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Article

A Generalization of Gegenbauer Polynomials and Bi-Univalent Functions

1
Department of Mathematics, Faculty of Science and Technology, Irbid National University, Irbid 21110, Jordan
2
Department of Mathematics, Al-Leith University College, Umm Al-Qura University, Mecca 24231, Saudi Arabia
3
Department of Basic Sciences, Faculty of Arts and Science, Al-Ahliyya Amman University, Amman 19328, Jordan
4
Department of Mathematics, Faculty of Science, Zarqa University, Zarqa 13110, Jordan
5
Department of Basic Scientific Sciences, Applied Science Private University, Amman 11931, Jordan
*
Authors to whom correspondence should be addressed.
Axioms 2023, 12(2), 128; https://doi.org/10.3390/axioms12020128
Submission received: 30 December 2022 / Revised: 17 January 2023 / Accepted: 22 January 2023 / Published: 28 January 2023
(This article belongs to the Special Issue Recent Advances in Complex Analysis and Applications)

Abstract

:
Three subclasses of analytic and bi-univalent functions are introduced through the use of q Gegenbauer polynomials, which are a generalization of Gegenbauer polynomials. For functions falling within these subclasses, coefficient bounds a 2 and a 3 as well as Fekete–Szegö inequalities are derived. Specializing the parameters used in our main results leads to a number of new results.

1. Introduction

Legendre first made the discovery of orthogonal polynomials in 1784 [1]. Under specific model restrictions, orthogonal polynomials are frequently employed to solve ordinary differential equations. Furthermore, a crucial function in the approximation theory is performed by orthogonal polynomials [2].
P m and P n are two polynomials of order m and n, respectively, and are orthogonal if
a b P n ( x ) P m ( x ) s ( x ) d x = 0 , for m n ,
where s ( x ) is a suitably specified function in the interval ( a , b ) ; therefore, all finite order polynomials P n ( x ) have a well-defined integral.
Gegenbauer polynomials are orthogonal polynomials of a specified type. As found in [3], when traditional algebraic formulations are used, the generating function of Gegenbauer polynomials and the integral representation of typically real functions T R are related to each other in a symbolic way T R . This undoubtedly caused a number of helpful inequalities to emerge from the world of Gegenbauer polynomials.
q orthogonal polynomials are now of particular relevance in both physics and mathematics due to the development of quantum groups. The q deformed harmonic oscillator, for instance, has a group-theoretic setting for the q Laguerre and q Hermite polynomials. Jackson’s q exponential plays a crucial role in the mathematical framework required to characterize the properties of these q polynomials, such as the recurrence relations, generating functions, and orthogonality relations. Jackson’s q exponential has recently been expressed by Quesne [4] as a closed-form multiplicative series of regular exponentials with known coefficients. In this case, it is crucial to look into how this discovery might affect the theory of q orthogonal polynomials. An effort in this regard was made in the current work. To obtain novel nonlinear connection equations for q Gegenbauer polynomials in terms of their respective classical equivalents, we used the aforementioned result in particular.
This study analyzed various features of the class under consideration after associating some bi-univalent functions with q Gegenbauer polynomials. The following part lays the foundation for mathematical notations and definitions.

