Research article

The Fekete-Szegö functional and the Hankel determinant for a certain class of analytic functions involving the Hohlov operator

  • Received: 07 August 2022 Revised: 08 September 2022 Accepted: 20 September 2022 Published: 29 September 2022
  • MSC : Primary 30C45; Secondary 30C55, 33C05

  • In this paper, we introduce and study a new subclass of normalized functions that are analytic and univalent in the open unit disk U={z:zCand|z|<1}, which satisfies the following geometric criterion:

    (Lwu,vf(z)z(1e2iϕμ2z2)eiϕ)>0,

    where zU, 0μ1 and ϕ(π2,π2), and which is associated with the Hohlov operator Lwu,v. For functions in this class, the coefficient bounds, as well as upper estimates for the Fekete-Szegö functional and the Hankel determinant, are investigated.

    Citation: Hari Mohan Srivastava, Timilehin Gideon Shaba, Gangadharan Murugusundaramoorthy, Abbas Kareem Wanas, Georgia Irina Oros. The Fekete-Szegö functional and the Hankel determinant for a certain class of analytic functions involving the Hohlov operator[J]. AIMS Mathematics, 2023, 8(1): 340-360. doi: 10.3934/math.2023016

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  • In this paper, we introduce and study a new subclass of normalized functions that are analytic and univalent in the open unit disk U={z:zCand|z|<1}, which satisfies the following geometric criterion:

    (Lwu,vf(z)z(1e2iϕμ2z2)eiϕ)>0,

    where zU, 0μ1 and ϕ(π2,π2), and which is associated with the Hohlov operator Lwu,v. For functions in this class, the coefficient bounds, as well as upper estimates for the Fekete-Szegö functional and the Hankel determinant, are investigated.



    Geometric function theory is one of the most exciting areas of research in complex analysis, with applications in a wide range of mathematical fields including mathematical physics. Due to its many uses in analytical solutions to issues such as those in electrostatics, aerodynamics and fluid mechanics, researchers in the field of complex analysis have been investigating various families of analytic (or holomorphic) functions.

    Analytic functions such as ψ(z) can be expressed in the Taylor-Maclaurin series expansion about the origin z=0 as follows:

    ψ(z)=C0+C1z+C2z2+C3z3+C4z4+(zU),

    which can be normalized in the following way:

    f(z)=ψ(z)C0C1=z+j=2bjzj, (1.1)

    where

    C10,bj=CjC1,U={z:zCand|z|<1},

    and the series expansion in (1.1) is convergent in the open unit disk U. Let A denote a class of functions f(z) that are analytic (or holomorphic) in U, have the form (1.1) and are normalized by the constraints f(0)1=f(0)=0.

    The class of functions φ that are holomorphic in U and have the form

    φ(z)=1+r1z+r2z2+(zU),

    with

    φ(0)=1and(φ(z))>0(zU),

    is denoted by P.

    In the geometric function theory of complex analysis, studies of the concept of convolution are crucial. Various new and interesting subclasses of holomorphic and univalent functions have been introduced and investigated through the use of the Hadamard product (or convolution) in the direction of well-known ideas such as the integral mean, Hankel determinant, subordination, partial sums, superordination inequalities and so on. The Hadamard product (or convolution) of f and g, represented by fg, is defined by

    (fg)(z):=z+j=2bjajzj=:(gf)(z)

    for functions f and g in A given by the following series:

    f(z)=z+j=2bjzjg(z)=z+j=2ajzj(zU).

    The Gauss hypergeometric function 2F1(u,v,w;z) is defined as follows:

    2F1(u,v,w;z)=j=0(u)j(v)j(w)jzj(1)j(zU),

    where (δ)j signifies the Pochhammer symbol (or the shifted factorial) defined in terms of the Gamma function Γ, as follows:

    (δ)j=Γ(δ+j)Γ(δ)={1(j=0)δ(δ+1)(δ+2)(δ+3)(δ+j1)(j0).

