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Article

Coefficient Estimates of New Families of Analytic Functions Associated with q-Hermite Polynomials

by
Isra Al-Shbeil
1,*,
Adriana Cătaş
2,†,
Hari Mohan Srivastava
3,4,5,6,† and
Najla Aloraini
7,†
1
Department of Mathematics, Faculty of Science, The University of Jordan, Amman 11942, Jordan
2
Department of Mathematics and Computer Science, University of Oradea, 1 University Street, 410087 Oradea, Romania
3
Department of Mathematics and Statistics, University of Victoria, Victoria, BC V8W 3R4, Canada
4
Department of Medical Research, China Medical University Hospital, China Medical University, Taichung 40402, Taiwan
5
Department of Mathematics and Informatics, Azerbaijan University, 71 Jeyhun Hajibeyli Street, AZ1007 Baku, Azerbaijan
6
Section of Mathematics, International Telematic University Uninettuno, I-00186 Rome, Italy
7
Department of Mathematics, College of Sciences and Arts Onaizah, Qassim University, P.O. Box 6640, Buraydah 51452, Saudi Arabia
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Axioms 2023, 12(1), 52; https://doi.org/10.3390/axioms12010052
Submission received: 20 November 2022 / Accepted: 27 December 2022 / Published: 3 January 2023
(This article belongs to the Special Issue Mathematical Analysis and Applications III)

Abstract

:
In this paper, we introduce two new subclasses of bi-univalent functions using the q-Hermite polynomials. Furthermore, we establish the bounds of the initial coefficients υ 2 , υ 3 , and υ 4 of the Taylor–Maclaurin series and that of the Fekete–Szegö functional associated with the new classes, and we give the many consequences of our findings.

