1. Introduction and Background
In this article, we employ the calculus on time scales to prove some properties of Muckenhoupt and Gehring weights and some relations between them. The study of dynamic equations and inequalities on time scales has been developed by Stefan Hilger in [
1]. The two books by Bohner and Peterson [
2,
3] have summarized and organized most time scale calculus. A time scale
is an arbitrary nonempty closed subset of
the set of real numbers. The three well-known time scale calculus are differential calculus when
, differential calculus when
and quantum calculus when
We assume that a time scale
has the topology that it is inherited from the standard topology on
, the set of real numbers. The backward and forward jump operators defined on
are given by
and
, respectively, where
. We define the time-scale interval
by
. The graininess function
for a time scale
is defined by
, and for any function
, the notation
denotes
. Recall the following product and quotient rules for the derivative of the product
and the quotient
of two (delta) differentiable functions
and
where
, and
. The (delta) integral is defined as follows: If
, then the delta integral of
is given by
. The Cauchy integral
exists,
, and satisfies
for
. A simple consequence of Keller’s chain rule is given by (see [
2])
and the integration by parts formula on time scales is given by
We say that
belongs to
provided that
Hölder’s inequality on time scales is given by
for
and
and
. We say that
satisfies a reverse Hölder inequality if for
there exists a constant
such that the inequality
holds for
. The Jensen inequality for convex functions is given by
A special case of (
6), when
we have the inequality
for
or
, and for
, we have that
We assume that a weight
is a non-negative locally
-integrable weight defined on
and
be a positive real number and
and denote by
the Lebesgue
-measure of
S.
The non-negative weight
is said to belong to the Muckenhoupt class
for
and
(independent of
) if the inequality
The weight
is said to belong to the Muckenhoupt class
if the inequality
The weight
is said to belong to the Muckenhoupt class
if the inequality
The weight
is said to belong to the Gehring class
(satisfies the reverse Hölder inequality) for
and
(independent of
) if the inequality
holds for every subinterval
. The weight
is said to belong to the Gehring class
if the inequality
holds for every
. The weight
is said to belong to the Gehring class
if the inequality
holds for every
. We note that when
, the class
becomes the classical Muckenhoupt class
of functions that satisfy
for
and
(independent of
) and
. In [
4], Muckenhoupt proved that if
and
satisfies the
-condition (
11), with constant
, there exist constants
and
depending on
and
such that
and
satisfies the
-condition
for every
Muckenhoupt’s result (see also Coifman and Fefferman [
5]), which is the
self-improving property states that if
, then there exists a constant
and a positive constant
such that
and
We note that when
, the class
becomes the classical the Gehring class
, of functions that satisfy
for
and every
. Gehring in [
6] proved that if (
14) holds, then there exist
and a positive constant
such that
In other words, Gehring’s result for the
self-improving property states that if
, then there exist
and a positive constant
such that
and then
The relations between Gehring and Muckenhoupt classes (inclusions properties) was given by Coifman and Fefferman in [
5]. In [
7,
8], the author proved that any Gehring class is contained in some Muckenhoupt class and vice versa. In other words, they proved the following inclusions
and
For more details of the structure of the Muckenhoupt and Gehring classes of weights, we refer the reader to the recent paper [
9,
10] and the references cited therein.
When
, the class
becomes the classical Muckenhoupt class
of sequences. A discrete weight on
is a sequence
of non-negative real numbers. The
space is the Banach space of sequences defined on
and is given by
A discrete non-negative sequence
belongs to the discrete Muckenhoupt class
for
and
if the inequality
holds for every
A discrete weight
belongs to the discrete Muckenhoupt class
for
and
if the inequality
holds for every subinterval
and
is the cardinality of the set
A discrete weight
is said to be belongs to the discrete Muckenhoupt class
for
and
if the inequality
holds for every subinterval
. Ariño and Muckenhoupt [
11] proved that if
is nonincreasing and satisfies (
21), then the space
is the dual space of the discrete classical Lorentz space
where
is the nonincreasing rearrangement of
and
is the conjugate of
The class
has been used by Pavlov [
12] to give a full description of all complete interpolating sequences on the real line. In [
13], the authors proved that if
is a nonincreasing sequence and satisfies (
21) for
, then for
, the inequality
holds for every subinterval interval
. We also note that when
, the class
becomes that the discrete Gehring class
of discrete weights that satisfy the reverse Hölder inequality
for a given exponent
and a constant
, for every subinterval
. In [
14], Böttcher and Seybold proved that if
satisfies the Muckenhoupt condition, then there exist a constant
and
depending only on
and
such that the reverse of the Hölder inequality
holds (
a transition property) for all
and all
of the form
with
.
The authors in [
15] mentioned that what goes for sums goes, with the obvious modifications, for integrals, which in fact proved the first part of the basic principle of Hardy, Littlewood, and Polya [
16] (p. 11).