    Hohlov (see [19,20]) proposed and investigated a linear operator denoted by Lwu,v and defined by Lwu,vf:AA, with

    Lwu,vf(z):=z2F1(u,v,w;z)f(z)=z+j=2(u)j1(v)j1(w)j1(1)j1bjzj(zU). (1.2)

    The above-specified three-parameter family of operators unifies several other linear operators that have been introduced and explored previously when the parameters are appropriately chosen. The works in [7,9,11,12,40,41,42,43,51,53,59,72] provide special examples of this operator. For more details, see [17,47,70,71]. It should be remarked in passing that much more general convolution operators, such as the Dziok-Srivastava operator (see [14,15]) and the Srivastava-Wright operator (see [62]), have also been investigated rather extensively in the vast literature in geometric function theory of complex analysis.

    The nth coefficient of a function belonging to the class S is well-known to be bounded by n, and the coefficient bounds provide information about the geometric properties of the function. For example, the nth coefficient of functions in the family S yields the growth and distortion properties of the function, whereas the second coefficient of functions in the family S yields the growth and distortion properties of the function itself. Studying a functional composed of combinations of the coefficients of the original function is a common issue in the geometric function theory of complex analysis. In most cases, the extremal value of the functional is required across a parameter. Some of our findings are related to the Fekete-Szegö functional, which is a key functional of this kind.

    The famous problem solved by Fekete and Szegö [16] is to determine the greatest value of the coefficient functional Ωσ(f):=|a3σa22| over the class S for each σ[0,1], which was demonstrated by using the Loewner chain technique. For various subclasses of the class of S and associated subclasses of functions in A, several scholars solved the Fekete-Szegö issue. For example, see [8,13,23,25,28,29,30,40,44], and so on. We refer to [68] for a thorough study on the Fekete-Szegöproblem of the traditional univalent function class S. Srivastava et al. claimed that the inequality was sharp in [68]. However, Peng (see [54]) has demonstrated that the extremal function presented there for the situation of ϱ(2/3,1) is not sharp. Cho et al. [10] discovered the Fekete-Szegö inequalities for close-to-convex functions with regard to a certain convex function, which improves the bound explored in [68]. Using the Hankel or Toeplitz determinants is another approach to look at the sharp bound for the nonlinear functional. We recall that Noonan and Thomas [49] introduced and investigated the qth Hankel determinant of f for q1 and n1 as follows:

    Hq(j)=|bjbj+1bj+2bj+q1bj+1bj+2bj+3bj+qbj+2bj+3bj+4bj+q+1bj+q1bj+qbj+q+1bj+2(q1)|(q,jN). (1.3)

    Several writers, notably Noor [50], have investigated the determinant Hq(j), with topics ranging from the rate of development of Hq(j) (as j) to the determinant of exact limits for particular subclasses of analytic functions in the unit disk U with specified values of j and q. When q=2, j=1, and b1=1, the Hankel determinant is H2(1)=|b3b22|. The Hankel determinant simplifies to H2(2)=|b2b4b23| when j=q=2. Fekete and Szegö [12] consider the Hankel determinant H2(1) and refer to H2(2) as the second Hankel determinant. If f is univalent in U, then the sharp upper inequality H2(1)=|b3b22|1 is known (see[16]). Janteng et al. [21] obtained sharp bounds for the functional H2(2) for the function f in the subclass RT of S, which was introduced by MacGregor [37] and which consists of functions whose derivative has a positive real part. They demonstrated that H2(2)=|b2b4b23|4/9 for each fRT. They also discovered the sharp second Hankel determinant for the classical subclasses of S, namely, the classes S and K of starlike and convex functions, respectively (see [22]). These two classes have bounds of |b2b4b23|1/8 and |b2b4b23|1. The Hankel determinants for starlike and convex functions with respect to symmetric points were recently discovered by Reddy and Krishna [57]. For functions belonging to subclasses of the Ma-Minda type starlike and convex functions, Lee et al. [34] found bounds for the second Hankel determinant.

    Mishra and Gochhayat [41] found the sharp bound to the nonlinear functional |b2b4b23| for the subclass of analytic functions given by

    Rρ(ω,t)(0t<1;0ρ<1;|ω|<π2),

    and defined as follows:

    (eiωΩρzf(z)z)>tcosω,

    using the Owa-Srivastava operator in [53]. Similar coefficient constraints are found for a variety of analytic function subclasses that are constructed by using other appropriate linear operators (see, for example, [1,32,45,46,74,75]).

