Improved estimates for the argument and zero-counting of Riemann zeta-function
(With an appendix by Andrew Fiori)
Abstract.
In this article, we improve the recent work of Hasanalizade, Shen, and Wong by establishing
for every , where is the number of non-trivial zeros , with , of the Riemann zeta-function . The main source of improvement comes from implementing new subconvexity bounds for on some -lines inside the critical strip.
Key words and phrases:
Riemann zeta-function, zero-density estimates, explicit estimates2020 Mathematics Subject Classification:
Primary 11M06, 11M26. Secondary 11Y351. Introduction
The main objective of this article is to improve the known estimates for the number of non-trivial zeros , with , of the Riemann zeta-function . More precisely, we shall study
for . The first explicit bound for was obtained by von Mangoldt [VM05], and it has been studied and improved since then. It shall be worthwhile mentioning that the importance of improving explicit bounds for allows one to estimate sums over zeros of , it leads to the explicit bounds for the prime-counting functions and (see, e.g., [FK15]).
Our main theorem is the following estimate that improves the recent work of Hasanalizade, Shen, and Wong [HSW22]:
Theorem 1.1.
For every , we have
and
For the convenience of the reader, writing
(1.1) |
we summarise the advances that have been made in Table 1 below.111Regrettably, as pointed out in [HSW22], there is an error in [Tru14]. Also, there is a typo in [HSW22] regarding the constant . The value is now substituted with .
von Mangoldt [VM05] (1905) | 0.4320 | 1.9167 | 13.0788 | 28.5580 |
Grossmann [Gro13] (1913) | 0.2907 | 1.7862 | 7.0120 | 50 |
Backlund [Bac16] (1918) | 0.1370 | 0.4430 | 5.2250 | 200 |
Rosser [Ros41] (1941) | 0.1370 | 0.4430 | 2.4630 | 2 |
Trudgian [Tru12] (2012) | 0.1700 | 0 | 2.8730 | |
Trudgian [Tru14] (2014) | 0.1120 | 0.2780 | 3.3850 | |
Platt–Trudgian [PT15] (2015) | 0.1100 | 0.2900 | 3.165 | |
Hasanalizade, Shen, and Wong [HSW22] (2022) | 0.1038 | 0.2573 | 9.4925 |
Note that the second estimate in Theorem 1.1 is sharper than Trudgian’s bound [Tru14] for .222This, together with Platt’s computation of as stated in (1.2), assures that Trudgian’s bound [Tru14] and all the explicit results relying on it remain valid.
Theorem 1.2.
Let be positive real numbers satisfying
and , where is defined in (3.32). Let defined in (2.2), defined in (2.3), and denote with the largest that we consider when using (2.4).
Let be fixed. Then for any , we have
where the constants , , , , are defined in (3.44), (3.45), (3.46), (3.47), (3.48) respectively and some admissible values can be found in Table 2.
Remark.
The proof of Theorem 1.2 has its roots in the works of [Ben+21, Tru14, HSW22] and flourished by the following new inputs.
(i) We used various improved bounds for , including the estimates of Yang [Yan24] inside the critical strip. To implement these bounds, we further considered “-splitting” of in Section 3.1 ( gives nearly-optimal result for ). This is one of our key observations and leads us to refined estimates for and .
(ii) Instead of just using the trivial bound for , we provided an alternative method by applying a non-trivial estimate obtained by Leong recently (as stated in Lemma 2.2). In fact, the constants and in Theorem 1.2 are calculated via the trivial bound, while and are obtained by Leong’s bound. As may be noticed, Leong’s bound allows one to get a relatively small at the expense of a larger , which might be useful for certain applications.
(iii) We directly estimated (which is useful for most applications). This particularly reduces in the previous estimate of Hasanalizade, Shen, and Wong [HSW22] by roughly .
We shall remark that the constant in Theorem 1.1 is the nearly-optimal value that one can obtain from Theorem 1.2 with the current knowledge on explicit estimates for . Also, it is possible to have smaller values of or of , at the expense of larger values for the other constants. Here, we provide two bounds with the smallest admissible and , respectively. (Particularly, the first estimate below is always sharper than Rosser’s bound [Ros41] for .)
Corollary 1.3.
The following estimates hold for :
and
Another important consequence of Theorem 1.2 is the following general bound for the argument of the Riemann zeta-function along the -line. (Recall that , where is the path formed by the straight line from to and then to ).
Theorem 1.4.