2. Preliminaries

Let A denote the class of all analytical functions f that are defined on the open unit disk U = { ξ C : ξ < 1 } and normalized by the formula f ( 0 ) =   f ( 0 ) 1 = 0 . As a result, each f A has the following Taylor–Maclaurin series expansion:
f ( ξ ) = ξ + n = 2 a n ξ n , ( ξ U ) .
In addition, let S denote the class of all functions f A that are univalent in U .
Let the functions g ( ξ ) and f ( ξ ) be analytic in U . We say that the function f ( ξ ) is subordinate to g ( ξ ) , written as f ( ξ ) g ( ξ ) , if there exists a Schwarz function ω that is analytic in U with
| ω ( ξ ) | < 1 and ω ( 0 ) = 0 ( ξ U )
such that
g ( ω ( ξ ) ) = f ( ξ ) .
Beside that, if the function g is univalent in U , then the following equivalence holds:
f ( ξ ) g ( ξ ) if g ( 0 ) = f ( 0 )
and
f ( U ) g ( U ) .
It is well known that every function f S has an inverse f 1 , defined by
ξ = f 1 ( f ( ξ ) ) ( ξ U )
and
f 1 ( f ( w ) ) = w ( r 0 ( f ) 1 4 ; w < r 0 ( f ) )
where
f 1 ( w ) = w a 2 w 2 w 3 ( a 3 2 a 2 2 ) + w 4 ( 5 a 2 a 3 a 4 5 a 2 3 ) + .
If both f 1 ( ξ ) and f ( ξ ) are univalent in U , then a function is said to be bi-univalent in U .
Let Σ denote the class of bi-univalent functions in U given by (1). Examples of functions in the class Σ are ξ 1 ξ , log 1 + ξ 1 ξ .
Fekete and Szegö achieved a sharp bound of the functional η a 2 2 a 3 , with real η ( 0 η 1 ) for a univalent function f in 1933 [5]. Since that time, it has been known as the classical Fekete and Szegö problem of establishing the sharp bounds for this functional of any compact family of functions f A with any complex η .
In 1983, Askey and Ismail [6] found a class of polynomials that can be interpreted as q–analogues of the Gegenbauer polynomials. These are essentially the polynomials B q ( λ ) ( ξ , z )
G q ( λ ) ( x , ξ ) = n = 0 C n ( λ ) ( x ; q ) ξ n ,
where x [ 1 , 1 ] and ξ U .
In 2006, Chakrabarti et al. [7] found a class of polynomials that can be interpreted as q–analogues of the Gegenbauer polynomials by the following recurrence relations:
C 0 ( λ ) ( x ; q ) = 1 , C 1 ( λ ) ( x ; q ) = [ λ ] q C 1 1 ( x ) = 2 [ λ ] q x ,
C 2 ( λ ) ( x ; q ) = [ λ ] q 2 C 2 1 ( x ) 1 2 [ λ ] q 2 [ λ ] q 2 C 1 2 ( x ) = 2 [ λ ] q 2 + [ λ ] q 2 x 2 [ λ ] q 2 .
where 0 < q < 1 and λ N = 1 , 2 , 3 , .
In 2021, Amourah et al. [8,9] considered the classical Gegenbauer polynomials G ( λ ) ( x , ξ ) , where ξ U and x [ 1 , 1 ] . For fixed x, the function G ( λ ) is analytic in U , so it can be expanded in a Taylor series as
G ( λ ) ( x , ξ ) = n = 0 C n α ( x ) ξ n ,
where C n α ( x ) is the classical Gegenbauer polynomial of degree n.
Recently, several authors have begun examining bi-univalent functions connected to orthogonal polynomials (such as [10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28]).
As far as we are aware, there is no published work on bi-univalent functions for q Gegenbauer polynomials. The major objective of this work is to start an investigation of the characteristics of bi-univalent functions related to q Gegenbauer polynomials. To perform this, we consider the following definitions in the next section.

