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Variation inequalities related to Schrödinger operators on weighted Morrey spaces

  • Jing Zhang EMAIL logo
Published/Copyright: July 31, 2019

Abstract

This paper establishes the boundedness of the variation operators associated with Riesz transforms and commutators generated by the Riesz transforms and BMO-type functions in the Schrödinger setting on the weighted Morrey spaces related to certain nonnegative potentials belonging to the reverse Hölder class.

MSC 2010: 42B20; 42B35

1 Introduction

Given a family of bounded operators 𝓣 = {Tϵ}ϵ>0 acting between spaces of functions, one of the most significative problems in harmonic analysis is the existence of limits limϵ→0+Tϵ f and limϵ→∞Tϵ f, when f belongs to a certain space of functions. A question that arises naturally is what is the speed of convergence of the above limits. A classical way to measure the speed of convergence of {Tϵ}ϵ>0 is to study “square function” of the type (i=1|TϵifTϵi+1f|2)1/2 , where ϵi ↘ 0. Recently, other expressions have been considered, among which is the q -variation operator defined by

Vq(Tf)(x):=supϵi0(i=1|Tϵi+1f(x)Tϵif(x)|q)1/q, (1.1)

where the supremum is taken over all sequence {ϵi} decreasing to zero. We denote Fq the space that includes all the functions φ: (0, ∞) → ℝ, such that

φFq=sup{ϵi}iN(i=0|φ(ϵi)φ(ϵi+1)|q)1/q<. (1.2)

Then ∥⋅∥Fq is a seminorm on Fq. It can be written that

Vq(Tϵ)(f)=TϵfFq. (1.3)

The variation for martingales and some families of operators have been studied in many recent papers on probability, ergodic theory, and harmonic analysis. We refer the readers to [1, 2, 3, 4, 5, 6] and the references therein for more background information.

Recently, Betancor et al. [7] studied the bounded behaviors of variation operators for some Schrödinger type operators in Lebesgue spaces. Precisely, let n ≥ 3 and 𝓛 = −Δ + V be the Schrödinger operator defined on ℝn associated with a fixed non-negative potential V ∈ RHs (the reverse Hölder class) for s ≥ n/2, that is, there exists C > 0 such that

(1|B|BV(x)sdx)1/sC|B|BV(x)dx (1.4)

for every ball B in ℝn. For = 1, ⋯ n, consider the -th Riesz transform in the 𝓛-context, which can be defined by

RL(f)(x)=limε0+R,εL(f)(x):=limε0+|xy|>εRL(x,y)f(y)dy,a.e.xR,

and its adjoint operator by

RL,(f)(x)=limε0+R,εL,(f)(x):=limε0+|xy|>εRL(y,x)f(y)dy,a.e.xR.

Here, for every x, y ∈ ℝn, xy,

RL(x,y)=12πR(iτ)1/2xΓ(x,y,τ)dτ,

where Γ(x, y, τ) represents the fundamental solution for the operator 𝓛+iτ (see [7, 8]).

Betancor et al. [7] proved that when n/2 ≤ s < n, for = 1, 2, ⋯, n, the variation operators Vq(R,εL) (resp., Vq(R,εL,) ) associated with the family of truncations {Rl,εL}ε>0(resp.,{R,εL,}ε>0) are bounded from Lp(ℝn) into itself for 1 < p < p0 (resp., p0 < p < ∞) with 1/p0 = 1/s−1/n, and Vq(R,εL) are of weak type (1, 1); moreover, when sn, both Vq(R,εL) and Vq(R,εL,) are bounded from Lp(ℝn) into itself for 1 < p < ∞ and of weak type (1, 1). More recently, Tang and Zhang [9] extend the results above to the weighted Lp space. They established the weighted Lp boundedness for Vq(R,εL) and Vq(R,εL,) with the weight Apγ,θ class (see section 2 for the defination), which includes the Mukenhoupt weight class. By different method, Zhang and Wu in [10] also obtained Lp boundedness for Vq(R,εL) and Vq(R,εL,) and the weighted weak type (1,1) estimation Vq(R,εL) with the weight Apγ,θ class.

In addition, for every VRHn/2, Shen [11] introduced the function γ, which is called as the critical radius and defined as

γ(x)=sup{r>0:1rn2B(x,r)V(y)dy1},xRn, (1.5)

and plays key roles in the theory of harmonic analysis operators associated to 𝓛. In [12], Bongioann et al defined the space BMOθ(γ), θ ≥ 0, as follows.

