Volume 2022, Issue 1 9021391
Research Article
Open Access

Atomic Decompositions and John-Nirenberg Theorem of Grand Martingale Hardy Spaces with Variable Exponents

Libo Li

Libo Li

College of Mathematics and Computing Science, Hunan University of Science and Technology, Xiangtan, Hunan 411201, China hnust.edu.cn

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Zhiwei Hao

Corresponding Author

Zhiwei Hao

College of Mathematics and Computing Science, Hunan University of Science and Technology, Xiangtan, Hunan 411201, China hnust.edu.cn

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First published: 19 January 2022
Citations: 1
Academic Editor: Tianqing An

Abstract

Let θ ≥ 0 and p(·) be a variable exponent, and we introduce a new class of function spaces Lp(·),θ in a probabilistic setting which unifies and generalizes the variable Lebesgue spaces with θ = 0 and grand Lebesgue spaces with p(·) ≡ p and θ = 1. Based on the new spaces, we introduce a kind of Hardy-type spaces, grand martingale Hardy spaces with variable exponents, via the martingale operators. The atomic decompositions and John-Nirenberg theorem shall be discussed in these new Hardy spaces.

1. Introduction

The martingale theory is widely studied in the field of mathematical physics, stochastic analysis, and probability. Weisz [1] presented the atomic decomposition theorem for martingale Hardy spaces. Herz [2] established the John-Nirenberg theorem for martingales. Since then, the study of martingale Hardy spaces associated with various functional spaces has attracted a steadily increasing interest. For instance, martingale Orlicz-type Hardy spaces were investigated in [36], martingale Lorentz Hardy spaces were studied in [79], and variable martingale Hardy spaces were developed in [1014].

Let 1 < p < ∞, and the grand Lebesgue space Lp)(E) introduced by Iwaniec and Sbordone [15] is defined as the Banach function space of the measurable functions f on finite E such that
(1)

Such spaces can be used to integrate the Jacobian under minimal hypotheses [15]. The grand Lebesgue spaces as a kind of Banach function space were investigated in the papers of Capone et al. [16, 17], Fiorenza et al. [1821], Kokilashvili et al. [22, 23], and so forth. In particular, grand Lebesgue spaces with variable exponents were studied in [24, 25].

We find that the framework of grand Lebesgue spaces with variable exponents has not yet been studied in martingale theory. This paper is aimed at discussing the variable grand Hardy spaces defined on the probabilistic setting and showing the atomic decompositions and John-Nirenberg theorem in these new Hardy spaces. More precisely, we first present the atomic characterization of grand Hardy martingale spaces with variable exponents. To do so, we introduce the following new notations of atom.

Definition 1. Let p(·) be a variable exponent and θ ≥ 0. A measurable function a is called a (1, p(·), θ) -atom (resp. (2, p(·), θ) -atom, (3, p(·), θ) -atom) if there exists a stopping time τ such that

(a1), ∀ nτ

(a2)

See Section 2 for the notation Lp(·),θ. Denote by (resp. , ) the collection of all sequences of triplet (ak, τk, μk), where ak are (1, p(·), θ)-atoms (resp. (2, p(·), θ)-atoms, (3, p(·), θ)-atoms), τk are stopping times satisfying (a1) and (a2) in Definition 1, and μk are nonnegative numbers and also
(2)
Under these definitions, we show the atomic decompositions of the grand Hardy martingale spaces with variable exponents (see Section 3). To be precise, we prove that for any , (resp. Qp(·),θ, Dp(·),θ) iff there exists a sequence of triplet (resp. , ) so that for each n ≥ 0,
(3)
Moreover, we extend the classical John-Nirenberg theorem to the grand variable Hardy martingale spaces. To be precise, under suitable conditions, we present the following one:
(4)

See Theorem 11 for the details. This conclusion improves the recent results [12, 26], respectively.

Throughout this paper, , , and denote the integer set, nonnegative integer set, and complex numbers set, respectively. We denote by C the absolute positive constant, which can vary from line to line. The symbol AB stands for the inequality ACB. If we write AB, then it stands for ABA.

2. Preliminaries

2.1. Grand Lebesgue Spaces with Variable Exponents

Let be a probability space. An -measurable function p(·): Ω⟶(0, ∞) which is called a variable exponent. For convenience, we denote
(5)
Denote by the collection of all variable exponents p(·) satisfying with 1 < pp+ < ∞. The variable Lebesgue space Lp(·) = Lp(·)(Ω) consists of all -measurable functions f such that for some λ > 0,
(6)
This leads to a Banach function space under the Luxemburg-Nakano norm
(7)

Based on this, we begin with the definition of the grand Lebesgue space with variable exponent.