3. Coefficient Bounds of the Class B Σ ( x , α ; q )

Here, we introduce some new bi-univalent function subclasses that are subordinate to the q Gegenbauer polynomial.
Definition 1. 
For x ( 1 2 , 1 ] and 0 < q < 1 , if the following subordinations are satisfied, a function f belonging to Σ is said to be in the class B Σ ( x , α ; q ) given by (1):
q f ( ξ ) G q ( λ ) ( x , ξ )
and
q g ( w ) G q ( λ ) ( x , w ) ,
where λ N = 1 , 2 , 3 , , α is a nonzero real constant, the function f 1 ( w ) = g ( w ) is defined by (2), and G q ( λ ) is the generating function of q–analogues of the Gegenbauer polynomials given by (3).
We start by providing the coefficient estimates for the class B Σ ( x , α ; q ) specified in Definition 1.
Theorem 1. 
Let f Σ given by (1) be in the class B Σ ( x , α ; q ) . Then,
a 2 2 x | [ λ ] q | 2 [ λ ] q x [ 2 ] q 4 [ 3 ] q [ 2 ] q 2 2 [ λ ] q 2 2 [ λ ] q 2 x 2 + [ λ ] q ,
and
a 3 4 [ λ ] q 2 x 2 [ 2 ] q 2 + 2 | [ λ ] q | x [ 3 ] q .
Proof. 
Let f B Σ ( x , α ; q ) . From Definition 1, for some analytic functions w and v such that w ( 0 ) = 0 = v ( 0 ) and | w ( ξ ) | < 1 , | v ( w ) | < 1 for all w , ξ U ; then, we can write
q f ( ξ ) = G q ( λ ) ( x , w ( ξ ) )
and
q g ( w ) = G q ( λ ) ( x , v ( w ) ) ,
From the Equations (8) and (9), we obtain that
q f ( ξ ) = 1 + C 1 ( λ ) ( x ; q ) c 1 ξ + C 1 ( λ ) ( x ; q ) c 2 + C 2 ( λ ) ( x ; q ) c 1 2 ξ 2 +
and
q g ( w ) = 1 + C 1 ( λ ) ( x ; q ) d 1 w + C 1 ( λ ) ( x ; q ) d 2 + C 2 ( λ ) ( x ; q ) d 1 2 ) w 2 + .
It is generally understood that if
w ( ξ ) = c 1 ξ + c 2 ξ 2 + c 3 ξ 3 + < 1 , ( ξ U )
and
v ( w ) = d 1 w + d 2 w 2 + d 3 w 3 + < 1 , ( w U ) ,
then
| c j | 1 and | d j | 1 for all j N .
As a result, we have the following after comparing the relevant coefficients in (10) and (11):
[ 2 ] q a 2 = C 1 ( λ ) ( x ; q ) c 1 ,
[ 3 ] q a 3 = C 1 ( λ ) ( x ; q ) c 2 + C 2 ( λ ) ( x ; q ) c 1 2 ,
[ 2 ] q a 2 = C 1 ( λ ) ( x ; q ) d 1 ,
and
[ 3 ] q 2 a 2 2 a 3 = C 1 ( λ ) ( x ; q ) d 2 + C 2 ( λ ) ( x ; q ) d 1 2 .
From the Equations (13) and (15), we have
c 1 = d 1
and
2 [ 2 ] q 2 a 2 2 = C 1 ( λ ) ( x ; q ) 2 c 1 2 + d 1 2 .
By adding (14) to (16), yields
2 [ 3 ] q a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + d 2 + C 2 ( λ ) ( x ; q ) c 1 2 + d 1 2 .
