) to obtain a formula valid for ℜs<0: η(s)=−sin⁡(sπ2)∫0∞t−ssinh⁡(πt)dt.

Numerical algorithms

Most of the series acceleration techniques developed for alternating series can be profitably applied to the evaluation of the eta function. One particularly simple, yet reasonable method is to apply Euler's transformation of alternating series, to obtain η(s)=∑n=0∞12n+1∑k=0n(−1)k(nk)1(k+1)s.

Note that the second, inside summation is a forward difference.

Borwein's method

Peter Borwein used approximations involving Chebyshev polynomials to produce a method for efficient evaluation of the eta function.[3] If dk=n∑ℓ=0k(n+ℓ−1)!4ℓ(n−ℓ)!(2ℓ)! then η(s)=−1dn∑k=0n−1(−1)k(dk−dn)(k+1)s+γn(s), where for ℜ(s)≥12 the error term Template:Math is bounded by |γn(s)|≤3(3+8)n(1+2|ℑ(s)|)exp⁡(π2|ℑ(s)|).The factor of 3+8≈5.8 in the error bound indicates that the Borwein series converges quite rapidly as n increases.


The result for η(s) can also be expressed as: η(s)=∑k=1n(−1)k−1ks(1−dk−1dn)+γn(s)This form appears similar to the definition of the eta function but with finitely many terms, with each term being multiplied by a scaling factor.

Particular values

Template:Further

Also:

  • η(1)=ln⁡2, this is the alternating harmonic series
  • η(2)=π212 Template:OEIS2C
  • η(4)=7π4720≈0.94703283
  • η(6)=31π630240≈0.98555109
  • η(8)=127π81209600≈0.99623300
  • η(10)=73π106842880≈0.99903951
  • η(12)=1414477π121307674368000≈0.99975769

The general form for even positive integers is: η(2n)=(−1)n+1B2nπ2n(22n−1−1)(2n)!.

Taking the limit Template:Tmath, one obtains Template:Tmath.

Derivatives

The derivative with respect to the parameter Template:Mvar is for s≠1 η′(s)=∑n=1∞(−1)nln⁡nns=21−sln⁡(2)ζ(s)+(1−21−s)ζ′(s). η′(1)=ln⁡(2)γ−ln⁡(2)22−1

References

Template:Reflist

  1. ↑ Template:Cite web
  2. ↑ Hardy, G. H. (1922). A new proof of the functional equation for the Zeta-function. Matematisk Tidsskrift. B, 71–73. http://www.jstor.org/stable/24529536
  3. ↑ Template:Cite book