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Article

Applications of the q-Derivative Operator to New Families of Bi-Univalent Functions Related to the Legendre Polynomials

1
Department of Mathematics, Yangzhou University, Yangzhou 225002, China
2
Department of Mathematics and Statistics, University of Victoria, Victoria, BC V8W 3R4, Canada
*
Author to whom correspondence should be addressed.
Axioms 2022, 11(11), 595; https://doi.org/10.3390/axioms11110595
Submission received: 5 October 2022 / Revised: 23 October 2022 / Accepted: 23 October 2022 / Published: 27 October 2022
(This article belongs to the Special Issue Mathematical Analysis and Applications III)

Abstract

:
By using the q-derivative operator and the Legendre polynomials, some new subclasses of q-starlike functions and bi-univalent functions are introduced. Several coefficient estimates and Fekete–Szegö-type inequalities for functions in each of these subclasses are obtained. The results derived in this article are shown to extend and generalize those in some earlier works.

1. Introduction

In the development of the Geometric Function Theory of Complex Analysis, the q-derivative is an important research tool. The application of q-calculus was first considered by Jackson (see [1,2,3,4]). Recently, many scholars have defined new subclasses of analytic functions by combining the q-derivative operator with the principle of differential subordination and studied their geometric properties (see [5,6,7,8,9,10,11,12,13,14,15]). In this article, we investigate two new subclasses I 𝒜 q [ A , B , λ , β ] and I Σ q [ ϕ , λ , β ] of the class of q-starlike functions and bi-univalent functions associated with the q-derivative operator and the Legendre polynomials. For each of these subclasses, we obtain certain coefficient estimates and Fekete–Szegö-type inequalities. The results obtained in this article are also shown to extend and generalize those in some earlier works. For motivation and incentive for further researches, the reader’s attention is drawn toward some of the related recent developments in [12,16,17,18,19] dealing with the coefficient inequalities and coefficient estimates of various subclasses of analytic, univalent, and bi-univalent functions involving the second, third, and fourth Hankel determinants and the Fekete–Szegö functional.
Let 𝒜 be the class of analytic functions in the open unit disk
U = { z : z C and | z | < 1 } ,
which have the following normalized form:
f ( z ) = z + n = 2 a n z n .
Also, let 𝒮 𝒜 be the class of functions that are univalent in U . Obviously, each function f 𝒮 has an inverse f 1 , so that
f 1 f ( z ) = z ( z U )
and
f 1 f ( w ) = w | w | < r 0 ( f ) ; r 0 ( f ) 1 4 ,
where
g ( w ) : = f 1 ( w ) = w a 2 w 2 + ( 2 a 2 2 a 3 ) w 3 ( 5 a 2 3 5 a 2 a 3 + a 4 ) w 4 + .
A function f 𝒜 is said to be bi-univalent in U if both f and f 1 are univalent in U . We denote this class using Σ . We remark that the study of the normalized class Σ of analytic and bi-univalent functions in U was revived in recent years by a pioneering article on the subject by Srivastava et al. [20], which has flooded the literature on the Geometric Function Theory of Complex Analysis with a large number of sequels to [20].
For a function f 𝒜 , given by (1), and a function g 𝒜 , given by
g ( z ) = z + n = 2 b n z n ( z U ) ,
the Hadamard product (or convolution) of f and g is defined by
( f g ) ( z ) : = z + n = 2 a n b n z n = : ( g f ) ( z ) ( z U ) .
Let 𝒫 be the class of Carathéodory functions h that are analytic in U and that satisfy
h ( z ) = 1 + n = 1 c n z n
and
R h ( z ) > 0 ( z U ) .
For two analytic functions f and g, we say that f is subordinate to g and it is written as f g or f ( z ) g ( z ) , if there is a Schwarz function w such that f ( z ) = g w ( z ) . Further, if g is univalent in U , then
f g f ( 0 ) = g ( 0 ) and f ( U ) g ( U ) .
Let q ( 0 , 1 ) and define the q-number [ λ ] q as follows:
[ λ ] q : = 1 q λ 1 q ( λ C ) 1 + j = 1 n 1 q j ( λ = n N ) .
Especially, we note that [ 0 ] q = 0 .
Let q ( 0 , 1 ) and define the q-factorial [ n ] q ! by
[ n ] q ! : = 1 ( n = 0 ) k = 1 n [ k ] q ( n N ) .