We determine that, by replacing the value of c 1 2 + d 1 2 from (18) on the right side of (19),
2 [ 3 ] q 2 C 2 ( λ ) ( x ; q ) [ 2 ] q 2 C 1 ( λ ) ( x ; q ) 2 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + d 2 .
Through computations using (11), (5) and (20), we find that
a 2 2 | [ λ ] q | x 2 [ λ ] q x [ 2 ] q 4 [ 3 ] q [ 2 ] q 2 2 [ λ ] q 2 2 [ λ ] q 2 x 2 + [ λ ] q .
In addition, if we subtract (16) from (14), we obtain
2 [ 3 ] q a 3 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 d 2 + C 2 ( λ ) ( x ; q ) c 1 2 d 1 2 .
Then, in view of (18) and (21), we obtain
a 3 = C 1 ( λ ) ( x ; q ) 2 2 [ 2 ] q 2 c 1 2 + d 1 2 + C 1 ( λ ) ( x ; q ) 2 [ 3 ] q c 2 d 2 .
By applying (4), we conclude that
a 3 4 [ λ ] q 2 x 2 [ 2 ] q 2 + 2 | [ λ ] q | x [ 3 ] q .
The proof of the theorem is now complete. □
Using the values of a 2 2 and a 3 , we prove the following Fekete–Szegö inequality for functions in the class B Σ ( x , α ; q ) .
Theorem 2. 
Let f Σ given by (1) be in the class B Σ ( x , α ; q ) . Then,
| a 3 σ a 2 2 | 2 x [ λ ] q [ 3 ] q , | σ 1 | 2 [ 3 ] q [ 2 ] q 2 [ λ ] q 2 [ 2 ] q 2 [ λ ] q 2 x 2 + 2 [ 2 ] q 2 [ λ ] q 2 2 [ 3 ] q [ λ ] q 2 x 2 , 2 2 [ λ ] q x h ( η ) , | σ 1 | 2 [ 3 ] q [ 2 ] q 2 [ λ ] q 2 [ 2 ] q 2 [ λ ] q 2 x 2 + 2 [ 2 ] q 2 [ λ ] q 2 2 [ 3 ] q [ λ ] q 2 x 2 .
Proof. 
From (20) and (21),
a 3 σ a 2 2 = 1 σ C 1 ( λ ) ( x ; q ) 3 c 2 + d 2 2 [ 3 ] q C 1 ( λ ) ( x ; q ) 2 2 [ 2 ] q 2 C 2 ( λ ) ( x ; q ) + C 1 ( λ ) ( x ; q ) 2 [ 3 ] q c 2 d 2 = C 1 α ( x ) h ( η ) + 1 2 [ 3 ] q c 2 + h ( η ) 1 2 [ 3 ] q d 2 ,
where
K ( σ ) = C 1 ( λ ) ( x ; q ) 2 1 σ 2 [ 3 ] q C 1 ( λ ) ( x ; q ) 2 2 [ 2 ] q 2 C 2 ( λ ) ( x ; q ) ,
In view of (4) and (5), we conclude that
| a 3 σ a 2 2 | C 1 ( λ ) ( x ; q ) [ 3 ] q , K ( σ ) 1 2 [ 3 ] q , 2 C 1 ( λ ) ( x ; q ) K ( σ ) , K ( σ ) 1 2 [ 3 ] q .
The proof of the theorem is now complete. □
Corollary 1. 
Let f Σ given by (1) belong to the class B Σ ( x , α ; 1 ) . Then,
a 2 α x 2 α x α 2 x 2 + 1 α .
a 3 λ 2 x 2 + 2 | λ | x 3 ,
and a 3 η a 2 2 2 α x 3 , 2 α x 3 1 η α 2 x 2 + 1 α , η 1 α 2 x 2 + 1 3 α x 2 η 1 α 2 x 2 + 1 3 α x 2 .
Corollary 2. 
Let f Σ given by (1) belong to the class B Σ ( x , 1 ; 1 ) . Then,
a 2 x 2 x 1 x 2 ,
a 3 x 2 + 2 x 3 ,
and
a 3 η a 2 2 2 x 3 , 2 x 3 1 η 1 x 2 , η 1 1 x 2 3 x 2 η 1 1 x 2 3 x 2 .