Definition 1.1

A locally integrable function b inn is BMOθ(γ) provided that

1|B(x,r)|B(x,r)|b(y)bB(x,r)|dyC(1+rγ(x))θ (1.6)

for all x ∈ ℝn and r > 0, where bB = ∣B−1 Bb(x) − bBdx. We denote for bBMOθ(γ)

bBMOθ(γ)=supxRn,r>01|B(x,r)|B(x,r)|b(y)bB(x,r)|dy(1+rγ(x))θ.

It is easy to check that BMO(ℝn) = BMO0(γ) ⊂ BMOθ(γ) ⊂ BMOθ(γ) for 0 ≤ θθ′. Set BMO(γ) = ∪θ>0BMOθ(γ). Then BMO(γ) is larger than BMO(ℝn) in general (see [12]).

For bBMO(γ) and = 1, ⋯, n, the commutators Rb,L and Rb,L, are defined by

Rb,L(f)=bRLRL(bf),andRb,L,(f)=bRL,RL,(bf)forfCc(Rn).

It was shown in [12] that, for every bBMO(γ) and = 1, ⋯, n, the operators Rb,L (resp., Rb,L, ) are bounded on Lp(ℝn), provided that 1 < p < p0 (resp., p0 < p < ∞) with 1/p0 = (1/s−1/n)+ for V ∈ RHs, sn/2. In [7], Betancor et al obtained the following point-wise representations of the commutator operators by a principal value integral:

Rb,L(f)(x)=limε0Rb,,εL(f)(x):=limε0|xy|>ε(b(x)b(y))RL(x,y)f(y)dy,a.e.xRn,

and

Rb,L,(f)(x)=limε0Rb,,εL,(f)(x):=limε0|xy|>ε(b(x)b(y))RL(y,x)f(y)dy,a.e.xRn.

Moreover, the authors in [7] proved that for every bBMO(γ) and = 1, ⋯, n, the variation operators Vq(Rb,,εL)(resp.,Vq(Rb,,εL,)) associated with the family of truncations {Rb,,εL}ε>0(resp.,{Rb,,εL,}ε>0) are bounded from Lp(ℝn) into itself, provided that 1 < p < p0 (resp., p0 < p < ∞) with 1/p0 = (1/s−1/n)+ for V ∈ RHs, sn/2. In [9], the above results have been extend to the weighted Lebesgue space.

On the other hand, in order to extend the boundedness of Schrödinger type operators in Lebesgue spaces, Pan and Tang [13] introduced the following weighted Morrey spaces related to the non-negative potential V, denoted by Lα,V,ωp,λ (ℝn).

Definition 1.2

Let k > 1, p ∈ [1, ∞), α ∈ (−∞, +∞) and λ ∈ [0, 1). For f Llocp (ℝn) and VRHq (q > 1), we say f Lα,V,ωp,λ (ℝn) provided that

fLα,V,ωp,λ(Rn)p=supB(x0,r)Rn(1+rγ(x0))αω(B(x0,kr))λB(x0,r)|f(x)|pω(x)dx<, (1.7)

where B = B(x0, r) denote a ball with centered at x0 and radius r, γ(x0) is the critical radius at x0 defined as in (1.5) and the weight function ω Apγ, .

Clearly, when α = 0 or V = 0, ω = 1 and 0 < λ < 1, the spaces Lα,V,ωp,λ (ℝn) are the classical Morrey spaces Lp,λ(ℝn), which were introduced by Morrey [14] in 1938 and were subsequently found to have many important applications to the elliptic equations (see [15, 16, 17, 18, 19, 20]), the Navier-Stokes equations (see [21, 22, 23]) and the Schrödinger equations (see [24, 25, 26, 27]) etc. When α = 0 or V = 0 and 0 < λ < 1, the spaces Lωp,λ (ℝn) is first introduced in [28], where ωAp(ℝn)(Muckenhoupt weights class). It is easy to see that Lα,V,ωp,λ (ℝn) ⊂ Lωp,λ (ℝn) for α > 0 and Lωp,λ (ℝn) ⊂ Lα,V,ωp,λ (ℝn) for α < 0. In [29], the authors established the Lα,Vp,λ (ℝn)-boundedness of the Riesz transforms Vq(RL),Vq(RL,), and the corresponding commutators with VBn/2.