A sharper bound for , up to certain given height, can be obtained using the database of non-trivial zeros of computed by Platt and made available at [Lmf]. More precisely, one has
(1.2) |
for Hence, by Theorem 1.4 (with and Table 2) and (1.2), we can get the following explicit estimate for .
Corollary 1.5.
The following estimate holds for :
Two final consequences of Theorems 1.2 and 1.4 are bounds for the number of zeros in a unit interval and a short interval. These types of estimates have several applications in number theory, such as providing an effective disproof of the Mertens conjecture [Pin87, RK23], improving the error term in the explicit version of the Riemann–von Mangoldt formula [Dud16], and consequently obtaining improvements related to primes between consecutive cubes and consecutive powers [JCH24]. More generally, these two types of estimates are useful for any problems that require an estimate for the sum over the zeros of restricted to a certain range.
Corollary 1.6.
Remark.
Note that the optimal constants that one could hope to get in front of the main terms in the upper bounds of and in Corollary 1.6 are and respectively and it will be shown in Section 6. Furthermore, we omit the lower bound for when . Indeed, following the method used in Section 6 for results in a negative lower bound for , which is worse than the trivial non-negativity of .
2. Preliminaries
In this section, we recall some known results involving the Riemann zeta-function, which will be used throughout the proof of our theorems.
As already explained in [Tru14, HSW22], bounds of when and play a crucial role.
The sharpest known estimates for and are the following333Recently E. H. Qingyi and L.-P. Teo [QT24] found a new explicit bound for , which might lead to some small improvements.:
(2.1) |
In order of appearance, the estimates are due to Patel [Pat22], Hiary–Leong–Yang [HLY24] and the last one is a direct consequence of Theorem 1 in [Bel24].
In order to apply Lemma 2.6, we actually need an estimate of the form
(2.2) |
for , where are constants which depend on . Hence, for the middle range we will use the slightly worse upper bound .
The sharpest known estimates for up to date are instead:
In order of appearance, these estimates are due to Hiary [Hia16], Hiary–Patel–Yang [HPY24], Patel–Yang [PY24]. We will denote
(2.3) |
for , where are constants which depend on . Meanwhile, there exists another set of vertical lines inside the critical strip on which explicit bounds for are known. More precisely, Yang [Yan24] provided the following explicit estimate for , with , for every :
(2.4) |
For instance, substituting gives
The bound (2.4) will be the main innovative tool which will lead to improved values of both and in Theorem 1.1.
2.1. Other useful results
We recall other useful results which will be used to prove Theorem 1.1 and Theorem 1.2.
First of all, for , we consider the following function that will be fundamental in our argument:
Then, denoting with the open disk centred at with radius , for any , we define
where is the set of zeros of in .
Lemma 2.1 ([HSW21] Prop. 3.5).
Let , and be real numbers such that
Let be an even function such that . Then there is an infinite sequence of natural numbers such that
Lemma 2.1 uses the following trivial lower bound for zeta when :
(2.5) |
However, recently Leong [Leo24] proved a non-trivial lower bound for when which does not depend on the real part but only on the imaginary part .
Lemma 2.2 ([Leo24]).
The following estimate holds for and :
If instead of the trivial bound (2.5) we use Lemma 2.2 inside the proof of Lemma 2.1, we get the following result.
Lemma 2.3.
Under the same assumption as in Lemma 2.1, if there is an infinite sequence of natural numbers such that
Backlund’s trick is another important tool we will use for the proof of Theorem 1.1. To end this section, we recall the following version of Backlund’s trick (see [HSW21, Prop. 3.7]), a tool according to which if has zeros in , then there are zeros in .
Lemma 2.4 (Backlund’s trick).
We also recall the estimate for due to [Ben+21, Lemma 3.4].
Lemma 2.5 ([Ben+21]).
For and , one has
Also, for and , one has
To conclude the section, we mention the Phragmén–Lindelöf principle, as stated in [Tru14, Lemma 3], which will be used to construct a suitable function , given Lemmata 2.1, 2.3, and 2.4.
Lemma 2.6 (Phragmén-Lindelöf principle).
Let be real numbers such that and . Let be a holomorphic function on the strip such that
for some and . Suppose, further, that there are such that and
Then for , one has
3. Proof of Theorem 1.2
As in [Tru14, HSW22], we will work with the completed Riemann zeta-function , which is defined by
It is widely known that the function is an entire function of order 1 , which satisfies the functional equation
Furthermore, as in [HSW22], instead of working directly with the quantity , we will work with the quantity which is defined as
for and it is related to the quantity by the equality .