4. Coefficient Bounds of the Class S Σ * ( x , α ; q )

Definition 2. 
For x ( 1 2 , 1 ] and 0 < q < 1 , if the following subordinations are satisfied, a function f belonging to Σ is said to be in the class S Σ * ( x , α ; q ) given by (1):
ξ q f ( ξ ) f ( ξ ) G q ( λ ) ( x , ξ ) ,
and
w q g ( w ) g ( w ) G q ( λ ) ( x , w ) ,
where λ N = 1 , 2 , 3 , , α is a nonzero real constant, the function g ( w ) = f 1 ( w ) is defined by (2), and G q ( λ ) is the generating function of the q–analogues of Gegenbauer polynomials given by (3).
Theorem 3. 
Let f Σ given by (1) belong to the class S Σ * ( x , α ; q ) . Then, we have
| a 2 | 2 | [ λ ] q | x 2 [ λ ] q x q 2 [ λ ] q 2 [ λ ] q 2 x 2 + [ λ ] q 2 ,
and
| a 3 | 4 [ λ ] q 2 x 2 q 2 + 2 [ λ ] q x q 1 + q .
Proof. 
Let f S Σ * ( x , α ; q ) . From Definition 2, for some analytic functions w and v such that w ( 0 ) = 0 = v ( 0 ) and | w ( ξ ) | < 1 , | v ( w ) | < 1 for all ξ , w U ,
ξ q f ( ξ ) f ( ξ ) = G q ( λ ) ( x , w ( ξ ) ) ,
and
ξ q g ( w ) g ( w ) = G q ( λ ) ( x , v ( w ) ) .
From the equalities (24) and (25), we obtain that
ξ q f ( ξ ) f ( ξ ) = 1 + C 1 ( λ ) ( x ; q ) ξ + C 1 ( λ ) ( x ; q ) c 2 + C 2 ( λ ) ( x ; q ) c 1 2 ξ 2 +
and
ξ q g ( w ) g ( w ) = 1 + C 1 ( λ ) ( x ; q ) d 1 w + C 1 ( λ ) ( x ; q ) d 2 + C 2 ( λ ) ( x ; q ) d 1 2 ) w 2 + .
Thus, upon comparing the corresponding coefficients in (26) and (27), we have
q a 2 = C 1 ( λ ) ( x ; q ) c 1 ,
q 1 + q a 3 q a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + C 2 ( λ ) ( x ; q ) c 1 2 ,
q a 2 = C 1 ( λ ) ( x ; q ) d 1 ,
and
q 1 + 2 q a 2 2 q 1 + q a 3 = C 1 ( λ ) ( x ; q ) d 2 + C 2 ( λ ) ( x ; q ) d 1 2 .
From the Equations (28) and (30), it follows that
c 1 = d 1
and
2 q 2 a 2 2 = C 1 ( λ ) ( x ; q ) 2 c 1 2 + d 1 2 .
By adding (29) to (31), yields
2 q 2 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + d 2 + C 2 ( λ ) ( x ; q ) c 1 2 + d 1 2 .
We determine that, by replacing the value of c 1 2 + d 1 2 from (33) on the right side of (34),
2 q 2 1 C 2 ( λ ) ( x ; q ) C 1 ( λ ) ( x ; q ) 2 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + d 2 .
Moreover, through computations using (5) and (35), we find that
| a 2 | 2 | [ λ ] q | x 2 [ λ ] q x q 2 [ λ ] q 2 [ λ ] q 2 x 2 + [ λ ] q 2 .
Now, if we subtract (31) from (29), we obtain
2 q 1 + q a 3 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 d 2 + C 2 ( λ ) ( x ; q ) c 1 2 d 1 2 .
By viewing of (33) and (36), we conclude that
a 3 = C 1 ( λ ) ( x ; q ) 2 2 q 2 c 1 2 + d 1 2 . + C 1 ( λ ) ( x ; q ) 2 q 1 + q c 2 d 2 .
By applying (4) and (5), we have
| a 3 | 4 [ λ ] q 2 x 2 q 2 + 2 [ λ ] q x q 1 + q .
This completes the proof of the Theorem 3. □
Theorem 4. 
Let f Σ given by (1) belong to the class S Σ * ( x , α ; q ) . Then,
| a 3 σ a 2 2 | [ λ ] q x q ( 1 + q ) , 1 σ q 2 2 [ λ ] q 2 [ λ ] q 2 x 2 + [ λ ] q 2 8 ( 1 + q ) | [ λ ] q x | 3 , 8 | [ λ ] q x | 3 1 σ q 2 2 [ λ ] q 2 [ λ ] q 2 x 2 + [ λ ] q 2 , 1 σ q 2 2 [ λ ] q 2 [ λ ] q 2 x 2 + [ λ ] q 2 8 ( 1 + q ) | [ λ ] q x | 3 .
Proof. 
From (35) and (36),
a 3 σ a 2 2 = ( 1 σ ) C 1 ( λ ) ( x ; q ) 3 2 q 2 C 1 ( λ ) ( x ; q ) 2 C 2 ( λ ) ( x ; q ) c 2 + d 2 + C 1 ( λ ) ( x ; q ) 2 q 1 + q c 2 d 2 = C 1 ( λ ) ( x ; q ) 2 q K ( σ ) + 1 1 + q c 2 + K ( σ ) 1 1 + q d 2 ,
where
K ( σ ) = C 1 ( λ ) ( x ; q ) 2 1 σ q C 1 ( λ ) ( x ; q ) 2 C 2 ( λ ) ( x ; q ) ,
1 σ q 2 2 [ λ ] q 2 [ λ ] q 2 x 2 + [ λ ] q 2 8 ( 1 + q ) | [ λ ] q x | 3 ,
then, in view of (4) and (5), we conclude that
| a 3 σ a 2 2 | C 1 ( λ ) ( x ; q ) 2 q ( 1 + q ) , K ( σ ) 1 1 + q , 1 q C 1 ( λ ) ( x ; q ) K ( σ ) , K ( σ ) 1 1 + q .
This completes the proof of the Theorem 4. □
Corollary 3. 
Let f Σ given by (1) belong to the class S Σ * ( x , α ; 1 ) . Then, we have
| a 2 | 2 | λ | x 2 x 2 λ 1 x 2 1 , | a 3 | λ 4 λ x + 1 ,
and
| a 3 σ a 2 2 | λ x 2 , 1 σ 2 λ 1 x 2 + 1 16 | λ | 2 x 3 , 8 λ 2 x 3 1 σ 2 λ 1 x 2 + 1 , 1 σ 2 λ 1 x 2 + 1 16 | λ | 2 x 3 .