Indeed, the proofs for series translate immediately and become much simpler when applied to integrals, but the converse sometimes is not true.
In recent years, increasing interest has been paid to the study of properties of Muckenhoupt and Gehring weights on time scales. For example, the authors used the tools on time scales and proved the self-improving properties of the Muckenhoupt and Gehring weights in [
13] and proved some higher integrability theorems on time scales in [
17]. Motivated by this work, the natural question that arises now is:
Is it possible to prove some new properties of Muckenhoupt and Gehring weights on time scales, which, as special cases, cover the properties of the continuous and discrete Muckenhoupt and Gehring weights?
In this paper, we give an affirmative answer to this question. Our main results are valid on different types of time scales, like
,
and the quantum space
. This paper is organized as follows: In
Section 2, we state and prove some basic lemmas that will be needed in the proof of the main results. Some fundamental properties of the Muckenhoupt and Gehring classes on time scales are provided in
Section 3. In
Section 4, we prove some essential relations between the norms (will be defined later) of these classes on time scales. Our results as particular cases when
cover the results following David Cruz-Uribe [
18], Neugebauer [
19], and Popoli [
20].
Our motivation for proving these results is our belief of the great importance of the applications of the fundamental properties of the Muckenhoupt and Gehring classes in developing the boundedness of operators and extrapolation theorems on time scales. The applications of class of functions of Muckenhoupt’s type have appeared in weighted inequalities in the 1970s, and the full characterization of the weights
w for which the Hardy–Littlewood maximal operator is bounded on
by means of the so-called the Muckenhoupt
-condition on the weight
w has been achieved by Muckenhoupt (see [
4]).
The result of Muckenhoupt became a landmark in the theory of weighted inequalities for classical operators like the Hardy operator, the Hilbert operator, Calderón-Zygmund singular integral operators, fractional integral operators, etc. On the other hand, the extrapolation theorems following Rubio de Francia, that are announced in [
21], and the detailed proof given in [
22], have been proved by the properties of
-Muckenhoupt weights. The integrability properties of the gradient of quasiconformal mappings of functions has been developed by Gehring [
6] in connection with the properties of weights satisfying the reverse Hölder inequality (Gehring weights).
2. Some Essential Lemmas
Throughout this section, we assume that a weight is a non-negative locally -integrable function defined on .
Definition 1. We define the operator , for any non-negative weight θ, byfor any real number , where . We note that when
, and
, the operator (
25) becomes the integral Hardy operator
which has been studied by Ariňo and Muckenhoupt [
23] on the space
and the characterizations of the weighted function
u in connection with the boundedness of Hardy operator (
26) have been established. When
, and
, the operator (
25) becomes the discrete Hardy operator
The authors in [
24] proved that the Hardy operator (
27) is bounded in
if and only if
. In the following lemma, we state and prove some basic properties of the operator
, which will be needed in the proof of the main results.
Lemma 1. If is a non-negative weight and α, are real numbers, then the following properties hold:
- (1)
.
- (2)
for all
- (3)
for all
- (4)
for all
Proof. By applying inequality (
7) with
, we have
Then,
which is the desired result.
By applying inequality (
7) with
, we have
Then,
which is the desired result.
Since , we consider the two cases: and .
If
, by applying inequality (
7) with
, then we have
By taking into account that
is negative, we have
If
, by applying inequality (
8) with
, then we have
Then,
This is the desired result.
We discuss three cases: , , and .
If
, then
, and hence using property
, we have
. That is,
Thus,
If
, then
, and hence, using Property
, we have
. That is,
Thus, by taking into account that
is negative, we have
If
, then
, and hence using Property
, we have
. That is,
Thus,
From these three cases, we obtain the desired result. The proof is complete. □
Lemma 2. Let β be a positive real number. If for and , then , and consequently, for all .
Proof. Since
then for every interval
, for
and
we have that
By the definition of the operator
, (
28) is written as
Furthermore, by Property
in Lemma 1, we have
for all
. By using (
29) and (
30), we obtain
for
and all
. This is the desired result. The proof is complete. □
In the following, we prove some basic properties of the Muckenhoupt -weights and the Gehring -weights on time scales.
Lemma 3. If , and , thenholds. Proof. Since
on time scales, for
, we have
for all
. By applying Jensen’s inequality for the convex function
and
replaced by
we have
The left-hand side of (
34) can be written as follows:
From (
34) and (
35), we obtain
and then
From (
33) and (
36), we obtain
which is the desired inequality. The proof is complete. □
Remark 1. The lemma proves the inclusion of the Muckenhoupt classes for in the -class.
Lemma 4. Let θ be a non-negative weight and β be a non negative number. If for , thenholds for all Proof. If
for
, then there exists
such that
for all
, or equivalently
Taking the limit in (
38) as
tends to 1, we obtain
The proof is complete. □
Remark 2. This lemma proves the inclusion of the Gehring’s classes of weights in the -class.