Based on the above, it is a natural and interesting question whether we can establish the Lα,V,ωp,λ (ℝn)-boundedness of the variation operators aforementioned in Schrödinger setting. The main purpose of this paper is to answer this question. Our results can be formulated as follows:

Theorem 1.3

Let = 1, ⋯ n, q > 2 and VRHs. Assume α ∈ (−∞, +∞) and λ ∈ (0, 1). Then

  1. If n/2 ≤ s < n and p0 is such that 1/p0 = 1/s−1/n, then the variation operator Vq(Rl,εL,) is bounded on Lα,V,ωp,λ (ℝn) for p0 p < ∞ and ω Ap/p0γ,.

  2. If n/2 ≤ s < n and p0 is such that 1/p0 = 1/s−1/n, then the variation operator Vq(Rl,εL) is bounded on Lα,V,ωp,λ (ℝn) for 1 < pp0 and ω1p1Ap/p0γ,.

  3. If sn, then the variation operators Vq(Rl,εL,) and Vq(Rl,εL) are bounded on Lα,V,ωp,λ (ℝn) for 1 < p < ∞ and ω Apγ,

Theorem 1.4

Let = 1, ⋯, n. Assume that q > 2 and VRHs. (i) If n/2 ≤ s < n then for p = 1, η > 0 and ωp0A1γ,,

η(1+rγ(x))αω(B(x,2r))λω{yB(x,r):|Vq(R,εLf)(y)|>η}CfLα,V,ω1,λ(Rn),

(ii) If sn, then for p = 1, η > 0 and ω A1γ,,

η(1+rγ(x))αω(B(x,2r))λω{yB(x,r):|Vq(R,εLf)(y)|>η}CfLα,V,ω1,λ(Rn),

and

η(1+rγ(x))αω(B(x,2r))λω{yB(x,r):|Vq(R,εL,f)(y)|>η}CfLα,V,ω1,λ(Rn),

holds for all balls B, where C is independent of x, r, η and f.

Theorem 1.5

Let = 1, ⋯, n, q > 2, b BMOθγ with θ > 0 and VRHs, Assume that α ∈ (−∞, +∞) and λ ∈ (0, 1).

  1. If n/2 ≤ s < n and p0 is such that 1/p0 = 1/s−1/n, then the variation operator Vq(Rb,l,εL,) is bounded on Lα,V,ωp,λ (ℝn) for p0 p < ∞ and ω Ap/p0γ,.

  2. If n/2 ≤ s < n and p0 is such that 1/p0 = 1/s−1/n, then the variation operator Vq(Rb,l,εL) is bounded on Lα,V,ωp,λ (ℝn) for 1 < pp0, with ω1p1Ap/p0γ,.

  3. If sn, then the variation operator Vq(Rb,l,εL,) and Vq(Rb,l,εL) are bounded on Lα,V,ωp,λ (ℝn) for 1 < p < ∞ and ω Apγ,.

Remark 1.6

In [8], it was proved that if V is a nonnegative polynomial, then VRHs for any 1 < s < ∞. Therefore, as special cases of our results, the corresponding ones to the Hermite operator: H = −Δ+∣x2 hold. This can be regarded as the generalization of the corresponding results in [2, 30].

The rest of this paper is organized as follows. In Section 2, we will recall some properties of the function γ and some basic facts concerning weights Apγ , which will play a crucial roles in our arguments. In Section 3, we will prove Theorem 1.3 and 1.4, the proof of Theorem 1.5 will be given in Section 4. Throughout this paper, the letter C always denotes a positive constant that is independent of main parameters involved but whose value may differ from line to line. We use fg to denote fCg. If fgf, we write fg. For any t ∈ (0, ∞), we denote the ball B(x, tr) by tB. Given any p ∈ [1, ∞], p′ = pp1 denote its conjugate index. In particular, it should be pointed out that these weighted Morrey spaces in Definition 1.2 are equivalent for different k > 1.

2 Preliminaries

In this section, we recall some known results, which will be used in our next proofs. We first recall some properties of the auxiliary function γ(x), which will be used below.

