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Article

Two Families of Bi-Univalent Functions Associating the (p, q)-Derivative with Generalized Bivariate Fibonacci Polynomials

by
Sondekola Rudra Swamy
1,†,
Basem Aref Frasin
2,†,
Daniel Breaz
3,*,† and
Luminita-Ioana Cotîrlă
4,*,†
1
Department of Infomation Science and Engineering, Acharya Institute of Technology, Bengaluru 560 107, Karnataka, India
2
Department of Mathematics, Faculty of Science, Al al-Bayt University, Mafraq, Jordan
3
Department of Computing, Mathematics and Electronics, “1 Decembrie 1918” University of Alba Iulia, 510009 Alba Iulia, Romania
4
Department of Mathematics, Tehnical University of Cluj-Napoca, 400114 Cluj-Napoca, Romania
*
Authors to whom correspondence should be addressed.
These authors contributed equally to this work.
Mathematics 2024, 12(24), 3933; https://doi.org/10.3390/math12243933
Submission received: 20 October 2024 / Revised: 8 December 2024 / Accepted: 10 December 2024 / Published: 13 December 2024

Abstract

:
Making use of generalized bivariate Fibonacci polynomials, we propose two families of regular functions of the type ϕ ( ζ ) = ζ + j = 2 d j ζ j , which are bi-univalent in the disc { ζ C : | ζ | < 1 } involving the (p, q)-derivative operator. We find estimates on the coefficients | d 2 | , | d 3 | and the of Fekete–Szegö functional for members of these families. Relevant connections to the existing results and new consequences of the main result are presented.