3. Properties of Muckenhoupt and Gehring Classes
In this section, we prove some basic inclusion properties of Muckenhoupt and Gehring classes on time scales.
Theorem 1. Let θ be a non-negative weight and α and β be positive real numbers. Then, the following inclusion properties of Muckenhoupt classes hold:
- (1)
for all
- (2)
Let then
- (3)
with and
Proof. Assume that
, then there exists a constant
such that for all
, we have that
Since
, we see that
and then using Property
in Lemma 1, we have that
Then, for all
we obtain that
which implies that
.
Since
, then there exists
such that for all
, we have
By using (
39), we have for all
that
which implies that
and then
Now, assume that
, for
. Then, by applying Lemma 3, we have
That is,
, which implies
.
By Property
, for any
,
. Then,
Conversely assume that
and assume, on the contrary, that for all
,
. Then, for all
, we see that
which, by taking the limit as
, tends to
∞ implies that
This contradicts the assumption that
. Then,
implies that
for some
, and hence
Thus,
From (
40) and (
41), we obtain
By Property
, for any
then
The proof is complete. □
Theorem 2. Let be a non-negative weight and α and β be non-negative real numbers. Then, the following inclusion properties of Gehring classes hold:
- (1)
for all
- (2)
for all
- (3)
with
Proof. If
on a time scale, then there exists
such that for all
, the inequality
holds. Property (4) in Lemma 1 implies that
for all
. Then, for
we have
Then, by substituting (
43) into (
42), we have
That is,
, which is the desired result.
If
then by the definition of
there exists
such that for all
holds. For all
by applying (
44), we have
That is,
, and hence
and the inclusion
are proved in Lemma 4. This is the desired result.
From Property
, we have that
for all
and then
Conversely, let
and assume, on the contrary, that
for all
. That is, for all
, we have
Taking the limit on both sides of (
46) as
tends to
we have
This contradicts the assumption that
, which implies that
for some
and then
From (
45) and (
47), we have
. The proof is complete. □
Here, we prove some additional properties of the Muckenhoupt classes of weights on time scales. We define the
-norm of the weight
on time scales by
and we define
-norm on time scales by
We define the
-norm on time scales by
and the
-norm is defined by
Theorem 3. Let be a non-negative weight and α and β be positive real numbers. Then, the following properties hold:
- (1)
if and only if with where is the conjugate of
- (2)
If for , then for each such that
Proof. From the definition of the class
and since
we have for
that
with
This is the desired result.
Let
and
, then
and by applying Lemma 1 for
. Then, we have
hence,
. This is the desired result. This completes our proof. □
In the next theorem, we discuss the power rule for weights in the Muckenhoupt classes on time scales.
Theorem 4. Let be a positive real number. Then, the following properties hold:
- (1)
If then for with
- (2)
If then for with
Proof. For
and
on time scales, we have
, and by Lemma 1 for
for all
, we have
that is,
, with
. This is the desired result.
Since
, on time scales, we obtain that
and
where
. By applying Hölder’s inequality on time scales (note that
) with
and
and using (
48) and (
49), we have
By applying the Hölder inequality on time scales with
and
on the term
we have
By substituting (
51) into (
50), and since
, we have
This proves that
implies that
, for
, with
The proof is complete. □
Theorem 5. Let be a non-negative weight and α be a non negative real number. If , then
Proof. Let
then there exists a constant
such that the inequality
holds for all
. From Property
in Lemma 1, we have
and (
52) becomes
That is,
The proof is complete. □
Theorem 6. Suppose that and Then, the following properties hold:
- (1)
If then - (2)
If then
Proof. Since
, then
for all
. By applying Hölder’s inequality on time scales with
and
we obtain
Since
, we can easily see that
and by using the fact that
, we have
and then
From (
57) and by applying Hölder’s inequality on time scales with
and
, and taking into account that
, we obtain
By using (
56) and (
58), (
55) becomes
Taking supremum over all
, we obtain the desired result (
53).
Assume that
then
For
, we have
and hence (
59) can be written as
By applying Hölder’s inequality on time scales with exponents
and
we obtain
and by applying Hölder’s inequality on time scale with exponents
and
and taking into account that
, we obtain
By substituting (
61) and (
62) into (
60), we have
Taking supremum over all
, we obtain the desired result (
54). The proof is complete. □
Theorem 7. Let be a positive real number. Then, the following properties hold:
- (1)
If then for with and - (2)
if and only if and are in
Proof. Assume that
then
for all
. Note that
and
then by letting
, we have
and (
63) can be written as
By applying Hölder’s inequality on time scales with exponents
and
we obtain
and
By substituting (
65) and (
66) into (
64), we have
Taking supremum over all
, we obtain the desired result
Using Property (3) in Theorem 1, since , it is clear that for some , if and only if . Now, we have by Property (1) in Theorem 3 that if and only if . That is, (since ) if and only if . The proof is complete. □