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Research article

Regions of variability for a subclass of analytic functions

  • Received: 31 December 2019 Accepted: 26 March 2020 Published: 31 March 2020
  • MSC : 30C45, 30C55, 30C80

  • Let AC, B[1,0) and α(π2,π2). Then Cα[A,B] denotes the class of analytic functions f in the open unit disc with \lt i \gt f \lt /i \gt (0) = 0 = \lt i \gt f \lt /i \gt '(0)-1 such that eiα(1+zf(z)f(z))=cosαp(z)+isinα, with p(z)=1+Aw(z)1+Bw(z), where w(0)=0 and |w(z)|<1. Region of variability problems provides accurate information about a class of univalent functions than classical growth distortion and rotation theorems. In this article we find the regions of variability Vλ(z0,A,B) for logf(z0) when f ranges over the class Cα[λ,A,B] defined as Cα[λ,A,B]={fCα[A,B]:f(0)=(AB)eiαcosα} for any fixed z0E and λ¯E. As a consequence, the regions of variability are also illustrated graphically for different sets of parameters.

    Citation: Mohsan Raza, Wasim Ul Haq, Jin-Lin Liu, Saddaf Noreen. Regions of variability for a subclass of analytic functions[J]. AIMS Mathematics, 2020, 5(4): 3365-3377. doi: 10.3934/math.2020217

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  • Let AC, B[1,0) and α(π2,π2). Then Cα[A,B] denotes the class of analytic functions f in the open unit disc with \lt i \gt f \lt /i \gt (0) = 0 = \lt i \gt f \lt /i \gt '(0)-1 such that eiα(1+zf(z)f(z))=cosαp(z)+isinα, with p(z)=1+Aw(z)1+Bw(z), where w(0)=0 and |w(z)|<1. Region of variability problems provides accurate information about a class of univalent functions than classical growth distortion and rotation theorems. In this article we find the regions of variability Vλ(z0,A,B) for logf(z0) when f ranges over the class Cα[λ,A,B] defined as Cα[λ,A,B]={fCα[A,B]:f(0)=(AB)eiαcosα} for any fixed z0E and λ¯E. As a consequence, the regions of variability are also illustrated graphically for different sets of parameters.


    Let X and Y be two separable metric spaces and let M(X) be the family of compactly supported Borel probability measures on X. We say that μM(X) satisfies the doubling condition if

    lim supr0(supxsupp(μ)μ(B(x,ar))μ(B(x,r)))<

    for some a>1 (or, equivalently, any a>1), where B(x,r) is closed ball with a center x and a radius r. We use M0(X) to denote the family of compactly supported Borel probability measures on X that fulfill the doubling condition [1]. To study the multifractal analysis of measures introduced by Mandelbrot in [2,3], we must turn back to the study of sets related to the local behavior of such measures, called level sets, defined, for βR, as :

    Eμ(β)={xsupp(μ);limr0logμ(B(x,r))logr=β},

    where supp(μ) is the topologic support of μ, and B(x,r) stands for the closed ball with a center x and a radius r>0. Thus, this study is essentially linked to its punctual nature and falls under set theory. However, some geometric sets are essentially known by means of the measures that are supported by them, i.e.,

    ν(A)=sup{ν(B),  BA},

    for a given measure ν and a given set A. Hence, when we consider a set A, we focus on the properties of the measure ν rather than the geometric structure of A. The set A is thus partitioned into α-level sets Eμ(β). This allows the inclusion of μ into the computation of the fractal measures and dimensions. Olsen, in [1], introduced the multifractal generalizations of the fractal dimensions. This is achieved by constructing the generalization of Hausdorff and the packing measures, denoted Hq,tμ and Pq,tμ in Rd, where d1, respectively. Later, in [4], the authors introduced a new multifractal formalism that deviates from the classical approach. To achieve this, they constructed two distinct measures known as the lower and upper Hewitt-Stromberg (H-S) measures, denoted, respectively, by Hq,tμ and Pq,tμ. These measures serve as fundamental tools in the analysis of multifractal structures. Given the importance of these measures in this study, it is crucial to examine their properties, including their behavior on product sets and their density characteristics both of which play a critical role in understanding the broader implications of this new formalism. In particular, in [5], the author proved the existence of a constant c>0 such that, for any measurable sets ARd and BRl, the following inequality holds:

    Hq,s+tμ×ν(A×B)c1Hq,sμ(A)Hq,tν(B)c2Pq,s+tμ×ν(A×B)c3Pq,sμ(A)Pq,tν(B), (1.1)

    provided that we have the measures μM0(Rd) and νM0(Rl) and with the convention that

    0×=0.

    The constant ci (i=1,2,3) depends only on certain structural parameters, such as the dimensions d and l, but is independent of the specific choice of E and F. Moreover, in the specific case q=0, the associated dimensional inequalities for the products of these measures have been derived in [6,7,8]. For additional related discussions, the readers may consult [9,10]. Furthermore, the inequalities above are explicitly stated in this case in [8,11,12,13]. In particular, if

    d=l=1andμ=ν

    are basically the Lebesgue measure on R, one has, for

    q+s=q+t=log2/log3

    and E=F as the middle third Cantor [14,15]

    Hq,sμ(A)Pq,tμ(B)=1×4t<Pq,s+tμ×ν(A×B)=4s+t=Pq,sμ(A)Pq,tν(B).

    Remark 1. The equation of (1.1) has important physical interpretations depending on the context. Note, for q=0, that

    H1=L1,

    is the one-dimensional Lebesgue measure. In particular, if A,BR, then the product set A×B forms a subset of R2, and then (1.1) gives an approximation of the Hausdorff measure of A×B using the area of the region covered by the Cartesian product. These prove, in particular, that

    H2(A×B)H1(A)H1(B).

    A Hausdorff function

    h:R+R+

    is a function that is increasing, continuous, and satisfies

    h(0)=0.

    These functions are often used in the context of geometric measure theory, particularly in defining Hausdorff measures. Let F denote the set of all such dimension functions, i.e., the set of all Hausdorff functions. Additionally, a Hausdorff function h is considered to fulfill the doubling condition if a positive constant γ exists such that the following inequality holds:

    h(2r)γh(r),  for all r>0.

    This condition essentially ensures that h does not grow too quickly and is often used to ensure specific regularity properties of the corresponding measures. The subset of F consisting of all Hausdorff functions that satisfy the doubling condition is denoted by F0. Recently, in [16], the authors introduced the generalized pseudo-packing measure Rq,hμ and they proved that

    Hq,hgμ×ν(A×B)Hq,hμ(A)Rq,gν(B)Rq,hgμ×ν(A×B), (1.2)

    for all AX and BY, provided that we do not have 0 case; that is, the product on the medium side does not take the form 0× or ×0. Note that we do not any restriction on the measures μ,ν,h, and g; that is, they do not satisfy necessary the doubling condition. In addition, one has (see again [16])

    Pq,hgμ×ν(A×B)Qq,hμ(A)Pq,gν(B), (1.3)

    except in the 0 case, where Qq,hμ is the weighted generalized packing measure. In particular, one can obtain (1.1) under appropriate geometric conditions on X and Y (amenable to packing) [8,16].

    Traditional packing and Hausdorff measures are defined using packings and coverings made up of collections of balls with diameters less than a given positive value δ. An alternative approach to constructing fractal measures utilizes packings and coverings by using families of balls with a fixed diameter δ. These measures, known as H-S measures, were first introduced in [17, Exercise (10.51)]. They were later explicitly described in Pesin's monograph [18] and are also referenced, albeit in an implicit manner, in foundational works such as Mattila's [19]. The importance of H-S measures goes beyond their theoretical definition; they offer a flexible framework for analyzing fractals and their complex characteristics. Numerous studies, including [20,21,22,23] for H-S measures and [24,25,26] for Standard measures, have demonstrated their utility in exploring the local properties of fractals and the behavior of fractal products. These works underscore the adaptability of H-S measures across various contexts, thus enriching the field of fractal geometry and its applications. Furthermore, Edgar's comprehensive exposition of these measures [27, pp. 32–36] provides a clear and accessible introduction, thoroughly detailing their construction, properties, and potential applications.

    In Section 3, we are interested in studying the counterpart of the formula (1.1) related to the lower and upper H-S measures in Euclidean space. This result was shown for q=0 in [28] in Euclidean space. We will prove the following theorem.

    Theorem 1. Let ARd, BRl, μM0(Rd), νM0(Rl), h,gF0 and qR. Positive constants c1c4 exist such that

    Hq,hμ(A)Hq,gν(B)c1Hq,hgμ×ν(A×B)c2Hq,hμ(A)Pq,gν(B)c3Pq,hgμ×ν(A×B)c4Pq,hμ(A)Pq,gν(B), (1.4)

    except in the 0 case.

    To prove the first inequality, we introduce a new multifractal measure that parallels the lower H-S measure and is notably simpler to analyze. This is achieved by utilizing a class of half-open dyadic cubes as covering sets in the definition, instead of using closed balls. The use of half-open dyadic cubes provides a new framework for the analysis, simplifying the structure of the measure. For the second inequality, we extend the technique by replacing the traditional dyadic cubes with half-open semi-dyadic cubes. This adjustment leads to the definition of two distinct measures that correspond to the upper and lower H-S measures. This choice arises from the fact that semi-dyadic cubes vn(x) are less sensitive to the position of x compared with the corresponding dyadic cubes un(x). Semi-dyadic cubes have been utilized in works such as [5,13,29]. It is important to note that this construction is specific to Euclidean space, making our proof distinct from those in [30].