1. Introduction and Preliminaries

Let M U denote the class of analytic functions in the open unit disk
U = z : z C and z < 1 .
Let A be the subclass of M U whose functions f satisfy the normalization condition given by
f 0 = f 0 1 = 0 ,
that is, each function f in A can be represented by the following Taylor–Maclaurin series expansion:
f z = z + k = 2 υ k z k z U .
Moreover, let S be the subclass of A whose functions are univalent in U . The Koebe one-quarter theorem ensures that the image of U under every f 𝒮 contains a disk of radius 1 / 4 .
It is known that every function f S has an inverse f 1 defined by
f 1 f z = z ( z U ) ,
and
f 1 f ω = ω ω < r 0 f ; r 0 f 1 4 ,
where
f 1 ω = g ( ω ) = ω υ 2 ω 2 + 2 υ 2 2 υ 3 ω 3 5 υ 2 3 5 υ 2 υ 3 + υ 4 ω 4 + .
A function is said to be bi-univalent in U if both f and f 1 are univalent in U . Let Σ denote the class of bi-univalent functions in U given by (1).
Lewin [1] investigated the class Σ and showed that v 2 < 1.51 . Subsequently, Brannan and Clunie [2] conjectured that v 2 < 2 . Netanyahu [3], on the other hand, showed that
max f Σ v 2 = 4 3 .
The Taylor–Maclaurin coefficients v n n 3 , n N in (1) are still unknown, and it is an open problem.
Similar to the subclasses S * ζ and K ζ of the starlike and convex functions of the order ζ 0 ζ < 1 , respectively, that we are familiar with, Brannan and Taha [4] gave two subclasses of Σ , which are called S Σ * ζ and K Σ ζ of the bi-starlike functions and bi-convex functions of the order ζ 0 ζ < 1 , respectively. It should be remarked here that, in their pioneering work, Srivastava et al. [5] actually revived the study of analytic and bi-univalent functions in recent years.
Moreover, for two analytic functions s 1 and s 2 , the function s 1 is called subordinated to the function s 2 , denoted as
s 1 ( z ) s 2 ( z ) z U ,
if there is an analytic function w in U with
w 0 = 0 and w z < 1 ,
such that
s 1 ( z ) = s 2 ( w ( z ) ) .
If the function s 2 S , then
s 1 ( z ) s 2 ( z ) s 1 ( 0 ) = s 2 ( 0 ) and s 1 ( U ) s 2 ( U ) .
In 2008, Babalola [6] defined the operator I n σ : A A as
I m τ f ( z ) = ( ν τ ν τ , m 1 f ) ( z )
where
ν τ , m ( z ) = z ( 1 z ) τ ( m 1 ) , τ ( m 1 ) > 0 , ν τ = ν τ , 0
and ν τ , m 1 is such that
( ν τ , m ν τ , m 1 ) ( z ) = z 1 z ( τ , m N ) .
Let f A , then (3) is equivalent to
I m τ f ( z ) = z + j = 2 [ τ + j 1 ] ! τ ! [ τ m ] ! [ τ + j m 1 ] ! υ j z j .
The q-derivative operator D q of a function was introduced and researched by Jackson [7,8].
D q f ( z ) = f ( q z ) f ( z ) z ( q 1 ) = z 1 z + k = 2 [ k ] q υ k z k
and D q f ( 0 ) = f ( 0 ) . In particular, f ( z ) = z k for k is a positive integer, the q-derivative of f ( z ) is given by
D q z k = ( z q ) k z k z ( q 1 ) = [ k ] q z k 1 ,
lim q 1 [ k ] q = lim q 1 q k 1 q 1 = k .
For function f ( z ) given by (1) and g ( z ) given by
g ( z ) = z + k = 2 c k z k
the convolution of f ( z ) and g ( z ) is defined by
( f g ) ( z ) = z + k = 2 υ k c k z k = ( g f ) ( z ) .
Let
D q ( z ) = z ( 1 q z ) ( 1 z ) = z + ( 1 + e 1 ) z 2 + ( 1 + e 1 + e 2 ) z 3 + = z + k = 2 [ k ] e z k
where
[ k ] e = 1 + e 1 + e 2 + + e k 1 , e k = q k .
See [9,10] for additional information on q-derivative theories.
Quantum (or q-) calculus is a strong instrument for investigating a wide range of analytic functions, and it has sparked new research in mathematics and other fields. The first time it was used in the context of univalent functions was by Srivastava [11]. Many academics have studied q-calculus and its many applications due to the usefulness of q-analysis in mathematics and other areas. With the help of certain higher-order q-derivative operators, Khan et al. [12] constructed and analyzed a number of subclasses of q-starlike functions. Shi et al. (see also [13]) created a novel subclass of multivalent q-starlike Janowski functions using the q-differential operator. A variety of adequate requirements as well as some other noteworthy characteristics were investigated in both articles [12,14].
Because of the large range of applications and the usefulness of q-operators above fundamental operators, many scholars have looked into q-calculus in depth. Furthermore, Srivastava’s recently published survey-cum-expository review study [15,16,17] is useful for academics and scholars studying these topics.
The q-Hermite polynomial was first introduced by Rogers [18] (see also [19,20]) and is usually defined by means of their generating function as follows
