Research article Special Issues

Sharp coefficient problems of functions with bounded turning subordinated to the domain of cosine hyperbolic function

  • In the current article, we consider a class of bounded turning functions associated with the cosine hyperbolic function and give some results containing coefficient functionals using the familiar Carathéodory functions. An improvement on the bound of the third-order Hankel determinant for functions in this class is provided. Furthermore, we obtain sharp estimates of the Fekete-Szegö, Krushkal, and Zalcman functionals with logarithmic coefficients as entries. All the findings are proved to be sharp.

    Citation: Zhen Peng, Muhammad Arif, Muhammad Abbas, Nak Eun Cho, Reem K. Alhefthi. Sharp coefficient problems of functions with bounded turning subordinated to the domain of cosine hyperbolic function[J]. AIMS Mathematics, 2024, 9(6): 15761-15781. doi: 10.3934/math.2024761

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  • In the current article, we consider a class of bounded turning functions associated with the cosine hyperbolic function and give some results containing coefficient functionals using the familiar Carathéodory functions. An improvement on the bound of the third-order Hankel determinant for functions in this class is provided. Furthermore, we obtain sharp estimates of the Fekete-Szegö, Krushkal, and Zalcman functionals with logarithmic coefficients as entries. All the findings are proved to be sharp.



    Complex analysis is one of the major disciplines nowadays due to its numerous applications in mathematical science and other fields. Geometric function theory is an intriguing topic of complex analysis that involves the geometrical characteristics of analytic functions. This area is crucial to applied mathematics, particularly in fields such as engineering, electronics, nonlinear integrable system theory, fluid dynamics, modern mathematical physics, and partial differential equation theory. The key problem that led to the rapid emergence of geometric function theory is the Bieberbach conjecture. It is about the coefficient bounds for functions belonging to the class S of univalent functions. This conjecture states that if gS with the Taylor-Maclaurin series expansion of the form

    g(z)=z+k=2dkzk,zD, (1.1)

    where D:={zC:|z|<1}, then |dk|k for all k2. Let A be the class of analytic functions with the series representation given in (1.1). The set S is a subclass of A which was first taken into account by Koebe in 1907. The above famous conjecture was proposed by Bieberbach [1] in 1916. He proved this for k=2, and subsequent researchers, including L öwner [2], Garabedian and Schiffer [3], Pederson and Schiffer [4], and Pederson [5], confirmed it for k=3, 4, 5, and 6, respectively. However, settling the conjecture for k7 remained elusive until 1985 when de Branges [6] used hypergeometric functions to prove it for every k2. Lawrence Zalcman proposed the inequality |d2kd2k1|(k1)2 with k2 for gS in the late 1960's as a way of establishing the Bieberbach conjecture. Due to this, a number of articles [7,8,9] have been published on the Zalcman hypothesis and its generalized form |λd2kd2k1|λk22k+1 with λ0 for different subclasses of the class S. This conjecture has remained unsolved for a long time. Krushkal [10] established this hypothesis for k6. In an attempt to solve the Zalcman conjecture, Krushkal [11] investigated the inequality |dlkdl(k1)2|2l(k1)kl with k,l2 for gS. A broader Zalcman hypothesis for gS was proposed by Ma [12] later, in 1999, and is given by

    |djdkdj+k1|(j1)(k1),j,k2.

    He only proved it for a subclass of S. The challenge is still open for the class S.

    Now, we recall the definition of subordination, which actually provides a relationship between analytic functions. We write g1g2 to illustrate that g1 is subordinate to g2. It is explained that for two given functions g1,g2A, a Schwarz function w exists such that g1(z)=g2(w(z)) for zD. Once g2 is univalent in D, then this relation is equivalent to saying that

    g1(z)g2(z),zD

    if and only if

    g1(0)=g2(0)  and  g1(D)g2(D).

    The three classic subclasses of univalent functions are C, S and K, of which their functions are known respectively as convex functions, starlike functions and close-to-convex functions. These classes are defined by

    C:={gS:(zg(z))g(z)1+z1z,zD},
    S:={gS:zg(z)g(z)1+z1z,zD},

    and

    K:={gS:zg(z)h(z)1+z1z,zD}

    for some hS. Taking h(z)=z, the class K reduces to the class BT of bounded turning functions. Further, replacing 1+z1z by some other special functions, various interesting subfamilies of the class S were studied; interested readers may refer to [13,14,15,16,17,18].