1. Preliminaries

The q-analysis is a generalization of the ordinary analysis that does not employ limit notation. Jackson presented the use and application of the q-calculus in [1]. The q-analogue of the derivative and integral operator were first defined in [2], along with some of their applications. The multifaceted uses of the q-derivative operator make it extremely important in the study of geometric function theory. Initially, Ismail et al. proposed the concept of q-extension of the class of q-starlike functions in [3]. Later, a number of mathematicians studied q-calculus in the context of geometric functions theory: the Ruscheweyh differential operator’s q-analogue was first presented in [4]; some applications for multivalent functions were examined in [5,6]; q-starlike functions associated with the generalized conic domain, by applying the convolution concept was investigated in [7]; an operator associated with q-hypergeometric function was investigated in [8], and so forth. Numerous authors have recently released a number of articles that examine a class of q-starlike functions from different perspectives (see [9,10,11,12,13,14]).
An extension of the q-calculus to the (p, q)-calculus, was taken into consideration by the researchers. The (p, q)-number, was first examined around the same time (1991) and subsequently on its own by [15,16,17,18]. Fibonacci oscillators were studied with the presentation of the (p, q)-number in [15]. The investigation of the (p, q)-number in [16] allows for the construction of a (p, q)-Harmonic oscillator. The (p, q)-number was investigated in [17] as a means of combining different types of q-oscillator algebras and in [18], the (p, q)-number was examined in order to determine the (p, q)-Stirling numbers.
Building on the aforementioned publications, since 1991, a large number of scientists have investigated (p, q)-calculus in a range of research domains. The results in [19] provided a syntax for embedding the q-series into a (p, q)-series. They also investigated (p, q)-hypergeometric series and found some results corresponding to (p, q)-extensions of the known q-identities. The q-identities are extended correspondingly to yield the (p, q)-series (see, e.g., [20]). We provide some basic definitions of the (p, q)-calculus concepts used in this paper. The (p, q)-bracket number is given by [ j ] p , q = p j 1 + p j 2 q + p j 3 q 2 + + p q j 2 + q j 1 = p j q j p q ( p q ) , which is an extension of q-number (see [2]), that is [ j ] q = 1 q j 1 q ( q 1 ) . Note that [ j ] p , q is symmetric and if p = 1, then [ j ] p , q = [ j ] q .
Let { ζ C : | ζ | < 1 } = D be the open unit disk, and C be the complex plane. Let N represent the natural number set and R be the real number set.
Definition 1 
([21]). Let φ be a function defined on C and 0 < q < p 1 . Then, the (p, q)-derivative of φ is defined by
D p , q φ ( ζ ) = φ ( p ζ ) φ ( q ζ ) ( p q ) ζ ( ζ 0 ) ,
and D p , q φ ( 0 ) = φ ( 0 ) , provided φ ( 0 ) exists.
We note that D p , q ζ j = [ j ] p , q ζ j 1 , D p , q ln ( ζ ) = ln ( p / q ) ( p q ) ζ and [ j ] p , q j , if p = 1 and q 1 . Therefore, D p , q φ ( ζ ) φ ( ζ ) as p = 1 and q 1 . For any constants δ and κ , it is obvious that D p , q ( δ φ 1 ( ζ ) + κ φ 2 ( ζ ) ) = δ D p , q φ 1 ( ζ ) + κ D p , q φ 2 ( ζ ) . The product rules and quotient rules are satisfied by the (p, q)-derivative (see [22]). The exponential functions are used to define the (p, q)-analogues of many functions, including sine, cosine, and tangent, in the same way as their well-known Euler expressions. Duran et al. [23] examined the (p, q)-derivatives of these functions.
The set of functions ϕ , which are regular in D and have the following form, is represented by A :
ϕ ( ζ ) = ζ + j = 2 d j ζ j , ( ζ D ) ,
with ϕ ( 0 ) = 0 = ϕ ( 0 ) 1 , and we denote a sub-set of A containing univalent functions in D by S . If ϕ A is of the form (1), then
D p , q ϕ ( ζ ) = 1 + j = 2 [ j ] p , q d j ζ j 1 , ( ζ D ) .
The Koebe theorem (see [24]) states that the inverse of each function ϕ in S is given by
ϕ 1 ( ϖ ) = ψ ( ϖ ) = ϖ d 2 ϖ 2 + ( 2 d 2 2 d 3 ) ϖ 3 ( 5 d 2 3 5 d 2 d 3 + d 4 ) ϖ 4 + .
satisfying ζ = ϕ 1 ( ϕ ( ζ ) ) and ϖ = ϕ ( ϕ 1 ( ϖ ) ) , | ϖ | < r 0 ( ϕ ) , r 0 ( ϕ ) 1 / 4 , ζ , ϖ D . In D , a member ϕ of A given by (1) is called bi-univalent if ϕ S and ϕ 1 S . The set of such functions in D is represented by σ . 1 2 log 1 + ζ 1 ζ , log ( 1 ζ ) , and ζ 1 ζ are some of the functions in the σ family. Nevertheless, despite being in S , ζ ζ 2 2 , ζ 1 ζ 2 , and the Koebe function does not belong to σ . For a concise analysis and to discover some of the remarkable characteristics of the family σ , see [25,26,27,28] and the citation provided in these papers. Srivastava et al. [29] introduced several subclasses of the family σ , which are similar to the well-known subclasses of the family S . As follow-ups, numerous authors have since examined a number of different subfamilies of σ (see, for instance, [30,31,32,33,34]).
Several subclasses of the class σ were studied using the (p, q)-calculus. In [35], the (p, q)-derivative operator and the subordination principle were used to introduce the new generalized classes of (p, q)-starlike and (p, q)-convex functions. The Fekete-Szegö inequalities are also examined and the (p, q)-Bernardi integral operator for analytic functions is defined. The (p, q)-Bernardi integral operator was used to obtain some applications of the main results. Several studies have also introduced and investigated novel subclasses of the class σ related to the (p, q)-differential operator (see [36,37,38,39,40,41]).
Let k ( ϰ , y ) and l ( ϰ , y ) be polynomials with real coefficients. For, j 2 , the generalized bivariate Fibonacci polynomials (GBFP) are defined by the recurrence relation:
F j ( ϰ , y ) = k ( ϰ , y ) F j 1 ( ϰ , y ) + l ( ϰ , y ) F j 2 ( ϰ , y ) ,
where F 0 ( ϰ , y ) = 0 , F 1 ( ϰ , y ) = 1 and k 2 ( ϰ , y ) + 4 l ( ϰ , y ) > 0 . The generating function of GBFP is (see [42])
F ( ϰ , y , ζ ) = j = 0 F j ( ϰ , y ) ζ j = ζ 1 k ( ϰ , y ) ζ l ( ϰ , y ) ζ 2 .
For specific selections of k ( ϰ , y ) and l ( ϰ , y ) , GBFP leads to various known polynomials (see [43]). Readers with an interest in GBFP can find a brief history and extensive information in [44] and its references. Interesting findings regarding coefficient estimates and Fekete–Szegö functional have been presented in [45,46,47] for members of certain subclasses of σ associated with GBFP.
For brevity, we write hereafter that k ( ϰ , y ) = k and l ( ϰ , y ) = l . F 2 ( ϰ , y ) = k and F 3 ( ϰ , y ) = k 2 + l are evident from (4).
Remark 1. 