B k ( s | q ) = k = 0 H k x ; q t k q ; q k = k = 0 1 1 2 x t q k + t 2 q 2 k 0 < q < 1 .
The q-derivative of the q-Hermite polynomial is
D q B k + 1 ( s | q ) = [ k ] q B k ( s | q ) .
Moreover, Ismail et al. [18] were able to define the recursion relation as
t B k ( s | q ) = B k + 1 ( s | q ) + [ k ] q B k 1 ( s | q )
with
B 0 ( s | q ) = 1 and B 1 ( s | q ) = 0 .
Also from (11), we have
B 1 ( s | q ) = s B 2 ( s | q ) = s 2 1 B 3 ( s | q ) = s 3 ( 2 + q ) s B 4 ( s | q ) = s 4 ( 3 + 2 q + q 2 ) s 2 + ( 1 + q + q 2 ) .
Remark 1. 
It is clear that
B k ( s | q = 1 ) = B c k ( s )
is the Hermite polynomials. Moreover, when
B k ( s | q = 0 ) = U k ( s / 2 ) ,
we have Chebyshev polynomials of the first kind, and they are defined by the recursion relation,
2 s U k ( s ) = U k 1 ( s ) + U k + 1 ( s )
with
U 0 ( s ) = 1 a n d U 1 ( s ) = 0 .
Next, we define the q-Babalola convolution operator which will be used throughout this paper.
Definition 1. 
Let f A . Denote by I γ , q f ( z ) the q-Babalola convolution operator defined by
I γ , q f ( z ) = ( ν τ , q ν γ , q ( 1 ) f ) ( z )
where
ν γ , q = z ( 1 q z ) γ ( 1 z ) , γ > 1 a n d ν γ , q ( 1 )
is such that
( ν γ , q ν γ , q ( 1 ) ) ( z ) = z 1 z .
Hence,
I γ , q f ( z ) = z + k = 2 [ k ] e σ [ k ] e γ υ k z k = z + k = 2 ( k ] e γ υ k z k .
where
( k ] e γ = 1 + e 1 ( τ ) + e 2 ( τ ) e k 1 ( τ ) 1 + e 1 ( γ ) + e 2 ( γ ) e k 1 ( γ )
and
e k 1 ( τ ) = ( τ + k 2 ) ! ( τ 1 ) ! q k 1 ( k 1 ) ! , e k 1 ( γ ) = ( γ + k 2 ) ! ( γ 1 ) ! q k 1 ( k 1 ) ! .
Remark 2. 
It is easily seen that, upon setting q 1 , the extended Babalola convolution operator I γ , q f ( z ) reduces to the Babalola convolution operator I σ m f ( z ) which was introduced and studied by Babalola [6]. For m = τ = 1 , the extended Babalola convolution operator I γ , q f ( z ) reduces to the q-derivative operator introduced and studied by Jackson [7,8]. Moreover, if m = τ and q 1 , we have the Ruscheweyh’s operator [21].
Consider the univalent normalized functions of the kind (1); the Fekete–Szegö functional | υ 3 φ υ 2 2 | has a long history in geometric function theory. The authors in [22] disproved Paley’s conjecture and Littlewood’s that the coefficients of odd univalent functions are confined by unity in 1933. Since then, the functional has gotten much attention, especially in subclasses of the family of univalent functions. This problem appears to have piqued the interest of scholars in recent years (see, for example, [23,24]).
We know that the q-Hermite polynomials and q-convolution operators still have not been studied with bi-univalent functions. The main goal of this paper is to start looking at the properties of the bi-univalent functions that are connected to q-Hermite polynomials and the q-convolution operator. In this study, the initial coefficient estimates for the Fekete–Szegö problem of analytic and bi-univalent functions are determined using the q-Hermite polynomial expansions and the q-convolution operator.
In Definition 2, we describe a class of convex bi-univalent functions that are defined by the q-convolution operator and linked to the q-Hermite polynomial.
Definition 2. 
Let N ( z , s , q ) be defined as follows:
N ( z , s , q ) = k = 2 B k ( s | q ) z k .
A function f Σ given by (1) is said to be in the class Γ Σ q ( s , γ , τ ) , if the following conditions are satisfied:
1 + z D q 2 ( I γ , q f ( z ) ) D q ( I γ , q f ( z ) ) N ( z , s , q )
and
1 + ω D q 2 ( I γ , q f 1 ( ω ) ) D q ( I γ , q f 1 ( ω ) ) N ( ω , s , q ) .
Where s 1 2 , 1 , 0 < q < 1 , z U , ω U , γ = τ m > 1 .
In Definition 3, we describe a class of starlike bi-univalent functions that are defined by the q-convolution operator and linked to the q-Hermite polynomial.
Definition 3. 
Let N ( z , s , q ) be defined as follows:
N ( z , s , q ) = k = 2 B k ( s | q ) z k .
A function f Σ given by (1) is said to be in the class Π Σ q ( s , γ , τ ) , if the following conditions are satisfied:
z D q ( I γ , q f ( z ) ) I γ , q f ( z ) N ( z , s , q )
and
ω D q ( I γ , q f 1 ( ω ) ) I γ , q f 1 ( ω ) N ( ω , s , q ) .
We must recall the following lemma in order to arrive at our primary conclusions.
As is usually the case, we let P be the family of functions p ( z ) = 1 + p 1 z + p 2 z 2 + . . . regular with positive real part, for z U .
Lemma 1 
([25]). Let φ ( z ) P , then
| p j | 2 j N .