    Remark 2. It is important to emphasize that our analysis was not conducted for an arbitrary subset ΓR2, but specifically for cases where Γ takes the form of a Cartesian product

    Γ=A×B.

    Addressing such a problem is far from straightforward, as it necessitates the application of integral versions of product set. For a deeper exploration of these techniques and their implications, we refer the reader to [5,31,32].

    When

    h(r)=rt,

    the measures Hq,hμ and Pq,hμ are simply denoted as Hq,tμ and Pq,tμ, respectively. In this case, these measures assign, in the standard manner, a multifractal dimension to each subset A of Rd, defined as follows:

    bqμ(A)=inf{tR,Hq,tμ(A)=}andBqμ(A)=inf{tR,Pq,tμ(A)=}.

    If q=0, bμ(A) and Bμ(A) do not depend on μ and are simply denoted b and B, respectively. Theorem A implies, when all the hypothesis are satisfied, that

    bqμ1(A)+bqμ2(B)bqμ1×μ2(A×B)bqμ1(A)+Bqμ2(B)Bqμ1×μ2(A×B). (1.5)

    Moreover, all these inequalities may be strict. Indeed, one can construct two sets A and B such that

    bqμ1(A)+bqμ2(B)<bqμ1×μ2(A×B),

    (see [33] for q=0). However, in Example 2, we give a sufficient condition to get the first equality in Eq (1.5):

    bqμ1(A)+bqμ2(B)=bqμ1×μ2(A×B).

    One can define also the multifractal separator functions

    bμ(q)=bqμ(supp(μ))

    and

    Bμ(q)=Bqμ(supp(μ)).

    Where bμ is known to be a decreasing function, while Bμ is both a decreasing and convex function [4]. In addition, it holds that

    bμBμ.

    As a consequence, since

    supp(μ1×μ2)=supp(μ1)×supp(μ2),

    we get the following result:

    bμ1(q)+bμ2(q)bμ1×μ2(q)bμ1(q)+Bμ2(q)Bμ1×μ2(q), (1.6)

    by taking

    E=supp(μ1)

    and

    F=supp(μ2)

    in Theorem 1. Similar results were also proven for the s-dimensional Hausdorff measure Hs and the s-dimensional packing measure Ps [6,13,34,35]. In addition, a variety of related results and further developments on this problem can be found in the works of [36,37].

    Now, given μ,θP(Rd), qR, h,gF0, and xsupp(μ), we define the upper and lower (q,s)-densities of θ at x with respect to μ as

    ¯dq,hμ(x,θ)=lim supr0θ(B(x,r))μ(B(x,r))qh(2r) and d_q,hμ(x,θ)=lim infr0θ(B(x,r))μ(B(x,r))qh(2r). (1.7)

    If

    d_q,hμ(x,θ)=¯dq,hμ(x,θ),

    we use dq,hμ(x,θ) to denote the common value. In [30], the authors used some density inequalities as "local versions" of the product inequalities. In particular, they proved that the inequality

    Pq,hgμ×ν(A×B)cPq,hμ(A)Pq,gν(B)

    may be deduced from the following density inequality:

    cd_q,hgμ×ν((x,y),θ1×θ2)d_q,hμ(x,θ1)d_q,gν(y,θ2),

    where θ1 is the restriction of Pq,hμ to E and θ2 is the restriction of Pq,gν to B.

    The set A satisfies the condition

    bqμ(A)=Bqμ(A)

    for measures μ under consideration, which will be called regular set. Regularity is defined with respect to various measures, such as the packing measure [29,38], the Hausdorff measure [39,40,41,42], and the H-S measure [43,44,45]. Notably, Tricot et al. [38,46] demonstrated that a subset A of Rd has integer Hausdorff and packing dimensions if it is strongly regular, meaning that

    Ht(A)=Pt(A)

    for t0. Furthermore, as a consequence of (1.5), it follows that if either E or F is regular, then

    bqμ1(A)+bqμ2(B)=bqμ1×μ2(A×B)=Bqμ1×μ2(A×B). (1.8)

    In Theorem 1, we assume that the products do not take the form 0× or ×0. In Section 4, by estimating the measure of d-dimensional symmetric generalized Cantor sets, we demonstrate that this assumption is essential and can not be omitted. Specifically, let 0<α,β<1, to establish the second inequality in (1.4), we then need to prove that

    ¯Hq,α+βμ×ν,0(H)c¯Hq,αμ,0(A)¯Pq,βν(B),

    for all

    HA×B

    and some positive constant c, where ¯Hq,αμ,0 and ¯Pq,βν are the pre-lower and pre-upper H-S measures, respectively (see Section 3.2 and Eq (3.2)). We establish the following result.

    Theorem 2. One-dimensional generalized Cantor sets K1, K12, K22, and K32 such that

    ¯Hq,αμ,0(K1)=0,¯Pq,βμ(Kj2)=,

    and ¯Hq,α+βμ×ν,0(K1×K2) and ¯Pq,α+βμ×ν(K1×K2) are infinite, positive finite, and zero according as j=1,2,3, respectively.

    In this paper, we use formulas containing too many different variables, which is unpleasant, and omitting these extra parameters will create no confusion. To this end, for μP(Rd),νP(Rl), and h,gF, we define the gauge functions ξ and ζ as

    ξ(x,r)=μ(B(x,r)qh(2r)andζ(x,r)=ν(B(x,r)qg(2r), (2.1)

    where qR, r>0, with the conventions

    0q=

    for q0 and

    0q=0

    for q>0. The reader should note that we have simply used ξ (respectively, ζ) to denote the gauge function depending on μ (respectively, ν), q, and h (respectively, g). If

    h(r)=rsandg(r)=rt

    for s,tR, then ξ and ζ will be denoted as ξs and ζt respectively. In this section, we construct the different fractal measures used in this paper. Let δ>0,

    Asupp(μ),

    and {B(xi,ri)}i is a δ-packing of the A, that is, a countable family of disjoint closed balls such that xiA and

    0<2ri<δ

    for all i. Write

    Pξδ(A)=supξ(xi,ri)andPξ0(A)=infδ>0Pξδ(A),

    where the supremum is taken over all δ-packings of the set E. The generalized packing measure Pξ of A with respect to ξ is defined by

    Pξ(A)=infAiAiPξ0(Ai)

    and

    Pξ()=0.

    In a similar way, we define

    Hξδ(A)=infξ(xi,ri)andHξ0(A)=supδ>0Hξδ(A),

    where the infimum is taken over all δ-coverings {B(xi,ri)}i of E; that is, xiE, 0<2ri<δ, and

    AiB(xi,ri).

    We define the generalized Hausdorff measure as

    Hξ(A)=supEAHξ0(E)

    and

    Hξ()=0.

    We refer to [1,5] for more details (see also [46,47] for q=0). Moreover, an integer κN exists such that

    HξκPξ.

    Similarly, we define

    ¯Pξ(A)=lim supr0Mqμ,r(A)h(2r),

    where

    Mqμ,r(A)=sup{iμ(B(xi,r))q|{B(xi,r)}iis a centered packing ofA}.

    It is clear that ¯Pξ is increasing and

    ¯Pξ()=0.

    However it is not σ-additive. For this, we define the Pξ-measure defined as

    Pξ(A)=inf{i¯Pξ(Ai)|AiAiand theAis are bounded}.

    In a similar way, we define

    ¯Hξr(A)=Nqμ,r(A)h(2r)and¯Hξ0(A)=lim infr0¯Hξr(A),

    where

    Nqμ,r(A)=inf{iμ(B(xi,r))q|{B(xi,r)}iis a centered covering ofA}.

    Clearly, ¯Hξ0 is not countably subadditive and not increasing; one needs some modification to obtain an outer measure. More precisely, let

    ¯Hξ(A)=inf{i¯Hξ0(Ai)|AiAiand theAis are bounded}

    and

    Hξ(A)=supEA¯Hξ(E).

    It is well known (see, for instance, [48]) that Hξ and Pξ are metric outer measures, which implies that they are measures on the Borel algebra. Moreover, for some integer κN, the following inequality holds:

    Hξ(A)Hξ(A)κPξ(A)κPξ(A).

    In the following, we recall the construction of the one-dimensional generalized Cantor set K. Let L be a positive number, let {nk}k1 be a sequence of integers, and let {λk}k1 be a sequence of positive numbers such that

    nk>1,   n1λ1<L   and   λk+1nk+1<λk (2.2)

    for all k1. The construction of the generalized Cantor set {L,{nk}k1,{λk}k1} is as follows. In the first step, from a given closed interval with the length L, remove (n11) open intervals and then leaves n1 closed intervals with the length λ1, denoted by I1,,In1. Let

    J1=n1j1=1Ij1.

    In the second step, from each remaining closed interval with the length λ1, remove (n21) open intervals and leaves n2 closed intervals with the length λ2. These are denoted as Ij1,j2, and we can write

    J2=n1j1=1n2j2=1Ij1,j2.

