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Research article Special Issues

Extended suprametric spaces and Stone-type theorem

  • Received: 28 March 2023 Revised: 01 July 2023 Accepted: 13 July 2023 Published: 20 July 2023
  • MSC : 47H10, 54E35, 54E99

  • Extended suprametric spaces are defined, and the contraction principle is established using elementary properties of the greatest lower bound instead of the usual iteration procedure. Thereafter, some topological results and the Stone-type theorem are derived in terms of suprametric spaces. Also, we have shown that every suprametric space is metrizable. Further, we prove the existence of a solution of Ito-Doob type stochastic integral equations using our main fixed point theorem in extended suprametric spaces.

    Citation: Sumati Kumari Panda, Ravi P Agarwal, Erdal Karapínar. Extended suprametric spaces and Stone-type theorem[J]. AIMS Mathematics, 2023, 8(10): 23183-23199. doi: 10.3934/math.20231179

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  • Extended suprametric spaces are defined, and the contraction principle is established using elementary properties of the greatest lower bound instead of the usual iteration procedure. Thereafter, some topological results and the Stone-type theorem are derived in terms of suprametric spaces. Also, we have shown that every suprametric space is metrizable. Further, we prove the existence of a solution of Ito-Doob type stochastic integral equations using our main fixed point theorem in extended suprametric spaces.



    Assume that A denotes the set of all analytic functions h(z) in the open symmetric unit disk

    U={z:|z|<1},

    which are normalized by

    h(0)=0andh(0)=1.

    Thus, every function hA can be expressed in the form given in (1.1)

    h(z)=z+k=2akzk. (1.1)

    Let an analytic function h is said to be univalent if it satisfy the following condition:

    h(z1)h(z2)z1z2,z1,z2U.

    Furthermore, S is the subclass of A whose members are univalent in U. The idea of subordination was initiated by Lindelof [30] and Little-wood and Rogosinski have further improved this idea, see [31,35,36]. For h, yA, and h subordinate to y in U, denoted by

    h(z)y(z),zU,

    if we have a function u, such that

    uB={u:uA,|u(z)|<1,andu(0)=0,zU}

    and

    h(z)=y(u(z)),zU.

    According to the Koebe one-quarter theorem (see [13]), the image of U under hS contains a disk of radius one-quarter centered at origin. Thus, every function hS has an inverse h1=g, defined as:

    g(h(z))=z,zU

    and

    h(g(w))=w,|w|<r0(h),r0(h)14.

    The power series for the inverse function g(w) is given by

    g(w)=wa2w2+(2a22a3)w3Q(a)w4+,, (1.2)

    Where

    Q(a)=(5a325a2a3+a4).

    An analytic function h is called bi-univalent in U if h and h1 are univalent in U and class of all bi-univalent functions are denoted by Σ. In 1967, for hΣ, Levin [32] showed that |a2|<1.51 and after twelve years Branan and Clunie [8] gave the improvement of |a2| and proved that |a2|2. Furthermore, for hΣ, Netanyahu [34] proved that max|a2|=43 and an intriguing subclass of analytic and bi-univalent functions was proposed and studied by Branan and Taha [9], who also discovered estimates for the coefficients of the functions in this subclass. Recently, the investigation of numerous subclasses of the analytic and bi-univalent function class Σ was basically revitalized by the pioneering work of Srivastava et al. [41]. In 2012, Xu et al. [44] defined a general subclass of class Σ and investigated coefficient estimates for the functions belonging to the new subclass of class Σ. Recently, several different subclasses of class Σ were introduced and investigated by a number of authors (see for details ([23,29,38]). In these recent papers only non-sharp estimates on the initial coefficients were obtained.