2. Coefficient Estimates for the Class Γ Σ q ( s , γ , τ )

The initial coefficient bounds of the class Γ Σ q ( s , γ , τ ) of bi-univalent functions are investigated in this section.
Theorem 1. 
Let f Γ Σ q ( s , γ , τ ) . Then,
| υ 2 | Ψ 1 ( s , q , γ ) ,
| υ 3 | s 2 [ 2 ] b 2 ( ( 2 ] e γ ) 2 + s 4 [ 2 ] b [ 3 ] b ( 3 ] e γ ,
and
| υ 4 | s 3 ( 2 ( 1 + e 1 ) [ 3 ] e ( 3 ] e γ [ 2 ] e 2 ( ( 2 ] e γ ) 2 ) [ 2 ] e 3 [ 4 ] e ( 4 ] e γ ( ( 2 ] e γ ) 2 s 2 ( 2 e 1 [ 2 ] e ( 2 ] e γ ( 3 ] e γ + 5 [ 4 ] e ( 4 ] e γ ) 2 [ 2 ] e 3 [ 4 ] e ( 2 ] e γ ( 3 ] e γ ( 4 ] e γ + s 3 2 s 2 q s 4 [ 2 ] e [ 4 ] e ( 4 ] e γ
where
Ψ 1 ( s , q , γ ) = s 3 | s 2 ( [ 2 ] e [ 3 ] e ( 3 ] e γ [ 2 ] e 2 ( ( 2 ] e γ ) 2 ) [ 2 ] e 2 ( ( 2 ] e γ ) 2 ( s 2 s 1 ) | .
Proof. 
Let f Σ be given by (1) be in the class Γ Σ q ( s , γ , τ ) . Then,
1 + z D q 2 ( I γ , q f ( z ) ) D q ( I γ , q f ( z ) ) = N ( d ( z ) , s , q )
and
1 + z D q 2 ( I γ , q f 1 ( ω ) ) D q ( I γ , q f 1 ( ω ) ) = N ( ϖ ( ω ) , s , q ) ,
Let ϱ , η P be defined as
ϱ ( z ) = 1 + d ( z ) 1 d ( z ) = 1 + ϱ 1 z + ϱ 2 z 2 + ϱ 3 z 3 + d ( z ) = ϱ ( z ) 1 ϱ ( z ) + 1 , ( z U )
and
η ( ω ) = 1 + ϖ ( ω ) 1 ϖ ( ω ) = 1 + η 1 ω + η 2 ω 2 + η 3 ω 3 + ϖ ( ω ) = η ( ω ) 1 η ( ω ) + 1 , ( ω U ) .
It follows that from (26) and (27) that
d ( z ) = 1 2 ϱ 1 z + ϱ 2 ϱ 1 2 2 z 2 + ϱ 3 ϱ 1 ϱ 2 + ϱ 1 3 4 z 3 +
and
ϖ ( ω ) = 1 2 η 1 ω + η 2 η 1 2 2 ω 2 + η 3 η 1 η 2 + η 1 3 4 ω 3 + .
From (28) and (29), applying N ( z , s , q ) as given in (18), we see that
N ( d ( z ) , s , q ) = 1 + B 1 ( s | q ) 2 ϱ 1 z + B 1 ( s | q ) 2 ϱ 2 ϱ 1 2 2 + B 2 ( s | q ) 4 ϱ 1 2 z 2                           + B 1 ( s | q ) 2 ϱ 3 ϱ 1 ϱ 2 + ϱ 1 3 4 + B 2 ( s | q ) 2 ϱ 1 ϱ 2 ϱ 1 2 2 + B 3 ( s | q ) 8 ϱ 1 3 z 3 +
and
N ( ϖ ( ω ) , s , q ) = 1 + B 1 ( s | q ) 2 η 1 ω + B 1 ( s | q ) 2 η 2 η 1 2 2 + B 2 ( s | q ) 4 η 1 2 ω 2 + B 1 ( s | q ) 2 η 3 η 1 η 2 + η 1 3 4 + B 2 ( s | q ) 2 η 1 η 2 η 1 2 2 + B 3 ( s | q ) 8 η 1 3 ω 3 + .
It follows from (24), (30), and (25), we have
[ 2 ] e ( 2 ] e γ υ 2 = B 1 ( s | q ) 2 ϱ 1 ,
[ 2 ] e [ 3 ] e ( 3 ] e γ υ 3 [ 2 ] e 2 ( ( 2 ] e γ ) 2 υ 2 2 = B 1 ( s | q ) 2 ϱ 2 ϱ 1 2 2 + B 2 ( s | q ) 4 ϱ 1 2 ,
[ 3 ] e [ 4 ] e ( 4 ] e γ υ 4 [ 2 ] e [ 3 ] e ( 2 ] e γ ( 3 ] e γ e 1 υ 2 υ 3 + [ 2 ] e 3 ( ( 2 ] e γ ) 3 υ 2 3 = B 1 ( s | q ) 2 ϱ 3 ϱ 1 ϱ 2 + ϱ 1 3 4 + B 2 ( s | q ) 2 ϱ 1 ϱ 2 ϱ 1 2 2 + B 3 ( s | q ) 8 ϱ 1 3 ,
[ 2 ] e ( 2 ] e γ υ 2 = B 1 ( s | q ) 2 η 1 ,
