1. Introduction
Recall that the
mth harmonic number is the sum of the reciprocals of the first
m positive integers:
Harmonic numbers appear frequently in many different areas, such as combinatorial problems, expressions involving special functions in analytic number theory, probability and statistics, analysis of algorithms, etc. Sometimes they appear unexpectedly [
1], but they mainly can be found in many beautiful identities. For instance, in 1775, Euler proved the following identity:
where
is the Riemann zeta function. See, e.g., [
2,
3], for a short proof of this and similar identities involving zeta functions, logarithms and polylogarithms. In [
4], there are many identities of a different type, such as the following:
for
. Other more complicated identities have been proven with the help of computers. See also [
5,
6,
7].
It is well known that
is the only integer among all the harmonic numbers
(see, e.g., Section 1.2.7 in [
8]). Thus, the fractional parts of other harmonic numbers
, where
, all belong to the open interval
. Note that the
mth harmonic number can be written in the form
, where
is the least common multiple of the integers
and
. Here,
and
are not necessarily coprime. In [
9], Wu and Chen conjectured that
for infinitely many
. This conjecture is still open despite some progress in [
10], showing that
cannot be too large for all
m. In the opposite direction, the set of
for which
has been recently studied by Yan and Wu [
11].
In particular, from the representation
, even in the worst case, when there is no cancellation by the factor
, it follows that
for each
. By the prime number theorem, it is well known that
as
. This gives the exponential bound
for each positive constant
and each sufficiently large integer
m. Calculations show that this bound is far from optimal. However, the question of whether this bound can be replaced by the bound
is completely open (see, e.g., Question 258097 at MathOverflow). One should also mention recent progress on the question of Erdős and Graham [
12], who were interested in the question of how close the difference
can be to 1. In [
13], it was shown that for any
, there are infinitely many pairs of positive integers
such that
.
Since
as
, the sequence of the fractional parts
,
, is everywhere dense in
. However, as
tends to a finite limit
, which is called
Euler’s constant, and the sequence
,
, is not uniformly distributed modulo 1, the sequence of the fractional parts
,
, is not uniformly distributed in
. For a sequence
,
, which is uniformly distributed in
, one has the following:
We do not have this property for , so it seems a natural problem to investigate the limit points of the sequence of arithmetic means , . In this paper, we determine the upper and lower limits of this sequence and show that all its possible limit points consist of the closed interval between them.
Theorem 1 follows from the following more general result:
Theorem 2. For each , we havewherefor each . Indeed, since the sequence of the fractional parts
,
, is everywhere dense in the closed interval
, by (
1) and (
2), the set of limit points of the sequence of arithmetic means,
,
, is actually the set of all values attained by the function
for
. Since
is continuous in
, the latter set is obviously the following closed interval:
In particular, for
, the function
defined in (
2) equals
In the closed interval , the maximum of is attained at and at and equals . The minimum of is attained at the point and is equal to the same value . Consequently, all limit points of the sequence , , form the closed interval , which implies Theorem 1.
Observe that, for any fixed
, the derivative of the function
in
equals
, such that
is increasing in
from a negative value at
to a positive value at
. (The inequality
is immediate, while the inequality
follows from
.) By continuity, this implies that there is a unique
in
satisfying
such that
for
and
for
. Therefore, the function
is decreasing in
and increasing in
. Consequently, the maximum of
in
is attained at
or at
. Since
, the maximum of the function
in the interval
equals
, while its minimum is
. Hence,
However, unlike in the case where
, the smallest limit point
cannot be determined by an explicit expression as before. For example, for
, we have the following:
Here,
, and hence, we obtain
The minimum of the function
in
is attained at point
satisfying the following:
where
. Therefore,
In fact, we will prove a result more precise than that stated in Theorem 2, which not only gives the asymptotical Formula (
1) but also an estimate for the error term:
Theorem 3. For each , with the notation of Theorem 2, we havefor some constant independent of n. In the next section, we prove several auxiliary results. The proof of Theorem 3 is given in
Section 3. Finally, in
Section 4, we will show that
in (
1) can be replaced by a more general function
with an appropriate change in the definition of
in (
2); see (
29). Some examples of
f giving explicit upper and lower limits for the sequence
,
, will be presented there as well.
4. Concluding Remarks
In the proof of Theorem 3 and Lemma 3, we mainly used the fact that the function
is continuous, non-negative and non-decreasing in
, implying that the function
is as well. By exactly the same argument, one can show that, for every continuous, non-negative and non-decreasing function
f in
, we have
where
for each
. (The specific form of
f, namely
, has been used only in the estimate of the error term as in Theorem 3, which we will not do for a general
f.)
Thus, Theorem 2 can be generalized as follows:
Theorem 4. Let be an absolutely continuous function on . Then,as , where is defined in (29). Indeed, since
f is absolutely continuous, it is a function of bounded variation. (The definition and basic properties of functions of bounded variation can be found in the following monographs [
17,
18]). Next, every function of bounded variation is the difference between two monotonically non-decreasing functions. Adding an appropriate positive constant to both of them, we conclude that
f is expressible in the form
where the functions
and
are both continuous, positive, and non-decreasing in
. In view of (
29), we clearly have
Thus, applying the asymptotic Formula (
28) to
and
and then subtracting one formula from another, we derive Theorem 4.
Selecting in (
29), for instance,
, we find that
The maximum of this function for
is attained at
and
and equals
, while its minimum is attained at
and equals
. Hence, by Theorem 4, it follows that
and
Likewise, selecting in (
29), for instance,
, we obtain
This time, unlike in all previous examples, not the maximum but the minimum of the function
is attained at
and
, and it equals
. Its maximum is attained at
and equals
. Therefore, by Theorem 4,
and