    The determinant Dλ,n(g), where n,λN={1,2,}, is known as the Hankel determinant and was presented by Pommerenke [19,20]. It is formed by the coefficients of the function gS and is defined by

    Dλ,n(g):=|dndn+1dn+λ1dn+1dn+2dn+λdn+λ1dn+λdn+2λ2|.

    Hankel matrices are used in both pure mathematics and technological applications, including the theory of Markov processes, the theory of non-stationary signals in the Hamburger moment problem, and many other topics, see for example [21,22,23,24]. There are relatively few publications on the bounds of the Hankel determinant for functions in the general class S. The best estimate for gS was determined by Hayman in [25], which asserted that |D2,n(g)||η|, where η is a constant. Additionally, for gS, it was shown in [26] that the second-order Hankel determinant |D2,2(g)|η for 0η11/3. The two determinants D2,1(g) and D2,2(g) have been extensively studied in the literature for various subfamilies of univalent functions. The works [27,28,29,30,31], in which the sharp bounds of the second-order Hankel determinant for some subclasses of S are determined, are particularly noteworthy.

    In comparison to the second-order Hankel determinant, the sharp bound of the third-order Hankel determinant D3,1(g) for certain analytic univalent functions is much harder to find. The investigation on D3,1(g) for S was initiated by Babalola [32] in 2010. The exact bounds of this determinant were proved recently for the classes C, S, and BT in [33], [34], and [35], respectively. These bounds are given by

    |D3,1(g)|{4135,forgC,49,forgS,14,forgBT.

    By employing similar techniques, Khalil Ullah et al. [36] and Lecko et al. [37] derived the sharp bounds for |D3,1(g)| when considering functions belonging to the families Stanh and S(1/2), respectively. Additionally, the works [38,39,40,41,42,43] proved the sharp bounds for the same third-order Hankel determinant in various novel subfamilies of analytic univalent functions.

    Let us consider the two function classes defined respectively by

    Scosh:={gS:zg(z)g(z)coshz (zD)}

    and

    BTcosh:={gS:g(z)coshz (zD)}.

    These classes were introduced and studied by Mundalia et al. [44] and Ghaffar et al. [45], respectively. In this paper, we improved the bound of the third-order Hankel determinant |D3,1(g)|, which was determined by Ghaffar et al. and published recently in AIMS Mathematics [45]. Furthermore, we obtain the sharp estimates of the Fekete-Szegö, Krushkal, and Zalcman functionals with logarithmic coefficients as entries.

    In the theory of univalent functions, the Carathéodory functions are well studied. They are analytic in D with positive real part and take series representations of the form

    p(z)=1+n=1τnzn (zD). (2.1)

    We denote by P the set of these functions.

    To prove the main theorems, we need the following lemmas.

    Lemma 2.1 [46] Let pP be the form of (2.1) with τ10. Then

    2τ2=τ21+β(4τ21), (2.2)
    4τ3=τ31+2(4τ21)τ1βτ1(4τ21)β2+2(4τ21)(1|β|2)η, (2.3)
    8τ4=τ41+(4τ21)β[τ21(β23β+3)+4β]4(4τ21)(1|β|2)[τ1(β1)η+¯βη2(1|η|2)κ] (2.4)

    for some β,η,κ¯D:={zC:|z|1}.

    Lemma 2.2 [47] If pP is of the form (2.1) and ϑC, we have

    |τnϑτkτnk|2max{1,|2ϑ1|} (2.5)

    for all 1kn1.

    Lemma 2.3 [48] Let μ, λ, ζ, and ς satisfy λ(0,1), ζ(0,1) and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ). (2.6)

    If pP is of the form (2.1), then

    |μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|2.

    Lemma 2.4 [49] Suppose that pP is provided by (2.1). If R[0,1] and R(2R1)SR, then we have

    |τ32Rτ1τ2+Sτ31|2. (2.7)

    Theorem 3.1 If gBTcosh is of the form (1.1), then

    |d5d2d4|110.

    This inequality is sharp.

    Proof. Let gBTcosh. Then g can be easily expressed by using the Schwarz function as

    g(z)=coshw(z), zD.