( 2 [ 2 ] e [ 3 ] e ( 3 ] e γ [ 2 ] e 2 ( ( 2 ] e γ ) 2 ) υ 2 2 [ 2 ] e [ 3 ] e ( 3 ] e γ υ 3 = B 1 ( s | q ) 2 η 2 η 1 2 2 + B 2 ( s | q ) 4 η 1 2 ,
( 2 ( 2 + e 1 ) [ 2 ] e [ 3 ] e ( 2 ] e γ ( 3 ] e γ 5 [ 3 ] e [ 4 ] e ( 4 ] e γ [ 2 ] e 3 ( ( 2 ] e γ ) 2 ) υ 2 3 + ( 5 [ 3 ] e [ 4 ] e ( 4 ] e γ + [ 2 ] e [ 3 ] e ( 2 ] e γ ( 3 ] e γ e 1 ) υ 2 υ 3 [ 3 ] e [ 4 ] e ( 4 ] e γ υ 4 = B 1 ( s | q ) 2 η 3 η 1 η 2 + η 1 3 4 + B 2 ( s | q ) 2 η 1 η 2 η 1 2 2 + B 3 ( s | q ) 8 η 1 3 .
Adding (31) and (34), we have
ϱ 1 = η 1 , ϱ 1 2 = η 1 2 and ϱ 1 3 = η 1 3
and
υ 2 2 = ( B 1 ( s | q ) ) 2 ( ϱ 1 2 + η 1 2 ) 8 [ 2 ] e 2 ( ( 2 ] e γ ) 2 .
Moreover, adding (32) and (35) and applying (37) yields
4 υ 2 2 [ [ 2 ] e [ 3 ] e ( 3 ] e γ [ 2 ] b 2 ( ( 2 ] e γ ) 2 ] = B 1 ( s | q ) ( ϱ 2 + η 2 ) η 1 2 B 1 ( s | q ) B 2 ( s | q ) .
Applying (37) in (38) gives
η 1 2 = 4 [ 2 ] e 2 ( ( 2 ] e γ ) 2 υ 2 2 ( B 1 ( s | q ) ) 2 .
Putting (40) into (39) and with some calculations, we have
| υ 2 | 2 = ( B 1 ( s | q ) ) 3 ( ϱ 2 + η 2 ) 4 [ [ 2 ] e [ 3 ] e ( 3 ] e γ [ 2 ] b 2 ( ( 2 ] e γ ) 2 ] ( B 1 ( s | q ) ) 2 + 4 [ 2 ] e 2 ( ( 2 ] e γ ) 2 ( B 1 ( s | q ) B 2 ( s | q ) ) .
Applying triangular inequality and Lemma 1, we have
| υ 2 | Ψ 1 ( s , q , γ ) .
Subtracting (35) from (32) and with some calculations, we have
υ 3 = υ 2 2 + B 1 ( s | q ) [ ϱ 2 η 2 ] 4 [ 2 ] e [ 3 ] e ( 3 ] e γ
υ 3 = ( B 1 ( s | q ) ) 2 ϱ 1 2 4 [ 2 ] e 2 ( ( 2 ] e γ ) 2 + B 1 ( s | q ) [ ϱ 2 η 2 ] 4 [ 2 ] e [ 3 ] e ( 3 ] e γ .
Applying triangular inequality and Lemma 1, we have
| υ 3 | s 2 [ 2 ] b 2 ( ( 2 ] e γ ) 2 + s 4 [ 2 ] b [ 3 ] b ( 3 ] e γ .
Subtracting (36) from (33), we have
2 [ 2 ] e [ 4 ] e ( 4 ] e γ υ 4 = ( 2 ( 1 + e 1 ) [ 3 ] e ( 3 ] e γ [ 2 ] e 2 ( ( 2 ] e γ ) 2 ) ( B 1 ( s | q ) ) 3 ϱ 1 3 4 [ 2 ] e 2 ( ( 2 ] e γ ) 2 ( 2 e 1 [ 2 ] e ( 2 ] e γ ( 3 ] e γ + 5 [ 4 ] e ( 4 ] e γ ) ( B 1 ( s | q ) ) 2 ϱ 1 ( ϱ 2 η 2 ) 8 [ 2 ] e 2 ( 2 ] e γ ( 3 ] e γ + B 1 ( s | q ) ( ϱ 3 η 3 ) 2 + [ B 2 ( s | q ) B 1 ( s | q ) ] ϱ 1 ( ϱ 2 + η 2 ) 2 + ( B 1 ( s | q ) 2 B 2 ( s | q ) + B 3 ( s | q ) ) ϱ 1 3 4 .
Applying triangular inequality and Lemma 1, we have
| υ 4 | s 3 ( 2 ( 1 + e 1 ) [ 3 ] e ( 3 ] e γ [ 2 ] e 2 ( ( 2 ] e γ ) 2 ) [ 2 ] e 3 [ 4 ] e ( 4 ] e γ ( ( 2 ] e γ ) 2 s 2 ( 2 e 1 [ 2 ] e ( 2 ] e γ ( 3 ] e γ + 5 [ 4 ] e ( 4 ] e γ ) 2 [ 2 ] e 3 [ 4 ] e ( 2 ] e γ ( 3 ] e γ ( 4 ] e γ + s 3 2 s 2 q s 4 [ 2 ] e [ 4 ] e ( 4 ] e γ .
 □