Following [HSW22], given a parameter we will choose later, we consider the rectangle with vertices , , , and , and, since is entire, we apply the argument principle, getting
As per [HSW22, eq. (2.8)], the previous expression for is equivalent to
(3.1) |
where
and is the part of the contour of in the region and . The estimate is given by [Ben+21, Prop. 3.2] and holds for every . Then, denoting with the vertical line from to and with the horizontal line from to , one has
and for ,
Furthermore, we know that [HSW22, eq. (5.5)]
(3.2) |
and
(3.3) |
Let fixed. Instead of estimating the usual quantity
as in [HSW22] (or instead of if we work with instead of as in [Tru14]), we aim to estimate
which is the quantity that is usually required in the majority of applications.
Remark.
This choice will allow us to save an extra in the final constant in Theorem 1.1.
One has
(3.4) | ||||
where
Since (it will be approximately ), quite large (), and being the function increasing for , we can estimate as
(3.5) |
Now, we will focus on improving the bound for
for which the main new ideas which lead to improvements are used.
3.1. Convexity/subconvexity bounds and generalisation to -splitting of
While outside the range we consider the same cases as in [HSW22], we will split the interval in sub-intervals using the lines corresponding to (2.4). As already mentioned, this splitting will be the main tool which allows us to get an improved value of .
More precisely, the first sub-interval is of the form , the last interval will be of the form and the intervals in the middle will be of the form , where and, for every , is defined as
A careful analysis shows that the nearly-optimal value for is . Indeed, a higher number of subintervals of the form would lead to an improvement on only at the seventh decimal place, while it would cause a worse constant , in which a factor of containing (multiplied by other quantities) appears in for each interval we are considering.
Following [HSW22], we start estimating in each of the intervals for we are considering.
-
•
Case . The trivial bound for the zeta-function immediately implies
- •
- •
-
•
Case with . By (2.4), for every fixed , there exist depending on so that
(3.8) and
(3.9) Hence, by Lemma 2.6, we have
where .
Remark.
When , , with given in (3.7).
- •
- •
-
•
Case . As in [HSW22], we have
(3.14) -
•
Case . We shall use the same estimate as in [HSW22]:
(3.15)
3.2. Estimating
Given the function
(3.16) |
we want to bound
(3.17) |
inside the different ranges we considered in the previous subsection.
-
•
Case . As per [HSW22], we have the bound
(3.18) -
•
Case . Following [HSW22], we use
(3.19) -
•
Case . Observe that
Hence, taking the logarithms of both sides and dividing by , we obtain
-
•
Case , where . It follows from
that
-
•
Case . One has
and thus
-
•
Case . As in [HSW22], we have
(3.20) -
•
Case . By [HSW22], we know
(3.21) -
•
Case . Finally, as per [HSW22], we use the bound
(3.22)
3.3. Defining
We start recalling some auxiliary functions already defined in [HSW22] which will appear in the definition of . For , we let , with , and . We define
(3.23) |
and
(3.24) |
3.4. Conclusion
From (3.4) and (3.5), following [HSW22], if we use Lemma 2.1 we obtain
(3.29) | ||||
and hence, being , we have
(3.30) | ||||
If instead we use Lemma 2.3, we have
(3.31) | ||||
As in [Tru14, HSW22], we define
(3.32) |
Now, we let , and be positive real numbers satisfying444Note that . Indeed, by the definition of , if we take , then by the assumption (3.33).
(3.33) |
and . To bound , we consider the splitting
First, we recall two estimates [HSW22] for defined in (3.23) and defined in (3.24) which hold for and . Defining, for ,
we have
(3.34) |
and
(3.35) |
Now, we proceed with the estimate of each integral as in [HSW22] to derive
(3.36) |
(3.37) | ||||
(3.38) | ||||
(3.39) | ||||
and
(3.40) | ||||
Observe that
(3.41) | ||||
Hence, for every , we have
(3.42) | ||||
Finally, we have
(3.43) | ||||
With the above estimates in hand, we are ready to estimate the constants.
3.4.1. Constant
Setting
we can express as
(3.44) |
3.4.2. Constants and
3.4.3. Constants and
4. Proof of Theorem 1.4
5. Proofs of Theorem 1.1 and Corollary 1.5
First, we apply Theorem 1.2 and Theorem 1.4 with . Furthermore, we take , and we choose the following parameters :
The first row of Table 2 gives Theorem 1.1 and Corollary 1.5 for .