    In the case when q=3 and j=1, the Hankel determinant, represented by H3(1), is given by

    H3(1)=b3(b2b4b23)b4(b4b2b3)+b5(b3b22).

    Clearly, we have

    |H3(1)||b3||b2b4b23|+|b4||b4b2b3|+|b5||b3b22|. (1.4)

    Babalola (see [5]) recently obtained the sharp upper bound of H3(1) for functions in the classes S, K and RT classes.

    Krishna et al. [31] defined RT(α) as (h(z))>α and found the bound on H3(1). Ayinla and Opoola [4] introduced the class defined by using the Sălăgean derivative operator as follows:

    (eiγ(1e2iγβ2z2)Dn+1f(z)z)>0

    and obtained inequalities for the Fekete-Szegö functional and the second Hankel determinant. Additionally, Bansal et al. [6] and Raza and Malik [56] found the bound for H3(1) for a subclass of univalent functions. Gochhayat et al. [17] recently introduced the class Rca,b and obtained the sharp bounds of H2(2) and H3(1) in terms of the Gauss hypergeometric function by utilizing the Hohlov operator. See also [2,3,26,27,33,48,55,61,65,69,73,76] for some of the recent works on the third Hankel determinant and [66] for some developments on the fourth Hankel determinant.

    Here, in this paper, we introduce a subclass of the normalized univalent function class S by using the Hohlov operator, as inspired by some of the above-mentioned researches.

    Definition 1.1. A function f(z) of the form (1.1) that is holomorphic and univalent in U is said to belong to the class Jϕμ(u,v,w) if it satisfies the following geometric criterion:

    (Lwu,vf(z)z(1e2iϕμ2z2)eiϕ)>0, (1.5)

    where zU, 0μ1 and ϕ(π2,π2).

    Remark 1.1. Choosing u=2, v=w=1 and μ=0 gives we get the class

    Jϕ0(2,1,1):=Jϕ.

    This class Jϕ was introduced and studied by Noshiro [52].

    Remark 1.2. Choosing u=2, v=w=1 and μ=ϕ=0 gives we get the class

    J00(2,1,1)=:J.

    This class J was introduced and studied by MacGregor [37].

    Remark 1.3. Choosing u=2, v=w=1, ϕ=0 and μ=1 gives we get the class

    J01(2,1,1)=:J1.

    This class J1 was introduced and studied by Hengartner and Schober [18].

    Remark 1.4. Choosing u=2, v=w=1 and μ=1 gives we get the class

    Jϕ1(2,1,1)=:Jϕ1.

    This class Jϕ1 was introduced and studied by Royster and Ziegl [58].

    Remark 1.5. Choosing u=2, v=w=1 and ϕ=0 gives we get the class

    J0μ(2,1,1)=:Jμ.

    This class Jμ was introduced and studied by Kanas and Lecko [24].

    Remark 1.6. Choosing u=2 and v=w=1 gives we get the class

    Jϕμ(2,1,1)=:Jϕμ.

    This class Jϕμ was introduced and studied by Lecko [35].

    In this article, we establish the coefficient estimates, Fekete-Szegö type inequality, and the bounds for the second and the third Hankel determinants for functions belonging to the class Jϕμ(u,v,w).

    Lemma 1.1. (see [12]) Let φ(z)P. Then

    |rj|2(jN).

    Lemma 1.2. (see [38]) Let φ(z)P. Then

    |r2υr212|{2(1υ),(υ0)2(0υ2)2(υ1)(υ2)

    for υR.

    Lemma 1.3. (see [36]) Let φ(z)P. Then

    2r2=r21+x(4r21),4r3=r31+2r1(4r21)xr1(4r21)x2+2(4r21)(1|x|2)z,

    for some complex numbers x and z such that |x|1 and |z|1.