Lemma 2.1

(cf. [8]) If VRHn/2, then there exist c0 and l0 ≥ 1 such that for all x, y ∈ ℝn,

1c0γ(x)(1+|xy|γ(x))l0γ(y)c0γ(x)(1+|xy|γ(x))l0/(l0+1). (2.1)

In particular, γ(x) ∼ γ(y) ifxy∣ < (x), and the ball B(x, γ(x)) is called critical.

According to [31], we recall a new class of weights Apγ,=θ0Apγ,θ for p ≥ 1, where Apγ,θ (p > 1) is the set of those weights satisfying

(Bω(y)dy)1/p(Bω1p1(y)dy)1/pC|B|(1+rγ(x))θ, (2.2)

and A1γ,θ is the set of those weights ω such that

1|B|Bω(y)dyC(1+rγ(x))θinfByω(y) (2.3)

for every ball B = B(x, r).

Clearly, the classes Apγ,θ are increasing with θ and for θ = 0, they are just the Munkenhoupt classes Ap. From [32], we know that the following properties for Apγ,θ hold.

Lemma 2.2

([32]) Let 1 < p < ∞, 0 < θ < ∞. Then

  1. Ap1γ,θAp2γ,θ for 1 ≤ p1 < p2 < ∞;

  2. ω Apγ,θ if and only if ω1p1Apγ,θ, where 1/p+1/p′ = 1;

  3. if ω Apγ,θ for 1 ≤ p < ∞, then there exists a constant such that for any κ > 1,

    ω(κB(x0,r))C(1+κrγ(x0))(l0+1)θω(B(x0,r)). (2.4)

Lemma 2.3

([32]) Let 0 < θ < ∞, 1 ≤ p < ∞. If ω Apγ,θ , then there exist positive constant δ > 1, σ and C such that

ω(E)ω(B)C(|E||B|)1/δ(1+rγ(x0))σ (2.5)

for any measurable subset E of a ball B(x0, r).

Lemma 2.4

([32]) If ω Apγ, , 1 ≤ p < ∞, then there exist positive constant β, τ and C such that

1|B|Bω1+β11+βC1|B|Bω(1+rγ(x))τ, (2.6)

for every ball B = B(x, r).

Lemma 2.5

([32]) If ω Apγ, , 1 ≤ p < ∞, then there exist positive constant ϵ > 0 such that ω Apϵγ, for every ball B = B(x, r).

3 Proof of Theorems 1.3 and 1.4

This section is devoted to the proof of Theorem 1.3 and 1.4. We first recall several auxiliary results. Let ℜ and R be the kernel function of RL and RL,, respectively. The following estimates for the kernel functions were established in [8] and will be very useful in the sequel.

Lemma 3.1

[8] Let l = 1, ⋯, n, VRHs with s > n/2. Then:

  1. For every N ∈ ℕ, there exist C > 0 such that

    |R(x,z)|C(1+|xz|/γ(x))N|xz|n1(B(z,|xz|4)V(u)|uz|n1du+1|xz|). (3.1)

    Moreover, the last inequality also holds with γ(x) replaced by γ(z).

  2. When s > n, the term involving V can be dropped from inequalities (3.1).

Proof of Theorem 1.3

To prove (i), without loss of generality, we may assume α < 0 and ω Ap/p0γ,. Pick any ball B := B(x0, r) and write f(x) = f0(x) + i=1 fi(x), where f0 = 2B, fi = 2i+1B∖2iB for i ≥ 1. By the weighted Lp-boundedness of Vq(R,εL) (f) (see [9]). Hence, we have

B|Vq(R,εL,)(f0)(x)|pω(x)dx2B|f(x)|pω(x)dx(1+rγ(x0))αω(4B)λfLα,V,ωp,λ(Rn)p. (3.2)

From (1.3), we have

Vq(R,εL,)(fi)(x)=εi+1<|xy|<εiRL,(x,y)fi(y)dyFqRnχ{εi+1<|xy|<εi}(y)Fq|RL,(x,y)||fi(y)|dy2i+1B2iB|RL,(x,y)||f(y)|dy. (3.3)

In the term last but one, we used that ∥χεi+1<∣xy∣<εiFq ≤ 1.

Now it follows from Lemma 3.1 that

B|Vq(R,εL,)(fi)(x)|pω(x)dxB(2i+1B2iB|RL,(x,y)||f(y)|dy)pω(x)dxB(2i+1B2iB(1+|xy|γ(x))N|xy|n|f(y)|dy)pω(x)dx+B(2i+1B2iB(1+|xy|γ(x))N|xy|1n|f(y)|(B(y,|xy|/4)V(z)dz|zy|n1)dy)pω(x)dx=:A1+A2.