    If pP, then we can write it in the form of

    p(z)=1+w(z)1w(z)=1+τ1z+τ2z2+τ3z3+.

    It follows that

    w(z)=12τ1z+14(2τ2τ21)z2+18(τ314τ1τ2+4τ3)z3+116(τ41+6τ21τ28τ1τ34τ22+8τ4)z4+. (3.1)

    From (1.1), we have

    g(z)=1+2d2z+3d3z2+4d4z3+5d5z4+. (3.2)

    Using the series expansion of (3.1) with simple calculation, we get

    coshw(z)=1+14τ1z+(14τ21196τ21)z2+(3015760τ311148τ1τ2+14τ3)z3+(14τ41196τ22+3011920τ21τ215287645120τ411148τ1τ3)z4+. (3.3)

    Comparing the coefficients in (3.2) and (3.3), we obtain

    d2=18τ1, (3.4)
    d3=112τ211288τ21, (3.5)
    d4=30123040τ31+116τ311192τ1τ2, (3.6)
    d5=11480τ22152873225600τ41+120τ4+3019600τ21τ211240τ1τ3. (3.7)

    Employing (3.4), (3.6) and (3.7), we may write

    |d5d2d4|=120|13703107520τ41+1124τ22+2(103192)τ1τ332(493960)τ21τ2τ4|.=120|μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|, (3.8)

    where

    μ=13703107520,     λ=1124,     ζ=103192,     ς=493960.

    These constants satisfy λ(0,1), ζ(0,1), and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ).

    Hence, by Lemma 2.3 and (3.8), we deduce that

    |d5d2d4|110.

    This required result is sharp and determined by

    g4(z)=z0(cosht4)dt=z+110z5+1216z9+, (3.9)

    where we choose the branch of the square root function so that

    coshz4=1+12!z4+14!z8+16!z12+ (3.10)

    Theorem 3.2 If gBTcosh is of the form of (1.1), then

    |d5d23|110.

    This inequality is sharp.

    Proof. From (3.5) and (3.7), we obtain

    |d5d23|=120|1799331451520τ41+4372τ22+2(1124)τ1τ332(32596480)τ21τ2τ4|=120|μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|, (3.11)

    where

    μ=1799331451520,  λ=4372,  ζ=1124,  ς=32596480.

    These constants satisfy λ(0,1), ζ(0,1), and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ).

    Hence, by Lemma 2.3 and (3.11), we deduce that

    |d5d23|110.

    This required outcome is sharp for the function g4 given in (3.9).

    Theorem 3.3 If gBTcosh is of the form of (1.1), then

    |d4d32|18.

    This inequality is sharp.

    Proof. Using (3.4) and (3.6), we have

    |d4d32|=116|τ32(1124)τ1τ2+(845)τ31|.

    Let R=1124 and S=845. It is clear that

    R(2R1)=11288SR.

    All the conditions of Lemma 2.4 are satisfied, and thus we have

    |d4d32|18.

    This result is the best possible and equality is attained by

    g3(z)=z0(cosht3)dt=z+18z4+1168z7+, (3.12)

    where we choose the branch of the square root function so that

    coshz3=1+12!z3+14!z6+16!z9+ (3.13)

    Theorem 3.4 If gBTcosh is of the form of (1.1), then

    |d5d42|110.

    This inequality is sharp.

    Proof. From (3.4) and (3.7), we obtain

    |d5d42|=120|32149322560τ41+1124τ22+2(1124)τ1τ332(301720)τ21τ2τ4|=120|μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|, (3.14)

    where

    μ=32149322560, λ=1124,  ζ=1124, ς=301720.

    These constants satisfy λ(0,1), ζ(0,1), and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ).

    Hence, by Lemma 2.3 and (3.14), we deduce that

    |d5d42|110.

    This required inequality is sharp for the function g4 given in (3.9).

    Theorem 3.5 If gBTcosh has the form of (1.1), then

    |D3,1(g)|164.

    This inequality is sharp.