    Theorem 1.1. Let f(z)Jϕμ(u,v,w). Then

    |b2|2(w)1r1cosϕ(u)1(v)1, (1.6)
    |b3|2(w)2(u)2(v)2(2cosϕ+μ2), (1.7)
    |b4|12cosϕ(w)3(u)3(v)3(1+μ2), (1.8)
    |b5|24(w)4(u)4(v)4(2cosϕ+2μ2cosϕ+μ4) (1.9)

    and

    |b6|240cosϕ(w)5(u)5(v)5(1+μ2+μ4), (1.10)

    where μ[0,1] and ϕ(π2,π2).

    Proof. Consider the function ϑ(z) given by

    ϑ(z)=cosϕ+isinϕ+j=1κjzjφ(z)=ϑ(z)isinϕcosϕ. (1.11)

    Then, by (1.5), we can have

    Lwu,vf(z)z(1e2iϕμ2z2)eiϕ=ϑ(z). (1.12)

    Also, from (1.11) and (1.12), we get

    Lwu,vf(z)z(1e2iϕμ2z2)eiϕ=φ(z)cosϕ+isinϕ. (1.13)

    As a result, the right-hand side of (1.13) is given by

    cosϕ+r1zcosϕ+r2z2cosϕ+=cosϕ+κ1z+κ2z2+,

    which implies that

    κj=rjcosϕ(jN). (1.14)

    Furthermore, from the left-hand side of (1.13), we have

    Lwu,vf(z)z(1e2iϕμ2z2)eiϕ=eiϕ[(1e2iϕμ2z2)(1+j=2(u)j1(v)j1(w)j1(1)j1bjzj1)]=eiϕ+(u)(v)(w)eiϕb2z+((u)2(v)22(w)2eiϕb3eiϕμ2)z2+((u)3(v)36(w)3eiϕb4eiϕ(u)1(v)1(w)1μ2b2)z3+((u)4(v)424(w)4eiϕb5eiϕ(u)2(v)22(w)2μ2b3)z4+((u)5(v)5120(w)5eiϕb6eiϕ(u)3(v)36(w)3μ2b4)z5+. (1.15)

    Now, upon comparing the coefficients of z,z2,z3,z4 and z5 in (1.14) and (1.15), we get

    b2=(w)1r1cosϕeiϕ(u)1(v)1, (1.16)
    b3=2(w)2(r2cosϕeiϕ+e2iϕμ2)(u)2(v)2. (1.17)
    b4=6(w)3(r3cosϕeiϕ+e3iϕr1cosϕμ2)(u)3(v)3, (1.18)
    b5=24(w)4(r4cosϕeiϕ+r2μ2e3iϕcosϕ+e4iϕμ4)(u)4(v)4 (1.19)

    and

    b6=120(w)5(r5cosϕeiϕ+r3μ2e3iϕcosϕ+e5iϕr1cosϕμ4)(u)5(v)5. (1.20)

    The desired estimate is obtained by first applying the triangle inequality to (1.16) to (1.20) and then using Lemma 1.1. The proof of Theorem 1.1 is thus completed.

    Theorem 1.2. Let f(z)Jϕμ(u,v,w), 0μ1 and π2<ϕ<π2. Then

    |b3σb22|{2(w)2(u)2(v)2(μ2+2cosϕ)eiϕσ(2(w)1cosϕ(u)1(v)1)2,(σ0),2(w)2(u)2(v)2(μ2+2cosϕ),(0σA1),2(w)2(u)2(v)2(μ22cosϕ)+eiϕσ(2(w)1cosϕ(u)1(v)1)2,(σA1),

    where

    A1=2(w)2eiϕ(u)2(v)2cosϕ((u)1(v)1(w)1)2

    for any real number σ.