5. Coefficient Bounds of the Class C Σ ( x , α ; q )

Definition 3. 
For x ( 1 2 , 1 ] and 0 < q < 1 , if the following subordinations are satisfied, a function f belonging to Σ is said to be in the class C Σ ( x , α ; q ) given by (1):
1 + ξ q 2 f ( ξ ) q f ( ξ ) G q ( λ ) ( x , ξ )
and
1 + ξ q 2 g ( w ) q g ( w ) G q ( λ ) ( x , w ) ,
where λ N = 1 , 2 , 3 , , α is a nonzero real constant, the function g ( w ) = f 1 ( w ) is defined by (2), and G q ( λ ) is the generating function of the q–analogues of Gegenbauer polynomials given by (3).
Theorem 5. 
Let f Σ given by (1) belong to the class C Σ ( x , α ; q ) . Then,
| a 2 | 2 [ λ ] q x 2 | [ λ ] q | x [ 2 ] q 2 [ 3 ] q 3 [ 2 ] q [ λ ] q 2 2 [ 2 ] q [ λ ] q 2 x 2 + [ 2 ] q [ λ ] q 2 ,
and
| a 3 | 4 [ λ ] q 2 x 2 [ 2 ] q 2 + 2 [ λ ] q x [ 2 ] q [ 3 ] q .
Proof. 
Let f C Σ ( x , α , μ ; q ) . From Definition 3, for some analytic functions w , v such that w ( 0 ) = v ( 0 ) = 0 and | w ( ξ ) | < 1 , | v ( w ) | < 1 for all ξ , w U ,
1 + ξ q 2 f ( ξ ) q f ( ξ ) = G q ( λ ) ( x , w ( ξ ) ) ,
and
1 + ξ q 2 g ( w ) q g ( w ) = G q ( λ ) ( x , v ( w ) ) .
By expanding the Equations (39) and (40), we obtain that
1 + ξ q 2 f ( ξ ) q f ( ξ ) = 1 + C 1 ( λ ) ( x ; q ) c 1 ξ + C 1 ( λ ) ( x ; q ) c 2 + C 2 ( λ ) ( x ; q ) c 1 2 ξ 2 +
and
1 + ξ q 2 g ( w ) q g ( w ) = 1 + C 1 ( λ ) ( x ; q ) d 1 w + C 1 ( λ ) ( x ; q ) d 2 + C 2 ( λ ) ( x ; q ) d 1 2 ) w 2 + .
Upon comparing the corresponding coefficients in (41) and (42), we have
[ 2 ] q a 2 = C 1 ( λ ) ( x ; q ) c 1 ,
[ 2 ] q [ 3 ] q a 3 [ 2 ] q 2 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + C 2 ( λ ) ( x ; q ) c 1 2 ,
[ 2 ] q a 2 = C 1 ( λ ) ( x ; q ) d 1 ,
and
[ 2 ] q 2 [ 3 ] q [ 2 ] q a 2 2 [ 2 ] q [ 3 ] q a 3 = C 1 ( λ ) ( x ; q ) d 2 + C 2 ( λ ) ( x ; q ) d 1 2 .
We get from (43) and (45) that
c 1 = d 1
and
2 [ 2 ] q 2 a 2 2 = C 1 ( λ ) ( x ; q ) 2 c 1 2 + d 1 2 .
By adding (44) to (46), we obtain
2 [ 2 ] q [ 3 ] q [ 2 ] q a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + d 2 + C 2 ( λ ) ( x ; q ) c 1 2 + d 1 2 .
We determine that, by replacing the value of c 1 2 + d 1 2 from (48) on the right side of (49),