    Faber polynomials was introduced by Faber [15] and first time he used it to determine the general coefficient bounds |ak| for k4. Gong [16] interpreted significance of Faber polynomials in mathematical sciences, particularly in Geometric Function Theory. In 1913, Hamidi et al. [18] first time used the Faber polynomials expansion technique on meromorphic bi-starlike functions and determined the coefficient estimates. The Faber polynomials expansion method for analytic bi-close-to-convex functions was examined by Hamidi and Jahangiri [21,22], who also discovered some new coefficient bounds for new subclasses of close-to-convex functions. Furthermore, many authors [3,4,7,11,12,14,20] used the same technique and determined some interesting and useful properties for analytic bi-univalent functions. For hΣ, by using the Faber polynomial expansions methods, only a few works have been done so far and we recognized very little over the bounds of Maclaurin's series coefficient |ak| for k4 in the literature. Recently only a few authors, used the Faber polynomials expansion technique and determined the general coefficient bounds |ak| for k4, (see for detail [6,11,24,39,40,42]).

    A domain U is said to be the υ-fold symmetric if

    hυ(ek(2πυ)(z))=ek(2πυ)hυ(z),zU,υZ+,hA

    and every hυ has the series of the form

    hυ=z+k=1aυk+1zυk+1. (1.3)

    The class Sυ represents the set of all υ-fold symmetric univalent functions. For υ=1, then Sυ reduce to the class S of univalent functions. If the inverse gυ of univalent h is univalent then h is called υ-fold symmetric bi-univalent functions in U and denoted by Συ. The series expansion of inverse function gυ investigated by Srivastava et al. in [43]:

    gυ(w)=waυ+1wυ+1+((υ+1)a2υ+1a2υ+1)w2υ+1{12(υ+1)(3υ+2)a3υ+112(υ+1)(υ+2)a3υ+1((3υ+2)aυ+1a2υ+1+a3υ+1)}w3υ+1. (1.4)

    For υ=1, the series in (1.4) reduces to the (1.2) of the class Σ. In [43] Srivastava et al. defined a subclass of υ-fold symmetric bi-univalent functions and investigated coeffiients problem for υ-fold symmetric bi-univalent functions. Hamidi and Jahangiri [19] defined υ-fold symmetric bi-starlike functions and discussed the unpredictability of the coefficients of υ-fold symmetric bi-starlike functions.

    Many researchers have used the q-calculus and fractional q-calculus in the field of Geometric Function Theory (GFT) and they defined and studied several new subclasses of analytic, univalent and bi-univalent functions. In 1909, Jackson ([26,27]), gave the idea of q-calculus operator and defined the q-difference operator (Dq) while in [25], Ismail et al. was the first who used Dq in order to define a class of q-starlike functions in open unit disk U. The most signifcant usages of q-calculus in the perspective of GFT was basically furnished and the basic (orq) hypergeometric functions were first used in GFT in a book chapter by Srivastava (see, for details, [37]). For more study about q-calculus operator theory in GFT, see the following articles [5,28,33].

    Now we recall, some basic definitions and concepts of the q-calculus which will be used to define some new subclasses of the this paper.

    For a non-negative integer t, the q-number [t,q], (0<q<1), is defined by

    [t,q]=1qt1q,and[0,q]=0

    and the q-number shift factorial is given by

    [t,q]!=[1,q][2,q][3,q][t,q],
    [0,q]!=1.

    For q1, then [t,q]! reduces to t!.

    The q-generalized Pochhammer symbol is defined by

    [t,q]k=Γq(t+k)Γq(t),kN,tC.

    Remark 1.1. For q1, then [t,q]k reduces to (t)k=Γ(t+k)Γ(t).

    Definition 1.2. Jackson [27] defined the q-integral of function h(z) as follows:

    h(z)dq(z)=k=0z(1q)h(qk(z))qk.

    Jackson [26] introduced the q-difference operator for analytic functions as follows:

    Definition 1.3. [26]. For hA, the q-difference operator is defined as:

    Dqh(z)=h(qz)h(z)z(q1),zU.

    Note that, for kN and zU and

    Dq(zk)=[k,q]zk1,Dq(k=1akzk)=k=1[k,q]akzk1.

