Abel's summation formula

From testwiki
Jump to navigation Jump to search

Template:Short description Template:Dablink

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)=∑0≤n≤tan

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

∑x<n≤yanϕ(n)=A(y)ϕ(y)−A(x)ϕ(x)−∫xyA(u)ϕ′(u)du.

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

Variations

Taking the left endpoint to be −1 gives the formula

∑0≤n≤xanϕ(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

∑1≤n≤xanϕ(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=0∞anϕ(n)=limx→∞(A(x)ϕ(x))−∫0∞A(u)ϕ′(u)du,∑n=1∞anϕ(n)=limx→∞(A(x)ϕ(x))−∫1∞A(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 n≥0. In this case, A(x)=⌊x+1⌋. For this sequence, Abel's summation formula simplifies to

∑0≤n≤xϕ(n)=⌊x+1⌋ϕ(x)−∫0x⌊u+1⌋ϕ′(u)du.

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

∑1≤n≤xϕ(n)=⌊x⌋ϕ(x)−∫1x⌊u⌋ϕ′(u)du.

Upon taking the limit as x→∞, we find

∑n=0∞ϕ(n)=limx→∞(⌊x+1⌋ϕ(x))−∫0∞⌊u+1⌋ϕ′(u)du,∑n=1∞ϕ(n)=limx→∞(⌊x⌋ϕ(x))−∫1∞⌊u⌋ϕ′(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<n≤yanϕ(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 n≥1 and ϕ(x)=1/x, then A(x)=⌊x⌋ and the formula yields

∑n=1⌊x⌋1n=⌊x⌋x+∫1x⌊u⌋u2du.

The left-hand side is the harmonic number H⌊x⌋.

Representation of Riemann's zeta function

Fix a complex number s. If an=1 for n≥1 and ϕ(x)=x−s, then A(x)=⌊x⌋ and the formula becomes

∑n=1⌊x⌋1ns=⌊x⌋xs+s∫1x⌊u⌋u1+sdu.

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

ζ(s)=s∫1∞⌊u⌋u1+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)=x−s, then A(x)=M(x)=∑n≤xμ(n) is Mertens function and

1ζ(s)=∑n=1∞μ(n)ns=s∫1∞M(u)u1+sdu.

This formula holds for ℜ(s)>1.

See also

References