    Proof. By applying (1.16) and (1.17), we have

    |b3σb22|=|2r2cosϕeiϕ(w)2(u)2(v)2+2μ2e2iϕ(w)2(u)2(v)2σr21cos2ϕe2iϕ(w)21(u)21(v)21|2μ2(w)2(u)2(v)2+2(w)2cosϕ(u)2(v)2|r2r21σ(w)21(u)2(v)2cosϕeiϕ2(u)21(v)21(w)2|2μ2(w)2(u)2(v)2+2(w)2cosϕ(u)2(v)2|r2υr212|,

    where

    υ=σ(w)21(u)2(v)2cosϕeiϕ(u)21(v)21(w)2. (1.21)

    By Lemma 1.2 and for υ0, we get

    |b3σb22|2(w)2(u)2(v)2(μ2+2cosϕ)eiϕσ(2(w)1cosϕ(u)1(v)1)2 (1.22)

    and, for υ0 in (1.21), we have

    σ(w)21(u)2(v)2cosϕeiϕ(u)21(v)21(w)20. (1.23)

    Also, by applying Lemma 1.2, and for 0υ2, we obtain

    |b3σb22|2(w)2(u)2(v)2(μ2+2cosϕ) (1.24)

    and for 0υ2 in (1.21), we get

    0σ2(w)2eiϕ(u)2(v)2cosϕ((u)1(v)1(w)1)2. (1.25)

    Next, for υ2 in Lemma 1.2, we have

    |b3σb22|2μ2(w)2(u)2(v)2+2(w)2cosϕ(u)2(v)2[2(σ(w)21(u)2(v)2cosϕeiϕ(u)21(v)21(w)21)], (1.26)

    which gives

    |b3σb22|2(w)2(u)2(v)2(μ22cosϕ)+eiϕσ(2(w)1cosϕ(u)1(v)1)2 (1.27)

    and, for υ2 in (1.21), we get

    σ2(w)2eiϕ(u)2(v)2cosϕ((u)1(v)1(w)1)2.

    This completes the proof of Theorem 1.2.

    Theorem 1.3. Let f(z)Jϕμ(u,v,w), 0μ1 and π2<ϕ<π2. Then

    H2(1)=|b3b22|2(w)2(u)2(v)2(μ2+2cosϕ). (1.28)

    Proof. By applying (1.16) and (1.17), we have

    |b3b22|=|2r2cosϕeiϕ(w)2(u)2(v)2+2μ2e2iϕ(w)2(u)2(v)2r21cos2ϕe2iϕ(w)21(u)21(v)21|2μ2(w)2(u)2(v)2+2(w)2cosϕ(u)2(v)2|r1(w)21(u)2(v)2cosϕeiϕ(u)21(v)21(w)2r212|.

    Thus, by applying Lemma 1.2, we find that

    |b3b22|2(w)2(u)2(v)2(μ2+2cosϕ).

    Theorem 1.4. Let f(z)Jϕμ(u,v,w), 0μ1 and π2<ϕ<π2. Then

    H2(2)=|b2b4b23|(2(w)2(u)2(v)2)2(μ4+4μ2cosϕ+4cos2ϕ)+3cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3(μ4+6μ2+9). (1.29)

    Proof. From the equations (1.16) to (1.18), we have

    |b2b4b23||6r1r2(w)1(w)3cos2ϕe2iϕ(u)1(v)1(u)3(v)3+6r21(w)1(w)3cos2ϕe4iϕμ2(u)1(v)1(u)3(v)34r22e2iϕcos2ϕ(w)22(u)22(v)228r2μ2e3iϕcosϕ(w)22(u)22(v)224μ4e4iϕ(w)22(u)22(v)22|.

    Applying Lemma 1.3, and after some simplification, we find that

    X|b2b4b23|=|3r41e2iϕcos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r21(4r21)e2iϕxcos2ϕ(w)1(w)3(u)1(v)1(u)3(v)33r21(4r21)e2iϕx2cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r1(4r21)(1|x|2)e2iϕcos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+6r21μ2e4iϕcos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3r41e2iϕcos2ϕ(w)22(u)22(v)222r21xe2iϕcos2ϕ(4r21)(w)22(u)22(v)22x2e2iϕcos2ϕ(4r21)2(w)22(u)22(v)224r21μ2e3iϕcosϕ(w)22(u)22(v)224μ2x(4r21)e3iϕcosϕ(w)22(u)22(v)224μ4e4iϕ(w)22(u)22(v)22|.