3. Coefficient Estimates for the Class Π Σ q ( s , γ , τ )

The initial coefficient bounds of the class Π Σ q ( s , γ , τ ) of bi-univalent functions are investigated in this section.
Theorem 2. 
Let f Π Σ q ( s , γ , τ ) . Then,
| υ 2 | X 1 ( s , q , γ ) ,
| υ 3 | s 2 e 1 2 ( ( 2 ] e γ ) 2 + s ( e 1 + e 2 ) ( 3 ] e γ ,
and
| υ 4 | s 3 ( ( 2 ] e γ ( 3 ] e γ ( 4 e 1 + 2 e 2 ) 2 ( ( 2 ] e γ ) 3 e 1 10 ( e 1 + e 2 + e 3 ) ( 4 ] e γ ) 2 ( e 1 + e 2 + e 3 ) ( ( 2 ] e γ ) 3 ( 4 ] e γ e 1 3 5 s 2 2 ( 2 ] e γ ( 3 ] e γ e 1 ( e 1 + e 2 ) + s 3 2 s 2 q s 4 ( e 1 + e 2 + e 3 ) ( 4 ] e γ
where
X 1 ( s , q , γ ) = 2 s 3 | s 2 { 2 ( e 1 + e 2 ) ( 3 ] e γ + ( 2 ] e γ ( ( 2 ] e γ ) 2 ( 1 + 2 e 1 ) } 2 ( ( 2 ] e γ ) 2 e 1 2 ( s 2 s 1 ) | .
Proof. 
Let f Σ be given by (1) be in the class Π Σ q ( s , γ , τ ) . Then,
z D q ( I γ , q f ( z ) ) I γ , q f ( z ) = N ( d ( z ) , s , q )
and
ω D q ( I γ , q f 1 ( ω ) ) I γ , q f 1 ( ω ) = N ( ϖ ( ω ) , s , q ) .
Let ϱ , η P be defined by
ϱ ( z ) = 1 + d ( z ) 1 d ( z ) = 1 + ϱ 1 ( z ) + ϱ 2 z 2 + ϱ 3 z 3 + d ( z ) = ϱ ( z ) 1 ϱ ( z ) + 1 , ( z U )
and
η ( ω ) = 1 + ϖ ( ω ) 1 ϖ ( ω ) = 1 + η 1 ( ω ) + η 2 ω 2 + η 3 ω 3 + ϖ ( ω ) = η ( ω ) 1 η ( ω ) + 1 , ( ω U ) .
It follows that from (51) and (52) that
d ( z ) = 1 2 ϱ 1 z + ϱ 2 ϱ 1 2 2 z 2 + ϱ 3 ϱ 1 ϱ 2 + ϱ 1 3 4 z 3 +
and
ϖ ( ω ) = 1 2 η 1 ω + η 2 η 1 2 2 ω 2 + η 3 η 1 η 2 + η 1 3 4 ω 3 + .
From (53) and (54), applying N ( z , s , q ) as given in (18), we see that
N ( d ( z ) , s , q ) = 1 + B 1 ( s | q ) 2 ϱ 1 z + B 1 ( s | q ) 2 ϱ 2 ϱ 1 2 2 + B 2 ( s | q ) 4 ϱ 1 2 z 2                                 + B 1 ( s | q ) 2 ϱ 3 ϱ 1 ϱ 2 + ϱ 1 3 4 + B 2 ( s | q ) 2 ϱ 1 ϱ 2 ϱ 1 2 2 + B 3 ( s | q ) 8 ϱ 1 3 z 3 +
and
N ( ϖ ( ω ) , s , q ) = 1 + B 1 ( s | q ) 2 η 1 ω + B 1 ( s | q ) 2 η 2 η 1 2 2 + B 2 ( s | q ) 4 η 1 2 ω 2 + B 1 ( s | q ) 2 η 3 η 1 η 2 + η 1 3 4 + B 2 ( s | q ) 2 η 1 η 2 η 1 2 2 + B 3 ( s | q ) 8 η 1 3 ω 3 + .
It follows from (49), (55), and (50), we have
( 2 ] e γ e 1 υ 2 = B 1 ( s | q ) 2 ϱ 1 ,
( e 1 + e 2 ) ( 3 ] e γ υ 3 ( ( 2 ] e γ ) 2 e 1 υ 2 2 = B 1 ( s | q ) 2 ϱ 2 ϱ 1 2 2 + B 2 ( s | q ) 4 ϱ 1 2 ,
( e 1 + e 2 + e 3 ) ( 4 ] e γ υ 4 ( 2 e 1 + e 2 ) ( 2 ] e γ ( 3 ] e γ υ 2 υ 3 + e 1 ( ( 2 ] e γ ) 3 υ 2 3 = B 1 ( s | q ) 2 ϱ 3 ϱ 1 ϱ 2 + ϱ 1 3 4 + B 2 ( s | q ) 2 ϱ 1 ϱ 2 ϱ 1 2 2 + B 3 ( s | q ) 8 ϱ 1 3 ,
( 2 ] e γ e 1 υ 2 = B 1 ( s | q ) 2 η 1 ,
2 ( 3 ] e γ ( e 1 + e 2 ) υ 2 2 e 1 ( ( 2 ] e γ ) 2 υ 2 2 ( e 1 + e 2 ) ( 3 ] e γ υ 3 = B 1 ( s | q ) 2 η 2 η 1 2 2 + B 2 ( s | q ) 4 η 1 2 ,
( ( 2 ] e γ ( 3 ] e γ ( 4 e 1 + 2 e 2 ) 5 ( 4 ] e γ ( e 1 + e 2 + e 3 ) ( ( 2 ] e γ ) 2 e 1 ) υ 2 3 ( ( 2 ] e γ ( 3 ] e γ ( 2 e 1 + e 2 ) + 5 ( 4 ] e γ ( e 1 + e 2 + e 3 ) ) υ 2 υ 3 ( 4 ] e γ ( e 1 + e 2 + e 3 ) υ 4 = B 1 ( s | q ) 2 η 3 η 1 η 2 + η 1 3 4 + B 2 ( s | q ) 2 η 1 η 2 η 1 2 2 + B 3 ( s | q ) 8 η 1 3 .
Adding (56) and (59), we have
ϱ 1 = η 1 , ϱ 1 2 = η 1 2 and ϱ 1 3 = η 1 3
and
υ 2 2 = ( B 1 ( s | q ) ) 2 ( ϱ 1 2 + η 1 2 ) 8 ( ( 2 ] e γ ) 2 e 1 2 .
Moreover, adding (57) and (60) and applying (62) yields
2 υ 2 2 { 2 ( e 1 + e 2 ) ( 3 ] e γ + ( 2 ] e γ ( ( 2 ] e γ ) 2 ( 1 + 2 e 1 ) } = B 1 ( s | q ) ( ϱ 2 + η 2 ) η 1 2 B 1 ( s | q ) B 2 ( s | q ) .
Applying (62) in (63) gives
η 1 2 = 4 ( ( 2 ] e γ ) 2 e 1 2 υ 2 2 ( B 1 ( s | q ) ) 2 .
Putting (65) into (64) and with some calculations, we have
| υ 2 | 2 = ( B 1 ( s | q ) ) 3 ( ϱ 2 + η 2 ) 2 [ 2 ( e 1 + e 2 ) ( 3 ] e γ + ( 2 ] e γ ( ( 2 ] e γ ) 2 ( 1 + 2 e 1 ) ] ( B 1 ( s | q ) ) 2 + 4 ( ( 2 ] e γ ) 2 e 1 2 ( B 1 ( s | q ) B 2 ( s | q ) ) .
Applying triangular inequality and Lemma 1, we have
| υ 2 | X 1 ( s , q , γ ) .
Subtracting (60) from (57) and with some calculations, we have
υ 3 = υ 2 2 + B 1 ( s | q ) [ ϱ 2 η 2 ] 4 ( e 1 + e 2 ) ( 3 ] e γ
υ 3 = ( B 1 ( s | q ) ) 2 ϱ 1 2 4 e 1 2 ( ( 2 ] e γ ) 2 + B 1 ( s | q ) [ ϱ 2 η 2 ] 4 ( e 1 + e 2 ) ( 3 ] e γ .
Applying triangular inequality and Lemma 1, we have
| υ 3 | s 2 e 1 2 ( ( 2 ] e γ ) 2 + s ( e 1 + e 2 ) ( 3 ] e γ .
Subtracting (61) from (58), we have
2 ( e 1 + e 2 + e 3 ) ( 4 ] e γ υ 4 = ( 3 ] e γ ( 4 e 1 + 2 e 2 ) ( B 1 ( s | q ) ) 3 ϱ 1 3 8 e 1 2 ( ( 2 ] e γ ) 2 ( B 1 ( s | q ) ) 3 ϱ 1 3 4 e 1 2 5 ( 4 ] e γ ( e 1 + e 2 + e 3 ) ( B 1 ( s | q ) ) 3 ϱ 1 3 4 ( ( 2 ] e γ ) 3 e 1 3 5 ( 4 ] e γ ( e 1 + e 2 + e 3 ) ( B 1 ( s | q ) ) 2 ϱ 1 ( ϱ 2 η 2 ) 8 ( 2 ] e γ ( 3 ] e γ e 1 ( e 1 + e 2 ) + B 1 ( s | q ) ( ϱ 3 η 3 ) 2 + [ B 2 ( s | q ) B 1 ( s | q ) ] ϱ 1 ( ϱ 2 + η 2 ) 2
+ ( B 1 ( s | q ) 2 B 2 ( s | q ) + B 3 ( s | q ) ) ϱ 1 3 4 .
Applying triangular inequality and Lemma 1, we have
| υ 4 | s 3 ( ( 2 ] e γ ( 3 ] e γ ( 4 e 1 + 2 e 2 ) 2 ( ( 2 ] e γ ) 3 e 1 10 ( e 1 + e 2 + e 3 ) ( 4 ] e γ ) 2 ( e 1 + e 2 + e 3 ) ( ( 2 ] e γ ) 3 ( 4 ] e γ e 1 3 5 s 2 2 ( 2 ] e γ ( 3 ] e γ e 1 ( e 1 + e 2 ) + s 3 2 s 2 q s 4 ( e 1 + e 2 + e 3 ) ( 4 ] e γ .
 □