    Here, we introduce the q-difference operator for υ-fold symmetric functions related to the q-calculus as follows:

    Definition 1.4. Let hυΣυ, of the form (1.3). Then q-difference operator will be defined as

    Dqhυ(z)=hυ(qz)hυ(z)(q1)z,zU, (1.5)
    =1+k=1[υk+1,q]aυk+1zυk

    and

    Dq(k=1aυk+1zυk+1)=k=1[υk+1,q]aυk+1zυk,
    Dq(z)υk+1=[υk+1,q]zυk.

    Now we define Salagean q-differential operator for υ-fold symmetric functions as follows:

    Definition 1.5. For mN, the Salagean q-differential operator for hυΣυ is defined by

    0qhυ(z)=hυ(z),1qhυ(z)=zDqhυ(z)=hυ(qz)hυ(z)(q1),,
    mqhυ(z)=zDq(m1qhυ(z))=(z+k=1([υk+1,q])mzυk+1),
    mqhυ(z)=z+k=1([υk+1,q])maυk+1zυk+1. (1.6)

    Remark 1.6. For υ=1, we have Salagean q-differential operator for analytic functions proved in [17].

    Motivated by the following articles [1,10,25] and using the q-analysis in order to define new subclasses of class Συ, we apply Faber polynomial expansions technique in order to determine the estimates for the general coefficient bounds |aυk+1|. We also derive initial coefficients |aυ+1| and |a2υ+1| and obtain Feketo-Sezego coefficient bounds for the functions belonging to the new subclasses of Συ.

    Definition 1.7. A function hυΣυ is in the class Rυ,γb,q(φ) if and only if

    1+1b{(Dqhυ(z)+γzD2qhυ(z))1}φ(z)

    and

    1+1b{(Dqgυ(w)+γwD2qgυ(w))1}φ(w),

    where, φP, γ0, bC{0}, z, wU, and gυ(w) is defined by (1.4).

    Remark 1.8. For q1, υ=1, and γ=0, then Rυ,γb,q(φ)=Rb(φ) introduced in [22].

    Definition 1.9. A function hυΣυ, is in the class Rυb(b,α,γ) if and only if

    |(1+1b{(Dqhυ(z)+γzD2qhυ(z))1})1αq1q|<1α1q

    and

    |(1+1b{(Dqgυ(w)+γzD2qgυ(w))1})1αq1q|<1α1q.

    Or equivalently by using subordination, we can write the above conditions as:

    1+1b{(Dqhυ(z)+γzD2qhυ(z))1}1+[1α(1+q)]z1qz

    and

    1+1b{(Dqgυ(w)+γwD2qgυ(w))1}1+[1α(1+q)]w1qw,

    where, 0α<1, γ0, bC{0}, z, wU, gυ(w) is defined by (1.4).

    Remark 1.10. For q1, υ=1, α=0 and γ=0, then Rυb(b,α,γ)=Rb(φ) introduced in [22].

    Definition 1.11. A function hυΣυ, is in the class Rυ,γ,mb,q(φ) if and only if

    1+1b{(mqhυ(z)z+γzDq(mqhυ(z)z))1}φ(z)

    and

    1+1b{(mqgυ(w)w+γwDq(mqgυ(w)w))1}φ(w),

    where, φP, γ0,mN, bC{0}, z, wU, gυ(w) is defined by (1.4).

    Using the Faber polynomial technique for the analytic function h, then the coefficient of its inverse map g can be written as follows (see [2,4]):

    gυw)=w+k=21kkk1(a2,a3,...)wk,

    where

    kk1=(k)!(2k+1)!(k1)!ak12+(k)![2(k+1)]!(k3)!ak32a3+(k)!(2k+3)!(k4)!ak42a4+(k)![2(k+2)]!(k5)!ak52[a5+(k+2)a23]+(k)!(2k+5)!(k6)!ak62[a6+(2k+5)a3a4]+i7aki2Qi,

    and Qi is a homogeneous polynomial in the variables a2,a3,...ak, for 7ik. Particularly, the first three term of kk1 are

    1221=a2,1332=2a22a3,1443=(5a325a2a3+a4).