    We continue this process and, in the k-th step, obtain n1n2nk closed intervals with the length λk, denoted Ij1,j2,,jk and denote their union as Jk. Then let

    K=k=0Jk.

    Let

    μ=ν

    be the uniform measure on K, that is

    μ(Qk)=λk

    and define

    Sk=μ(Qk+1)μ(Qk)=λk+1λk. (2.3)

    This construction can be generalized in Rd and Kd, denoting the generalized Cantor set. Let Fk be the product set of d copies Jk. Thus, Fk is the union of (n1n2nk)d closed cubes with the side λk, each of which may be denoted as Q(k), and

    Kd=k=0Fk.

    The next lemma will be used in Section 4 to estimate the measure of Kd.

    Lemma 1. Let Kd be the d-dimensional symmetric generalized Cantor set (d1). A set function Ψ, defined on every non-empty closed subset in Rd and r0, exists such that, for every open cube I with the side rr0, we have

    Ψ(I)23dh(r)λqk, (2.4)

    where k is the unique integer such that

    λk+1r<λk.

    Proof. We start the proof by constructing the set function Ψ. Assume that

    lim infk(n1n2nk)dh(λk)λqk>0.

    Let

    0<b<lim infk(n1n2nk)dh(λk)λqk,

    then there is a k0 such that

    λk0<t0

    and

    h(λk)>b/(n1n2nk)dλqk

    for all k>k0. We define the sequence (λk) such that

    h(λk)=b(n1n2nk)dλqk. (2.5)

    Clearly, we have λk>λk (since h is increasing) and

    h(λk+1)=b(n1n2nk+1)dλqk+1=(2.3)b(n1n2nk+1)dSqkλqk=h(λk)ndk+1Sqk.

    Let A be any open set and define

    Nqμ,k(A)=inf{iμ(Qi)q,QiFk,and meeting A}.

    Then, we have

    Nqμ,k+1(A)=inf{iμ(Qi)q,QiFk+1,and meeting A}inf{iμ(Qi)qμ(Qk)qμ(Qk)qQiFk+1,and meeting A}kdk+1Sqkinf{iμ(Qi)q,QiFk,and meeting A}=kdk+1SqkNqμ,k(A).

    It follows that the sequence {Nqμ,k(A)h(λk)} is decreasing, and we may define the function

    Ψ(A)=limk0Nqμ,k(A)h(λk).

    Now, we will prove (2.4). Let I be an open cube, k exists such that

    1jnk+1andλk+1r<λk.

    Moreover, take a positive sequence (δk)k1 such that

    nkλk+(nk1)δk=λk1. (2.6)

    Then the following exists:

    1jnk+1,

    such that

    jλk+1+(j1)δk+1r<(j+1)λk+1+jδk+1. (2.7)

    Observe that

    Nqμ,k+1(I)=inf{iμ(Qi)q,QiFk+1,and meetingA}2d(j+1)dμ(Qk+1)q22djdμ(Qk+1)q.

    It follows that

    Ψ(I)22djdμ(Qk+1)qh(λk+1),

    ● If j=1, then

    Ψ(I)22dμ(Qk+1)qh(λk+1)22dμ(Qk+1)qh(r);

    ● If 1<j<nk+1, then

    jdμ(Qk+1)qh(λk+1)=(2.5)jdμ(Qk+1)qb(n1n2nk+1)=(j/n1n2nk+1)db=(j/nk+1)dh(λk)μ(Qk)q.

    Since

    λkjkr+1λk,

    and

    th(t)/td

    is decreasing, we get

    (j/nk+1)dh(λk)h(jλk/nk+1),

    and then

    jdμ(Qk+1)qh(λk+1)μ(Qk)qh(jλk/nk+1).

    Now, observe that

    jλk/nk+1jλk/nk+1(2.6)jnk+1nk+1(λk+1+δk+1)2(jλk+1+(j1)δk+1)(2.7)2r.

    As a consequence, we obtain

    Ψ(I)22djdμ(Qk+1)qh(λk+1)22dμ(Qk)qh(2r)23dμ(Qk)qh(r).

    This completes the proof.

    We set, for nN,

    Un={di=1[li2n,li+12n[,l1,,ldZ}

    and

    Vn={di=1[12li2n,12li+12n[,l1,,ldZ}.

    The family Un denotes the set of half-open dyadic cubes of order n. For xRd, let un(x) denote the unique cube uUn that contains x. Similarly, the family Vn consists of half-open dyadic semi-cubes of order n. For xRd, let vn(x) represent the unique semi-cube vVn that contains x and has its complement at a distance of 2n2 from un+2(x). Define

    K={(k1,,kd)ki=0 or 12}.

    For each

    k=(k1,,kd)K,

    let

    Vk,n={di=1[ki+li2n,ki+li+12n[,l1,,ldZ}.

    Note that for

    vvVk,n,

    we have

    vv=.

    Additionally, the collection (Vk,n)kK forms a partition of the family Vn. Moreover, if

    v,vVk:=n0Vk,n,

    then either

    vv=

    or one is contained within the other. Finally, for ARd, define

    Vn(A)={vn(x):xA}andVk,n(A)=Vn(A)Vk,n.

    In what follows, we construct measures on Rd analogous to the generalized lower and upper H-S measures. However, instead of using the collection of all closed balls in the definition, we employ the class of all half-open dyadic semi-cubes. For ARd, we define

    ¯Hξ(A)=lim infn+Nqμ,n(A)h(2n)and¯Pξ(A)=lim supn+Mqμ,n(A)h(2n),

    where the numbers Nn(A) and Mn(A) are defined as

    Nqμ,n(A)=inf{iμ(vi)q|(vi)iIis a family of coverings ofAsuch that viVn(A)}

    and

    Mqμ,n(A)=sup{iμ(vi)qviVn(A),iI,and¯vi¯vj=for ij}.

    The functions ¯Hξ and ¯Pξ are increasing and satisfy

    ¯Hξ()=¯Pξ()=0.

    However these functions are not σ-additive. For this, we consider

    Hξ(A)=inf{i¯Hξ(Ai)|AiAiAiis bounded},
    Pξ(A)=inf{i¯Pξ(Ai)|AiAiAiis bounded}.

    Lemma 2. For every set ARd, a constant c>0 exists such that

    c1Pξ(A)Pξ(A)cPξ(A)andc1Hξ(A)Hξ(A)cHξ(A). (3.1)

    Proof. This arises from the fact that

    B(x,2n2)vn(x)B(x,d2n).

    This completes the proof.

    Similarly, we may define Hξ and Pξ, by using the class of all half-open dyadic cubes in the definition instead of the class of all half-open dyadic semi-cubes. However, it is important to note the resulting pre-measure, denoted ¯Pξ, is not equivalent to the pre-measure ¯Pξ. For more discussion, consult [29, Example 3.5], where the interplay between the two pre-measures is explored. This highlights how seemingly minor changes in the class of sets used can lead to significant differences in the resulting pre-measures and their properties.

    In this section, for the sake of simplicity and clarity, we focus on results that pertain specifically to subsets of the plane. However, it is worth noting that these results can be extended to higher-dimensional spaces without significant complications. Let ΠR2 represent a subset of the plane. For a given x-coordinate, we use Πx to denote the set of all points in Π whose abscissa (x-coordinate) equals x. Given an arbitrary subset A of the x-axis, we will only prove that, if xA, we have

    Hζ(Πx)>a

    or some constant a, and then

    ¯Hξζ(Π)ΠaHξ(A).

    Let n be a non-negative integer and let {Ii×Ij}i,j be a collection of half-open dyadic cubes of order n covering Π. Set

    An={xE,Nqν,n(Πx)g(2n)>b11a}.

    Note that

    Nqμ×ν,n(Π)h(2n)g(2n)Nqμ,n(An)inf{Nqν,n(Πx),xAn}h(2n)g(2n)b11aNqμ,n(An)h(2n).

    This holds for any covering of Π by the binary squares {Ii×Ij}i,j with 2n sides. Hence,

    b11a¯Hξn(An)¯Hξζn(Π)¯Hξζ(Π).

    Since An increases to A as n+, then for any pn, we have

    b11a¯Hξn(Ap)b11a¯Hξn(Ak)¯Hξζ(Π).

    Thus, we obtain

    b11aHξn(Ap)b11a¯Hξn(Ep)¯Hq,hgμ×ν(Π)α1¯Hq,hgμ×ν(Π)

    for p1. Thereby, the continuity of the measure H implies that

    b11aHξ(A)α1¯Hq,hgμ×ν(Π).

    Thus, using Lemma 2, we get

    b21aHξ(A)b11aHq,hμ(A)α1¯Hξζ(Π).

    Finally, by taking

    Π=b21α11,

    we get the result.

    Let ARd and BRl. We prove that a constant c>0 exists such that

    Hξζ(A×B)cHξ(A)Pζ(B).

    Let

    HA×B,

    r>0, and let {B(xi,r)}i be a centered r-covering of A. We denote n as the integer such that

    l2n<rl2n+1.

    For vVn(B) with

    (B(xi,r)×v)H)

    and each i, choose a point

    yi,vB(xi,r)

    and a point yi,vv such that

    (yi,v,yi,v)(B(xi,r)×v)H).