By specializing k and l, many polynomial sequences can be inferred from GBFP. They are as follows: (i) the bivariate Fibonacci polynmials are obtained if k = ϰ and l = y ; (ii) the Pell polynomials are achieved if k = 2 ϰ and l = 1 ; (iii) we derive the Jacobsthal polynomials if k = 1 and l = ϰ ; and (iv) we arrive at the Fermat polynomials, if k = 3 ϰ and l = 2 , and so forth.
For Ω 1 , Ω 2 A holomorphic in D , Ω 1 is subordinate to Ω 2 , if there is h ( ζ ) a Schwarz function that is holomorphic in D with h ( 0 ) = 0 and | h ( ζ ) | < 1 , such that Ω 1 ( ζ ) = Ω 2 ( h ( ζ ) ) . The notation Ω 1 Ω 2 or Ω 1 ( ζ ) Ω 2 ( ζ ) ( ζ D ) denotes this subordination. Specifically, when Ω 2 S , we have
Ω 1 ( ζ ) Ω 2 ( ζ ) Ω 1 ( 0 ) = Ω 2 ( 0 ) a n d Ω 1 ( D ) Ω 2 ( D ) .
We present two new families of σ subordinate to GBFP F j ( ϰ , y ) as in (4), with the generating function F ( ϰ , y , z ) as in (5). These families are motivated by the aforementioned trends on coefficient-related problems and the Fekete–Szegö functional [48] on certain subclasses of σ linked to GBFP. F ( ϰ , y , z ) is as in (5), ϕ 1 ( ϖ ) = ψ ( ϖ ) , an inverse function as in (3), ϰ R , ζ D , and ϖ D are assumed throughout this paper, unless otherwise mentioned.
Definition 2. 
A function ϕ given by (1), which is said to be in the set Y σ , p , q λ , η ( γ , F ) , γ 1 , 0 < η 1 a n d λ 1 , if
1 2 γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) + γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) 1 η F ( ζ )
= F ( ϰ , y , ζ ) ζ ,
and
1 2 γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) + γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) 1 η F ( ϖ )
= F ( ϰ , y , ϖ ) ϖ ,
where
F ( ζ ) = 1 1 k ζ l ζ 2 , k 0 , a n d k 2 + 4 l > 0 .
For specific choices of p , q , γ and λ , the family Y σ , p , q λ , η ( γ , F ) includes many new and existing subfamilies of σ . This is shown below:
1. let λ = 1 . Then H σ , p , q η ( γ , F ) Y σ , p , q 1 , η ( γ , F ) , γ 1 , 0 < η 1 is the collection of members ϕ of σ that satisfy
1 2 γ D p , q ( ζ D p , q ϕ ( ζ ) ) + ( 1 γ ) D p , q ϕ ( ζ ) + γ D p , q ( ζ D p , q ϕ ( ζ ) ) + ( 1 γ ) D p , q ϕ ( ζ ) 1 η F ( ζ )
= F ( ϰ , y , ζ ) ζ ,
and
1 2 γ D p , q ( ϖ D p , q ψ ( ϖ ) ) + ( 1 γ ) D p , q ψ ( ϖ ) + γ D p , q ( ϖ D p , q ψ ( ϖ ) ) + ( 1 γ ) D p , q ψ ( ϖ ) 1 δ F ( ϖ )
= F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
2. Assume that γ = 1 . Then I σ , p , q λ , η ( F ) Y σ , p , q λ , η ( 1 , F ) , 0 < η 1 and λ 1 , is the collection of elements ϕ of σ that satisfy
1 2 [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ D p , q ϕ ( ζ ) + [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ D p , q ϕ ( ζ ) 1 η F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
and
1 2 [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ D p , q ψ ( ϖ ) + [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ D p , q ψ ( ϖ ) 1 η F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
3. If p = 1 and q 1 in the class Y σ , p , q λ , η ( γ , F ) , then we obtain a subset Υ σ λ , η ( γ , F ) ( λ 1 , 0 < η 1 , γ 1 ) which is the collection of members ϕ of σ that satisfy
1 2 γ [ ( ζ ϕ ( ζ ) ) ] λ + ( 1 γ ) ϕ ( ζ ) + γ [ ( ζ ϕ ( ζ ) ) ] λ + ( 1 γ ) ϕ ( ζ ) 1 η F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
and
1 2 γ [ ( ϖ ψ ( ϖ ) ) ] λ + ( 1 γ ) ψ ( ϖ ) + γ [ ( ϖ ψ ( ϖ ) ) ] λ + ( 1 γ ) ψ ( ϖ ) 1 η F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
4. Let η = 1 . Then Z σ , p , q λ ( γ , F ) Y σ , p , q λ , 1 ( γ , F ) , γ 1 a n d λ 1 is the set of elements ϕ of σ that satisfy
γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
and
γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
Remark 2. 
(i). H σ , p , q η ( 1 , F ) I σ , p , q 1 , η ( F ) , (ii). H σ , p , q 1 ( γ , F ) Z σ , p , q 1 ( γ , F ) , and (iii). Z σ , p , q λ ( 1 , F ) I σ , p , q λ , 1 ( F ) .
Definition 3. 
A function ϕ given by (1) is said to a member of the set T σ , p , q λ , η ( ν , F ) , 0 ν 1 , 0 < η 1   a n d   λ 1 , if
1 2 ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ + ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ 1 η F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
and
1 2 ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ + ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ 1 η F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
The family T σ , p , q λ , η ( ν , F ) contains numerous new and existing subfamilies of σ for specific choices of ν and λ , as shown below:
  • Let ν = 0 . Then, C σ , p , q λ , η ( F ) T σ , p , q λ , η ( 0 , F ) , 0 < η 1 a n d λ 1 , is the collection of elements ϕ of σ that satisfy
    1 2 ( D p , q ϕ ( ζ ) ) λ + ( D p , q ϕ ( ζ ) ) λ η F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
    and
    1 2 ( D p , q ψ ( ϖ ) ) λ + ( D p , q ψ ( ϖ ) ) λ η F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
    where F ( ζ ) is as mentioned in (6).
  • Let ν = 1 . Then, D σ , p , q λ , η ( F ) T Σ , p , q λ , η ( 1 , F ) , 0 < η 1 a n d λ 1 , is the family of members ϕ of σ that satisfy
    1 2 ζ ( D p , q ϕ ( ζ ) ) λ ϕ ( ζ ) + ζ ( D p , q ϕ ( ζ ) ) λ ϕ ( ζ ) 1 η F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
    and
    1 2 ϖ ( D p , q ψ ( ϖ ) ) λ f ( ϖ ) + ϖ ( D p , q ψ ( ϖ ) ) λ f ( ϖ ) 1 η F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
    where F ( ζ ) is as mentioned in (6).
  • If p = 1 and q 1 in the class T σ , p , q λ , η ( ν , F ) , then we get a subclass Γ σ λ , η ( ν , F ) ( λ 1 , 0 < η 1 , 0 ν 1 ) of functions ϕ σ satisfying
    1 2 ζ ( ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ + ζ ( ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ 1 η F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
    and
    1 2 ϖ ( ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ + ϖ ( ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ 1 η F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
    where F ( ζ ) is as mentioned in (6).
  • Suppose η = 1 . Then, O σ , p , q λ ( ν , F ) T σ , p , q λ , 1 ( ν , F ) , 0 ν 1 a n d λ 1 , is the set of functions ϕ σ that satisfy
    ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ F ( ζ ) = F ( ϰ , y , ζ ) ζ , a n d ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
    where F ( ζ ) is as mentioned in (6).
Remark 3. 
( i ) . D σ , p , q λ , 1 ( F ) O σ , p , q λ ( 1 , F ) , a n d (ii). Γ σ λ , 1 ( ν , F ) O σ , p = 1 , q 1 λ ( ν , F ) .
Estimates for bounds on | d 2 | , | d 3 | , and | d 3 μ d 2 2 | , μ R for functions in the class Y σ , p , q λ , η ( γ , F ) are found in Section 2. The upper bounds for | d 2 | , | d 3 | , and | d 3 μ d 2 2 | , μ R for functions in the class T σ , p , q λ , η ( ν , F ) are derived in Section 3. Along with pertinent connections to the published research, interesting results are also presented.