Definition 2. Suppose that and θ ≥ 0. We define the grand Lebesgue space with variable exponent Lp(·),θ = Lp(·),θ(Ω) as the set of all -measurable functions f satisfying

(8)

The Grand Lebesgue space with variable exponent can unify and generalize the various function spaces. To be precise, if θ = 0, Lp(·),θ degenerates to the variable Lebesgue space Lp(·). If θ = 1 and p(·) ≡ p, Lp(·),θ becomes the grand Lebesgue space Lp).

2.2. Martingale Grand Hardy Spaces via Variable Exponents

Let be a nondecreasing sequence of sub-σ-algebras of sets with . The expectation operator and the conditional expectation operator relative to are denoted by and , respectively. A sequence of random variables is said to be a martingale, if fn is -measurable, , and for every n ≥ 0. Denote to be the set of all martingales with respect to such that f0 = 0. For , write its martingale difference by dnf = fnfn−1(n ≥ 0, f−1 = 0). Define the maximal function, the square function, and the conditional square function of f, respectively, as follows:
(9)
Let Γ be the set of all sequences of nondecreasing, nonnegative, and adapted functions, and . For , , and θ ≥ 0, denote
(10)
Now we introduce the grand martingale Hardy spaces associated with variable exponents as follows:
(11)
The bounded Lp(·),θ-martingale spaces
(12)
where
(13)

Remark 3. If θ = 0, then we obtain the definitions of , , , Qp(·), and Dp(·), respectively (see [10, 12, 27]). If we consider the special case θ = 1 and p(·) ≡ p with the notations above, we obtain the definitions of , , , Qp), and Dp), respectively (see [26]). In addition, if p(·) ≡ p and θ = 0, we obtain the martingale Hardy spaces , , , Qq, and Dq, respectively (see [28]).

Refer to [29, 30] for more information on martingale theory.

3. Atomic Characterization

The method of atomic characterization plays an useful tool in martingale theory (see for instance [1, 4, 6, 3133]). We shall construct the atomic characterizations for grand Hardy martingale spaces with variable exponents in this section.

Theorem 4. Let and θ ≥ 0. If the martingale , then there exists a sequence of triplet so that for each n ≥ 0,

(14)
(15)

Conversely, if the martingale f has a decomposition of (14), then

(16)
where the infimum is taken over all the admissible representations of (14).

Proof. Let . Now consider the stopping time for each k:

(17)

It is easy to see that the sequence of these stopping times is nondecreasing. For each stopping time τ, denote . It is easy to write that

(18)

For each k, let . If μk ≠ 0, we set

(19)

If μk = 0, we set for each n. For each fixed k, is a martingale. Since , we get

(20)

We can easily check that is a bounded L2-martingale. Hence, there exists an element akL2 such that . If nτk, then , and . Consequently, it implies that ak is really a (1, p(·), θ)-atom.

Denote Λk≔{τk<∞}. Knowing that {τk<∞} = {s(f) > 2k} and τk is nondecreasing for each k, we obtain Λk+1Λk. Now, we point out that

(21)

Indeed, for a fixed x0Ω, there is k0 so that and , then we have

(22)

This means

(23)

For the converse part, according to the definition of (1, p(·), θ)-atom, we easily conclude

(24)
where ak is the (1, p(·), θ)-atom and τk is the stopping time associated with ak which, when combined with the subadditivity of the operator s, yields
(25)

This implies

(26)

Taking over all the admissible representations of (14) for f, we obtain the desired result.

Next, we will characterize Qp(·),θ and Dp(·),θ by atoms, respectively. The proof is similar to the proof of Theorem 4. For the completeness of this paper, we provide some details.

Theorem 5. Suppose and θ ≥ 0. If the martingale (resp. Dp(·),θ), then there exists a sequence of triplet (resp. ) so that for each n,

(27)
(28)

Conversely, if the martingale has admissible representation (27), then fQp(·),θ (resp. Dp(·),θ) and

(29)
where the infimum is taken over all the admissible representations of (27).

Proof. The proof follows the ideas in Theorem 4, so we omit some details. Suppose (resp. Dp(·),θ). We define stopping times as follows:

(30)
where is an adapted, nondecreasing sequence such that almost everywhere ∣Sn(f) | ≤λn−1 (resp.∣fn | ≤λn−1) and λLp(·),θ.

Let and be defined as in the proof of Theorem 4. And replace Λk = {τk<∞} = {s(f) > 2k} by the Λk = {τk<∞} = {λ > 2k}. Then, we obtain that and (28) still hold.