    Note that

    Hi(vVn(B)(B(xi,r)×v)HB(xi,r)×v)i(vVn(B)(B(xi,r)×v)HB(yi,v,2r)×B(yi,v,2r))i(vVn(B)(B(xi,r)×v)HB((yi,v,yi,v),2r)).

    As a consequence, we have the family (B((yi,v,yi,v),2r))iN,vVn(B),B(xi,r)×v)H, which forms a centered (2r)-covering of H. Furthermore, we get

    B(yi,v,ηr)B(yi,v,2n2)

    for

    ηr=23lr.

    It follows, for each kK, that the family

    (B(yi,v,ηr),iN,vVk,n(B),B(xi,r)×v)H

    is a centered ηr-packing of B. It follows that

    ¯Hξζ2r(H)i(vVn(B)(B(xi,r)×v)Hμ(B(yi,v,2r))qν(yi,v,2r)qh(4r)g(4r))mhmgmqνiμ(B(yi,v,2r))qh(2r)(kKvVk,n(B)(B(xi,r)×v)Hν(yi,v,ηr)qg(2ηr))mhmgmqνiμ(B(yi,v,2r))qh(2r)(kK¯Pζηr(B))2lmhmgmqν¯Pζηr(B)iμ(B(yi,v,2r))qh(2r).

    Thus, by considering the infimum over all possible centered r-coverings of the set A, we get

    ¯Hξζ2r(H)2lmhmgmqν¯Hξr(A)¯Pζηr(B).

    Therefore,

    ¯Hξζ0(H)clim infr0¯Hξr(A)lim supr0¯Pζηr(B)=c¯Hξ0(A)¯Pζ(B), (3.2)

    where

    c=2lmhmgmqν.

    Now, assume that

    AiAi

    and

    BjBj.

    Then

    HA×Bi,jAi×Bj.

    It follows that

    ¯Hξζ(H)i,j¯Hq,hgμ×ν,0(Ai×Bj)ci,j¯Hq,hμ,0(Ai)¯Pq,gν(Bj).c(i¯Hξ0(Ai))(j¯Pζ(Bj)).

    Since the cover (A_i) of A and the cover (B_j) of B were arbitrarily chosen, we obtain

    \overline {\mathsf H}^{\xi\zeta}(H)\le c \overline {\mathsf H}^{\xi}(A) {\mathsf P}^{\zeta}(B) \le c {\mathsf H}^{\xi}(A) {\mathsf P}^{\zeta}(B).

    This holds for all for all

    H\subseteq A\times B

    which implies that

    {\mathsf H}^{\xi\zeta}(A\times B) \le c {\mathsf H}^{\xi}(A) {\mathsf P}^{\zeta}(B).

    Let

    A \subseteq \mathbb{R}^d \; \; \; \text{and}\; \; \; B \subseteq \mathbb{R}^l .

    We aim to show that a constant c > 0 exists such that the following inequality holds:

    {\mathsf P}^{\xi\zeta}(A \times B) \ge c {\mathsf H}^{\xi}(A) {\mathsf P}^{\zeta}(B).

    For simplicity, we limit our discussion to subsets of the plane, although the result can be extended to higher dimensions without without significant complications. Let \mathcal Q be any packing of B consisting of semi-dyadic intervals, and let \mathcal C be any covering of A composed of semi-dyadic intervals. We define the following

    \begin{align*} \mathcal C_1& = \Big\{ \mathrm u_i \in \mathcal C, \mathrm u_i \; \text{is dyadic and}\;\; \overline{ \mathrm u}_i \cap \overline{ \mathrm u}_j = \emptyset\;\; \text{for}\;\; i\neq j \Big\},\\ \mathcal C_2& = \Big\{ \mathrm u_i \in \mathcal C, \mathrm u_i \; \text{is not dyadic and}\;\; \overline{ \mathrm u}_i \cap \overline{ \mathrm u}_j = \emptyset\;\; \text{for}\;\; i\neq j \Big\},\\ \mathcal C_3& = \Big\{ \mathrm u_i \in \mathcal C, \mathrm u_i \; \text{is dyadic} \Big\}\bigcap \mathcal C\backslash \mathcal C_1,\\ \mathcal C_4& = \Big\{ \mathrm u_i \in \mathcal C, \mathrm u_i \; \text{is not dyadic} \Big\}\bigcap \mathcal C\backslash \mathcal C_2. \end{align*}

    Clearly, we have each of \mathcal C_i is a packing of E and \mathcal C_i\times \mathcal Q is a packing of A\times B . Therefore,

    4 M_{\mu\times \nu, n}^{*q, hg} (A\times B) h(2^{-n}) g(2^{-n})\ge \sum\limits_{ \mathrm u\in \mathcal Q} \nu( \mathrm u)^q h(2^{-n})g(2^{-n}) \Big( \sum\limits_{ \mathrm v\in \mathcal C_1} \mu( \mathrm v)^q + \sum\limits_{ \mathrm v\in \mathcal C_2} \mu( \mathrm v)^q+\sum\limits_{ \mathrm v\in \mathcal C_3} \mu( \mathrm v)^q+\sum\limits_{ \mathrm v\in \mathcal C_4} \mu( \mathrm v)^q\Big).

    This holds for any packing \mathcal Q of B and

    \mathcal C = \bigcup\limits_i \mathcal C_i,

    so we have

    4 M_{\mu\times \nu, n}^{*q, hg} (A\times B) h(2^{-n}) g(2^{-n})\ge M_{\nu,n}^{*q,g}(B) g(2^{-n}) \sum\limits_{ \mathrm v\in \mathcal C} \mu(v)^q h(2^{-n}) \ge M_{\nu,n}^{*q,g}(B) g(2^{-n}) N_{\mu,n}^{*q,h}(A) h(2^{-n}).

    Thus,

    \overline{ {\mathsf P}}^{*\xi\zeta}(A\times B) \ge \frac14 \overline{ {\mathsf P}}^{*\zeta}(B) \overline{ {\mathsf H}}^{*\xi}(A) \ge \frac14 { {\mathsf P}}^{*\zeta}(B) { {\mathsf H}}^{*\xi}(A).

    Finally, we get the desired result using (3.1).

    Let A\subseteq \mathbb R^d and B\subseteq \mathbb R^l . We will prove that a constant c > 0 exists such that

    {\mathsf P}^{*\xi\zeta}(A\times B) \le c {\mathsf P}^{*\xi}(A) {\mathsf P}^{*\zeta}(B).

    Here again, we limit our study to subsets of the plane, since the extension to higher dimensions does not involve significant complications. Let \mathcal B represent any packing of the set A\times B containing semi-dyadic squares, where each square is formed as the Cartesian product of two semi-dyadic intervals. We define the sets as follows:

    \mathcal C = \Big\{ \mathrm u_n(x) : \exists \mathrm v_n(y) \;\; \text{such that }\;\; w_n(x,y) = \mathrm u_n(x)\times \mathrm v_n(y) \in {\mathcal B}, \;\; x\in A, y\in B\Big\}

    and

    \mathcal Q = \Big\{ \mathrm v_n(x) : \exists \mathrm u_n(y) \;\; \text{such that }\;\; w_n(x,y) = \mathrm u_n(x)\times \mathrm v_n(y) \in {\mathcal B}, \;\; x\in A, y\in B\Big\}.

    Next, we examine the subclasses

    \begin{align*} \mathcal C_1 & = \Big\{ \mathrm u_n(x) \in \mathcal C,\;\; \mathrm u_n(x) \;\; \text{is dyadic} \Big\},\\ \mathcal Q_1 & = \Big\{ \mathrm v_n(x) \in \mathcal Q,\;\; \mathrm v_n(x) \;\; \text{is dyadic} \Big\},\\ \mathcal C_2 & = \Big\{ \mathrm u_n(x) \in \mathcal C,\;\; \mathrm u_n(x) \;\; \text{is not dyadic} \Big\},\\ \mathcal Q_2 & = \Big\{ \mathrm v_n(x) \in \mathcal Q,\;\; \mathrm v_n(x) \;\; \text{is not dyadic} \Big\}. \end{align*}

    It is not difficult to note that each of \mathcal C_1, \mathcal C_2 is a packing of A and, similarly, each of \mathcal Q_1 , \mathcal Q_2 is a packing of B . Moreover, each square of the packing {\mathcal B} is in the collection \mathcal C_i\times \mathcal Q_j , i, j\in \{1, 2\} . Therefore,

    \begin{align*} \sum\limits_{(u, \mathrm v)\in\mathcal B} \mu( \mathrm u)^q \nu( \mathrm v)^q h(2^{-n}) g(2^{-n}) \le& \Big[ \sum\limits_{ \mathrm u\in \mathcal C_1}\mu( \mathrm u)^q h(2^{-n}) + \sum\limits_{ \mathrm u\in \mathcal C_2} \mu( \mathrm u)^q h(2^{-n})\Big] \\ &\cdot\Big[ \sum\limits_{ \mathrm v\in \mathcal Q_1} \nu( \mathrm u)^q g(2^{-n}) + \sum\limits_{ \mathrm v\in \mathcal Q_2} \nu( \mathrm u)^q g(2^{-n})\Big]\\ \le& 4 M_{\mu,n}^{*q,h}(A) h(2^{-n} )M_{\nu, n}^{*q,g}(B) g(2^{-n}). \end{align*}

    This holds, for any packing of A\times B , so we have

    M_{\mu\times \nu,n}^{*q,hg}(A\times B) h(2^{-n)}g(2^{-n)} \le 4 M_{\mu,n}^{*q,h}(A) h(2^{-n} )M_{\nu, n}^{*q,g}(B) g(2^{-n})

    and then

    \overline{ {\mathsf P}}^{*\xi\zeta}(A\times B) \le 4 \overline{ {\mathsf P}}_{n}^{*\xi}(A)\; \overline{ {\mathsf P}}_{n}^{*\zeta}(B).