For term A1, using Lemma 2.1, we have

A1B(1+2irγ(x0))Np/(l0+1)(2ir)np(2i+1B|f(y)|dy)pω(x)dx(1+2irγ(x0))Np/(l0+1)(2ir)npω(B)(2i+1B|f(y)|dy)p(1+2irγ(x0))Np/(l0+1)(2ir)npω(B)×(2i+1B|f(y)|pω(y)dy)(2i+1Bω(y)p/pdy)p/pfLα,V,ωp,λ(Rn)p(1+2irγ(x0))Np/(l0+1)α+θp×ω(2B)ω(2i+1B)λω(2i+1B)1fLα,V,ωp,λ(Rn)p1+rγ(x0)αω(2B)λ×1+2irγ(x0)Np/(l0+1)α+θp+(l0+1)θω(2B)ω(2i+1B)1λfLα,V,ωp,λ(Rn)p(1+rγ(x0))αω(2B)λ|2B||2i+1B|(1λ)/δ×(1+2irγ(x0))Np/(l0+1)α+θp+(l0+1)θ+σ(1λ)fLα,V,ωp,λ(Rn)p(1+rγ(x0))αω(2B)λ2in(1λ)/δ×(1+2irγ(x0))Np/(l0+1)α+θp+(l0+1)θ+σ(1λ). (3.4)

Now, we will estimate the term A2. Using (2.1) and Hölder’s inequality, we can write

A2B(2ir)(1n)p(1+2irγ(x0))Np/(l0+1)(2i+1B|f(y)|×(2i+1BV(z)dz|zy|n1)dy)pω(x)dx(2ir)(1n)p(1+2irγ(x0))Np/(l0+1)ω(B)(2i+1B|f(y)|×J1(Vχ2i+1B)(y)dy)p. (3.5)

If we choose ϱ such that 1ϱ+1p0+1p=1. Then by Hölder’s inequality, we have

2i+1B|f(y)||J1(Vχ2i+2B)(y)|dypJ1(Vχ2i+2B)(y)Lp0pfχ2i+1BLp(ω)p2i+1Bω(y)ϱ/pdyp/ϱ. (3.6)

Using the boundedness of the 1-th Euclidean fractional integral 𝓙: LsLp0 with 1/p0 = 1/s−1/n, we obtain that

J1(Vχ2i+2B)Lp0pVχ2i+2BLsp. (3.7)

Recall that VBs for some s > 1 implies that V satisfies the doubling condition, i.e., there exist constants μ ≥ 1 and C such that,

tBV(x)dxCtnμBV(x)dx

holds for every ball B and t > 1. Therefore

Vχ2i+2BLsp(2ir)np/snp2i+1BV(x)dxp(2ir)np/snp(2irγ(x0))npμγ(x0)np2p. (3.8)

Since ω Ap/p0γ,θ and p/ϱ = p/ p0 − 1, we get

2i+1Bω(y)dy2i+1Bω(y)ϱ/pdyp/ϱ|2i+1B|p/p0(1+2irγ(x0))θp/p0. (3.9)

Go back to (3.10), we have

A2(2ir)(1n)p+pnp0+npqnp+np2p(1+2irγ(x0))Np/(l0+1)ω(2B)ω(2i+1B)×(2irγ(x0))npμ+2pnp2i+1B|f(y)|pω(y)dyfLα,V,ωp,λ(Rn)p(1+rγ(x0))αω(2B)λ(ω(2B)ω(2i+1B))1λ×(1+2irγ(x0))Np/(l0+1)+θp/p0+(l0+1)θλ+npμ+p(2n)+(1λ)σfLα,V,ωp,λ(Rn)p(1+rγ(x0))αω(2B)λ2in(1λ)/δ×(1+2irγ(x0))Np/(l0+1)+θp/p0+(l0+1)θλ+npμ+p(2n)+(1λ)σ. (3.10)

This together with (3.4) by choosing N which is big enough, we get

Vq(R,εL)(f)Lα,V,ωp,λ(Rn)CfLα,V,ωp,λ(Rn).