For , in order to estimate , we use the known bound (1.2) computed by Platt, which is in particular sharper than
for every . Hence, Corollary 1.5 follows by combining the two cases.
Now, it remains to prove Theorem 1.1 when . As per [HSW22], since
(5.1) |
for we have
(5.2) |
which is always smaller than
for every . Hence, combining the two cases, Theorem 1.1 follows.
6. Proof of Corollary 1.6
Since
(6.1) |
one has
(6.2) |
and
(6.3) | ||||
Writing
and using the Taylor expansions at and
with , , , we have, for ,
(6.4) | ||||
and, similarly,
(6.5) | ||||
Furthermore,
(6.6) | ||||
Finally, if , then Theorem 1.4 implies that
(6.7) |
and
(6.8) |
while if , by (1.2) we get
(6.9) |
and
(6.10) |
Substituting the estimates we found above into (6.2) and (6.3), we can conclude that, for , one has
(6.11) | ||||
and
where
On the other hand, if then
(6.12) |
and
(6.13) |
Finally, it remains to find the lower bounds. Similarly to what we did in (6.4), (6.5),
(6.14) |
and
(6.15) |
It follows that, for ,
(6.16) | ||||
where
On the other hand, if , then
and
Remark.
The goes inside the approximation of the last decimal place in the various constants.
Acknowledgments
The authors thank Andrew Fiori, Nathan Ng, David Platt and Tim Trudgian for the helpful discussions and comments. The first author also thanks the organizers of the workshop “Analytic and Explicit results of zeros of -functions” (Bȩdlewo, September 23-27, 2024), where helpful discussions with David Platt took place.
References
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Appendix A A Numerical Study
Andrew Fiori 555
Department of Mathematics and Statistics, University of Lethbridge,
4401 University Drive,
Lethbridge, Alberta,
T1K 3M4,
Canada
Andrew Fiori’s Research is supported by NSERC Discovery Grant RGPIN-2020-05316.
Under the Riemann Hypothesis one expects a bound of the form:
(A.1) |
However, it is conjectured in [FGH05] that the actual size is:
(A.2) |
One goal of this appendix is to provide numerical evidence for this stronger conjecture. A second goal is to provide useful input for future works to improve upon effective bounds on by summarizing what is known using the work of [Pla16]. We provide such a result in Theorem A.4.
Here we study by using the list of the zeros for the zeta function as computed by [Pla16] and made available at [Lmf]. This database of the first many zeros is broken up into 14 580 intervals. For practical reasons we analyze the data using these intervals. We note that although [PT21] has verified RH to , they have not produced a database of zeros.
We shall denote the imaginary part of the th zero, ordered by height . Because all the zeros up to are simple we know that in the interval under consideration .
A.1. Average Values
Observation A.1.
On each of the intervals of zeros produced by [Pla16], the average value of the function
evaluated at the zeros, , of zeta in that interval is approximately .
Excluding the first two intervals, where the deviation from the average is respectively and ,
on each of the intervals the deviation of these average values from is bounded by .
A.2. Range of Values
Proposition A.2.
On any interval beginning and ending at zeros of the maximum value of
will be taken at , the exact ordinate of a zero of . Moreover, if all zeros on the interval are simple, then the infimum of
will be exactly less than the value takes on at , the exact ordinate of a zero of .
Proof.
Notice that the respective functions are continuous and decreasing on any interval between consecutive zeros and that
The results follow immediately. ∎
As a result of the above, we focus our attention on the study of minimum values of and maximum values of at zeta zeros.
Observation A.3.
Theorem A.4.
For we have
Proof.
This is an immediate consequence of the previous observation and proposition. ∎
A.3. Extreme Values are Rare
The following observation says that in some sense extreme values are rare.
Observation A.5.
The function is almost always negative, indeed, it is negative at all zeros with except for those listed in Table 3. Similarly, the function is almost always positive, indeed, it is positive at all zeros with for those listed in Table 3. We notice that the frequency of the extreme values is decreasing as both and increase. We also note that there are no examples of consecutive extreme values.