    Let

    A\subseteq \bigcup\limits_i A_i

    for

    B\subseteq \bigcup\limits_j B_j,

    we have:

    \begin{align*} {\mathsf P}^{*\xi\zeta} (A\times B) &\le \sum\limits_{i,j} \overline{ {\mathsf P}}^{*\xi\zeta}(A_i\times B_j)\le 4 \sum\limits_{i,j} \overline{ {\mathsf P}}^{*\xi}(A_i)\; \overline{ {\mathsf P}}^{*\zeta}(B_j).\\ &\le 4 \Big(\sum\limits_i \overline{ {\mathsf P}}^{*\xi}(A_i)\Big) \; \Big( \sum\limits_j \overline{ {\mathsf P}}^{*\zeta}(B_j)\Big). \end{align*}

    Since (A_i) represents an arbitrary covering of E and (B_j) represents an arbitrary covering of B , we can deduce that

    {\mathsf P}^{*\xi\zeta} (A\times B) \le 4 {\mathsf P}^{*\xi} (A) {\mathsf P}^{*\zeta} ( B).

    Finally, by applying (3.1), we obtain the desired conclusion.

    Let \mu, \theta\in \mathcal{M} (\mathbb{R}^d) , q, s, t \in \mathbb R , and x\in\text{supp}(\mu) , and recall the upper and lower (q, h) -densities of \theta at x with respect to \mu as defined in (1.7). In this section, we assume that

    { \mathcal P}^{\xi_s}(A) < \infty

    and

    { \mathcal P}^{\zeta_t}(B) < \infty.

    When studying fractal measures, a common question that naturally arises is whether we can guarantee the existence of subsets that possess finite or positive Hausdorff measures. This question becomes crucial in understanding the intricate structure of fractals, as it involves determining whether certain subsets exhibit measurable properties in terms of the Hausdorff measure, either finite or positive. Assume that

    \begin{equation} \inf\limits_{0 < r\le \delta} \frac{q\ln \mu( \mathsf B(x,r) + s\ln (2r)}{\ln \delta}\le -\alpha \quad \text{and} \quad \inf\limits_{0 < r\le \delta} \frac{q\ln \nu( \mathsf B(x,r) +t \ln (2r)}{\ln \delta}\le -\alpha \end{equation} (3.3)

    for some positive real number \alpha . The assumption (3.3) implies, for every \delta > 0 that is small enough, that

    \mu( \mathsf B(x,r))^q \nu( \mathsf B(x,r))^q (2r)^{t+s} \ge \delta^{-2\alpha}.

    It follows that for

    G = \{x\}\times\{y\},\ \ \ \delta > 0,

    we then have

    \overline{ \mathcal H}^{q, s+t}_{\mu\times \nu, 2\delta}(G) \ge (2\delta)^{-2\alpha}.

    Letting \delta tend to zero, we get

    { {\mathsf H}}^{\xi_s\zeta_t}(\{G\}) \ge { \mathcal H}^{\xi_s\zeta_t}(\{G\}) = \overline{ \mathcal H}^{\xi_s\zeta_t}(\{G\}) = +\infty.

    Note that the assumption (3.3) is satisfied; for instance, if we take

    \mu = \nu

    to be the Lebesgue measure with

    q+t < 0.

    In this case, we see that the Hausdorff measure constructed above is the standard Hausdorff measure \mathcal H^\varphi with

    \varphi (r) = (2r)^{q+t}.

    Thus, for any closed nonempty set

    G \subseteq A \times B ,

    every subset of G , including the empty set, is a subset of infinite measures. Thus, we may construct the measures { {\mathsf H}}^{\xi_s\zeta_t} for which the subset of finite measure properties can fail to hold for every closed set of infinite measures. One can assume also that for every \delta > 0 , the following exists:

    0 < r\le \delta/2,

    such that

    \mu( \mathsf B(x,r))^q (2r)^t\le \delta.

    Using Theorem 1, we formulate a sufficient condition to obtain

    0\le {\mathsf H}^{\xi_s\zeta_t} (G) \le {\mathsf P}^{\xi_s\zeta_t} (G) < \infty.

    First, we will state the following result, which is a direct consequence of Theorem 1.

    Corollary 1. Let A\subset \mathbb R^d and B\subset \mathbb R^l , \mu, \theta\in \mathcal {P}(\mathbb R^d) , and \nu, \theta'\in \mathcal {P}(\mathbb R^l) such that \mu and \nu satisfy the doubling condition. Let

    G'\subset G\subseteq A\times B,

    such that

    \mathcal H_{\mu\times \nu}^{q, s+t} (G) = \infty.

    (1) Assume that if \inf_{(x, y)\in G'} \underline{d}^{q, h_s}_\mu(x, \theta) < \infty and \inf_{(x, y)\in G'} \underline{d}^{q, h_t}_\nu(x, \theta') > 0 , then {\mathsf P}^{\xi_s\zeta_t} (G') < \infty .

    (2) Assume that if \text{sup}_{(x, y)\in G'} \overline{d}^{q, h_s}_\mu(x, \theta) < \infty and \text{sup}_{(x, y)\in G'} \overline{d}^{q, h_t}_\nu(x, \theta') > 0 , then {\mathsf H}^{\xi_s\zeta_t} (G') > 0 .

    Proof. Using [30, Lemma 3], we have

    {\mathsf H}^{\xi_s} (A) \ge \gamma \theta(A)

    if

    \sup\limits_{x\in A} \overline{d}^{q, h_s}_\mu(x, \theta) < \infty

    and

    {\mathsf P}^{\xi_s}(A) \le \tilde \gamma \theta(A),

    whenever

    \inf\limits_{x\in A} \underline{d}^{q, h_s}_\mu(x, \theta) > 0,

    where \gamma, \tilde \gamma are positive constants. for all \theta\in \mathcal {P}(\mathbb R^d) . Thus, the result follows from Theorem 1.

    Example 1. Recall the construction of the Moran set given in Section 2.2.

    Lemma 3. [49] Let A \subset I be a Moran set that satisfies the strong separation condition, and let \theta be a finite Borel measure with

    \text{supp}(\theta) \subset A .

    Then there are some positive constants c_i ( 1 \leq i \leq 4 ) depending on \delta and t , such that the following inequalities hold for any \varphi(i) \in A :

    \begin{align*} &c_1 \substack{\underline{\lim} \\ {n\to \infty}} \frac{\theta(I_n(i))}{\mu(I_n(i))^q |I_n(i)|^t} \leq \substack{\underline{\lim} \\ {r\to 0}} \frac{\theta\big( B(\varphi(i), r)\big)}{\mu\big(B(\varphi(i), r)\big)^q (2r)^t} \leq c_2 \substack{\underline{\lim} \\ {n\to \infty}} \frac{\theta\big(I_n(i)\big)}{\mu\big(I_n(i)\big)^q |I_n(i)|^t},\\ &c_3 \substack{\overline{\lim} \\ {n\to \infty}} \frac{\theta\big(I_n(i)\big)}{\mu\big(I_n(i)\big)^q |I_n(i)|^t} \leq \substack{\overline{\lim} \\ {r\to 0}} \frac{\theta\big( B(\varphi(i), r)\big)}{\mu\big(B(\varphi(i), r)\big)^q (2r)^t} \leq c_4 \substack{\overline{\lim} \\ {n\to \infty}} \frac{\theta(I_n(i))}{\mu(I_n(i))^q |I_n(i)|^t}. \end{align*}

    Now consider the special case I = [0, 1] , n_k = 2 , and c_{kj} = \frac13 for all k\geq1 and 1\leq j\leq n_k . In this case, the Moran set A = B is the classical ternary Cantor set. Let

    \alpha = \frac{\log 2}{\log 3}

    and \theta and \theta' be probability measures on I defined by

    \begin{align*} \theta\big(I_n(i)\big)& = \begin{cases} |I_n(i)|^\alpha, & {if}\;\; i\in D,\\ 0, & {otherwise}, \end{cases}\\ \theta'\big(I_n(i)\big)& = \begin{cases} |I_n(i)|^\beta, & {if}\;\; i\in D,\\ 0, & {otherwise}, \end{cases} \end{align*}

    where

    \alpha = q+s\; \; {and}\; \; \beta = q+t.

    It is clear that

    \text{supp}(\theta)\subset E \; \; {and}\; \; \text{supp}(\theta)'\subset E.

    Moreover, we have

    \lim\limits_{ n\to \infty} \frac{\theta(I_n(i))}{\mu(I_n(i))^q |I_n(i)|^s} = 1 \quad {and}\quad \lim\limits_{ n\to \infty} \frac{\theta'(I_n(i))}{\mu(I_n(i))^q |I_n(i)|^t} = 1.

