Riesz mean

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In mathematics, the Riesz mean is a certain mean of the terms in a series. They were introduced by Marcel Riesz in 1911 as an improvement over the Cesàro mean[1][2]. The Riesz mean should not be confused with the Bochner–Riesz mean or the Strong–Riesz mean.

Definition

Given a series {sn}, the Riesz mean of the series is defined by

sδ(λ)=nλ(1nλ)δsn

Sometimes, a generalized Riesz mean is defined as

Rn=1λnk=0n(λkλk1)δsk

Here, the λn are a sequence with λn and with λn+1/λn1 as n. Other than this, the λn are taken as arbitrary.

Riesz means are often used to explore the summability of sequences; typical summability theorems discuss the case of sn=k=0nak for some sequence {ak}. Typically, a sequence is summable when the limit limnRn exists, or the limit limδ1,λsδ(λ) exists, although the precise summability theorems in question often impose additional conditions.

Special cases

Let an=1 for all n. Then

nλ(1nλ)δ=12πicic+iΓ(1+δ)Γ(s)Γ(1+δ+s)ζ(s)λsds=λ1+δ+nbnλn.

Here, one must take c>1; Γ(s) is the Gamma function and ζ(s) is the Riemann zeta function. The power series

nbnλn

can be shown to be convergent for λ>1. Note that the integral is of the form of an inverse Mellin transform.

Another interesting case connected with number theory arises by taking an=Λ(n) where Λ(n) is the Von Mangoldt function. Then

nλ(1nλ)δΛ(n)=12πicic+iΓ(1+δ)Γ(s)Γ(1+δ+s)ζ(s)ζ(s)λsds=λ1+δ+ρΓ(1+δ)Γ(ρ)Γ(1+δ+ρ)+ncnλn.

Again, one must take c > 1. The sum over ρ is the sum over the zeroes of the Riemann zeta function, and

ncnλn

is convergent for λ > 1.

The integrals that occur here are similar to the Nörlund–Rice integral; very roughly, they can be connected to that integral via Perron's formula.

References