2 [ 2 ] q [ 3 ] q [ 2 ] q [ 2 ] q C 2 ( λ ) ( x ; q ) C 1 ( λ ) ( x ; q ) 2 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 + d 2 .
Moreover, by doing computations along (12) and (50), we find that
| a 2 | 2 [ λ ] q x 2 | [ λ ] q | x [ 2 ] q 2 [ 3 ] q 3 [ 2 ] q [ λ ] q 2 [ 2 ] q [ λ ] q 2 x 2 + [ 2 ] q [ λ ] q 2 .
By subtracting (44) from (46), we obtain
2 [ 2 ] q [ 3 ] q a 3 a 2 2 = C 1 ( λ ) ( x ; q ) c 2 d 2 + C 2 ( λ ) ( x ; q ) c 1 2 d 1 2 .
In view of (48) and (51), we obtain
a 3 = C 1 ( λ ) ( x ; q ) 2 2 [ 2 ] q 2 c 1 2 + d 1 2 + C 1 ( λ ) ( x ; q ) 2 [ 2 ] q [ 3 ] q c 2 d 2 .
By applying (5), we conclude that
| a 3 | 4 [ λ ] q 2 x 2 [ 2 ] q 2 + 2 [ λ ] q x [ 2 ] q [ 3 ] q .
This completes the proof of the Theorem 5. □
Theorem 6. 
Let f Σ given by (1) belong to the class C Σ ( x , α ; q ) . Then,
| a 3 σ a 2 2 |
2 λ x [ 2 ] q [ 3 ] q , 1 σ ϝ , 16 1 σ [ λ ] q 3 x 3 [ 2 ] q 2 2 [ 3 ] q 2 3 [ 2 ] q [ λ ] q 2 2 [ 2 ] q [ λ ] q 2 x 2 + [ 2 ] q [ λ ] q 2 , 1 σ ϝ ,
where
ϝ = 2 2 [ 3 ] q 2 3 [ 2 ] q [ λ ] q 2 2 [ 2 ] q [ λ ] q 2 x 2 + [ 2 ] q [ λ ] q 2 16 [ 2 ] q [ 3 ] q [ λ ] q 2 x 2 .
Proof. 
From (50) and (51),
a 3 σ a 2 2 = 1 σ C 1 ( λ ) ( x ; q ) 3 2 [ 2 ] q q 2 C 1 ( λ ) ( x ; q ) 2 [ 2 ] q C 2 ( λ ) ( x ; q ) c 2 + d 2 + C 1 ( λ ) ( x ; q ) 2 [ 2 ] q [ 3 ] q c 2 d 2 = C 1 ( λ ) ( x ; q ) K ( σ ) + 1 2 [ 2 ] q [ 3 ] q c 2 + K ( σ ) 1 2 [ 2 ] q [ 3 ] q d 2 ,
where
K ( σ ) = 1 σ C 1 ( λ ) ( x ; q ) 2 2 [ 2 ] q q 2 C 1 ( λ ) ( x ; q ) 2 [ 2 ] q C 2 ( λ ) ( x ; q ) ,
1 σ 4 q 2 [ λ ] q 2 x 2 [ 2 ] q C 2 ( λ ) ( x ; q ) 4 [ 3 ] q [ λ ] q 2 x
Then, in view of (5), we conclude that
| a 3 σ a 2 2 | C 1 ( λ ) ( x ; q ) [ 2 ] q [ 3 ] q , K ( σ ) 1 2 [ 2 ] q [ 3 ] q , 1 [ 2 ] q C 1 ( λ ) ( x ; q ) K ( σ ) , K ( σ ) 1 2 [ 2 ] q [ 3 ] q .
This completes the proof of the last theorem. □
Corollary 4. 
Let f Σ given by (1) belong to the class C Σ ( x , α ; 1 ) . Then,
| a 2 | λ x 2 x 1 2 x 2 ,
| a 3 | λ 2 x 2 + λ x 3 .
and
| a 3 σ a 2 2 | 2 [ λ ] q x [ 2 ] q [ 3 ] q , | σ 1 | 1 2 λ x 2 24 λ x 2 , 1 [ 2 ] q C 1 ( λ ) ( x ; q ) K ( σ ) , | σ 1 | 1 2 λ x 2 24 λ x 2 .