    In general, for rN  and  k2, an expansion of rk of the form:

    rk=rak+r(r1)2E2k+r!(r3)!3!E3k+...+r!(rk)!k!Ekk,

    where,

    Erk=Erk(a2,a3,...)

    and by [2], we have

    Eυk(a2,a3,...ak)=k=1υ!(a2)μ1...(ak)μkμ1!,...,μk!,  for  a1=1  and  υk.

    The sum is taken over all non negative integer μ1,...,μk which is satisfying

    μ1+μ2+...+μk=υ,μ1+2μ2+...+(k)μk=k.

    Clearly,

    Ekk(a1,...,ak)=Ek1

    and

    Ekk=ak1  and  E1k=ak

    are first and last polynomials.

    Now, using the Faber polynomial expansion for hυ of the form (1.3) we have

    hυ(z)=z+k=1aυk+1zυk+1.

    The coefficient of inverse map gυ can be expressed of the form:

    gυ(z)=w+k=11(υk+1)(υk+1)k(aυ+1,a2υ+1,...aυk+1)wυk+1.

    Theorem 2.1. For bC{0}. Let hυRυ,γb,q(φ) by given by (1.3). If aυi+1=0,  1ik1, then

    |aυk+1|2|b|(1+γ[υk,q])[υk+1,q],  for  k2.

    Proof. For hυRυ,γb,q(φ) we have

    1+1b{(Dqhυ(z)+γzD2qhυ(z))1}
    =1+k=1(1+γ[υk,q])[υk+1,q]baυk+1zυk (2.1)

    and

    1+1b{(Dqgυ(w)+γwD2qgυ(w))1}
    =1+k=1(1+γ[υk,q])[υk+1,q]bAυk+1wυk, (2.2)

    where,

    Aυk+1=1(υk+1)(υk+1)k(aυ+1,a2υ+1,...aυk+1),  for  k1.

    Since hυRυ,γb,q(φ) and gυRυ,γb,q(φ) by definition, we have

    p(z)=k=1ckzυk (2.3)

    and

    r(w)=k=1dkwυk (2.4)

    where

    φ(p(z))=1+k=1l=1φllk(c1,c2,...,ck)zυk, (2.5)
    φ(r(w))=1+k=1l=1φllk(d1,d2,...,dk)wυk. (2.6)

    Equating the coefficient of (2.1) and (2.5) we obtain

    ((1+γ[υk,q])[υk+1,q]b)aυk+1=k1l=1φllk(c1,c2,...,ck). (2.7)

    Similarly, corresponding coefficient of (2.2) and (2.6), we have

    ((1+γ[υk,q])[υk+1,q]b)Aυk+1=k1l=1φllk(d1,d2...,dk). (2.8)

    Since, 1ik1,  and  aυi+1=0; we have

    Aυk+1=aυk+1

    and

    (1+γ[υk,q])[υk+1,q]baυk+1=φ1ck, (2.9)
    (1+γ[υk,q])[υk+1,q]bAυk+1=φ1dk. (2.10)

    Taking the modulus on both sides of (2.9) and (2.10), we have

    |(1+γ[υk,q])[υk+1,q]baυk+1|=|φ1ck|,
    |(1+γ[υk,q])[υk+1,q]bAυk+1|=|φ1dk|.

    Now using the fact |φ1|2,|ck|1, and |dk|1, we have

    |aυk+1||b|(1+γ[υk,q])[υk+1,q]|φ1ck|
    =|b|(1+γ[υk,q])[υk+1,q])|φ1dk|,
    |aυk+1|2|b|(1+γ[υk,q])[υk+1,q].

    Hence, Theorem 2.1 is completed.

    For υ=0,γ=0,q1,k=n1, in Theorem 2.1, we obtain known corollary proved in [22].

    Corollary 2.2. For bC{0}, Let hυRb(φ), If aυi+1=0,1in. Then

    |an|2|b|n,  for  n3.