Let r N 0 = N { 0 } . Define [ r ] q , n by
[ r ] q , n : = 1 ( n = 0 ) k = r r + n 1 [ k ] q ( n N ) .
Now, we recall here the q-derivative (or the q-difference) operator D q ( 0 < q < 1 ) of a function f 𝒜 as follows:
( D q f ) ( z ) = f ( z ) f ( q z ) ( 1 q ) z ( z 0 ) f ( 0 ) ( z = 0 ) ,
where f ( 0 ) exists. Also, we write
( D q ( 2 ) f ) ( z ) = D q ( D q f ) ( z ) .
The Legendre polynomials P n ( x ) are the particular solutions to the Legendre differential equation:
( 1 x 2 ) y 2 x y + n ( n + 1 ) y = 0 ( n N 0 ) .
The Legendre polynomials P n ( x ) are defined by
P n ( x ) = 1 2 n n ! d n d x n ( x 2 1 ) n ( n N 0 )
for arbitrary real or complex values of the variable x. The Legendre polynomials P n ( x ) are generated by (see, for details, [21])
( 1 2 x t + t 2 ) 1 2 = n = 0 P n ( x ) t n ,
where ( 1 2 x t + t 2 ) 1 2 is taken to be 1 when t 0 . The first few Legendre polynomials are given by
P 0 ( x ) = 1 , P 1 ( x ) = x , P 2 ( x ) = 1 2 ( 3 x 2 1 ) and P 3 ( x ) = 1 2 ( 5 x 3 3 x ) .
The function ϕ ( z ) given by
ϕ ( z ) = 1 z 1 2 z cos α + z 2
belongs to the class 𝒫 for every real number α (see [22]). By using (3), it is easy to see that
ϕ ( z ) = 1 + n = 1 [ P n ( cos α ) P n 1 ( cos α ) ] z n = 1 + n = 1 l n z n ,
where
l n = P n ( cos α ) P n 1 ( cos α ) .
We also note that
l 1 = cos α 1 and l 2 = 1 2 ( cos α 1 ) ( 1 + 3 cos α ) .
For more details, one can see the earlier work [23].
For f 𝒜 , the q-Ruscheweyh operator R q , λ is defined as follows (see [24]):
R q , λ f ( z ) = f ( z ) F q , λ + 1 ( z ) ( z U ; λ > 1 ) ,
where
F q , λ + 1 ( z ) = z + n = 2 [ λ + 1 ] q , n 1 [ n 1 ] q ! z n .
Let f 𝒜 . The q-integral operator R q , λ 1 is defined by (see [5,25])
R q , λ 1 ( z ) R q , λ ( z ) = z D q f ( z ) .
Further, we have
R q , λ 1 ( z ) = z + n = 2 ψ n 1 z n ,
where
ψ n 1 = [ n ] q ! [ λ + 1 ] q , n 1 ( n 2 ) .
When q 1 1 , the q-integral operator R q , λ 1 reduces to an integral operator studied by Noor [26].
For f 𝒜 , the q-integral operator I q λ is defined by (see [5])
I q λ f ( z ) = f ( z ) R q , λ 1 ( z ) = z + n = 2 ψ n 1 a n z n ,
where ψ n 1 is given by (5). Clearly, one can see that
I q 0 f ( z ) = z D q f ( z ) and I q 1 f ( z ) = f ( z ) .
Next, we will define the analytic function class I 𝒜 q [ A , B , λ , β ] and the bi-univalent function class I Σ q [ ϕ , λ , β ] .
Definition 1.
Let λ > 1 , 1 B < A 1 , and 0 β 1 . A function f 𝒜 is said to be in the class I 𝒜 q [ A , B , λ , β ] if
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z ( D q I q λ f ) ( z ) 1 + A z 1 + B z ( z U ) ,
or equivalently,
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z ( D q I q λ f ) ( z ) 1 A B z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z ( D q I q λ f ) ( z ) < 1 .
Remark 1.
(i) 
For λ = 1 and β = 0 , we have
I 𝒜 q [ A , B , 1 , 0 ] = 𝒮 q [ A , B ] ,
where the class 𝒮 q [ A , B ] was introduced by Srivastava et al. [27].
(ii) 
For λ = 1 , β = 0 , and q 1 , we get
lim q 1 I 𝒜 q [ A , B , 1 , 0 ] = 𝒮 [ A , B ] ,
where the class 𝒮 [ A , B ] was considered by Janowski [28].