2. Results for the Class Y σ , p , q λ , η ( γ , F )

First, for ϕ Y σ , p , q λ , η ( ν , F ) , the class as defined in Definition 2, we find the coefficient estimates.
Theorem 1. 
Let γ 1 , 0 < η 1 , a n d λ 1 . If ϕ Y σ , p , q λ , η ( γ , F ) , then
| d 2 |
2 η | k | | k | | ( 2 η ( η + 1 ) ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) + ( 1 η ) R 2 [ 2 ] p , q 2 ) k 2 ( η + 1 ) 2 R 2 [ 2 ] p , q 2 ( k 2 + l ) | ,
| d 3 | 4 η 2 k 2 ( η + 1 ) 2 R 2 [ 2 ] p , q 2 + 2 η | k | ( η + 1 ) P [ 3 ] p , q ,
and for μ R
| d 3 μ d 2 2 | 2 η | k | ( η + 1 ) P [ 3 ] p , q ; | 1 μ | J 4 η 2 | k | 3 | 1 μ | | ( 2 η ( η + 1 ) ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) + ( 1 η ) 2 R 2 [ 2 ] p , q 2 ) k 2 ( η + 1 ) 2 R 2 [ 2 ] p , q 2 ( k 2 + l ) | ; | 1 μ | J ,
where
J = ( 2 η ( η + 1 ) ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) + ( 1 η ) R 2 [ 2 ] p , q 2 ) k 2 ( η + 1 ) 2 R 2 [ 2 ] 2 ( k 2 + l ) 2 η ( 1 + η ) P [ 3 ] p , q k 2 ,
P = γ λ [ 3 ] p , q 1 ,
Q = 1 γ λ [ 2 ] p , q + γ λ ( λ 1 ) 2 [ 2 ] p , q 2 ,
and
R = γ λ [ 2 ] p , q 1 .
Proof. 
Let ϕ Y σ , p , q λ , η ( γ , ϰ ) . Then, due to Definition 2, we obtain
1 2 γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) + γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) 1 η = F ( m ( ζ ) )
and
1 2 γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) + γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) 1 η = F ( n ( ϖ ) )
where
m ( ζ ) = m 1 ζ + m 2 ζ 2 + m 3 ζ 3 + a n d n ( ϖ ) = n 1 ϖ + n 2 ϖ 2 + n 3 ϖ 3 + ,
are some holomorphic functions with | m ( ζ ) | < 1 , | n ( ϖ ) | < 1 , ζ , ϖ D and m ( 0 ) = 0 = n ( 0 ) . It is known that
| m i | 1 , a n d | n i | 1 , ( i N ) .
From (14)–(16), it follows that
1 2 γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) + γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) 1 η = 1 + F 2 ( ϰ , y ) m ( ζ ) + F 3 ( ϰ , y ) m 2 ( ζ ) + ,
and
1 2 γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) + γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) 1 η = 1 + F 2 ( ϰ , y ) n ( ϖ ) + F 3 ( ϰ , y ) n 2 ( ϖ ) + .
In light of (4), Equations (18) and (19) can be expressed as follows.
1 2 γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) + γ [ D p , q ( ζ D p , q ϕ ( ζ ) ) ] λ + ( 1 γ ) D p , q ϕ ( ζ ) 1 η = 1 + F 2 ( ϰ , y ) m 1 ζ + [ F 2 ( ϰ , y ) m 2 + F 3 ( ϰ , y ) m 1 2 ] ζ 2 + ,
and
1 2 γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) + γ [ D p , q ( ϖ D p , q ψ ( ϖ ) ) ] λ + ( 1 γ ) D p , q ψ ( ϖ ) 1 η = 1 + F 2 ( ϰ , y ) n 1 ϖ + [ F 2 ( ϰ , y ) n 2 + F 3 ( ϰ , y ) n 1 2 ] ϖ 2 + .
Comparing (20) and (21), we have
( η + 1 ) R [ 2 ] p , q 2 η d 2 = F 2 ( ϰ , y ) m 1 ,
η + 1 2 η P [ 3 ] p , q d 3 + Q [ 2 ] p , q 2 d 2 2 + 1 η 4 η 2 R 2 [ 2 ] p , q 2 d 2 2 = F 2 ( ϰ , y ) m 2 + F 3 ( ϰ , y ) m 1 2 ,
( η + 1 ) R [ 2 ] p , q 2 η d 2 = F 2 ( ϰ , y ) n 1 ,
and
η + 1 2 η P [ 3 ] p , q ( 2 d 2 2 d 3 ) + Q [ 2 ] p , q 2 d 2 2 + 1 η 4 η 2 R 2 [ 2 ] p , q 2 d 2 2 = F 2 ( ϰ , y ) n 2 + F 3 ( ϰ , y ) n 1 2 ,
where P, Q, and R are as mentioned in (11), (12) and (13), respectively. From (22) and (24), we easily obtain
m 1 = n 1
and also
( η + 1 ) 2 R 2 [ 2 ] p , q 2 2 η 2 d 2 2 = ( m 1 2 + n 1 2 ) F 2 2 ( ϰ , y ) .
By adding (23) and (25), we obtain
η + 1 η ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) + 1 η 2 η 2 R 2 [ 2 ] p , q 2 d 2 2 = F 2 ( ϰ , y ) ( m 2 + n 2 ) + F 3 ( ϰ , y ) ( m 1 2 + n 1 2 ) .
The value of m 1 2 + n 1 2 from (27) is substituted in (28), yielding
d 2 2 = 2 η 2 F 2 3 ( ϰ , y ) ( m 2 + n 2 ) ( 2 η ( η + 1 ) ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) + ( 1 η ) R 2 [ 2 ] p , q 2 ) F 2 2 ( ϰ , y ) ( η + 1 ) 2 R 2 [ 2 ] p , q 2 F 3 ( ϰ , y ) .
Applying (17) to the coefficients m 2 and n 2 yields (7).
We deduct (25) from (23) to get the bound on | d 3 | :
d 3 = d 2 2 + F 2 ( ϰ , y ) ( m 2 n 2 ) η + 1 η P [ 3 ] p , q .
Then in view of (26) and (27), (30) becomes
d 3 = 2 η 2 F 2 2 ( ϰ , y ) ( m 1 2 + n 1 2 ) ( η + 1 ) 2 R 2 [ 2 ] p , q 2 + η F 2 ( ϰ , y ) ( m 2 n 2 ) ( η + 1 ) P [ 3 ] p , q ,
and applying (17) for the coefficients m 1 , m 2 , n 1 and n 2 we obtain (8).
From (29) and (30), for μ R , we obtain
| d 3 μ d 2 2 | = | F 2 ( ϰ , y ) | B ( μ ) + η ( η + 1 ) P [ 3 ] p , q m 2 + B ( μ ) η ( η + 1 ) P [ 3 ] p , q n 2 ,
where
B ( μ ) = 2 η 2 ( 1 μ ) F 2 2 ( ϰ , y ) ( 2 η ( η + 1 ) ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) + ( 1 η ) R 2 [ 2 ] p , q 2 ) F 2 2 ( ϰ , y ) ( η + 1 ) 2 R 2 [ 2 ] p , q 2 F 3 ( ϰ , y ) .