    It follows, using Lemma 3, that

    0 < \underline{d}^{q, h_s}_\mu(x, \theta) \le \overline{d}^{q, h_s}_\mu(x, \theta) < \infty

    and

    0 < \underline{d}^{q, h_t}_\nu(x, \theta) \le \overline{d}^{q, h_t}_\nu(x, \theta) < \infty.

    Corollary 1 implies that

    0 < {\mathsf H}_{\mu\times \nu}^{q, s+t} (A\times A) \le {\mathsf P}_{\mu\times \nu}^{q, s+t} (A\times A) < \infty.

    Example 2. Let \mu, \nu\in \mathcal M(\mathbb R) , q\in \mathbb R , and let A and B be two sets of points in the x -axis and y -axis, respectively. In this example, we give a sufficient condition to obtain

    {\mathsf b}_{\mu\times \nu}^q (A\times B) = {\mathsf b}_\mu^q(A) + {\mathsf b}_{\nu}^q(B).

    From Theorem 1, we have

    {\mathsf b}_{\mu\times \nu}^q (A\times B) \ge {\mathsf b}_\mu^q(A) + {\mathsf b}_{\nu}^q(B),

    so we only have to prove the inverse inequality. For this, for t, s \in \mathbb R , we define the lower \zeta_t -dimensional density of A at the point y as

    D^{\zeta_t}(y) = \liminf\limits_{r\to 0} \inf\limits_{x\in B}\frac{ {\mathsf H}_\nu^{q,t}\Big(A\cap \mathsf B(y,r)\Big)}{\nu\big( \mathsf B(x,r) \big)^q (2r)^t}.

    Fix r > 0 and define the set I_y(r) as the centered interval on y with the length r . For n \ge 1 , consider the set

    B_n = \left\{ y\in B, \;\; {\mathsf H}^{\zeta_t} \Big(B\cap I_y(r)\Big ) > \sup\limits_{x\in B}\nu(I_x(r))^q r^t/n, \quad \forall r \le n^{-1} \right\}.

    Assume that D^{\zeta_t}(y) > 0 for all y\in F , which implies clearly that B_n \nearrow B . In addition, if we prove that

    \begin{equation} { {\mathsf H}}_{\mu\times\nu}^{q, s+t} (A\times B_n) < +\infty \end{equation} (3.4)

    for some n\in \mathbb N , then we deduce that

    {\mathsf b}_{\mu\times \nu} (A\times B) = s+t.

    This gives the result if we choose

    t = {\mathsf b}_{\nu}^q(B) \; \; {and}\; \; s = {\mathsf b}_{\mu}^q(A).

    Now, we will prove (3.4). Let

    \widetilde A \subseteq A \; \; {and}\; \; \widetilde B_n \subseteq B_n.

    Let n be an integer and 0 < r \le 1/n ; we then define

    I(r) = \big\{ I_y(r),\ \ \ y\in \widetilde B_n \big\}.

    We can extract f a finite subset J(r) rom I(r) such that \widetilde B_n \subset J(r) and no three intervals of J(r) have points in it.

    Lemma 4. For 0 < r \le 1/n , we have

    \begin{equation} J(r) \le 2 nr^{-t} \big(\sup\limits_{x\in B}\nu(I_x(r))\big)^{-q} {\mathsf H}^{\zeta_t}(B). \end{equation} (3.5)

    Proof. Divide the set J(r) into J_1(r) and J_2(r) such that in each of them the intervals do not overlap. Using the definition of the set F_n , we get

    \big(\sup\limits_{x\in F}\nu(I_x(r))\big)^{-q} r^{-t}n {\mathsf H}^{\zeta_t}(B) \ge \sum\limits_{I\in J_1(r)} \big(\sup\limits_{x\in B}\nu(I_x(r))\big)^{-q} r^{-t}n {\mathsf H}^{\zeta_t}(B \cap I) > \# J_1(r).

    Similarly, we obtain

    \# J_2(r)\le \big(\sup\limits_{x\in F}\nu(I_x(r))\big)^{-q} r^{-t}n {\mathsf H}^{\zeta_t}(B)

    as required.

    In the other hand, for \epsilon > 0 , a sequence of sets \{A_i\} exists such that

    \widetilde A\subseteq \bigcup\limits_i A_i

    and that

    \sum\limits_i \overline{ {\mathsf H}}^{\xi_s}_0(A_i) \le {\mathsf H}^{\xi_s}(A) +\epsilon.

    Thus, we have a sequence \{B_{i, j}\} of intervals of length r covering \widetilde A such that the family \{B_{i, j}\}_j , for each i , is a covering of A_i and

    \begin{equation} \sum\limits_i N_{\mu, r/2}^q (A_i) r^s\le {\mathsf H}^{\xi_s}(A) +2\epsilon. \end{equation} (3.6)

    Let [a, b] represent any interval within the set \{B_{i, j}\} . Enclose all points in this set that fall between the lines x = a and x = b with squares whose sides are parallel to these lines. The projections of these squares onto the y -axis correspond to intervals in J(r) . In a similar manner, construct sets of squares for each interval in \{B_{i, j}\} , and denote the set of squares associated with the interval [a, b] as C(a, b) . Since the number of squares in C(a, b) does not exceed the number of intervals in J(r) , and each square intersecting \widetilde A \times \widetilde B_n can be inscribed within a centered ball of diameter r' = 3r , it follows that:

    N_{\mu\times \nu, r'/2}^q ( \widetilde A \times \widetilde B_n) \le \# J(r)\; \sup\limits_{x\in F}\nu(I_x(r))^q \sum\limits_{i,j} \mu(B_{i, j})^q.

    Thus, using (3.5) and (3.6), we get

    \begin{align*} \overline{ {\mathsf H}}^{q, s+t}_{\mu\times \nu, r'/2}( \widetilde A \times \widetilde B_n) &\le 2 nr^{-t} {\mathsf H}^{\xi_t}(B) (3 r)^{s+t} \sum\limits_{i,j} \mu(B_{i, j})^q\\ &\le 2 \times 3^{s+t} n {\mathsf H}^{\zeta_t}(B) \sum\limits_i N_{\mu, r/2}^q (A_i) r^s\\ &\le 2 \times 3^{s+t} n {\mathsf H}^{\zeta_t}(B) ( {\mathsf H}^{\xi_s}(A)+ 2\epsilon). \end{align*}

    Since \epsilon is arbitrarily, we get

    { {\mathsf H}}^{s+t}_{0}( \widetilde A\times \widetilde B_n) \le 2 \times 3^{s+t} n {\mathsf H}^{\zeta_t}(B) {\mathsf H}^{\xi_s}(A).

    Finally, we have

    \overline{ {\mathsf H}}^{s+t} (A\times B_n) \le 2 \times 3^{s+t} n {\mathsf H}^{\zeta_t}(B) {\mathsf H}^{\xi_s}(A),

    from which the Eq (3.4) follows.

    The result given in this example can be summarized in the next theorem.

    Theorem 3. Let E and F be sets of points in x -axis and y -axis, respectively. Set

    s = {\mathsf b}_\mu^q(A) \; \; \mathit{\text{and}}\; \; t = {\mathsf b}_{\nu}^q(B)

    and assume that {\mathsf H}^{\xi_s}(A), {\mathsf H}^{\zeta_t}(B)\in (0, \infty) , and, for all y\in F , D^{\zeta_t}(y) > 0 . In this case,

    {\mathsf b}_{\mu\times \nu}^q (A\times B) = {\mathsf b}_\mu^q(A) + {\mathsf b}_{\nu}^q(B).

    We define the set \mathcal G of all continuous and increasing functions h on [0, t_0) for some t_0 > 0 satisfying h(0) = 0 , and the function

    t \longmapsto h(t)/t^d

    is decreasing. We assume in this section that h \in \mathcal G and that it t satisfies the doubling condition

    h(2t) \leq 2^d h(t),\; \;\text{for}\;\; 0 < t < t_{0} /2.

    A cube I(x, r) in \mathbb R^d is a subset of the form

    I(x,r) = \prod\limits_{i = 1}^{n} \left[ x_{i}-r,\; x_{i}+r \right].

    For a cube I , we use l(I) to denote its side length. In this section, using cubes with sides of a length less than \delta rather than closed balls, we define a generalized Hausdorff measure \widetilde{ \mathcal H}_{\mu}^{q, h} equivalent to the generalized Hausdorff measure { \mathcal H}_{\mu}^{q, h} . We prove that this measure is appropriate for estimating the measure of the generalized Cantor set. Let \mu \in \mathcal P_{D}(\mathbb R^d) , h \in \mathcal{F}_0, and q \in \mathbb R . Define

    \widetilde{ \mathcal H}_{\mu,0}^{q,h}(A) = \lim\limits_{\delta \to 0} \widetilde{ \mathcal H}_{\mu,\delta}^{q,h}(A),

    where

    \widetilde{ \mathcal H}_{\mu,\delta}^{q,h}(A) = \inf \sum\limits_i \mu( \mathsf B(x_i,\; r_i))^q h(|I_i|)

    with the infimum being taken over all coverings of A by cubes with sides of a length \leq \delta . Then a constant C exists such that

    C^{-1}\; \widetilde{ \mathcal H}_{\mu,0}^{q,h}(A) \leq { \mathcal H}_{\mu,0}^{q,h}(A) \leq C \; \widetilde{ \mathcal H}_{\mu,0}^{q,h}(A).