    Proof. From the definition, we know

    D3,1(g)=2d2d3d4d33d24+d3d5d22d5. (3.15)

    Let gBTcosh and gθ(z)=eiθg(eiθz) with θR. It is noted that gθ(z)=g(eiθz) and thus gθBTcosh for all θR. Since |D3,1(gθ)|=|D3,1(g)|, we may choose the coefficient d2 of g to be a non-negative real number when estimating the functional |D3,1(g)|. Then, since d2=18τ1 and τ1 is a coefficient of a function in P, it follows that τ1 is real and τ1=τ[0,2]. Putting the estimations of di's from (3.4), (3.5), (3.6), and (3.7) into D3,1(g) with τ1=τ, we have

    D3,1(g)=133443020800(513823τ64378896τ4τ2+7922880τ3τ3+5552064τ2τ2289994240τ2τ4+155312640ττ2τ383220480τ32+139345920τ2τ4130636800τ23).

    Let r=4τ2. Then, by (2.2), (2.3), and (2.4), we obtain

    D3,1(g)=133443020800{329τ610402560β3r3+34836480β3r2+10160640τ3rβ(1|β|2)η+10160640τ2r¯β(1|β|2)η210160640τ2r(1|β|2)(1|η|2)κ+8346240τr2β(1|β|2)η2177280τr2β2(1|β|2)η34836480r2¯ββη2(1|β|2)+34836480r2β(1|β|2)(1|η|2)κ+2476656τ2r2β210160640τ2rβ22540160τ4rβ312882240τ2r2β3+544320τ2r2β432659200r2η2(1|β|2)2+2555280τ4rβ2+12024τ4rβ30240τ3r(1|β|2)η}.

    It is seen that we can write D3,1(g) in the form of

    D3,1(g)=133443020800[l1(τ,β)+l2(τ,β)η+l3(τ,β)η2+l4(τ,β,η)κ],

    where β,η,κ¯D, and

    l1(τ,β)=329τ6+(4τ2)[(4τ2)(6773760β32479680τ2β3+2476656τ2β2+544320τ2β4)+2555280τ4β2+12024τ4β10160640τ2β22540160τ4β3],l2(τ,β)=30240(4τ2)(1|β|2)[(4τ2)(72τβ2+276τβ)+336τ3βτ3],l3(τ,β)=725760(4τ2)(1|β|2)[(4τ2)(3|β|245)+14τ2¯β],l4(τ,β,η)=725760(4τ2)(1|β|2)(1|η|2)[48β(4τ2)14τ2].

    By using |β|=ϰ,|η|=y and utilizing the fact |κ|1, we obtain

    |D3,1(g)|133443020800[|l1(τ,β)|+|l2(τ,β)|y+|l3(τ,β)|y2+|l4(τ,β,η)|].133443020800M(τ,ϰ,y), (3.16)

    where

    M(τ,ϰ,y)=m1(τ,ϰ)+m2(τ,ϰ)y+m3(τ,ϰ)y2+m4(τ,ϰ)(1y2),

    with

    m1(τ,ϰ)=329τ6+(4τ2)[(4τ2)(6773760ϰ3+2479680τ2ϰ3+2476656τ2ϰ2+544320τ2ϰ4)+2555280τ4ϰ2+12024τ4ϰ+10160640τ2ϰ2+2540160τ4ϰ3],m2(τ,ϰ)=30240(4τ2)(1ϰ2)[(4τ2)(72τϰ2+276τϰ)+336τ3ϰ+τ3],m3(τ,ϰ)=725760(4τ2)(1ϰ2)[(4τ2)(3ϰ2+45)+14τ2ϰ],m4(τ,ϰ)=725760(4τ2)(1ϰ2)[48ϰ(4τ2)+14τ2].

    Now, we have to maximize M in the closed cuboid Υ:=[0,2]×[0,1]×[0,1].

    In light of (τ,ϰ)[0,2]×[0,1], we observe that

    m3(τ,ϰ)725760(4τ2)(1ϰ2)[(4τ2)(3ϰ2+45)+14τ2]=:g3(τ,ϰ). (3.17)

    Taking gi(τ,ϰ)=mi(τ,ϰ) for i=1,2,4 and

    G(τ,ϰ,y)=g1(τ,ϰ)+g2(τ,ϰ)y+g3(τ,ϰ)y2+g4(τ,ϰ)(1y2), (3.18)

    it is not hard to see that M(τ,ϰ,y)G(τ,ϰ,y) in the cuboid Υ. In the following, we aim to find the maximum value of G in Υ.