7330779 | 3745331.534911 | 0.0045727 |
10014001 | 4998855.443421 | 0.0228842 |
30930930 | 14253736.600191 | 0.0215612 |
106941331 | 45420475.080263 | 0.0548687 |
121934174 | 51361501.783167 | 0.0633788 |
342331986 | 135399343.427052 | 0.0852310 |
486250460 | 188404036.065583 | 0.0077204 |
1333195695 | 487931556.151002 | 0.0711065 |
1819794287 | 654800601.959837 | 0.0016382 |
2953463649 | 1035537870.147914 | 0.0920937 |
4711070126 | 1611978781.026883 | 0.0552043 |
6020412879 | 2034221491.431262 | 0.0040533 |
6276413932 | 2116223525.742432 | 0.0136917 |
6916958115 | 2320709265.610272 | 0.0183240 |
7895552868 | 2631384288.230762 | 0.0134043 |
18019870103 | 5765666759.059866 | 0.0101465 |
29425625937 | 9196418366.325099 | 0.0141895 |
31587712923 | 9839079152.616086 | 0.0169750 |
43668302178 | 13396993184.932842 | 0.0314554 |
44121363503 | 13529486654.222228 | 0.0049450 |
71876944166 | 21550885080.446041 | 0.0076388 |
100093914039 | 29565113205.570534 | 0.0184384 |
337917 | 223936.368134 | -0.0206077 |
2009961 | 1137116.070608 | -0.0268423 |
10869861 | 5393528.443012 | -0.0021561 |
13999527 | 6820051.890986 | -0.0219395 |
37592217 | 17095484.271828 | -0.0359387 |
83088045 | 35862210.311523 | -0.0463096 |
88600097 | 38084045.549954 | -0.0491801 |
141617808 | 59096901.323297 | -0.0082036 |
164689303 | 68084444.336913 | -0.0322461 |
191297537 | 78359876.488247 | -0.0148321 |
225291159 | 91369499.494965 | -0.0092099 |
566415149 | 217536164.326180 | -0.0121163 |
1081300142 | 400354486.072002 | -0.0593335 |
1257893678 | 461849910.598599 | -0.0262264 |
1372703319 | 501584522.950737 | -0.0002137 |
1955876862 | 701027396.312615 | -0.0096394 |
2305634166 | 819113670.556185 | -0.0026561 |
5134032906 | 1748936581.577121 | -0.0142280 |
5136505385 | 1749735519.272913 | -0.0508501 |
8864769308 | 2937266043.546390 | -0.0418297 |
9430966584 | 3115208316.829027 | -0.0490178 |
9532704476 | 3147127461.727906 | -0.0055879 |
18629248201 | 5951053644.636571 | -0.0008106 |
19859326408 | 6324431638.934122 | -0.0452773 |
21082098810 | 6694540279.310641 | -0.0362361 |
22909699222 | 7245905144.854708 | -0.0030872 |
48227304665 | 14727556977.258993 | -0.0827069 |
77728515578 | 23222574401.823281 | -0.0515078 |
86585440777 | 25742609309.393488 | -0.0073926 |
87198634344 | 25916653877.755976 | -0.0017881 |
97495263831 | 28831591819.434777 | -0.0222335 |
103274388030 | 30461757456.864450 | -0.0421276 |
Conjecture A.6.
One could make a variety of conjectures of different strengths based on Table 3.
-
(1)
The number of extreme values up to height is less than for some constant .
-
(2)
The set of for which these functions are respectively positive or negative has natural density zero.
A.4. Extreme Values are Common
The following observation says that in some sense extreme values are common.
Observation A.7.
If for each interval of zeros produced by [Pla16], we compute the maximum value of on that interval, then the minimum of these values is .
Similarly, if for each interval of zeros produced by [Pla16] we compute the minimum value of on that interval, then the maximum of these values is .
For context note that is approximately and is approximately .
In particular, for each interval the function
takes on values relatively close to both the theoretical upper and lower extremes under consideration.
A.5. Clusters of Zeros
One common use of estimates on is to bound the number of zeros on an interval. The quality of the bounds one obtains using bounds on improves with . Consequently, it is useful to have explicit bounds on the number of zeros in intervals for small .
Observation A.8.
For , the maximum value for happens around where . Consequently, on this interval
Moreover, for each the smallest value of for which is given in Table 4, from which one may bound with a step function, or any other function which happens to exceed that step function.
n | t |
---|---|
1 | 13.1347251417346937904572 |
2 | 48.7738324776723021819167 |
3 | 356.952685101632273755128 |
4 | 2261.87830538116111223015 |
5 | 27134.3628475733906424560 |
6 | 221227.766664702101313669 |
7 | 2603074.61468824424587333 |
8 | 21297085.9439615105210553 |
9 | 254721517.418748602610351 |
10 | 2786055796.5252751861828 |
11 | 29731208527.9429140229012 |
12 | larger than 30610045999 |