    Let r1=r and recall that |r1|2. We may assume without restriction that r[0,2]. Then, by using the triangle inequality, we get

    |b2b4b23|3r4cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r2(4r21)|x|cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+3r2(4r2)|x|2cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r(4r2)(1|x|2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+6r2μ2cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+r4cos2ϕ(w)22(u)22(v)22+2r2|x|cos2ϕ(4r2)(w)22(u)22(v)22+|x|2cos2ϕ(4r2)2(w)22(u)22(v)22+4r2μ2cosϕ(w)22(u)22(v)22+4μ2|x|(4r2)cosϕ(w)22(u)22(v)22+4μ4(w)22(u)22(v)22.

    Now, putting λ=|x|1, we have

    |b2b4b23|3r4cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r2(4r21)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3λ+3r2(4r2)cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3λ2+3r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)33r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3λ2+6r2μ2cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+r4cos2ϕ(w)22(u)22(v)22+2r2cos2ϕ(4r2)(w)22(u)22(v)22λ+(4r2)2cos2ϕ(w)22(u)22(v)22λ2+4r2μ2cosϕ(w)22(u)22(v)22+4μ2(4r2)cosϕ(w)22(u)22(v)22λ+4μ4(w)22(1)22(u)22(v)22,

    which implies that

    |b2b4b23|{3r4cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+6r2μ2cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+r4cos2ϕ(w)22(u)22(v)22+4r2μ2cosϕ(w)22(u)22(v)22+4μ4(w)22(u)22(v)22}+{3r2(4r21)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+2r2(4r2)cos2ϕ(w)22(u)22(v)22+4μ2(4r2)cosϕ(w)22(u)22(v)22}λ+{3r2(4r2)cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)33r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+(4r2)2cos2ϕ(w)22(u)22(v)22}λ2=G1(r,λ).

    Now, maximizing the function G1(r,λ) in the closed interval 0λ1, we obtain

    G1(λ,r)λ={3r2(4r21)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+2r2(4r2)cos2ϕ(w)22(u)22(v)22+4μ2(4r2)cosϕ(w)22(u)22(v)22}+2{3r2(4r2)cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)33r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+(4r2)2cos2ϕ(w)22(u)22(v)22}λ>0

    for 0r1. Thus, clearly, G1(λ,r) is an increasing function. Hence, it has the maximum point at λ=1 and we have

    max0λ1G1(λ,r)=G1(1,r)3r4cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+6r2μ2cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+r4cos2ϕ(w)22(u)22(v)22+4r2μ2cosϕ(w)22(u)22(v)22+4μ4(w)22(u)22(v)22+3r2(4r21)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+2r2(4r2)cos2ϕ(w)22(u)22(v)22+4μ2(4r2)cosϕ(w)22(u)22(v)22+3r2(4r2)cos2ϕ(w)1(w)32(u)1(v)1(u)3(v)3+3r(4r2)cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3+(4r2)2cos2ϕ(w)22(u)22(v)22=G(r). (1.30)

    After simplifying and differentiating with respect to r, we have

    G(r)=[μ2+3]12cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3r12cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3r3.

    By equating G(r) to zero and doing some simple calculations, we have the critical points at

    r0=0,r1=μ2+3andr2=μ2+3.

    The maximum point occurs at r1=μ2+3, so by using (1.30), we get

    G(r)=4(w)22(u)22(v)22{μ4+4μ2cosϕ+4cos2ϕ}+6cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3{μ4+6μ2+9}3cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3{μ4+6μ2+9}.

    Hence, we have

    |b2b4b23|(2(w)2(u)2(v)2)2{μ4+4μ2cosϕ+4cos2ϕ}+3cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3{μ4+6μ2+9}.

    Theorem 1.5. Let f(z)Jϕμ(u,v,w), 0μ1 and π2<ϕ<π2. Then

    |b2b3b4|3cosϕ(w)3(u)3(v)3×[(2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2)32]+2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2×(2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2(μ2+2cosϕ))+(6cosϕ(w)3(u)3(v)3(μ3+3))×2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2. (1.31)

    Proof. Applying the equations (1.16) to (1.18), we have

    |b2b3b4||2r1r2e2iϕcos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+2r1μ2e3iϕcosϕ(w)1(w)2(u)1(v)1(u)2(v)26r3eiϕcosϕ(r)3(u)3(v)36μ2r1e3iϕcosϕ(r)3(u)3(v)3|.