    By partially differentiating G with respect to y, we have

    Gy=g2(τ,ϰ)+2[g3(τ,ϰ)g4(τ,ϰ)]y. (3.19)

    In view of g2(τ,ϰ)0 and

    g3(τ,ϰ)g4(τ,ϰ)=725760(4τ2)(1ϰ2)[(3ϰ248ϰ+45)(4τ2)]0 (3.20)

    on [0,2]×[0,1], we have Gy0 for all y[0,1]. It follows that

    G(τ,ϰ,y)G(τ,ϰ,1), (3.21)

    where

    G(τ,ϰ,1)=g1(τ,ϰ)+g2(τ,ϰ)+g3(τ,ϰ)=329τ6+72(4τ2)[q4(τ)ϰ4+q3(τ)ϰ3+q2(τ)ϰ2+q1(τ)ϰ+q0(τ)]=:Q(τ,ϰ),

    where

    q4(τ)=7560(4τ2)(τ24τ4),q3(τ)=840(τ430τ3+52τ2552τ+448),q2(τ)=84(13τ4365τ3+6678τ2+1440τ20160),q1(τ)=τ(167τ3+25200τ2+463680),q0(τ)=420(τ3744τ2+4320).

    Then the problem reduces to finding the maximum value of Q on [0,2]×[0,1]. By noting that q4(τ)0 for all τ[0,2], we obtain that

    Q(τ,ϰ)329τ6+72(4τ2)[q3(τ)ϰ3+q2(τ)ϰ2+q1(τ)ϰ+q0(τ)]=:W(τ,ϰ). (3.22)

    Setting τ=0, we obtain

    W(0,ϰ)=108380160ϰ3487710720ϰ2+522547200=108380160ϰ2(ϰ92)+5225472005225472005.2255×108

    for all ϰ[0,1]. Setting τ=2, we get

    W(2,ϰ)21056,ϰ[0,1].

    It is left to consider the case of τ(0,2). For the system of equations

    Wτ=0         and        Wϰ=0

    with (τ,ϰ)(0,2)×(0,1), a numerical computation indicates that all the real approximate solutions are listed as (1.6125,1.0547), (158.7578,0.6573), (2.0982,0.4927), (2.1274,0.3361), (1.0709,0.9834), (0,0), and (2,2.1500). Thus, the only critical point of W that lies in (0,2)×(0,1) is about (1.0709,0.9834). For this point, we have W(1.0709,0.9834)1.9621×108.

    Thus, from above cases, we conclude that

    M(τ,ϰ,y)G(τ,ϰ,y)G(τ,ϰ,1)Q(τ,ϰ)W(τ,ϰ)522547200

    on [0,2]×[0,1]×[0,1]. From (3.16) we get that

    |D3,1(g)|133443020800[M(τ,ϰ,y)]52254720033443020800=164.

    If gBTcosh, then the sharp bound for this Hankel determinant is determined by

    |D3,1(g)|=1640.01562,

    with an extremal function g3 given in (3.12).

    The logarithmic coefficients ξk of gS are given by

    Gg(z):=log(g(z)z)=2k=1ξkzk,zD.

    These coefficients contribute significantly in many estimations to the theory of univalent functions. In 1985, de Branges [6] completed the proof of the Milin conjecture [50], which asserted that for all positive integers k1,

    kl=1l(kl+1)|ξk|2kl=1kl+1l,

    and equality holds if and only if g takes the form z/(1eiφz)2 for some φR. This inequality leads to the famous Bieberbach–Robertson–Milin conjectures. In 2005, Kayumov [51] was able to solve the Brennans conjecture for conformal mappings by considering the logarithmic coefficients. For some recent works on the study of logarithmic coefficients, see, for example, [52,53,54,55,56].

    If gS is in the form of (1.1), then its logarithmic coefficients are given by

    ξ1=12d2, (4.1)
    ξ2=12(d312d22), (4.2)
    ξ3=12(d4d2d3+13d32), (4.3)
    ξ4=12(d5d2d4+d22d312d2314d42). (4.4)

    Plugging (3.4), (3.5), (3.6), and (3.7) into (4.1), (4.2), (4.3), and (4.4), we get

    ξ1=116τ1, (4.5)
    ξ2=124τ2532304τ21, (4.6)
    ξ3=717680τ31+132τ313384τ1τ2, (4.7)
    ξ4=191440τ221802099464486400τ41+140τ4+14861691200τ21τ21033840τ1τ3. (4.8)

    Define

    D2,1(Gg/2):=ξ1ξ3ξ22, (4.9)
    D2,2(Gg/2):=ξ2ξ4ξ23. (4.10)

    It is observed that D2,1(Gg/2) resembles the well-known functional D2,1(g)=d1d3d22 over the class S or its subclasses.