    We will compute the estimation of the generalized Hausdorff measure of the \mathcal K^d . More precisely, we have the following result.

    Theorem 4. Let \mathcal K^d be the d -dimensional symmetric generalized Cantor set ( d\geq 1 ) constructed by the system \Big\{ {\mathsf L}, \{n_k\}_{k\ge 1}, \{\lambda_k\}_{k\ge 1}\Big\} . We then have

    2^{-3d}\liminf\limits_{k\to \infty} (n_1n_2\ldots n_k)^d \lambda_k^q h(\lambda_k)\le { {\mathsf H}}_{\mu,0}^{q,h}( \mathcal K^d) \le { {\mathsf P}}_{\mu,0}^{q,h}( \mathcal K^d) \le M \limsup\limits_{k\to \infty} (n_1n_2\ldots n_k)^d \lambda_k^q h(\lambda_k).

    Proof. We focus on proving only the left-hand inequality; the validity of the right-hand inequality can be established using similar argument. Let \Psi be the set function in Lemma 1 . Let \varepsilon be a positive number with \varepsilon \leq r_0 and \{I_i\} be a \varepsilon -covering of \mathcal K^d by open cubes with the sides r_i\leq \varepsilon . We have

    \begin{align*} \sum\limits_i \mu(I_i)^q h(r_i) &\ge 2^{-3d} \sum\limits_i \Psi(I_i) \\ &\ge 2^{-3d} \Psi(\bigcup\limits_i I_i)\ge 2^{-3d} b. \end{align*}

    Since b is an arbitrary number such that

    b < \liminf\limits_{k\to \infty} (n_1n_2\ldots n_k)^d \lambda_k^q h(\lambda_k),

    then we get the desired result.

    In this example, we take d = 1 and we consider the one-dimensional generalized Cantor set \mathcal K_1 (resp. \mathcal K_2 ) constructed by the system \Big\{ {\mathsf L}, \{n_k\}_{k\ge 1}, \{\lambda_k\}_{k\ge 1}\Big\} (resp. \Big\{ {\mathsf L}, \{n_k\}_{k\ge 1}, \{\Lambda_k\}_{k\ge 1}\Big\} ) In the following, we consider l = 1, d = 1, n_k = 2 , and

    \lambda_k = k^{\xi_1} 2^{-k/\alpha}\qquad \Lambda_k = k^{-\xi_2} 2^{-k/\beta}\qquad h(t) = t^{\alpha}\qquad g(t) = t^{\beta}

    Theorem 5. The constants M and M' exist such that

    M \liminf\limits_{k\to \infty} 2^k \lambda_k^{q+\alpha} 2^k \Lambda_k^{q+\beta} \leq \overline {\mathsf H}_{\mu\times \nu,0 }^{q, hg}( \mathcal K_1\times \mathcal K_2) \leq \overline {\mathsf P}_{\mu\times \nu}^{q, hg}( \mathcal K_1\times \mathcal K_2)\leq M' \limsup\limits_{k \to \infty} 2^k \lambda_k^{q+\alpha} 2^k \Lambda_k^{q+\beta}.

    Proof. We focus on proving only the left-hand inequality; the validity of the right-hand inequality can be deduced using the same idea. Assume that

    A: = \liminf\limits_{k\to \infty} 2^k \lambda_k^{q+\alpha} 2^k \Lambda_k^{q+\beta} > 0;

    otherwise, the result remains trivial. Let

    0 < B < A

    and choose a positive integer k_1 satisfying the following inequality:

    B < 2^k \lambda_k^{q+\alpha} 2^k \Lambda_k^{q+\beta}

    for all k\ge k_1 . Now we define the sequence (\tilde \Lambda_k)_{k\ge k_1} as

    B = 2^k \lambda_k^{q+\alpha} 2^k \tilde\Lambda_k^{q+\beta}.

    It follows that

    \begin{equation} \tilde \Lambda_k < \Lambda_k \quad \text{and} \quad 2^2 \lambda_{k+1}^{q+\alpha}\; \tilde\Lambda_{k+1}^{q+\beta} = \lambda_{k}^{q+\alpha} \; \tilde\Lambda_{k}^{q+\beta} \end{equation} (4.1)

    for all k\ge k_1 .

    Let

    K\subset \mathcal K_1\times \mathcal K_2

    and use I_1^{k} (resp. I_2^{k}) to denote any of the closed intervals of the generation r of \mathcal K_1 (resp. \mathcal K_2 ). Then

    \begin{align*} N_{\mu\times \nu, k+1}^q (K)& = \inf \Big\{ \sum\limits_i \mu \times \nu(I_1^{r+1}\times I_2^{k+1})^q , \;\; I_1^{k+1}\times I_2^{k+1} \;\; \text{ meeting} \;\; K \Big\} \\ &\le \inf \Big\{ \sum\limits_i \mu (I_1^{r+1})^q \nu(I_2^{k+1})^q , \;\; I_1^{k+1}\times I_2^{k+1} \;\; \text{ meeting}\;\; K \Big\}. \end{align*}

    Note that

    \lambda_{k+1} = \lambda_k (\frac{k+1}{k})^{\xi_1} 2^{-1/\alpha}\quad \text{and} \quad \Lambda_{r+1} = \Lambda_k (\frac{k}{k+1})^{\xi_2} 2^{-1/\beta},

    and then

    \begin{align*} N_{\mu\times \nu, k+1}^q (K)&\le \inf \Big\{ \sum\limits_i \mu (I_1^{k+1})^q \nu(I_2^{k+1})^q , \;\; I_1^{k+1}\times I_2^{k+1} \;\; \text{ meeting} \;\;K \Big\} \\ &\le k_{k+1} 2^{-q/\alpha} 2^{-q/\beta} (\frac{k+1}{k})^{q\xi_1-q\xi_2} \inf \Big\{ \sum\limits_i \mu (I_1^{k})^q \nu(I_2^{k})^q , \;\; I_1^{k}\times I_2^{k} \;\; \text{ meeting} \;\; K \Big\} \\ & = 2^2 2^{-q/\alpha} 2^{-q/\beta} (\frac{k+1}{k})^{q\xi_1-q\xi_2} N_{\mu\times \nu, k}^q (K), \\ N_{\mu\times \nu, k+1}^q (K) \lambda_{k+1}^\alpha \tilde\Lambda_{k+1}^\beta &\le 2^2 2^{-q/\alpha} 2^{-q/\beta} (\frac{k+1}{k})^{q\xi_1-q\xi_2} \lambda_{k+1}^\alpha \tilde\Lambda_{k+1}^\beta N_{\mu\times \nu, k}^q (K)\\ &\le \frac{2^2 2^{-q/\alpha} 2^{-q/\beta}}{\lambda_{k+1}^q \tilde\Lambda_{r+1}^q} (\frac{k+1}{k})^{q\xi_1-q\xi_2} \lambda_{k+1}^{q+\alpha} \tilde\Lambda_{k+1}^{q+\beta} N_{\mu\times \nu, k}^q (K)\\ &\le^{(4.1)} \frac{ 2^{-q/\alpha} 2^{-q/\beta}}{\lambda_{k+1}^q \tilde\Lambda_{k+1}^q} (\frac{k+1}{k})^{q\xi_1-q\xi_2} \lambda_{k}^{q+\alpha} \tilde\Lambda_{k}^{q+\beta} N_{\mu\times \nu, k}^q (K)\\ &\le^{(4.1)}\Big[ \frac{ 2^{-1/\alpha} 2^{-1/\beta } \lambda_{k} \tilde\Lambda_{k} }{\lambda_{k+1} \tilde\Lambda_{k+1}} (\frac{k+1}{k})^{\xi_1-\xi_2} \Big]^q \lambda_{k}^{\alpha} \tilde\Lambda_{k}^{\beta} N_{\mu\times \nu, k}^q (K). \end{align*}

    It follows that the sequence \big\{ N_{\mu\times \nu, k}^q (K) \lambda_k^\alpha \tilde\Lambda_r^\beta \big\} is decreasing, and we may define the function

    \Phi(A) = \lim\limits_{k \to 0}N_{\mu\times \nu, k}^q (A) \lambda_k^\alpha \tilde\Lambda_k^\beta.

    Case \beta\le \alpha . We can choose k_2 > k_1 such that

    \Lambda_k < \lambda_{k+1} \qquad \text{for all } \ \ \ k\ge k_2.

    Let

    s_o = \Lambda_{k_2}

    and consider any two-dimensional open cube I with the side s\le s_0 . Let p and k be the unique positive integers such that

    \lambda_{p+1} < s\le \lambda_p \qquad \text{and} \qquad \Lambda_{k+1} < s\le \Lambda_k.