    Applying Lemma 1.3, we obtain

    |b2b3b4|=|r31e2iϕcos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+r1(4r21)e2iϕxcos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+2r1μ2e3iϕcosϕ(w)1(w)2(u)1(v)1(u)2(v)23r31eiϕcosϕ(w)32(u)3(v)33r1(4r21)eiϕxcosϕ(w)3(u)3(v)3+3r1(4r21)eiϕx2cosϕ(w)32(u)3(v)33(4r21)(1|x|2)eiϕcosϕz(w)3(u)3(v)36r1μ2e3iϕcosϕ(w)3(u)3(v)3|.

    Let r1=r, assuming that |r|=|r1|2, so that without restriction, r[0,2], and by applying triangle inequality with |x|=λ1 and |z|1, we find that

    |b2b3b4|{r3cos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+2rμ2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2+3r3cosϕ(w)32(u)3(v)3+3(4r2)cosϕ(w)3(u)3(v)3+6rμ2cosϕ(w)3(u)3(v)3}+{r(4r2)cos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+3r(4r2)cosϕ(w)3(u)3(v)3}λ+{3r(4r2)cosϕ(w)32(u)3(v)33(4r2)cosϕ(w)3(u)3(v)3}λ2=G2(λ,r). (1.32)

    By differentiating with respect to λ, we have

    G2(λ,r)λ={r(4r2)cos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+3r(4r2)cosϕ(w)3(u)3(v)3}+{3r(4r2)cosϕ(w)3(u)3(v)36(4r2)cosϕ(w)3(u)3(v)3}λ>0

    for 0λ1. Since G2(λ,r)>0 for 0λ1, it means that G2(λ,r) is an increasing function with its maximum point at λ=1. Hence, from (1.32), we have

    max0λ1G2(λ,r)=G2(1,r){r3cos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+2rμ2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2}+{3r3cosϕ(w)32(u)3(v)3+3(4r2)cosϕ(w)3(u)3(v)3+6rμ2cosϕ(w)3(u)3(v)3}+{r(4r2)cos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+3r(4r2)cosϕ(w)3(u)3(v)3}+{3r(4r2)cosϕ(w)32(u)3(v)33(4r2)cosϕ(w)3(u)3(v)3}=G(r). (1.33)

    After some simple calculations and simplification, we get

    G(r)=2rμ2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2+6rμ2cosϕ(w)3(u)3(v)3+4rcos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+12rcosϕ(w)3(u)3(v)33r3cosϕ(w)3(u)3(v)3+12cosϕ(w)3(u)3(v)3. (1.34)

    By differentiating G(r) with with respect to r and equating it to zero, the critical point will be seen to occur at

    2μ2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2+4cos2ϕ(w)1(w)2(u)1(v)1(u)2(v)2+18cosϕ(w)3(u)3(v)3+6μ2cosϕ(w)3(u)3(v)3=9cosϕ(w)3(u)3(v)3r2.

    Hence, we have

    r=2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2,
    r=2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2.

    Also, we have

    G(r)=18cosϕ(w)2(u)3(v)3r=18cosϕ(w)2(u)3(v)3×2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2.

    From (1.34), we get

    G(r)=3cosϕ(w)3(u)3(v)3×[(2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2)32]+2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2×(2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2(μ2+2cosϕ))+(6cosϕ(w)3(u)3(v)3(μ3+3))×2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2.

    Hence, we have

    |b2b3b4|3cosϕ(w)3(u)3(v)3×[(2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2)32]+2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2×(2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2(μ2+2cosϕ))+(6cosϕ(w)3(u)3(v)3(μ3+3))×2(w)1(w)2(u)3(v)3(μ2+2cosϕ)+6(w)3(u)1(v)1(u)2(v)2(3+μ2)9(w)3(u)1(v)1(u)2(v)2.