Clearly
| d 3 μ d 2 2 | 2 η | F 2 ( ϰ , y ) | ( η + 1 ) P [ 3 ] p , q ; 0 | B ( μ ) | η ( η + 1 ) P [ 3 ] p , q 2 | F 2 ( ϰ , y ) | | B ( μ ) | ; | B ( μ ) | η ( η + 1 ) P [ 3 ] p , q ,
which results in (9) and J as in (10). □
Corollary 1. 
Let λ = 1 in the above theorem. Then, for any function ϕ H σ , p , q η ( γ , F ) the upper bounds of | d 2 | , | d 3 | , and | d 3 μ d 2 2 | , μ , are given by (7), (8), and (9), respectively, with P = P 1 = γ [ 3 ] p , q 1 , Q = Q 1 = 1 γ [ 2 ] p , q a n d R = R 1 = Q 1 in (11), (12), and (13), respectively. P 1 , Q 1 , a n d R 1 are to be used in place of P , Q , a n d R for J in (10).
Corollary 2. 
Let γ = 1 in the above theorem. Then, for any function ϕ I σ , p , q λ , η ( ϰ ) the upper bounds of | d 2 | , | d 3 | , and | d 3 μ d 2 2 | , μ , are given by (7), (8), and (9), respectively, where P = P 2 = λ [ 3 ] p , q 1 , Q = Q 2 = 1 λ [ 2 ] p , q + λ ( λ 1 ) 2 [ 2 ] p , q 2 , a n d R = R 2 = λ [ 2 ] p , q 1 . P 2 , Q 2 , a n d R 2 are to be used in place of P , Q , and R for J in (10).
From Theorem 1, taking p = 1 and q 1 , we obtain
Corollary 3. 
Let γ 1 , 0 < η 1 , a n d λ 1 . If ϕ Υ σ λ , η ( γ , F ) , then
| d 2 |
η | k | 2 | k | | ( η ( η + 1 ) ( 8 γ λ 2 7 γ λ + 1 ) + 2 ( 1 η ) ( 2 γ λ 1 ) 2 ) k 2 2 ( η + 1 ) 2 ( 2 γ λ 1 ) 2 ( k 2 + l ) | ,
| d 3 | η k ( η + 1 ) ( 2 γ λ 1 ) 2 + 2 η | k | 3 ( η + 1 ) ( 3 γ λ 1 ) ,
and for μ R
| d 3 μ d 2 2 | 2 η | k | 3 ( η + 1 ) ( 3 γ λ 1 ) ; | 1 μ | J 1 2 η 2 | k | 3 | 1 μ | | ( η ( η + 1 ) ( 8 γ λ 2 7 γ λ + 1 ) + 2 ( 1 η ) ( 2 γ λ 1 ) 2 ) k 2 2 ( η + 1 ) 2 ( 2 γ λ 1 ) 2 ( k 2 + l ) | ; | 1 μ | J 1 ,
where
J 1 =
( η ( η + 1 ) ( 8 γ λ 2 7 γ λ + 1 ) + 2 ( 1 η ) ( 2 γ λ 1 ) 2 ) k 2 2 ( η + 1 ) 2 ( 2 γ λ 1 ) 2 ( k 2 + l ) η ( η + 1 ) ( 3 γ λ 1 ) k 2 ,
Here are a few examples of the above corollary’s special cases.
Example 1. 
Letting η = 1 in the class Υ σ λ , η ( γ , F ) , we obtain a subclass χ σ λ ( γ , F ) Υ σ λ , 1 ( γ , F ) of functions ϕ σ satisfying
γ [ ( ζ ϕ ( ζ ) ) ] λ + ( 1 γ ) ϕ ( ζ ) F ( ζ ) = F ( ϰ , y , ζ ) ζ
and
γ [ ( ϖ ψ ( ϖ ) ) ] λ + ( 1 γ ) ψ ( ϖ ) F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
The class χ σ λ ( γ , F ) is not an empty set, which is an important point to note. Consider the following example, where γ = λ = 1 , k = 1 a n d l = 0 . The function u ( ζ ) = ζ + ζ 2 6 + ζ 3 27 + = 3 log ( 1 ζ 3 ) S is in the class χ σ 1 ( 1 , F ) . Because, its inverse v ( ϖ ) = ϖ ϖ 2 6 + ϖ 3 54 = 3 ( e ϖ 3 1 ) e ϖ 3 S . So, we obtain that u ( ζ ) σ (see [46]).
Corollary 4. 
Let γ 1 , a n d λ 1 . If ϕ χ σ λ ( γ , F ) , then
| d 2 | | k | | k | | ( 8 γ λ 2 7 γ λ + 1 ) k 2 4 ( 2 γ λ 1 ) 2 ( k 2 + l ) | ,
| d 3 | k 2 ( 2 γ λ 1 ) 2 + | k | 3 ( 3 γ λ 1 ) ,
and for μ R
| d 3 μ d 2 2 | | k | 3 ( 3 γ λ 1 ) ; | 1 μ | J 2 2 | k | 3 | 1 μ | | ( 8 γ λ 2 7 γ λ + 1 ) k 2 4 ( 2 γ λ 1 ) 2 ( k 2 + l ) | ; | 1 μ | J 2 ,
where
J 2 = ( 8 γ λ 2 7 γ λ + 1 ) ) k 2 4 ( 2 γ λ 1 ) 2 ( k 2 + l ) ( 3 γ λ 1 ) k 2 .
Example 2. 
Letting γ = 1 in the class χ σ λ ( γ , F ) , we obtain a subclass χ σ λ ( 1 , F ) of functions ϕ σ satisfying
[ ( ζ ϕ ( ζ ) ) ] λ ϕ ( ζ ) F ( ζ ) = F ( ϰ , y , ζ ) ζ , and [ ( ϖ ψ ( ϖ ) ) ] λ ψ ( ϖ ) F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
Corollary 5. 
Let λ 1 . If ϕ χ σ λ ( 1 , F ) then
| d 2 | | k | | k | | ( 8 λ 2 7 λ + 1 ) k 2 4 ( 2 λ 1 ) 2 ( k 2 + l ) | , | d 3 | k 2 ( 2 λ 1 ) 2 + | k | 3 ( 3 λ 1 ) ,
and for μ R
| d 3 μ d 2 2 | | k | 3 ( 3 λ 1 ) ; | 1 μ | J 3 2 | k | 3 | 1 μ | | ( 8 λ 2 7 λ + 1 ) k 2 4 ( 2 λ 1 ) 2 ( k 2 + l ) | ; | 1 μ | J 3 ,
where
J 3 = ( 8 λ 2 7 λ + 1 ) ) k 2 4 ( 2 λ 1 ) 2 ( k 2 + l ) ( 3 γ λ 1 ) k 2 .
Remark 4. 
λ = 1 in Corollary 4 yields Corollaries 3 and 7 of Yilmaz and Aktas [43].
Taking η = 1 in the above theorem, we obtain
Corollary 6. 
Let γ 1 , a n d λ 1 . If ϕ Z σ , p , q λ ( γ , ϰ ) , then
| d 2 | | k | | k | | ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) k 2 R 2 [ 2 ] p , q 2 ( k 2 + l ) | , | d 3 | k 2 R 2 [ 2 ] p , q 2 + | k | P [ 3 ] p , q ,
and for μ R
| d 3 μ d 2 2 | | k | P [ 3 ] p , q ; | 1 μ | J 4 | k | 3 | 1 μ | | ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) k 2 R 2 [ 2 ] p , q 2 ( k 2 + l ) | ; | 1 μ | J 4 ,
where
J 4 = ( P [ 3 ] p , q + Q [ 2 ] p , q 2 ) k 2 R 2 [ 2 ] 2 ( k 2 + l ) P [ 3 ] p , q k 2 ,
and P, Q, and R are as detailed in (11), (12), and (13), respectively.
Remark 5. 
Z σ , p = 1 , q 1 λ ( γ , F ) χ σ λ ( γ , F )