    Theorem 4.1 If gBTcosh is of the form (1.1), then

    |ξ2ϑξ21|max{112,|9ϑ+5|576},ϑC.

    This inequality is sharp.

    Proof. By employing (4.5) and (4.6), we may write

    |ξ2ϑξ21|=124|τ29ϑ+5396τ21|.

    An application of Lemma 2.2 leads to

    |ξ2ϑξ21|max{112,|9ϑ+5|576}.

    The bound 112 is achieved by the function g2 given as

    g2(z)=z0(cosht2)dt=z+16z3+1120z5+. (4.11)

    The bound |9ϑ+5|576 for ϑC is attained by the function g1 given as

    g1(z)=z0(cosht)dt=z+14z2+172z3+. (4.12)

    Here, we choose the branch of the square root function so that

    coshz2=1+12!z2+14!z4+16!z6+ (4.13)

    and

    coshz=1+12!z+14!z2+16!z3+. (4.14)

    Substituting ϑ=1, we deduce the corollary stated below.

    Corollary 4.1 If the function gBTcosh has the form of (1.1), then

    |ξ2ξ21|112.

    This bound is achieved by the function g2 given in (4.11).

    Theorem 4.2 If gBTcosh has the form of (1.1), then

    |ξ1ξ2ξ3|116.

    This inequality is sharp.

    Proof. Using (4.5), (4.6), and (4.7), we have

    |ξ1ξ2ξ3|=132|τ32(712)τ1τ2+19695760τ31|.

    Let R=712 and S=19695760. It is clear that

    R(2R1)=772SR.

    By Lemma 2.4, we obtain

    |ξ1ξ2ξ3|116.

    The equality is attained by the function g3 given in (3.12).

    Theorem 4.3 Let gBTcosh have the series expansion (1.1). Then

    |ξ4ξ1ξ3|120.

    The inequality is sharp.

    Proof. From (4.5), (4.7), and (4.8), we have

    |ξ4ξ1ξ3|=140|207047911612160τ41+1936τ22+2(221384)τ1τ332(3264751840)τ21τ2τ4|=140|μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|, (4.15)

    where

    μ=207047911612160,     λ=1936,     ζ=221384,     ς=3264751840.

    These constants satisfy λ(0,1), ζ(0,1), and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ).

    Hence, by Lemma 2.3 and (4.15), we deduce that

    |ξ4ξ1ξ3|120.

    This equality is achieved by the function g4 given in (3.9).

    Theorem 4.4 Let gBTcosh be in the form of (1.1). Then

    |ξ4ξ22|120.

    This inequality is sharp.

    Proof. From (4.6) and (4.8), we obtain

    |ξ4ξ22|=140|409577323224320τ41+4372τ22+2(103192)τ1τ332(809312960)τ21τ2τ4|.=140|μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|, (4.16)

    where

    μ=409577323224320,     λ=4372,     ζ=103192,     ς=809312960.

    These constants satisfy λ(0,1), ζ(0,1), and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ).

    Hence, by Lemma 2.3 and (4.16), we deduce that

    |ξ4ξ22|120.

    The required inequality is sharp and determined by the function g4 given in (3.9).

    Theorem 4.5 If gBTcosh has the form of (1.1), then

    |ξ3ξ31|116.

    This inequality is sharp.

    Proof. Using (4.5) and (4.7), we have

    |ξ3ξ31|=132|τ32(1324)τ1τ2+5531920τ31|.

    Let R=1324 and S=5531920. It is clear that

    R(2R1)=13288SR.

    By Lemma 2.4, it follows that

    |ξ3ξ31|116.

    This result is the best possible and the extremal function is g3 as given in (3.12).

    Theorem 4.6 If gBTcosh is of the form (1.1), then

    |ξ4ξ41|120.

    This inequality is sharp.