(iii) 
For A = 1 2 α ( 0 α < 1 ) and B = 1 , the class 𝒮 [ A , B ] reduces to the class 𝒮 ( α ) , which was studied by Silverman [29].
Definition 2.
Let λ > 1 and 0 β 1 . A function f Σ is said to be in the class I Σ q [ ϕ , λ , β ] if
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z ( D q I q λ f ) ( z ) ϕ ( z ) w ( D q I q λ g ) ( w ) + β w 2 ( D q ( 2 ) I q λ g ) ( w ) ( 1 β ) I q λ g ( w ) + β w ( D q I q λ g ) ( w ) ϕ ( w ) ,
where the functions g and ϕ are given by (2) and (4), respectively.
To derive our main results, we need the following lemmas.
Lemma 1
(see [30]). Let φ ( z ) = 1 + ω 1 z + ω 2 z 2 + 𝒫 . Then,
| ω 2 ν ω 1 2 | 4 ν + 2 ( ν < 0 ) 2 ( 0 ν 1 ) 4 ν 2 ( ν > 1 ) .
Lemma 2
(see [13]). Let
M ( z ) = 1 + n = 1 C n z n H ( z ) = 1 + n = 1 d n z n .
If H ( z ) is univalent in U and H ( U ) is convex, then
| C n | | d 1 | ( n N ) .
Lemma 3
(see [31]). If p ( z ) = 1 + n = 1 c n z n 𝒫 , then
| c n | 2 ( n N ) .

2. Main Results

In this section, we derive certain coefficient estimates and the Fekete–Szegö-type inequalities for functions in the classes I 𝒜 q [ A , B , λ , β ] and I Σ q [ ϕ , λ , β ] , which are defined above (see Definitions 1 and 2). Many special cases and consequences of our main findings are pointed out.
Theorem 1.
Let a function f I 𝒜 q [ A , B , λ , β ] be of the form given by ( 1 ) . Then,
| a n | A B q ( 1 β ) + β [ n ] q ψ n 1 · j = 1 n 1 q ( 1 β ) + β [ j ] q [ j 1 ] q + ( 1 β ) + β [ j ] q ( A B ) q ( 1 β ) + β [ j ] q [ j ] q ( n 2 ) ,
where ψ n 1 is given by ( 5 ) .
Proof. 
For f I 𝒜 q [ A , B , λ , β ] , we have
ν ( z ) : = z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z ( D q I q λ f ) ( z ) 1 + A z 1 + B z ( z U ) ,
where
1 + A z 1 + B z = 1 + n = 0 ( A B ) ( B ) n z n + 1 = 1 + ( A B ) z B ( A B ) z 2 + .
Since ν ( z ) = 1 + n = 1 ν n z n , we get from Lemma 2 that
| ν n | A B ( n N ) .
From (12), we have
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) = ν ( z ) [ ( 1 β ) I q λ f ( z ) + β z D q I q λ f ( z ) ]
which shows that
z + n = 2 [ n ] q [ 1 + β [ n 1 ] q ] a n ψ n 1 z n = 1 + n = 1 ν n z n z + n = 2 [ 1 + β ( [ n ] q 1 ) ] a n ψ n 1 z n .
Comparing the coefficients of z n on both sides of the Equation (14), we get
[ n 1 ] q [ q ( 1 β ) + β [ n ] q ] a n ψ n 1 = l = 1 n 1 [ 1 + β ( [ l ] q 1 ) ] a l ψ l 1 ν n l ,
where a 1 = 1 , ν 1 = 1 and ψ 0 = 1 . The above equation gives
| a n | A B [ n 1 ] q [ q ( 1 β ) + β [ n ] q ] ψ n 1 l = 1 n 1 [ 1 + β ( [ l ] q 1 ) ] | a l | ψ l 1 .
Thus, we get
| a 2 | A B ( q + β ) ψ 1 ; | a 3 | A B ( q ( 1 β ) + β [ 3 ] q ) ψ 2 · ( q + β ) + ( 1 + β q ) ( A B ) [ 2 ] q ( q + β ) ; | a 4 | A B ( q ( 1 β ) + β [ 4 ] q ) ψ 3 · ( q + β ) + ( 1 + β q ) ( A B ) [ 2 ] q ( q + β ) · [ 2 ] q { q ( 1 β ) + β [ 3 ] q } + ( 1 β ) + β [ 3 ] q ( A B ) [ 3 ] q ; | a n | A B ( q ( 1 β ) + β [ n ] q ) ψ n 1 · j = 1 n 1 { q ( 1 β ) + β [ j ] q } [ j 1 ] q + { ( 1 β ) + β [ j ] q } ( A B ) { q ( 1 β ) + β [ j ] q } [ j ] q .