4. Fekete–Szego Inequalities for the Function Class Γ Σ q ( s , γ , τ )

Theorem 3. 
Let f Γ Σ q ( s , γ , τ ) . Then, for some φ R ,
υ 3 φ υ 2 2 2 | 1 φ | Ψ 1 ( s , q , γ ) | 1 φ | s [ 2 ] b [ 3 ] b ( 3 ] e γ Ψ 1 ( s , q , γ ) 2 s [ 2 ] b [ 3 ] b ( 3 ] e γ | 1 φ | s [ 2 ] b [ 3 ] b ( 3 ] e γ Ψ 1 ( s , q , γ ) ,
where
Ψ 1 ( s , q , γ ) = s 3 | s 2 ( [ 2 ] e [ 3 ] e ( 3 ] e γ [ 2 ] e 2 ( ( 2 ] e γ ) 2 ) [ 2 ] e 2 ( ( 2 ] e γ ) 2 ( s 2 s 1 ) | .
Proof. 
From (42), we have
υ 3 φ υ 2 2 = υ 2 2 + B 1 ( s | q ) [ ϱ 2 η 2 ] 4 [ 2 ] e [ 3 ] e ( 3 ] e γ φ υ 2 2 .
By triangular inequality, we have
| υ 3 φ υ 2 2 | s [ 2 ] e [ 3 ] e ( 3 ] e γ + | 1 φ | Ψ 1 ( s , q , γ ) .
Suppose
| 1 φ | Ψ 1 ( s , q , γ ) s [ 2 ] e [ 3 ] e ( 3 ] e γ
then we have
| υ 3 φ υ 2 2 | 2 | 1 φ | Ψ 1 ( s , q , γ )
where
| 1 φ | s [ 2 ] e [ 3 ] e ( 3 ] e γ Ψ 1 ( s , q , γ )
and suppose
| 1 φ | Ψ 1 ( s , q , γ ) s [ 2 ] e [ 3 ] e ( 3 ] e γ
then we have
| υ 3 δ υ 2 2 | 2 s [ 2 ] e [ 3 ] e ( 3 ] e γ
where
| 1 φ | s [ 2 ] e [ 3 ] e ( 3 ] e γ Ψ 1 ( s , q , γ )
and Ψ 1 ( s , q , γ ) is given in (72). □