    Theorem 2.3. For bC{0}. Let hυRυ,γb,q(φ) be given by (1.3). Then

    |aυ+1|{2|b|(1+γ[υk,q])[υ+1,q],  if  |b|<ψ1(υ,q),|b|ψ1(υ,q),  if  |b|ψ1(v,q),
    |a2υ+1|{|b|ψ2(υ,q)+2|b|2(1+γ[υ,q])[υ+1,q],  if  |b|<ψ2(υ,q),2|b|ψ2(υ,q),  if  |b|ψ2(υ,q),
    |a2υ+1(1+γ[υ,q])[υ+1,q]a2υ+1|2|b|ψ2(υ,q),
    |a2υ+11ψ2(υ,q)a2υ+1||b|ψ2(υ,q),

    where,

    ψ1(υ,q)=8((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q]),
    ψ2(υ,q)=2((1+γ[2υ,q])[2υ+1,q].

    Proof. Taking k=1 and k=2 in (2.7) and (2.8), then, we have

    (1+γ[υ,q])[υ+1,q]baυ+1=φ1c1, (2.11)
    (1+γ[2υ,q])[2υ+1,q]ba2υ+1=φ1c2+φ2c21, (2.12)
    (1+γ[υ,q])[υ+1,q]baυ+1=φ1d1, (2.13)
    {(1+γ[υ,q])[υ+1,q]a2υ+1a2υ+1}=b(φ1d2+φ2d21)(1+γ[2υ,q])[2υ+1,q]. (2.14)

    From (2.11) and (2.13) and using the fact |φ1|2,|ck|1 and |dk|1, we have

    |aυ+1||b|(1+γ[υ,q])[υ+1,q]|φ1c1|=|b|(1+γ[υ,q])[υ+1,q]|φ1d1|2|b|1+γ[υ,q])[υ+1,q]. (2.15)

    Adding (2.12) and (2.14) we have

    a2υ+1=b{φ1(c2+d2)+φ2(c21+d21)}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q]). (2.16)

    Taking absolute value of (2.16), we have

    |aυ+1|8|b|((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q]).

    Now the bounds given for |aυ+1| can be justified since

    |b|<8((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q])

    for

    |b|<8((1+γ[2υ,q])[2υ+q])((1+γ[υ,q])[υ+1,q]).

    From (2.12), we get

    |a2υ+1|=|b||φ1c2+φ2c21|(1+γ[2υ,q])[2υ+1,q]4b(1+γ[2υ,q])[2υ+1,q]. (2.17)

    Subtract (2.14) from (2.12), we have

    2(1+γ[2υ,q])[2υ+1,q]b{a2υ+1(1+γ[υ,q])[υ+1,q]2a2υ+1}=φ1(c2d2)+φ2(c21d21)=φ1(c2d2), (2.18)

    or

    a2υ+1=(1+γ[υ,q])[υ+1,q]2a2υ+1+φ1b(c2d2)2(1+γ[2v,q])[2v+1,q]. (2.19)

    Taking the absolute, we have

    a2v+1|φ1∣∣b∣∣c2d22(1+γ[2υ,q])[2υ+1,q]+(1+γ[υ,q])[υ+1,q]2a2υ+1|. (2.20)

    Using the assertion (2.15) on (2.20), we have

    a2υ+1∣≤2b(1+γ[2υ,q])[2υ+1,q]+2b2(1+γ[υ,q])[υ+1,q]. (2.21)

    Follows from (2.17) and (2.21) upon nothing that

    2b(1+γ[2υ,q])[2υ+1,q]+2b2(1+γ[υ,q])[υ+1,q]2b(1+γ[2υ,q])[2υ+1,q]  if  b∣<2(1+γ[2υ,q])[2υ+1,q].

    Now, rewrite (2.14) as follows:

    (1+γ[υ,q])[υ+1,q]a2υ+1a2υ+1=b(φ1d2+φ2d21)(1+γ[2υ,q])[2υ+1,q].

    Using the fact φ1∣≤2, ck∣≤1 and dk∣≤1, we have

    a2υ+1(1+γ[υ,q])[υ+1,q]a2υ+1∣≤4b(1+γ[2υ,q])[2υ+1,q].