This proves Theorem 1. □
For λ = 1 and β = 0 in Theorem 1, we obtain a result of the class 𝒮 q [ A , B ] , which was considered by Srivastava et al. [27].
Corollary 1.
Let a function f 𝒮 q [ A , B ] be of the form given by ( 1 ) . Then,
| a n | 1 q j = 1 n 1 q [ j 1 ] q + ( A B ) q [ j ] q ( n 2 ) .
Theorem 2.
Let a function f I Σ q [ ϕ , λ , β ] be given by ( 1 ) . Then,
| a 2 | min | cos α 1 | ( q + β ) ψ 1 , 2 | cos α 1 | | 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 |
and
| a 3 | min | cos α 1 | 2 ( q + β ) 2 ψ 1 2 + | cos α 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 , | cos α 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 + 2 ( cos α 1 ) 2 | { 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 } | .
Proof. 
From (9), we know that there are two Schwarz functions u ( z ) and ν ( w ) , such that
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z D q I q λ f ( z ) = ϕ u ( z )
and
w ( D q I q λ g ) ( w ) + β w 2 ( D q ( 2 ) I q λ g ) ( w ) ( 1 β ) I q λ g ( w ) + β w D q I q λ g ( w ) = ϕ ν ( w ) .
Now we define the functions s ( z ) and t ( w ) by
s ( z ) = 1 + u ( z ) 1 u ( z ) = 1 + s 1 z + s 2 z 2 + 𝒫
and
t ( w ) = 1 + ν ( w ) 1 ν ( w ) = 1 + t 1 z + t 2 z 2 + 𝒫 .
Since
ϕ ( z ) = 1 + n = 1 [ P n ( cos α ) P n 1 ( cos α ) ] z n = 1 + n = 1 l n z n ,
we get
ϕ u ( z ) = 1 + 1 2 l 1 s 1 z + 1 2 l 1 s 2 s 1 2 2 + 1 4 l 2 s 1 2 z 2 + , ϕ ν ( w ) = 1 + 1 2 l 1 t 1 w + 1 2 l 1 t 2 t 1 2 2 + 1 4 l 2 t 1 2 w 2 + .
Using the Taylor series formula, we have
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z D q I q λ f ( z ) = 1 + ( q + β ) ψ 1 a 2 z + { [ q ( q + 1 ) + ( q 2 + 1 ) [ 2 ] q β ] ψ 2 a 3 ( 1 + β q ) ( q + β ) ψ 1 2 a 2 2 } z 2 +
and
w ( D q I q λ g ) ( w ) + β w 2 ( D q ( 2 ) I q λ g ) ( w ) ( 1 β ) I q λ g ( w ) + β w D q I q λ g ( w ) = 1 ( q + β ) ψ 1 a 2 w + { [ q ( q + 1 ) + ( q 2 + 1 ) [ 2 ] q β ] ψ 2 ( 2 a 2 2 a 3 ) ( 1 + β q ) ( q + β ) ψ 1 2 a 2 2 } w 2 + .
Comparing the left-side and right-side coefficients of (17) and (18), we obtain
( q + β ) ψ 1 a 2 = 1 2 l 1 s 1 ,
[ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 a 3 ( 1 + β q ) ( q + β ) ψ 1 2 a 2 2 = 1 2 l 1 s 2 s 1 2 2 + 1 4 l 2 s 1 2 ,
( q + β ) ψ 1 a 2 = 1 2 l 1 t 1
and
[ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 ( 2 a 2 2 a 3 ) ( 1 + β q ) ( q + β ) ψ 1 2 a 2 2 = 1 2 l 1 t 2 t 1 2 2 + 1 4 l 2 t 1 2 .
From (20) and (22), we have
a 2 = l 1 s 1 2 ( q + β ) ψ 1 = l 1 t 1 2 ( q + β ) ψ 1 .