5. Fekete–Szego Inequalities for the Function Class Π Σ q ( s , γ , τ )

Theorem 4. 
Let f Π Σ q ( s , γ , τ ) . Then, for some φ R ,
υ 3 φ υ 2 2 2 | 1 φ | X 1 ( s , q , γ ) | 1 φ | s ( e 1 + e 2 ) ( 3 ] e γ X 1 ( s , q , γ ) 2 s ( e 1 + e 2 ) ( 3 ] e γ | 1 φ | s ( e 1 + e 2 ) ( 3 ] e γ X 1 ( s , q , γ ) ,
where
X 1 ( s , q , γ ) = 2 s 3 | s 2 { 2 ( e 1 + e 2 ) ( 3 ] e γ + ( 2 ] e γ ( ( 2 ] e γ ) 2 ( 1 + 2 e 1 ) } 2 ( ( 2 ] e γ ) 2 e 1 2 ( s 2 s 1 ) | .
Proof. 
From (67), we have
υ 3 φ υ 2 2 = υ 2 2 + B 1 ( s | q ) [ ϱ 2 η 2 ] 4 ( e 1 + e 2 ) ( 3 ] e γ φ υ 2 2 .
By triangular inequality, we have
| υ 3 φ υ 2 2 | s ( e 1 + e 2 ) ( 3 ] e γ + | 1 φ | X 1 ( s , q , γ ) .
Suppose
| 1 φ | X 1 ( s , q , γ ) s ( e 1 + e 2 ) ( 3 ] e γ
then we have
| υ 3 φ υ 2 2 | 2 | 1 φ | X 1 ( s , q , γ )
where
| 1 φ | s ( e 1 + e 2 ) ( 3 ] e γ X 1 ( s , q , γ )
and suppose
| 1 φ | Ψ 1 ( s , q , γ ) s ( e 1 + e 2 ) ( 3 ] e γ
then we have
| υ 3 δ υ 2 2 | 2 s ( e 1 + e 2 ) ( 3 ] e γ
where
| 1 φ | s ( e 1 + e 2 ) ( 3 ] e γ X 1 ( s , q , γ )
and X 1 ( s , q , γ ) is given in (75). □

6. Conclusions

As we mentioned earlier, q-calculus is a vital tool for understanding a large class of analytic functions and its applications. Several useful results related to the q-version of the starlike function and the q-derivative, bi-univalent functions, for instance, were provided in [26,27,28,29,30,31]. In recent decades, the orthogonal polynomials and special functions have played an essential role in mathematics, physics, engineering, and other research disciplines. In our current analysis, we used q-Hermite polynomials and q-convolution operators and systematically defined two new subclasses of bi-univalent functions, which was primarily prompted by the recent research cited in this paper. We then obtained several significant findings, such as bonds for the initial coefficients of υ 2 , υ 3 , and υ 4 of the Taylor–Maclaurin series and the Fekete–Szegö functional results for our established function classes.
Moreover, to have more new theorems under the present examinations, new generalizations and applications can be explored with some positive and novel outcomes in various fields of science, mainly in geometric function theory. These recent surveys will be presented in the future research work being processed by the authors of the present paper.
However, the purported trivial ( p , q )-calculus extension was clearly demonstrated to be a relatively insignificant variation of the classical q-calculus, the extra parameter p being redundant or superfluous (see, for details, [17], p. 340, and [32], pp. 1511–1512). This observation by Srivastava (see [17,32]) will indeed also apply to any future attempt to produce the rather straightforward ( p , q ) -variants of the results which we have presented in this paper.

Author Contributions

Conceptualization, I.A.-S.; Formal analysis, A.C.; Investigation, I.A.-S.; Resources, H.M.S. and N.A.; Data curation, H.M.S.; Writing—original draft, A.C.; Writing—review & editing, N.A. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Acknowledgments

The last author thanks the Deanship of Scientific Research at Qassim University for supporting her work.

Conflicts of Interest

The authors declare no conflict of interest.

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Al-Shbeil, I.; Cătaş, A.; Srivastava, H.M.; Aloraini, N. Coefficient Estimates of New Families of Analytic Functions Associated with q-Hermite Polynomials. Axioms 2023, 12, 52. https://doi.org/10.3390/axioms12010052

AMA Style

Al-Shbeil I, Cătaş A, Srivastava HM, Aloraini N. Coefficient Estimates of New Families of Analytic Functions Associated with q-Hermite Polynomials. Axioms. 2023; 12(1):52. https://doi.org/10.3390/axioms12010052

Chicago/Turabian Style

Al-Shbeil, Isra, Adriana Cătaş, Hari Mohan Srivastava, and Najla Aloraini. 2023. "Coefficient Estimates of New Families of Analytic Functions Associated with q-Hermite Polynomials" Axioms 12, no. 1: 52. https://doi.org/10.3390/axioms12010052

APA Style

Al-Shbeil, I., Cătaş, A., Srivastava, H. M., & Aloraini, N. (2023). Coefficient Estimates of New Families of Analytic Functions Associated with q-Hermite Polynomials. Axioms, 12(1), 52. https://doi.org/10.3390/axioms12010052

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