6. Conclusions

In the current study, we introduced and examined the coefficient issues related to each of the three new subclasses of the class of bi-univalent functions in the open unit disk U : B Σ ( x , α ; q ) , S Σ * ( x , α ; q ) , and C Σ ( x , α ; q ) . These bi-univalent function classes are described, accordingly, in Definitions 1 to 3. We calculated the estimates of the Fekete–Szegö functional problems and the Taylor–Maclaurin coefficients a 2 and a 3 for functions in each of these three bi-univalent function classes. Several more fresh outcomes are revealed to follow following specializing the parameters involved in our main results. Obtaining estimates on the bound of a n for n 4 ; n N for the classes that have been introduced here is still a problem.

Author Contributions

Conceptualization, A.A. (Ala Amourah) and A.A. (Abdullah Alsoboh); methodology, A.A. (Ala Amourah); validation, O.O., A.A. (Ala Amourah), A.A. (Abdullah Alsoboh), G.M.G. and R.S.; formal analysis, A.A. (Ala Amourah); investigation, A.A. (Ala Amourah), A.A. (Abdullah Alsoboh) and M.A.S.; writing—original draft preparation, A.A. (Ala Amourah) and A.A. (Abdullah Alsoboh); writing—review and editing, A.A. (Ala Amourah) and O.O.; supervision, A.A. (Abdullah Alsoboh). All authors have read and agreed to the published version of the manuscript.

Funding

The authors would like to thank the Deanship of Scientific Research at Umm Al-Qura University for supporting this work by Grant Code: (22UQU4320576DSR01).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

No data were used to support this study.

Conflicts of Interest

The authors declare that there are no conflict of interest.

References

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MDPI and ACS Style

Amourah, A.; Alsoboh, A.; Ogilat, O.; Gharib, G.M.; Saadeh, R.; Al Soudi, M. A Generalization of Gegenbauer Polynomials and Bi-Univalent Functions. Axioms 2023, 12, 128. https://doi.org/10.3390/axioms12020128

AMA Style

Amourah A, Alsoboh A, Ogilat O, Gharib GM, Saadeh R, Al Soudi M. A Generalization of Gegenbauer Polynomials and Bi-Univalent Functions. Axioms. 2023; 12(2):128. https://doi.org/10.3390/axioms12020128

Chicago/Turabian Style

Amourah, Ala, Abdullah Alsoboh, Osama Ogilat, Gharib Mousa Gharib, Rania Saadeh, and Maha Al Soudi. 2023. "A Generalization of Gegenbauer Polynomials and Bi-Univalent Functions" Axioms 12, no. 2: 128. https://doi.org/10.3390/axioms12020128

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