On the series expansion of a square-free zeta series
Abstract
In this article, we develop a square-free zeta series associated with the Möbius function into a power series, and prove a Stieltjes like formula for these expansion coefficients. We also investigate another analytical continuation of these series and develop a formula for in terms of the Möbius function, and in the last part, we explore an alternating series version of these results.
1 Introduction
In the recent work of Wolf [7] who investigated the divergence of a certain zeta series involving the Möbius function [3, p. 304], (thus essentially running over square-free integers) as such
(1) |
(as ) and determined a more refined estimate
(2) |
where a new constant
(3) | ||||
can be extracted in the limit in a much the same way as the classical Euler-Mascheroni constant
(4) | ||||
Recalling that the Riemann zeta function is defined by the simplest Dirichlet series
(5) |
is absolutely convergent for , and admits the Laurent series expansion about is given by
(6) |
which analytically extends to with residue and an only pole at . With the Euler’s constant () appearing as the order coefficient in the series, and consequently, the next higher order Stieltjes constants [4, p. 561] can be similarly generated by the well-known formula
(7) |
And in a similar fashion, a certain fraction of the zetas
(8) |
involves the Möbius function as in (1) [6, p.5], and based on some previous analysis its Laurent series expansion is given by
(9) |
also with a pole at and residue , and the proposed formula by Wolf for these expansion coefficients
(10) |
is an analogue of the Stieltjes formula (7) [7]. We also note that the radius of convergence of (9) is only limited to due to the pole at the first trivial zero when for from the center at .
We now prove (10) by following exactly the proof in Bohman-Fröberg [2][4, p. 561-562], but additionally inserting the Möbius function. We begin the proof by introducing a self-canceling telescoping series
(11) |
then one has
(12) |
which is still valid for , but since for the (lhs) limit is
(13) |
is inconsistent with (rhs) of (12). So if we consider another re-scaled sequence instead
(14) |
such that the (lhs) equals (rhs) at , and then proceeding with the exp-log expansion exactly about , then one obtains
(15) | ||||
and by collecting the terms (with ) and since , we obtain
(16) |
where
(17) |
and last term as self-cancels again leaving only the term leading to the final limit formula
(18) |
We next consider an alternative representation for these coefficients. If we take the Laurent series expansion about of
(19) |
to the order, and another expansion of
(20) |
to the order, then by multiplying them together yields
(21) |
As a result, the order coefficient in (21) is collected in the limit as
(22) |
gives a better closed-form formula in terms of other known constants. And the value for the zeta derivative can be computed directly from (5) as
(23) |
In Table 1, we compute the first higher order coefficients to high-precision ( decimal places) by the differentiation of the (lhs) of (16) in the limit as
(24) |
which is easily possible to do in software packages such as Mathematica or Pari/GP [5][8]. The error term for in (1) is , and this would roughly imply that in order to get decimal places using (3), one needs to compute the limit with on the order of , which is so large that even on modern computer workstations is still completely unfeasible to do in reasonable time (but perhaps on a supercomputer it could run faster), but one can still easily compute these constants to thousands of digits by differentiation in (24).
1.043894515711938297404563438509 | |
0.236152886477122974860578286060 | |
0.319384120408014249249465207074 | |
0.501294458741649566645935631332 | |
1.010739722784850417039579626049 | |
2.544030257932552280334481508980 | |
7.666100995112318690725728704276 | |
26.88797470534219199661349019865 | |
107.6566910334506652692812639473 | |
484.6934692784684121614213582581 | |
2424.080089640181055133479838894 |
2 On analytical continuation of the Dirichlet series
We saw earlier that the square-free Dirichlet series
(25) |
is convergent for . In the previous Section, the telescoping series (12) is also convergent for , but with the introduction of a scaling constant we propose that (14) is actually valid for (except at ) and assuming (RH). We reformulate the expression and bring over to the (rhs) we have
(26) |
and in another form
(27) |
and then self-canceling the telescoping series to last term we get
(28) |
which we numerically find is valid as stated. This limitation is due to the poles that arise at , where is the non-trivial root of . As evidenced by numerical computations, for example, for we compute the (lhs) of (28) to , while the (rhs) with is , an agreement to digits. And if then the (lhs) of (28) is , while the (rhs) with is computed as , where we see it is going to zero. And we checked many more random points and see that this formula is clearly converging to right values in the new domain , and as shown by the plot in Fig. 1, where we compare the (lhs) and (rhs) of equation (28) for , and observe a deviation starts to happen near . This means that all non-trivial roots are also roots of the (rhs) of (28).

Equation (28) can give many more interesting results. As previously seen, is a zero of (28), and so we obtain a special case
(29) |
as , or expressing in another way
(30) |
We also consider another expansion about of
(31) |
and seek to extract the first order zeta value by differentiation of the (rhs) of (28). We obtain the formula
(32) |
which is converging to this zeta value. We next verify this formula numerically and find that it is a rather noisy and fluctuating series. In Fig. 2, we plot (32) as a function of from to in increments of , on a logarithmic scale on the x-axis to capture all points. We note how it is fluctuating about the value , with a gradual decrease in amplitude as increases. Another form can be simplified by plugging in (30) into (32) to have
(33) |
and when we test this formula we reproduce an almost the same plot as in Fig. 2.

3 On an alternating series representation
There is a common alternating series representation for the zeta function
(34) |
which is valid for (but except at those points on the line where the leading factor becomes singular). A similar relation can be obtained for the square-free zeta series inspired by the MathOverflow post [9] by taking advantage of a certain connection to the Euler product
(35) |
valid for , where runs over all primes . Then, the application of the general Dirichlet series [3, p. 326] reads
(36) |
where is a multiplicative function, meaning that for any positive integers and must satisfy the relation and whenever and are co-prime holds. It turns out that an alternating sign function is multiplicative, and hence is multiplicative, then we get the following transformation
(37) | ||||
since , and and for . And this leads to the form analogue to the alternating zeta series (34) as
(38) |
It is rare get such a coincidence, since this transformation depends on the existence of such a Euler product form. But unfortunately, the domain of convergence of (37) is only valid for instead of as in the alternating zeta (34). One reason is that at the summation in (34) is conditionally convergent as
(39) |
while the for square-free alternating zeta at diverges for the reason being by equating (8) with (34), where they only differ by a factor of . And this leads to consider an estimate
(40) |
as , and an analogue constant for the alternating series
(41) | ||||
where the closed-form formula can be computed by
(42) |
by the virtue of expansion of the factor
(43) |
in conjunction with (19) to (22).
4 Acknowledgement
I would like to thank Professor Wolf for comments and suggestions for improving the paper.
References
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