For part (ii), we note that the adjoint R,εL of R,εL,, when VBs, with n/2 ≤ s < n. We write

Vq(R,εLf)(x)=εi+1<|xy|<εiR(x,y)f(y)dyFq=εi+1<|xy|<εiR(y,x)f(y)dyFq.

By proceeding as the previous proofs (i), we can prove that Vq(R,εL) is bounded on Lα,V,ωp,λ (ℝn) for 1 < pp0, with ω1p1Ap/p0γ. We omit the details.

The proof of part (iii) can be given analogously as in (i) and (ii), we leave the part to the part to the interested readers and complete the proof of therorem 1.3.□

Proof of Theorem 1.4

As for the case p = 1, by replacing (3.2) with the corresponding weak estimate. By the Vq(R,εL) (f) is bounded of weighted weak type (1,1) (see [10]), we have

ω({yB:|Vq(R,εL)(f0)(y)|>η2})1ηfLα,V,ωp,λ(Rn)(1+rγ(x0))αω(4B)λ. (3.11)

According (3.3) and (3.1), we get

ωyB:|Vq(R,εL)(i=1fi)(y)|>η21ηi=1B|Vq(R,εL)(fi)(y)|ω(y)dy1ηi=1B2i+1B2iB|RL(y,z)||f(z)|dzω(y)dy1ηi=1B2i+1B2iB|f(z)|(1+|yz|/γ(z))N|yz|ndzω(y)dy+1ηi=1B2i+1B2iB|f(z)|dz(1+|yz|/γ(z))N|yz|n1×B(y,|yz|/4)V(u)du|uy|n1ω(y)dy=:D1+D2. (3.12)

Note that for ωp0A1γ,, we have ωp0A1γ,θ0 for some θ0 ≥ 0. In this case it is true that ω A1γ,θ with θ = θ0/ p0 . Therefore, we obtain

D11ηi=1(1+2irγ(x0))Nl0+1(2ir)nω(B)2i+1B|f(z)|dz1ηi=1(1+2irγ(x0))Nl0+1+θ0/p0(2ir)n|2i+1B|×ω(B)ω(2i+1B)2i+1B|f(z)|ω(z)dz1ηfLα,V,ω1,λ(Rn)(1+rγ(x0))αω(2B)λ×i=1(1+2irγ(x0))N/l0+1+θ0/p0α(ω(2B)ω(2i+1B))1λ1ηfLα,V,ω1,λ(Rn)(1+rγ(x0))αω(2B)λ(2i)n(λ1)/δ×i=1(1+2irγ(x0))N/l0+1+θ0/p0α(1λ)δ.

By Hölder’s inequality and ωp0A1γ,θ0, we have

BJ1(Vχ2i+2B)(y)ω(y)dyJ1(Vχ2i+2B)(y)Lp0Bω(y)p0dy1/p0J1(Vχ2i+2B)(y)Lp0|B|1/p0(1+rγ(x0))θ0/p0(infByω(y)p0)1/p0J1(Vχ2i+2B)(y)Lp0|B|1/p0(1+rγ(x0))θ0/p0infByω(y).

From (3.7) and (3.8), we obtain

D21ηi=1(1+2irγ(x0))Nl0+1(2ir)1n2i+1B|f(z)|dz×BJ1(Vχ2i+2B)(y)ω(y)dy1ηi=1(1+2irγ(x0))Nl0+1+θ0p0+nμ+2n(2ir)nqn1×rnp02i+1B|f(z)|ω(z)dz1ηfLα,V,ω1,λ(Rn)(1+rγ(x0))αω(2B)λ×i=1(1+2irγ(x0))Nl0+1+θ0p0+nμ+2nα(2i)np0(ω(2B)ω(2i+1B))λ1ηfLα,V,ω1,λ(Rn)(1+rγ(x0))αω(2B)λ×i=1(1+2irγ(x0))Nl0+1+θ0p0+nμ+2nα(2i)n(λ/δ1/p0)

where we choose N which is big enough and we have

D11ηfLα,V,ω1,λ(Rn)(1+rγ(x0))αω(2B)λ,

and

D21ηfLα,V,ω1,λ(Rn)(1+rγ(x0))αω(2B)λ.

These together with (3.11) imply that

η(1+rγ(x))αω(2B)λω{yB(x,r):|Vq(R,εLf)(y)|>η}CfLα,V,ω1,λ(Rn),

which complete the proof of Theorem 1.4.□

4 Proof of Theorem 1.5

In what follows, we will prove Theorem 1.5. The following property of BMO(γ) functions.