    From (2.18), we have

    2(1+γ[2υ,q])[2υ+1,q]b{a2υ+1(1+γ[2υ,q])[2υ+1,q]2a2υ+1}=φ1(c2d2).

    Again using the fact φ1∣≤2, ck∣≤1 and dk∣≤1, we have

    |a2υ+1(1+γ[2υ,q])[2υ+1,q]2a2υ+1|2b(1+γ[2υ,q])[2υ+1,q].

    Take q1,γ=0,υ=1, and k=n1 in the Theorem 2.3, we get known corollary.

    Corollary 2.4. [22]. For bC{0}, let hRb(φ) be given by (1.1), then

    |a2|{|b|,  if  |b|<43,4|b|3,  if  |b|43,
    |a3|{2|b|3+|b|2,  if  |b|<23,4|b|3,  if  |b|23,
    |a32a22|4|b|3,
    |a3a22|2|b|3.

    Theorem 2.5. For bC{0}. Let hυRυq(b,α,γ) by given by (1.3). If aυi+1=0,1ik1. Then

    |aυk+1|(B0B1)|b|(1+γ[υk,q])[υk+1,q],fork2.

    where, B0=1α(1+q) and B1=q.

    Proof. Let hυRυq(b,α,γ). Then

    1+1b{(Dqhυ(z)+γzD2qhυ(z))1}=1+k=1(1+γ[υk,q])[υk+1,q]baυk+1zυk (2.22)

    and

    1+1b{(Dqgυ(w)+γwD2qgυ(w))1}=1+k=1(1+γ[υk,q])[υk+1,q]bAυk+1wυk. (2.23)

    where,

    Aυk+1=1(υk+1)(υk+1)(aυ+1,a2υ+1,...,aυk+1),  k1.

    Since hυRυq(b,α,γ) and gυRυq(b,α,γ) by definition, there exist two positive real functions p(z) and r(w) given in (2.3) and (2.4), then we have

    =1+B0(p(z))1+B1(p(z))=1k=1kl=1(B0B1)1k(c1,c2,...,ck,B1)zυk (2.24)
    =1+B0(r(w))1+B1(r(w))=1k=1kl=1(B0B1)1k(d1,d2,...,dk,B1)wυk. (2.25)

    Equating the corresponding coefficients of (2.22) and (2.24), we have

    (1+γ[υk,q])[υk+1,q]baυk+1=(B0B1)1k(c1,c2,...,ck,B1)zυk. (2.26)

    Similarly, corresponding coefficient of (2.23)and (2.25), we have

    (1+γ[υk,q])[υk+1,q]bAυk+1=(B0B1)1k(d1,d2,...,dk,B1)wυk. (2.27)

    For aυi+1=0;1ik1, we get

    Aυk+1=aυk+1

    and we have

    (1+γ[υk,q])[υk+1,q]baυk+1=(B0B1)ck, (2.28)

    and

    (1+γ[υk,q])[υk+1,q]bAυk+1=(B0B1)dk. (2.29)

    Taking modulus on (2.28) and (2.29), we have

    |(1+γ[υk,q])[υk+1,q]baυk+1|=|(B0B1)ck|,|(1+γ[υk,q])[υk+1,q]bAυk+1|=|(B0B1)dk|.

    Since

    |ck|1and|dk|1(see[14]),

    we have

    |aυk+1||b|(1+γ[υk,q])[υk+1,q]|(B0B1)ck|=|b|(1+γ[υk,q])[υk+1,q]|(B0B1)dk,||aυk+1|(B0B1)|b|(1+γ[υk,q])[υk+1,q],

    which complete the proof of Theorem.

    For b=1,k=1,υ=n1,q1,andγ0 in the above Theorem 2.5, we obtain the following result given in [40].

    Corollary 2.6. Let hυR(n,α,γ) be given by (1.3). If an1=0, and 1ik1, then

    |an|2(1α)n(1+γ(n1)),nN{1,2}.