3. Results for the Class T σ , p , q λ , η ( ν , ϰ )

First, for the class ϕ T σ , p , q λ , η ( ν , ϰ ) , as defined in Definition 3, we determine the coefficient estimates.
Theorem 2. 
Let 0 ν 1 , 0 < η 1 , a n d λ 1 . If ϕ T σ , p , q λ , η ( ν , ϰ ) , then
| d 2 | 2 η | k | | k | | ( 2 η ( η + 1 ) ( L + N ) + ( 1 η ) M 2 ) k 2 ( η + 1 ) 2 B 2 ( k 2 + l ) | ,
| d 3 | 4 η 2 k 2 ( η + 1 ) 2 M 2 + 2 η | k | ( η + 1 ) L ,
and for μ R
| d 3 μ d 2 2 | 2 η | k | ( η + 1 ) L ; | 1 μ | Q 4 η 2 | k | 3 | 1 μ | | ( 2 η ( η + 1 ) ( L + N ) + ( 1 η ) M 2 ) k 2 ( η + 1 ) 2 B 2 ( k 2 + l ) | ; | 1 μ | Q ,
where
Q = ( 2 η ( η + 1 ) ( L + N ) + ( 1 η ) M ) 2 ) k 2 ( η + 1 ) 2 M 2 ( k 2 + l ) 2 η ( 1 + η ) L k 2 ,
L = λ [ 3 ] p , q ν ,
N = λ ( λ 1 ) [ 2 ] p , q 2 2 ν λ [ 2 ] p , q + ν 2 ,
and
M = λ [ 2 ] p , q ν .
Proof. 
Let ϕ T σ , p , q λ , η ( ν , ϰ ) . Following that, due to Definition 3, we obtain
1 2 ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ + ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ 1 η = F ( m ( ζ ) ) ,
and
1 2 ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( w ) + ( 1 ν ) ϖ + ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ 1 η = F ( n ( ϖ ) ) ,
where m ( ζ ) and n ( ϖ ) are analytic functions as given in (16), with | m ( ζ ) | < 1 , | n ( ϖ ) | < 1 , ς , ϖ D , and it is known that
| m i | 1 , a n d | n i | 1 , ( i N ) .
It follows from (38), (39) and (16) that
1 2 ζ ( D p , q ϕ ( ζ ) ) τ ν ϕ ( ζ ) + ( 1 ν ) ζ + ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ 1 η = 1 + F 2 ( ϰ , y ) m ( ζ ) + F 3 ( ϰ , y ) m 2 ( ζ ) + ,
and
1 2 ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ + w ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ 1 η =
1 + F 2 ( ϰ , y ) n ( ϖ ) + F 3 ( ϰ , y ) n 2 ( ϖ ) + .
In light of (4), Equations (41) and (42) can be expressed as follows.
1 2 ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ + ζ ( D p , q ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ 1 η =
1 + F 2 ( ϰ , y ) m 1 ζ + [ F 2 ( ϰ , y ) m 2 + F 3 ( ϰ , y ) m 1 2 ] ζ 2 + ,
and
1 2 ϖ ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ + w ( D p , q ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ 1 η =
1 + F 2 ( ϰ , y ) n 1 ϖ + [ F 2 ( ϰ , y ) n 2 + F 3 ( ϰ , y ) n 1 2 ] ϖ 2 + .
Comparing (43) and (44), we have
( η + 1 ) M 2 η d 2 = F 2 ( ϰ , y ) m 1 ,
η + 1 2 η L d 3 + N d 2 2 + 1 η 4 η 2 M 2 d 2 2 = F 2 ( ϰ , y ) m 2 + F 3 ( ϰ , y ) m 1 2 ,
( η + 1 ) M 2 η d 2 = F 2 ( ϰ , y ) n 1 ,
and
η + 1 2 η L ( 2 d 2 2 d 3 ) + N d 2 2 + 1 η 4 η 2 M 2 d 2 2 = F 2 ( ϰ , y ) n 2 + F 3 ( ϰ , y ) n 1 2 ,
where L, N, and M are as in (35), (36) and (37), respectively. From (45) and (47), we easily obtain
m 1 = n 1
and also
( η + 1 ) 2 M 2 2 η 2 d 2 2 = ( m 1 2 + n 1 2 ) ( H 2 ( ϰ ) ) 2 .
The bound on | d 2 | , is obtained by adding (46) and (48).
η + 1 η ( L + N ) + 1 η 2 η 2 M 2 d 2 2 = F 2 ( ϰ , y ) ( m 2 + n 2 ) + F 3 ( ϰ , y ) ( m 1 2 + n 1 2 ) .
Substituting the value of m 1 2 + n 1 2 from (50) in (51), we obtain
d 2 2 = 2 η 2 F 2 3 ( ϰ , y ) ( ϰ ) ( m 2 + n 2 ) ( 2 η ( η + 1 ) ( L + N ) + ( 1 η ) M 2 ) F 2 2 ( ϰ , y ) ( η + 1 ) 2 M 2 F 3 ( ϰ , y ) .
Applying (40) for the coefficients m 2 and n 2 , we obtain (31).
To obtain the bound on | d 3 | , we deduct (48) from (46):
d 3 = d 2 2 + F 2 ( ϰ , y ) ( m 2 n 2 ) η + 1 η L .
Then, in view of (49) and (50), (53) becomes
d 3 = 2 η 2 F 2 2 ( ϰ , y ) ( m 1 2 + n 1 2 ) ( η + 1 ) 2 M 2 + η F 2 ( ϰ , y ) ( m 2 n 2 ) ( η + 1 ) L ,
and applying (40) for the coefficients m 1 , m 2 , n 1 and n 2 we obtain (32).
From (52) and (53), for μ R , we obtain
| d 3 μ d 2 2 | = | F 2 ( ϰ , y ) | B 1 ( μ , ϰ ) + η ( η + 1 ) L m 2 + B 1 ( μ , ϰ ) η ( δ + 1 ) L n 2 ,
where
B 1 ( μ , ϰ ) = 2 η 2 ( 1 μ ) F 2 2 ( ϰ , y ) ( 2 η ( η + 1 ) ( L + N ) + ( 1 η ) M 2 ) F 2 2 ( ϰ , y ) ( η + 1 ) 2 M 2 F 3 ( ϰ , y ) .
Clearly
| d 3 μ d 2 2 | 2 η | F 2 ( ϰ , y ) | ( η + 1 ) L ; 0 | B 1 ( μ , ϰ ) | η ( η + 1 ) L 2 | F 2 ( ϰ , y ) | | B 1 ( μ , ϰ ) | ; | B 1 ( μ , ϰ ) | η ( η + 1 ) L ,
from which we conclude (33) with Q as in (34). □
Corollary 7. 