Lemma 4.1

(cf. [12]) Let θ > 0 and 1 ≤ s < ∞. If bBMOθ(γ), then

(1|B|B|bbB|s)1/sCbBMOθ(γ)(1+rγ(x0))θ (4.1)

for all B = B, with x0 ∈ ℝn and r > 0, where θ′ = (l0 + 1)θ and l0 the constant appearing in (2.1).

Proof of Theorem 1.5

We will only prove the results of Vq(Rb,l,εL,) (f) in part (i). Without loss of generality, we may assume that α < 0. Pick any x0 ∈ ℝn and r > 0, and write

f(x)=f0(x)+i=1fi(x),

where f0 = B(x0,2r), fi = 2i+1B)∖2iB for i ≥ 1. By the weighted Lp-boundedness of Vq(Rb,l,εL,) (f) (see [9]), we have

B|Vq(Rb,,εL,)(f0)(x)|pω(x)dxbBMOθ(γ)p2B|f(x)|pω(x)dxCbBMOθ(γ)p(1+rγ(x0))αω(4B)λfLα,Vp,λ(Rn)p. (4.2)

set bB = ∣B−1 Bb(x)dx. For i ≥ 1, according to (1.3), we have

Vq(Rb,,εL,)(fi)(x)=Rb,,εL,(fi)(x))Fq=εi+1<|xy|<εi(b(x)b(y))RL,(x,y)fi(y)dyFqRnχ{εi+1<|xy|<εi}(y)Fq|b(x)b(y)||RL,(x,y)||fi(y)|dyRn|b(x)b(y)||RL,(x,y)||fi(y)|dy|b(x)bB|2i+1B2iB|RL,(x,y)||f(y)|dy+2i+1B2iB|b(y)bB||RL,(x,y)||f(y)|dy.

Applying Lemma 3.1, we can write

B|Vq(Rb,,εL,)(fi)(x)|pω(x)dxB|b(x)bB|p(2i+1B2iB(1+|xy|γ(y))N×|xy|n|f(y)|dy)pω(x)dx+B|b(x)bB|p(2i+1B2iB(1+|xy|γ(y))N×|xy|1n|f(y)|(B(y,|xy|/4)V(z)dz|zy|n1)dy)pω(x)dx+B(2i+1B2iB|b(y)bB|(1+|xy|γ(y))N×|xy|n|f(y)|dy)pω(x)dx+B(2i+1B2iB|b(y)bB|(1+|xy|γ(y))N×|xy|1n|f(y)|(B(y,|xy|/4)V(z)dz|zy|n1)dy)pω(x)dx=:B1+B2+B3+B4.

Using Lemma 2.1, Hölder’s inequality, Lemma 4.1 and Lemma 2.2-2.4, we have

B1B|b(x)bB|p(1+2irγ(x0))Npl0+1(2ir)np(2i+1B|f(y)|dy)pω(x)dxfLα,V,ωp,λ(Rn)p(1+2irγ(x0))αNpl0+1+(l0+1)θλ+θpω(2i+1B)λ1B|b(x)bB|pω(x)dxbθpfLα,V,ωp,λ(Rn)pω(2B)λ(1+2irγ(x0))αNpl0+1+(l0+1)θλ+θp+τ(ω(2B)ω(2i+1B))1λbθpfLα,V,ωp,λ(Rn)pω(2B)λ(1+2irγ(x0))αNpl0+1+(l0+1)θλ+θp+τ+σ(1λ)(2i)(λ1)n/δ. (4.3)

Similarly, we can get

B3B(2ir)np(1+2irγ(x0))Npl0+12i+1B|b(y)bB||f(y)|dypω(x)dx(2ir)np(1+2irγ(x0))Npl0+1ω(2B)2i+1B|b(y)bB||f(y)|dyp

we choose ϱ satisfies 1ϱ+1p0+1p=1. According to Hölder’s inequality, ωAp/p0 and (4.1), we have