    Theorem 2.7. For bC{0}, let hυRυq(b,α,γ) be given by (1.3), then

    |aυ+1|{(B0B1)|b|(1+γ[υ,q])[υ+1,q],if|b|<ψ3(υ,q),2|b|ψ3(υ,q)if|b|ψ3(υ,q),
    |a2υ+1|{|b|ψ4(υ,q)+ψ4(υ,q)|(B0B1)||b|2,if|b|<ψ4(υ,q),|b|(|B1|+1)ψ4(υ,q)if|b|ψ4(υ,q),
    |a2υ+1(1+γ[υ,q])[υ+1,q]a2υ+1||b|(|B1|+1|)ψ4(υ,q)

    and

    |a2υ+1(1+γ[2υ,q])[2υ+1,q]2a2υ+1||b|ψ4(υ,q),

    where

    ψ3(υ,q)=|B0B1|{|B1|+1}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q])ψ4(υ,q)=|B0B1|(1+γ[2υ,q])[2υ+1,q].

    Proof. Take k=1 and k=2 in (2.26) and (2.27). Then we have

    (1+γ[υ,q])[υ+1,q]baυ+1=(B0B1)c1, (2.30)
    (1+γ[2υ,q])[2υ+1,q]ba2υ+1=(B0B1)(B1c21+c2), (2.31)
    (1+γ[υ,q])[υ+1,q]baυ+1=(B0B1)d1, (2.32)
    (1+γ[υ,q])[υ+1,q]a2υ+1a2υ+1=b(B0B1)(B1d21+d2)(1+γ[2υ,q])[2υ+1,q]. (2.33)

    From (2.30) and (2.32) and using the fact |φ1|2,|ck|1 and |dk|1, we have

    |aυ+1||b|(1+γ[υ,q])[υ+1,q]|(B0B1)c1|=|b|(1+γ[υ,q])[υ+1,q]|(B0B1)d1|(B0B1)|b|(1+γ[υ,q])[υ+1,q]. (2.34)

    Adding (2.31) and (2.33) we have

    a2υ+1=b(B0B1){(c2+d2)+B1(c21+d21)}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q])

    and

    |aυ+1|22|b||B0B1|{|B1|+1}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q]). (2.35)

    Taking the square-root of (2.35), we have

    |aυ+1|2|b||B0B1|{|B1|+1}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q]).

    Now the bounds given for |aυ+1| can be justified since

    |b|<2|b||B0B1|{|B1|+1}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q])for|b|<2|b||B0B1|{|B1|+1}((1+γ[2υ,q])[2υ+1,q])((1+γ[υ,q])[υ+1,q]).

    From (2.31), we have

    |a2υ+1|=|b||(B0B1)(B1c21+c2)|(1+γ[2υ,q])[2υ+1,q]|b||B0B1|(|B1|+1)(1+γ[2υ,q])[2υ+1,q]. (2.36)

    Next we subtract (2.33) from (2.31), we get

    2(1+γ[2υ,q])[2υ+1,q]b{a2υ+1(1+γ[υ,q])[υ+1,q]2a2υ+1}=(B0B1){B1(d21c21)(c2d2)}=(B0B1)(c2d2), (2.37)

    or

    a2υ+1=(1+γ[υ,q])[υ+1,q]2a2υ+1+(B0B1)b(c2d2)2(1+γ[2υ,q])[2υ+1,q]. (2.38)

    Taking the absolute values yield

    |a2υ+1||(B0B1)||b||c2d2|2(1+γ[2υ,q])[2υ+1,q]+(1+γ[υ,q])[υ+1,q]2|a2υ+1|. (2.39)

    Using the assertion (2.34) on (2.39), we have

    |a2υ+1||(B0B1)||b|(1+γ[2υ,q])[2υ+1,q]+|(B0B1)|2|b|22(1+γ[υ,q])[υ+1,q]. (2.40)

    It follows from (2.36) and (2.40) upon noting that

    |(B0B1)||b|(1+γ[2υ,q])[2υ+1,q]+|(B0B1)|2|b|22(1+γ[υ,q])[υ+1,q].|(B0B1)||b|(1+γ[2υ,q])[2υ+1,q]if|b|<|(B0B1)|(1+γ[2υ,q])[2υ+1,q].