    Proof. From (4.5) and (4.8), we obtain

    |ξ4ξ41|=140|361837323224320τ41+1936τ22+2(103192)τ1τ332(1486125920)τ21τ2τ4|.=140|μτ41+λτ22+2ζτ1τ332ςτ21τ2τ4|, (4.17)

    where

    μ=361837323224320,     λ=1936,     ζ=103192,     ς=1486125920.

    These constants satisfy λ(0,1), ζ(0,1), and

    8λ(1λ)[(ζς2μ)2+(ζ(λ+ζ)ς)2]+ζ(1ζ)(ς2λζ)24λζ2(1ζ)2(1λ).

    Hence, by Lemma 2.3 and (4.17), we deduce that

    |ξ4ξ41|120.

    This required inequality is sharp and determined by using (4.1), (4.4) and (3.9).

    Theorem 4.7 If gBTcosh has the form of (1.1), then

    |D2,2(Gg/2)|1256.

    This inequality is sharp.

    Proof. Suppose that gBTcosh and gθ(z)=eiθg(eiθz) with θR. Since |D2,2(Ggθ/2)|=|D2,2(Gg/2)| for all θR, we still assume that τ1=τ[0,2]. Putting (4.6), (4.7), and (4.8) into (4.10) with τ1=τ, we obtain

    D2,2(Gg/2)=11070176665600(4047343τ632414400τ4τ2+41973120τ3τ3+56996352τ2τ22615444480τ2τ4+1068318720ττ2τ3588349440τ32+1114767360τ2τ41045094400τ23).

    Let r=4τ2. Then, by (2.2), (2.3), and (2.4), we obtain

    D2,2(Gg/2)=11070176665600{2237760τ3r(1|β|2)η73543680β3r3+278691840β3r2+29030400τ3rβ(1|β|2)η+29030400τ2r¯βη2(1|β|2)29030400τ2r(1|β|2)(1|η|2)κ+23224320τβr2η(1|β|2)17418240τβ2r2(1|β|2)η278691840βr2(1|β|2)¯βη2+278691840βr2(1|β|2)(1|η|2)κ261273600r2(1|β|2)2κ2+8376480τ4rβ2107424τ4βr+8443008τ2β2r229030400rτ2β27257600τ4rβ381285120β3r2τ2+4354560β4r2τ2+2671τ6}.

    It is observed that we can write D2,2(Gg/2) in the form of

    D2,2(Gg/2)=11070176665600[k1(τ,β)+k2(τ,β)η+k3(τ,β)η2+k4(τ,β,η)κ],

    where β,η,κ¯D, and

    k1(τ,β)=2671τ6+(4τ2)[(4τ2)(8443008τ2β215482880β37741440τ2β3+4354560τ2β4)29030400τ2β2+8376480τ4β2107424τ4β7257600τ4β3],k2(τ,β)=60480(4τ2)(1|β|2)[(4τ2)(288τβ2+384τβ)+480τ3β37τ3],k3(τ,β)=5806080(4τ2)(1|β|2)[(4τ2)(3|β|245)+5τ2¯β],k4(τ,β,η)=5806080(4τ2)(1|β|2)(1|η|2)[5τ2+48β(4τ2)].

    Now, by using |β|=ϰ,|η|=y and utilizing the fact |κ|1, we get

    |D2,2(Gg/2)|11070176665600[|k1(τ,β)|+|k2(τ,β)|y+|k3(τ,β)|y2+|k4(τ,β,η)|].11070176665600Λ(τ,ϰ,y), (4.18)

    where

    Λ(τ,ϰ,y)=t1(τ,ϰ)+t2(τ,ϰ)y+t3(τ,ϰ)y2+t4(τ,ϰ)(1y2),

    with

    t1(τ,ϰ)=2671τ6+(4τ2)[(4τ2)(8443008τ2ϰ2+15482880ϰ3+7741440τ2ϰ3+4354560τ2ϰ4)+29030400τ2ϰ2+8376480τ4ϰ2+107424τ4ϰ+7257600τ4ϰ3],t2(τ,ϰ)=60480(4τ2)(1ϰ2)[(4τ2)(288τϰ2+384τϰ)+480τ3ϰ+37τ3],t3(τ,ϰ)=5806080(4τ2)(1ϰ2)[(4τ2)(3ϰ2+45)+5τ2ϰ],t4(τ,ϰ)=5806080(4τ2)(1ϰ2)[5τ2+48ϰ(4τ2)].