2i+1B|b(y)bB||f(y)|dyp2i+1B|b(y)bB|p0dyp/p02i+1B|f(y)|pω(y)dy2i+1Bω(y)ϱ/pp/ϱbθpfLα,V,ωp,λ(Rn)p(2ir)pn(1+2irγ(x0))(θp)/p0αω(2i+1B)λ1

and we obtain

B3bθpfLα,V,ωp,λ(Rn)pω(B)λ(ω(2B)ω(2i+1B))1λ(1+2irγ(x0))Npl0+1+(θp)/p0αbθpfLα,V,ωp,λ(Rn)pω(B)λ(2i)(λ1)n/δ(1+2irγ(x0))Npl0+1+(θp)/p0α+σ(1λ)+θp. (4.4)

Imitating the estimation of term A2, using Lemma 2.1, Hölder’s inequality, Lemma 4.1 and Lemma 2.4, we obtain that

B2B|b(x)bB|p(2ir)(1n)p(1+2irγ(x0))Npl0+1×(2i+1B|f(y)|J1(Vχ2i+2B)(y)dy)pω(x)dx(2ir)(1n)p(1+2irγ(x0))Npl0+1+τbθpω(B)×(2i+1B|f(y)|J1(Vχ2i+2B)(y)dy)p.

According to (3.6)-(3.9), we have

(2i+1B|f(y)|J1(Vχ2i+2B)(y)dy)pfLα,V,ωp,λ(Rn)p(1+2irγ(x0))θp/p0+npμ2pnpα×ω(2i+1B)λ1(2ir)p(n1).

Then

B2bθpfLα,Vp,λ(Rn)pω(B)λ(ω(2B)ω(2i+1B))1λ×(1+2irγ(x0))Npl0+1+τ+θpp0+npμ2pnpαbθpfLα,V,ωp,λ(Rn)pω(B)λ(2i)(λ1)n/δ×(1+2irγ(x0))Npl0+1+τ+θpp0+npμ2pnpα+σ(1λ).

Similarly, we can estimate B4 as follows,

B4(2ir)(1n)p(1+2irγ(x0))Npl0+1ω(B)×2i+1BJ1(Vχ2i+2B)(y)||b(y)bB||f(y)|dypdy.

Now, Imitating the estimation of B3, but we use Hölder’s inequality with ν and t that 1p+1p0+1ν+1t=1. Furthermore, From lemma 2.5, we need choose ν that ω A1+p/tγ,.

2I+1BJ1(Vχ2i+2B)(y)||b(y)bB||f(y)|dypJ1(Vχ2i+2B)(y)Lp0pfχ2i+1BLp(ω)p×2i+1B|b(y)bB|μdyp/ν2i+1Bω(y)t/pdyp/tbθpfLα,V,ωp,λ(Rn)p(2ir)p(n1)×(1+2irγ(x0))np/sα2p+n+pn/t+pn/μω(2i+1B)λ1.

this yields that

B4bθpfLα,V,ωp,λ(Rn)pω(2B)λ(ω(2B)ω(2i+1B))1λ×(1+2irγ(x0))Npl0+1+np/sα2p+n+pn/t+pn/μbθpfLα,V,ωp,λ(Rn)pω(2B)λ(2i)n(λ1)/δ×(1+2irγ(x0))Npl0+1+np/sα2p+n+pn/t+pn/μ+σ(1λ). (4.5)

Then (4.3)-(4.5) by choosing N which is big enough, we can obtain that

Vq(Rb,,εL)(f)Lα,Vp,λ(Rn)CbBMOθ(γ)fLα,Vp,λ(Rn),

which completes the proof of Theorem 1.5.□

Remark 4.2

The fluctuations of a family 𝓣 = {Tt}t>0 of operators when t → 0+ can also be analyzed by using oscillation operators (see, for instance, [6, 33] etc.). If {tj}j∈ℕ is a real decreasing sequence that converges to zero, the oscillation operator 𝓞(𝓣f) is defined by

O(Tf)(x):=(i=1supti+1εi+1<εiti|Tεi+1f(x)Tεif(x)|2)1/2.

Then, by using the procedures developed in this paper, we can establish the corresponding conclusions in Theorem 1.3 for 𝓞 (R,εL) and O(R,εL,), Theorem 1.5 for O(Rb,,εL) and O(Rb,,εL,). The details are omitted.

Acknowledgement

Supported by the National Natural Science Foundation of xinjiang Province of China (No. 2016D01C381) and the Doctoral Scientific Research Foundation of Yili Normal University(No. 2017YSBS09).

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Received: 2017-12-08
Accepted: 2019-05-16
Published Online: 2019-07-31

© 2019 Zhang, published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 Public License.

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