Let ν = 0 in the above theorem. Then, for any function ϕ C σ , p , q λ , η ( F ) the upper bounds of | d 2 | , | d 3 | , and | d 3 μ d 2 2 | , μ , are given by (31), (32) and (33), respectively, with L = L 1 = λ [ 3 ] p , q , N = N 1 = λ ( λ 1 ) 2 [ 2 ] p , q 2 and M = M 1 = λ [ 2 ] p , q . L 1 , N 1 , a n d M 1 are to be used in place of L , N , a n d M for Q in (34).
Corollary 8. 
Let ν = 1 in the above theorem. Then, for any function ϕ D σ , p , q λ , η ( F ) the upper bounds of | d 2 | , | d 3 | , and | d 3 μ d 2 2 | , μ , are given by (31), (32) and (33), respectively, with L = L 2 = λ [ 3 ] p , q 1 , N = N 2 = λ ( λ 1 ) 2 [ 2 ] p , q 2 λ [ 2 ] p , q + 1 a n d M = M 2 = λ [ 2 ] p , q 1 . L 2 , N 2 , a n d M 2 are to be used in place of L , N , a n d M for Q in (34).
From Theorem 2, taking p = 1 and q 1 , we obtain
Corollary 9. 
Let 0 ν 1 , 0 < η 1 , a n d λ 1 . If ϕ Γ σ λ , η ( ν , F ) then
| d 2 |
2 η | k | | k | | ( 2 η ( η + 1 ) ( ( 2 λ + 1 ) ( λ ν ) + ν 2 ) + ( 1 η ) ( 2 λ ν ) 2 ) k 2 ( η + 1 ) 2 ( 2 λ ν ) 2 ( k 2 + l ) | ,
| d 3 | 2 η k ( η + 1 ) ( 2 λ ν ) 2 + 2 η | k | ( η + 1 ) ( 3 λ ν ) ,
and for μ R
| d 3 μ d 2 2 | 2 η | k | ( η + 1 ) ( 3 λ ν ) ; | 1 μ | Q 1 4 η 2 | k | 3 | 1 μ | | ( 2 η ( η + 1 ) ( ( 2 λ + 1 ) ( λ ν ) + ν 2 ) + ( 1 η ) ( 2 λ ν ) 2 ) k 2 ( η + 1 ) 2 ( 2 λ ν ) 2 ( k 2 + l ) | ; | 1 μ | Q 1 ,
where
Q 1 =
( 2 η ( η + 1 ) ( ( 2 λ + 1 ) ( λ ν ) + ν 2 ) + ( 1 η ) ( 2 λ ν ) 2 ) k 2 ( η + 1 ) 2 ( 2 λ ν ) 2 ( k 2 + l ) 2 η ( η + 1 ) ( 3 λ ν ) k 2 .
Here are a few examples of the above corollary’s special cases.
Example 3. 
Letting η = 1 in the class Γ σ λ , η ( ν , F ) , we obtain a subclass Ψ σ λ ( ν , F ) Γ σ λ , 1 ( ν , F ) of functions ϕ σ satisfying
ζ ( ϕ ( ζ ) ) λ ν ϕ ( ζ ) + ( 1 ν ) ζ F ( ζ ) = F ( ϰ , y , ζ ) ζ ,
and
ϖ ( ψ ( ϖ ) ) λ ν ψ ( ϖ ) + ( 1 ν ) ϖ F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6), 0 ν 1 , a n d λ 1 .
Corollary 10. 
Let 0 ν 1 , a n d λ 1 . If ϕ   Ψ σ λ ( ν , F ) then
| d 2 | | k | | k | | ( ( 2 λ + 1 ) ( λ ν ) + ν 2 ) k 2 ( 2 λ ν ) 2 ( k 2 + l ) | ,
| d 3 | k 2 λ ν 2 + | k | 3 λ ν ,
and for μ R
| d 3 μ d 2 2 | | k | 3 λ ν ; | 1 μ | Q 2 | k | 3 | 1 μ | | ( ( 2 λ + 1 ) ( λ ν ) + ν 2 ) k 2 ( 2 λ ν ) 2 ( k 2 + l ) | ; | 1 μ | Q 2 ,
where
Q 2 = ( ( 2 λ + 1 ) ( λ ν ) + ν 2 ) k 2 ( 2 λ ν ) 2 ( k 2 + l ) ( 3 λ ν ) k 2 .
Example 4. 
Letting ν = 1 , then Ψ σ λ ( 1 , F ) is the subclass of functions ϕ σ satisfying
ζ ( ϕ ( ζ ) ) λ ϕ ( ζ ) F ( ζ ) = F ( ϰ , y , ζ ) ζ , and ϖ ( ψ ( ϖ ) ) λ ψ ( ϖ ) F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in (6).
Corollary 11. 
Let λ 1 . If ϕ Ψ σ λ ( 1 , F ) then
| d 2 | | k | | k | | λ ( 2 λ 1 ) k 2 ( 2 λ 1 ) 2 ( k 2 + l ) | , | d 3 | k 2 λ 1 2 + | k | 3 λ 1 ,
and for μ R
| d 3 μ d 2 2 | | k | 3 λ 1 ; | 1 μ | λ ( 2 λ 1 ) k 2 ( 2 λ 1 ) 2 ( k 2 + l ) ( 3 λ 1 ) k 2 | k | 3 | 1 μ | | λ ( 2 λ 1 ) k 2 ( 2 λ 1 ) 2 ( k 2 + l ) | ; | 1 μ | λ ( 2 λ 1 ) k 2 ( 2 λ 1 ) 2 ( k 2 + l ) ( 3 λ 1 ) k 2 .
Remark 6. 
λ = 1 in Corollary 11 yields Corollaries 2 and 6 of Yilmaz and Aktas [43].
Example 5. 
Letting ν = 0 , then Ψ σ λ ( 0 , F ) is the subclass of functions ϕ σ satisfying
( ϕ ( ζ ) ) λ F ( ζ ) = F ( ϰ , y , ζ ) ζ , and ( ψ ( ϖ ) ) λ F ( ϖ ) = F ( ϰ , y , ϖ ) ϖ ,
where F ( ζ ) is as mentioned in ( ) .
The class Ψ σ λ ( 0 , F ) is not an empty set, which is an important point to note. Consider the following example, where λ = 1 , k = 1 a n d l = 0 . The function u ( ζ ) = = 1 2 log ( 1 + ζ 1 ζ ) S is in the class Ψ σ λ ( 0 , F ) . Because, its inverse v ( ϖ ) = e 2 ϖ 1 e 2 ϖ + 1 S . So, we get that u ( ζ ) σ (see [46]).
Corollary 12. 
Let λ 1 . If ϕ Ψ σ λ ( 0 , F ) , then
| d 2 | | k | | k | | ( 2 λ + 1 ) λ ) k 2 4 λ 2 ( k 2 + l ) | , | d 3 | k 2 λ 2 + | k | 3 λ ,
and for μ R
| d 3 μ d 2 2 | | k | 3 λ ; | 1 μ | ( 2 λ + 1 ) λ ) k 2 4 λ 2 ( k 2 + l ) 3 λ k 2 | k | 3 | 1 μ | | ( 2 λ + 1 ) λ ) k 2 4 λ 2 ( k 2 + l ) | ; | 1 μ | ( 2 λ + 1 ) λ ) k 2 4 λ 2 ( k 2 + l ) 3 λ k 2 .
Corollary 13. 
Let 0 ν 1 , a n d λ 1 . If ϕ O σ , p , q λ ( ν , F ) , then
| d 2 | | k | | k | | ( L + N ) k 2 M 2 ( k 2 + l ) | , | d 3 | k 2 M 2 + | k | L ,
and for μ R
| d 3 μ d 2 2 | | k | L ; | 1 μ | ( L + N ) k 2 M 2 ( k 2 + l ) L k 2 | k | 3 | 1 μ | | ( L + N ) k 2 M 2 ( k 2 + l ) | ; | 1 μ | ( L + N ) k 2 M 2 ( k 2 + l ) L k 2 ,
where L, N, and M are as mentioned in (31), (32), and (33), respectively.
Remark 7. 
O σ , p = 1 , q 1 λ ( ν , F ) Ψ σ λ ( ν , F ) .