    Now, we have to maximize Λ in the closed cuboid Υ.

    In view of

    t3(τ,ϰ)5806080(4τ2)(1ϰ2)[(4τ2)(3ϰ2+45)+5τ2]=:u3(τ,ϰ) (4.19)

    for all (τ,ϰ)[0,2]×[0,1], by setting ui(τ,ϰ)=ti(τ,ϰ)(i=1,2,4) and

    Θ(τ,ϰ,y)=u1(τ,ϰ)+u2(τ,ϰ)y+u3(τ,ϰ)y2+u4(τ,ϰ)(1y2),

    it is not hard to see that Λ(τ,ϰ,y)Θ(τ,ϰ,y) on Υ. In the following, we aim to discuss the maximum value of Θ on Υ.

    By partially differentiating Θ with respect to y, we get

    Θy=u2(τ,ϰ)+2[u3(τ,ϰ)u4(τ,ϰ)]y.

    Because u2(τ,ϰ)0 and

    u3(τ,ϰ)u4(τ,ϰ)=5806080(4τ2)(1ϰ2)[(3ϰ248ϰ+45)(4τ2)]0

    on [0,2]×[0,1], we have Θy0 for all y[0,1]. Hence, we obtain

    Θ(τ,ϰ,y)Θ(τ,ϰ,1), (4.20)

    where

    Θ(τ,ϰ,1)=u1(τ,ϰ)+u2(τ,ϰ)+u3(τ,ϰ)=2671τ6+288(4τ2)[v4(τ)ϰ4+v3(τ)ϰ3+v2(τ)ϰ2+v1(τ)ϰ+v0(τ)]=:V(τ,ϰ),

    where

    v4(τ)=15120(4τ2)(τ24τ4), (4.21)
    v3(τ)=1680(τ4+12τ332τ2+192τ128), (4.22)
    v2(τ)=21(11τ4+3250τ345904τ211520τ+161280), (4.23)
    v1(τ)=τ(373τ3+20160τ2+322560), (4.24)
    v0(τ)=30(259τ326880τ2+120960). (4.25)

    Taking the fact of v4(τ)0 for all τ[0,2], we obtain

    V(τ,ϰ)2671τ6+288(4τ2)[v3(τ)ϰ3+v2(τ)ϰ2+v1(τ)ϰ+v0(τ)]=:K(τ,ϰ). (4.26)

    Now, we need to find the maximum value of K on [0,2]×[0,1]. For τ=0, we have

    K(0,ϰ)=247726080ϰ2(ϰ634)+41803776004180377600 (4.27)

    for all ϰ[0,1]. If τ=2, it is calculated that K(2,ϰ)170944 with ϰ[0,1]. Hence, it is left to discuss the case of (τ,ϰ)(0,2)×(0,1).

    For the system of equations

    Kτ=0          and         Kϰ=0

    with (τ,ϰ)(0,2)×(0,1), a numerical computation indicates that the approximate solutions are (0,0), (1.7758,1.2237), (2.0405,0.4933), (52.7638,0.2085), (212.4757,0.2665), (2.0293,0.3246), (1.5447,1.0839), (5.1393,2.5129), (2,2.1720), and (2,1.1906). It is found that there are no critical points of K that lie in (0,2)×(0,1).

    From the above cases we conclude that

    Λ(τ,ϰ,y)Θ(τ,ϰ,y)Θ(τ,ϰ,1)=V(τ,ϰ)K(τ,ϰ)4180377600

    on [0,2]×[0,1]×[0,1]. Using (4.18), we have

    |D2,2(Gg/2)|11070176665600Λ(τ,ϰ,y)41803776001070176665600=12560.003906.

    If gBTcosh, then the sharp bound for this second-order Hankel determinant is determined by using (4.2), (4.3), (4.4), and (3.12).

    The authors declare that they have not used Artificial Intelligence tools in the creation of this article.

    The authors would like to extend their sincere-appreciation to the Researchers Supporting Project number (RSPD2024R802) King Saud University, Riyadh, Saudi Arabia.

    Prof. Dr. Nak Eun Cho is the Guest Editor of special issue “Geometric Function Theory and Special Functions” for AIMS Mathematics. Prof. Dr. Nak Eun Cho was not involved in the editorial review and the decision to publish this article.

    The authors declare that they have no conflicts of interest.



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