For the converse part, write

(31)

Clearly, is a nonnegative, nondecreasing, and adapted sequence with Sn+1(f) ≤ λn (resp.∣fn | ≤λn). Thus, we get

(32)

Taking over all the admissible representations of (27) for f, we obtain the desired result.

Remark 6. Suppose and θ ≥ 0. We conclude that the sum in Theorem 4 converges to f in as M⟶−∞, N⟶∞. Indeed, it follows by the subadditive of the operator s, we get, for any M, N with M < N,

(33)

Moreover, is decreasing and convergent to 0 (a.e.) as N⟶∞, and is decreasing and convergent to 0 (a.e.) as M⟶−∞. From this and the dominated convergence theorem in Lp(·)−ε for 0 < ε < p − 1 (see [34], Theorem 2.62), it follows that
(34)

Furthermore, we can also show the norm convergence of the summation in Theorems 5 as M⟶−∞, N⟶∞.

4. The Generalized John-Nirenberg Theorem

In the sequel of this section, we will often suppose that every is generated by countably many atoms. Recall that is called an atom, and if for any AB with satisfying (A) < (B), we have (A) = 0. We denote by the set of all atoms in . We shall present the generalized John-Nirenberg theorem on grand Lebesgue spaces with variable exponents. For each 1 ≤ p < ∞, the Banach space BMOp (bounded mean oscillation [35]) is defined as
(35)
It can be easily shown that the norm of BMOp is equivalent to
(36)
where consists of all stopping times relative to . It follows immediately from the John-Nirenberg theorem [2, 30] that
(37)
What is more, in [2], there has
(38)

Definition 7. For and θ ≥ 0, the generalized BMO martingale space is defined by

(39)
where
(40)

Remark 8. If θ = 0, BMOp(·),θ degenerates to the variable exponent BMO martingale space BMOp(·) introduced and studied in [12]. If θ = 1 and p(·) ≡ p, BMOp(·),θ becomes the grand BMO martingale space BMOp) studied in [26].

In order to establish the generalized John-Nirenberg theorem in the framework of BMOp(·),θ, we need the following lemmas and notations.

Lemma 9 (Hölder’s inequality, see [34]). Let satisfy

(41)

Then, there exists a constant C such that for all fLp(·) and gLq(·), we have fgLr(·) and

(42)

We mention that if the variable exponent p(x) meets the log-Hölder continuity condition in Euclidean spaces, the inverse Hölder’s inequality holds for characteristic functions in Lp(·)(n) (see [36]). Compared with Euclidean space n, the probability space (Ω, ) has no natural metric structure. Fortunately, Jiao et al. [11, 27] put forward the following condition: there exists an absolute constant κ ≥ 1 depending only on p(·) such that
(43)

Lemma 10 (see [27].)Suppose satisfying (43).

  • (1)

    For each , we get

(44)
  • (2)

    Let satisfy (43). If r(·) satisfies

(45)
then r(·) also satisfies condition (43). Moreover, for each , we deduce
(46)

Theorem 11. Suppose that satisfies (43) and θ ≥ 0. Then, for every f ∈ BMO1, there has

(47)

Proof. If satisfies (43), then we clearly get that p(·) − η also satisfies (43) for 0 < η < p − 1. It follows from Lemmas 9 and 10 that

(48)
for any 0 < η < p − 1. Here, the variable exponent (p(·) − η) is defined by
(49)

This is equivalent to the following inequality:

(50)

Hence, we have

(51)

Taking the supremum over all stopping times, we deduce

(52)

Conversely, from the definition of Lp(·),θ, we get

(53)

It follows from Lemma 9 that

(54)
where q(·) satisfies
(55)

Hence, by (38), we deduce that

(56)

From what has been discussed above, we draw the conclusion that

(57)

Theorem 11 improves the recent results [12, 26], respectively. More precisely, if we consider the case θ = 0, then the following result holds:

Corollary 12. If p(·) satisfies (43) with 1 < pp+ < ∞, then for f ∈ BMO1,

(58)

And especially for θ = 1 and p(·) ≡ p, we get the conclusion as follows.

Corollary 13 (see [26].)Suppose 1 < p < ∞, then for f ∈ BMO1,

(59)

Conflicts of Interest

The authors declare that they have no conflicts of interest.

Acknowledgments

This project is partially supported by the National Natural Science Foundation of China (Grant Nos. 11801001 and 12101223), Scientific Research Fund of Hunan Provincial Education Department (Grant No. 20C0780), and Scientific Research Fund of Hunan University of Science and Technology (Grant Nos. E51997 and E51998).

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