    Theorem 1.6. Let f(z)Jϕμ(u,v,w), 0μ1 and π2<ϕ<π2. Then

    H3(1)[2(w)2(u)2(v)2(2cosϕ+μ2)][(2(w)2(u)2(v)2)2{μ4+4μ2cosϕ+4cos2ϕ}+3cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3{μ4+6μ2+9}]+[12cosϕ(w)3(u)3(v)3(1+μ2)][3cosϕ(w)3(u)3(v)3(2A(μ2+2cosϕ)+2B(3+μ2)3B)32]+[12cosϕ(w)3(u)3(v)3(1+μ2)][2A(μ2+2cosϕ)+2B(3+μ2)3B2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2(μ2+2cosϕ)]+[12cosϕ(w)3(u)3(v)3(1+μ2)][2A(μ2+2cosϕ)+2B(3+μ2)3B6cosϕ(w)3(u)3(v)3(μ3+3)]+24(w)4(u)4(v)4(2cosϕ+2μ2cosϕ+μ4)[2(w)2(u)2(v)2(μ2+2cosϕ)], (1.35)

    where

    A=2(w)1(w)2(u)3(v)3andB=6(w)3(u)1(v)1(u)2(v)2.

    Proof. Taking it from (1.4), we have

    H3(1)=|b1b2b3b2b3b4b3b4b5|(b1=1) (1.36)
    =b3(b2b4b23)b4(b4b2b3)+b5(b3b22). (1.37)

    Applying Theorems 1.1 as well as 1.3 to 1.5, and by using the triangle inequality, we have

    H3(1)[2(w)2(u)2(v)2(2cosϕ+μ2)][(2(w)2(u)2(v)2)2{μ4+4μ2cosϕ+4cos2ϕ}+3cos2ϕ(w)1(w)3(u)1(v)1(u)3(v)3{μ4+6μ2+9}]+[12cosϕ(w)3(u)3(v)3(1+μ2)][3cosϕ(w)3(u)3(v)3(2A(μ2+2cosϕ)+2B(3+μ2)3B)32]+[12cosϕ(w)3(u)3(v)3(1+μ2)][2A(μ2+2cosϕ)+2B(3+μ2)3B2cosϕ(w)1(w)2(u)1(v)1(u)2(v)2(μ2+2cosϕ)]+[12cosϕ(w)3(u)3(v)3(1+μ2)][2A(μ2+2cosϕ)+2B(3+μ2)3B6cosϕ(w)3(u)3(v)3(μ3+3)]+24(w)4(u)4(v)4(2cosϕ+2μ2cosϕ+μ4)[2(w)2(u)2(v)2(μ2+2cosϕ)].

    Our present investigation was motivated by a number of recent developments on the Fekete-Szegö functional, the Hankel determinants of the third and the fourth kinds, and the associated Taylor-Maclaurin coefficient estimates and coefficient inequalities. Here, in this paper, we have introduced and systematically studied a new subclass of normalized analytic and univalent functions in the open unit disk U, which satisfies the following geometric criterion:

    (Lwu,vf(z)z(1e2iϕμ2z2)eiϕ)>0,

    where zU, 0μ1 and ϕ(π2,π2), and which is associated with the Hohlov operator Lwu,v. For functions in this class, we have investigated several coefficient bounds, as well as upper estimates for the Fekete-Szegö functional and the Hankel determinant.

    It should be remarked that, in many recent investigations dealing with some of the topics of our presentation in this paper, the basic or quantum (or q-) calculus was extensively used (see [39,60,67]).

    We conclude this paper by recalling a recently-published survey-cum-expository review article in which Srivastava [63] explored the mathematical applications of the q-calculus, the fractional q-calculus and the fractional q-derivative operators in geometric function theory of complex analysis, especially in the study of Fekete-Szegö functional. Srivastava [63] also exposed the not-yet-widely-understood fact that the so-called (p,q)-variation of the classical q-calculus is, in fact, a rather trivial and inconsequential variation of the classical q-calculus, the additional parameter p being redundant or superfluous (see, for details, [63,p. 340]; see also [64,pp. 1511-1512]).

    The authors declare that they have no conflicts of interest.



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