    Since

    \lambda_{p+1} < \Lambda_k < \lambda_{k+1}

    for k \ge k_2 , we deduce that k < p . Moreover, the open cube I meets at most 2^2 rectangles of the form I_1^{p}\times I_2^{k} and so meets at most 2^4 rectangles of the form I_1^{p+1}\times I_2^{k+1} . Therefore, since p > k , it follows that

    \begin{align*} N_{\mu\times \nu, p+1}^q (I)&\le \inf \Big\{ \sum\limits_i \mu (I_1^{p+1})^q \nu(I_2^{p+1})^q , \;\; I_1^{p+1}\times I_2^{p+1} \;\; \text{ meeting } I \Big\} \\ &\le 2^4 2^{p-r} \lambda_{p+1}^q \Lambda_{p+1}^q. \end{align*}

    Since 2^k \Lambda_k^\beta decrease as r increases, note that

    2^{p-k} \Lambda_{p+1}^\beta < \Lambda_{k+1}^\beta.

    Then,

    \begin{align*} \Phi(I) &\le N_{\mu\times \nu, p+1}^q (I) \lambda_{p+1}^\alpha \tilde\Lambda_{p+1}^\beta\le 2^{4+p-k} \lambda_{p+1}^q \Lambda_{p+1}^q \lambda_{p+1}^\alpha \tilde\Lambda_{p+1}^\beta\\ &\le 2^{4+p-k}\mu(Q^{p+1})^q \nu(Q^{(p+1)})^q \lambda_{(p+1)}^{\alpha} \; \Lambda_{p+1}^{\beta}\\ &\le 2^{4} \mu(Q^{(p+1)})^q \nu(Q^{(p+1)})^q s^{\alpha+\beta}. \end{align*}

    Example 3. As a consequence, we construct an estimate of the generalized packing measures of product sets of one-dimensional generalized Cantor sets. Let 0 < \alpha and \beta < 1 . In this example, we consider the one-dimensional generalized Cantor set \mathcal K_1 (resp. \mathcal K_2 ) constructed by the system \Big\{ l, \{k_r\}_{r\ge 1}, \{\lambda_r\}_{r\ge 1}\Big\} \left(\text{resp.}\; \Big\{ l, \{k_r\}_{r\ge 1}, \{\Pi_r\}_{r\ge 1}\Big\}\right) . Set l = 1 and n_k = 2 and consider in the following:

    \lambda_k = \left(k^2 2^{-k}\right)^{ \frac{1}{\alpha+q}},\; \; \Lambda_k = \left(k^{-j} 2^{-k}\right)^{ \frac{1}{\beta+q}},\;\; h(t) = t^{\alpha},\;{and}\;\;g(t) = t^{\beta}.

    (1) We have

    \begin{align*} \lim\limits_{k\to \infty} 2^k \lambda_k^{q+\alpha} 2^k \Lambda_k^{q+\beta}& = \lim\limits_{k\to \infty} 2^k \lambda_k^{q+\alpha} 2^k \Lambda_k^{q+\beta}\\ & = \lim\limits_{k\to \infty} (k^{2} 2^{-k}\big) \big( k^{-j} 2^{-k}\big) 2^k\\& = \lim\limits_{k\to \infty} k^{2-j} . \end{align*}

    Therefore, \overline{ {\mathsf H}}_{\mu\times \nu, 0}^{q, hg} (\mathcal K_1\times \mathcal K_2) (resp. \overline{ {\mathsf P}}_{\mu\times \nu}^{q, hg} (\mathcal K_1\times \mathcal K_2) ) is infinite, positive finite, and zero for j = 1, 2, 3 , respectively.

    (2) We have

    \begin{eqnarray*} \lim\limits_{k\to \infty} 2^k \lambda_k^{q+\alpha} = \lim\limits_{k\to \infty} 2^k (k^{2} 2^{-k}\big) = \infty. \end{eqnarray*}

    Therefore,

    \overline{ {\mathsf H}}_{\mu,0}^{q, h}( \mathcal K_1) = \overline{ {\mathsf P}}_{\mu}^{q, h}( \mathcal K_1) = \infty.

    (3) We have

    \begin{eqnarray*} \lim\limits_{k\to \infty} 2^k \Lambda_k^{q+\alpha} = \lim\limits_{k\to \infty} 2^k (k^{-j} 2^{-k}\big) = 0. \end{eqnarray*}

    Therefore,

    \overline{ {\mathsf H}}_{\nu,0}^{q, g} ( \mathcal K_2) = \overline{ {\mathsf P}}_{\nu}^{q, g} ( \mathcal K_2) = 0.

    Let A \subseteq \mathbb{R}^d and B \subseteq \mathbb{R}^l . In this work, we present a novel approach that is distinct from that in [30], as it is specifically tailored for Euclidean spaces, to establish the following inequality:

    {\mathsf H}_{\mu}^{q,h}(A) {\mathsf H}_{\nu}^{q,g}(B)\le c_1 {\mathsf H}_{\mu\times \nu}^{q, hg}(A\times B) \le c_2\; {\mathsf H}_{\mu}^{q,h}(A) {\mathsf P}_{\nu}^{q,g}(B)\le c_3\; {\mathsf P}_{\mu\times \nu}^{q, hg}(A\times B) \le c_4 {\mathsf P}_{\mu}^{q,h}(A) {\mathsf P}_{\nu}^{q,g}(B).

    This result holds under the assumption that \mu, \nu, h, g satisfy the doubling condition and that none of the products is of the form 0 \times \infty or \infty \times 0 . Furthermore, by analyzing the measures of symmetric generalized Cantor sets, we demonstrate that the exclusion of the 0 \infty condition is indispensable and thus cannot be omitted. Let (\mathcal X, \rho) and (\mathcal X', \rho') be two separable metric spaces. The result presented in this paper holds true for both \mathcal X and \mathcal X' , though the approach used in our proof does not extend to metric spaces.

    (1) Let {\mathcal B}(\mathcal X) denote the family of closed balls in \mathcal X , and let \Phi(\mathcal X) represent the class of pre-measures. A pre-measure is any increasing function

    \xi : {\mathcal B}( \mathcal X) \to [0, +\infty]

    satisfying

    \xi(\emptyset) = 0 .

    It is natural to consider a general construction of \mathcal H_\mu^{q, \xi}, defined using a measure \mu and a pre-measure \xi. Specifically, our result applies when

    \xi( \mathsf B(x,r)) = h(2r)

    and allows for the choice

    \xi( \mathsf B) = h(| \mathsf B|)

    for all \mathsf B \in {\mathcal B}(\mathcal X). Let

    \xi \in \Phi( \mathcal X)\; \; \text{and}\; \; \xi' \in \Phi( \mathcal X') .

    We define \xi_0, the Cartesian product measure generated from the functions \xi and \xi', on {\mathcal B}(\mathcal X \times \mathcal X') as

    \xi_0( \mathsf B \times \mathsf B') = \xi( \mathsf B)\xi'( \mathsf B'), \ \ \ \text{for all }\ \ \mathsf B \in {\mathcal B}( \mathcal X), \, \mathsf B' \in {\mathcal B}( \mathcal X').

    We strongly believe that the resulting measure is particularly well-suited for studying Cartesian product sets. Under a suitable doubling condition, we obtain the following result:

    \begin{equation} {\mathsf H}_{\mu \times \nu}^{q,\xi_0}(A \times B) = {\mathsf H}_\mu^{q,\xi}(A) {\mathsf H}_\nu^{q, \xi'}(B), \end{equation} (5.1)

    for all A \subset \mathcal X and B \subset \mathcal X'. This construction was first introduced by Kelly in [50]; see also [51].

    (2) To establish the equality presented in Eq (5.1), we draw inspiration from the work of Kelly [50]. Specifically, we propose constructing a weighted lower H-W measure, denoted \mathcal{W}_\mu^{q, h} , for any given Hausdorff measure h . This approach involves assigning non-negative weights to the covering sets, adhering to what is commonly referred to as the third method for constructing an outer measure. On the basis of this framework, we conjecture that the equality in (5.1) holds if the constructed weighted measure satisfies

    \mathcal{W}_\mu^{q,\xi} = {\mathsf H}_\mu^{q,\xi} .

    Similarly, one can construct a weighted upper H-W measure, denoted \mathcal{Q}_\mu^{q, h}, by following the same approach used for the weighted lower H-W measure but replacing covering with packing [8]. We conjecture that the equality

    {\mathsf P}_{\mu \times \nu}^{q,\xi_0}(A \times B) = {\mathsf P}_\mu^{q,\xi}(A) {\mathsf P}_\nu^{q,\xi'}(B),

    for all A \subset \mathcal X and B \subset \mathcal X', holds if the constructed weighted measure satisfies

    \mathcal{Q}_\mu^{q,\xi} = {\mathsf P}_\mu^{q,\xi} .

    (3) A similar result to (1.2) and (1.3) can be achieved by examining fractal pseudo-packings and weighted measures of the H-S type. The purpose of employing these generalizations is to eliminate the need for assuming the doubling condition.

    (4) Our results in this paper can be readily extended to the setting of generalized lower and upper H-S measures, denoted {\mathsf H}_{\mu_1\times \mu_2}^{q, h} and {\mathsf P}_{\mu_1\times \mu_2}^{q, h} . These fractal measures play a crucial role in the multifractal analysis of a measure relative to another measure [52].

    The author declares he has not used Artificial Intelligence (AI) tools in the creation of this article.

    This work was supported by the Deanship of Scientific Research, Vice Presidency for Graduate Studies and Scientific Research, King Faisal University, Saudi Arabia [KFU251033].

    The author declares no conflict of interest.



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