    Now, we rewrite (2.33) as follows:

    {(1+γ[υ,q])[υ+1,q]a2υ+1a2υ+1}=b(B0B1)(B1d21+d2)(1+γ[2υ,q])[2υ+1,q].

    Taking the modulus and using |φ1|2, |ck|1 and |dk|1, we have

    |a2υ+1(1+γ[υ,q])[υ+1,q]a2υ+1|(B0B1)(|B1|+1)|b|(1+γ[2υ,q])[2υ+1,q].

    Finally, from (2.37), we have

    {a2υ+1(1+γ[2υ,q])[2υ+1,q]2a2υ+1}=b(B0B1)(c2d2)2(1+γ[2υ,q])[2υ+1,q].

    Taking the modulus and using |ck|1 and |dk|1, we have

    |a2υ+1(1+γ[2υ,q])[2υ+1,q]2a2υ+1|(B0B1)|b|(1+γ[2υ,q])[2υ+1,q].

    For υ=1,γ=0,q1,k=n1 in Theorem 2.7, then we obtain result proved in [22].

    Corollary 2.8. [22]. For bC{0}, let hυRb(φ) be given by (1.1), then

    |a2|{|b|,  if  |b|<43,4|b|3,  if  |b|43,
    |a3|{2|b|3+|b|2,  if  |b|<23,4|b|3,  if  |b|23,
    |a32a22|4|b|3,
    |a3a22|2|b|3.

    Here, in this section, we consider the newly defined Salagean qdifferential operator for subclass of Rυ,γ,mb,q(φ) of class of υ and investigate some new application in the form of results

    Theorem 2.9. For bC{0}. Let hυRυ,γ,mb,q(φ) by given by (1.3). If aυi+1=0, and 1ik1, then

    |aυk+1|2|b|(1+γ[υk,q])(υk+1,q)m,fork2.

    Proof. We can prove Theorem 2.9 by using the similar method of Theorem 2.1.

    Theorem 2.10. For bC{0}. Let hυRυ,γ,mb,q(φ) by given by (1.3). Then

    |aυ+1|{2|b|(1+γ[υ,q])(υ+1,q)m,if|b|<ψ3(υ,q),|b|  ψ1(υ,q),if|b|ψ3(υ,q),
    |a2υ+1|{|b|ψ2(υ,q)+2|b|2(1+γ[υ,q])[υ+1,q]m,if|b|<ψ4(υ,q),2|b|ψ2(υ,q)if|b|ψ4(υ,q),
    |a2υ+1(1+γ[υ,q])[υ+1,q]ma2υ+1|2|b|ψ4(υ,q),
    |a2υ+11ψ2(υ,q)a2υ+1||b|ψ4(υ,q),

    where

    ψ3(υ,q)=8((1+γ[2υ,q])[2υ+1,q]m)((1+γ[υ,q])[υ+1,q]m),
    ψ4(υ,q)=2(1+γ[2υ,q])[2υ+1,q]m.

    Proof. We can prove Theorem 2.10 by using the similar method of Theorem 2.3.

    In this article, first of all, we used the q-difference operator for υ-fold symmetric functions in order to define some new subclasses of the υ-fold symmetric bi-univalent functions in the open symmetric unit disk U. We also used the basic concepts of q-calculus and defined the Salagean q-differential operator for υ-fold symmetric functions. We considered this operator and investigated a new subclass of υ-fold symmetric bi-univalent functions. Faber Polynomial expansion method and q-analysis are used in order to determined general coefficient bounds |aυ+1| for functions in each of these newly defined υ-fold symmetric bi-univalent functions classes. Feketo-Sezego problems and initial coefficient bounds |aυ+1| and |a2υ+1| for the function belonging to the subclasses of υ-fold symmetric bi-univalent functions in open symmetric unit disk U are also investigated.

    I would like to thank to the editor and referees for their valuable comments and suggestions.

    The author declares no conflict of interest.



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