4. Conclusions

The current work defines two subfamilies of σ associated with GBFP and derives upper bounds of | d 2 | , | d 3 | and the Fekete–Szegö functional | d 3 μ d 2 2 | , μ R for functions in these subfamilies. We have been able to draw attention to several implications by altering the parameters in Theorem 1 and Theorem 2. Relevant connections to the current research are also discovered. The subfamilies this paper studies may encourage researchers to concentrate on the (p, q) -derivative operator. Future studies might look into extending obtained results to fractional derivatives, higher-order Hankel determinants, or Toeplitz determinants. The findings presented here give these advancements a strong foundation and emphasize the importance of geometric factors in the study of analytic function theory.

Author Contributions

S.R.S. and B.A.F.: analysis, methodology, implementation, and original draft; D.B. and L.-I.C.: software and conceptualization, validation, resources, and editing. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

Data are contained within the article.

Conflicts of Interest

The authors declare that they have no conflicts of interest.

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MDPI and ACS Style

Swamy, S.R.; Frasin, B.A.; Breaz, D.; Cotîrlă, L.-I. Two Families of Bi-Univalent Functions Associating the (p, q)-Derivative with Generalized Bivariate Fibonacci Polynomials. Mathematics 2024, 12, 3933. https://doi.org/10.3390/math12243933

AMA Style

Swamy SR, Frasin BA, Breaz D, Cotîrlă L-I. Two Families of Bi-Univalent Functions Associating the (p, q)-Derivative with Generalized Bivariate Fibonacci Polynomials. Mathematics. 2024; 12(24):3933. https://doi.org/10.3390/math12243933

Chicago/Turabian Style

Swamy, Sondekola Rudra, Basem Aref Frasin, Daniel Breaz, and Luminita-Ioana Cotîrlă. 2024. "Two Families of Bi-Univalent Functions Associating the (p, q)-Derivative with Generalized Bivariate Fibonacci Polynomials" Mathematics 12, no. 24: 3933. https://doi.org/10.3390/math12243933

APA Style

Swamy, S. R., Frasin, B. A., Breaz, D., & Cotîrlă, L.-I. (2024). Two Families of Bi-Univalent Functions Associating the (p, q)-Derivative with Generalized Bivariate Fibonacci Polynomials. Mathematics, 12(24), 3933. https://doi.org/10.3390/math12243933

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