Abel's summation formula

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In mathematics, Abel's summation formula, introduced by Niels Henrik Abel, is intensively used in analytic number theory and the study of special functions to compute series.

Formula

Template:Wikibooks Let (an)n=0 be a sequence of real or complex numbers. Define the partial sum function A by

A(t)=0ntan

for any real number t. Fix real numbers x<y, and let ϕ be a continuously differentiable function on [x,y]. Then:

x<nyanϕ(n)=A(y)ϕ(y)A(x)ϕ(x)xyA(u)ϕ(u)du.

The formula is derived by applying integration by parts for a Riemann–Stieltjes integral to the functions A and ϕ.

Variations

Taking the left endpoint to be 1 gives the formula

0nxanϕ(n)=A(x)ϕ(x)0xA(u)ϕ(u)du.

If the sequence (an) is indexed starting at n=1, then we may formally define a0=0. The previous formula becomes

1nxanϕ(n)=A(x)ϕ(x)1xA(u)ϕ(u)du.

A common way to apply Abel's summation formula is to take the limit of one of these formulas as x. The resulting formulas are

n=0anϕ(n)=limx(A(x)ϕ(x))0A(u)ϕ(u)du,n=1anϕ(n)=limx(A(x)ϕ(x))1A(u)ϕ(u)du.

These equations hold whenever both limits on the right-hand side exist and are finite.

A particularly useful case is the sequence an=1 for all n0. In this case, A(x)=x+1. For this sequence, Abel's summation formula simplifies to

0nxϕ(n)=x+1ϕ(x)0xu+1ϕ(u)du.

Similarly, for the sequence a0=0 and an=1 for all n1, the formula becomes

1nxϕ(n)=xϕ(x)1xuϕ(u)du.

Upon taking the limit as x, we find

n=0ϕ(n)=limx(x+1ϕ(x))0u+1ϕ(u)du,n=1ϕ(n)=limx(xϕ(x))1uϕ(u)du,

assuming that both terms on the right-hand side exist and are finite.

Abel's summation formula can be generalized to the case where ϕ is only assumed to be continuous if the integral is interpreted as a Riemann–Stieltjes integral:

x<nyanϕ(n)=A(y)ϕ(y)A(x)ϕ(x)xyA(u)dϕ(u).

By taking ϕ to be the partial sum function associated to some sequence, this leads to the summation by parts formula.

Examples

Harmonic numbers

If an=1 for n1 and ϕ(x)=1/x, then A(x)=x and the formula yields

n=1x1n=xx+1xuu2du.

The left-hand side is the harmonic number Hx.

Representation of Riemann's zeta function

Fix a complex number s. If an=1 for n1 and ϕ(x)=xs, then A(x)=x and the formula becomes

n=1x1ns=xxs+s1xuu1+sdu.

If (s)>1, then the limit as x exists and yields the formula

ζ(s)=s1uu1+sdu.

where ζ(s) is the Riemann zeta function. This may be used to derive Dirichlet's theorem that ζ(s) has a simple pole with residue 1 at Template:Math.

Reciprocal of Riemann zeta function

The technique of the previous example may also be applied to other Dirichlet series. If an=μ(n) is the Möbius function and ϕ(x)=xs, then A(x)=M(x)=nxμ(n) is Mertens function and

1ζ(s)=n=1μ(n)ns=s1M(u)u1+sdu.

This formula holds for (s)>1.

See also

References