Thus, we find that
s 1 = t 1
and
8 ( q + β ) 2 ψ 1 2 a 2 2 = l 1 2 ( s 1 2 + t 1 2 ) .
Using Lemma 3, we find from (24) that
| a 2 | | cos α 1 | ( q + β ) ψ 1 .
Now from (21), (23), (24) and (25), we have
4 { [ 2 ] q [ q + β ( q 2 + 1 ) ] l 1 2 ψ 2 ( q + β ) [ ( 1 + β q ) l 1 2 + ( q + β ) ( l 2 l 1 ) ] ψ 1 2 } a 2 2 = l 1 3 ( s 2 + t 2 ) .
Since
l 1 = cos α 1 a n d l 2 = 1 2 ( cos α 1 ) ( 1 + 3 cos α ) ,
we obtain
a 2 2 = l 1 3 ( s 2 + t 2 ) 4 { [ 2 ] q [ q + β ( q 2 + 1 ) ] l 1 2 ψ 2 ( q + β ) [ ( 1 + β q ) l 1 2 + ( q + β ) ( l 2 l 1 ) ] ψ 1 2 } = ( cos α 1 ) 2 ( s 2 + t 2 ) 2 { 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 } .
Applying Lemma 3 to the coefficients s 2 and t 2 , we have
| a 2 | 2 | cos α 1 | | 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 | .
By subtracting (23) from (21), we have
2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( a 3 a 2 2 ) ψ 2 = 1 2 l 1 ( s 2 t 2 ) + 1 4 ( l 2 l 1 ) ( s 1 2 t 1 2 ) .
From (24), (25) and (29), we obtain
a 3 = a 2 2 + l 1 ( s 2 t 2 ) 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 .
Now taking the modulus of (30) and using Lemma 3, we get
| a 3 | | a 2 | 2 + l 1 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 .
Further, by using (27) and (31), we find
| a 3 | l 1 2 ( q + β ) 2 ψ 1 2 + | l 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 = | cos α 1 | ( q + β ) 2 ψ 1 2 + | cos α 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 .
Also, using (26) and (31), we derive
| a 3 |   | a 2 2 | + l 1 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 = | cos α 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 + 2 ( cos α 1 ) 2 | { 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 } | .
This completes the proof of Theorem 2. □
Theorem 3.
Let a function f I 𝒜 q [ A , B , λ , β ] be of the form given by ( 1 ) . Then,
| a 3 μ a 2 2 | A B ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 Λ ( q ) ( μ < σ 1 ) A B ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 ( σ 1 μ σ 2 ) B A ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 Λ ( q ) ( μ > σ 2 ) ,
where μ is real and
Λ ( q ) = ( q + β ) [ ( 1 + β q ) ( A B ) ( q + β ) B ] ψ 1 2 μ ( 1 + q ) [ q + ( q 2 + 1 ) β ] ( A B ) ψ 2 ( q + β ) 2 ψ 1 2 ,
σ 1 = ( q + β ) [ ( 1 + β q ) ( A B ) ( q + β ) ( B + 1 ) ] ψ 1 2 ( 1 + q ) [ q + ( q 2 + 1 ) β ] ( A B ) ψ 2
and
σ 2 = ( q + β ) [ ( 1 + β q ) ( A B ) ( q + β ) ( B 1 ) ] ψ 1 2 ( 1 + q ) [ q + ( q 2 + 1 ) β ] ( A B ) ψ 2 .
Proof. 
Let f I 𝒜 q [ A , B , λ , β ] . Using the Taylor series formula, we have
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z D q I q λ f ( z ) = 1 + ( q + β ) ψ 1 a 2 z + { [ q ( q + 1 ) + ( q 2 + 1 ) [ 2 ] q β ] ψ 2 a 3 ( 1 + β q ) ( q + β ) ψ 1 2 a 2 2 } z 2 + .
From (7), we know that there exists a Schwarz function h such that
z ( D q I q λ f ) ( z ) + β z 2 ( D q ( 2 ) I q λ f ) ( z ) ( 1 β ) I q λ f ( z ) + β z D q I q λ f ( z ) = 1 + A h ( z ) 1 + B h ( z ) .
We now define a function w 𝒫 by
w ( z ) = 1 + h ( z ) 1 h ( z ) = 1 + w 1 z + w 2 z 2 + .
This implies that
h ( z ) = w ( z ) 1 w ( z ) + 1 = 1 + 1 2 w 1 z + 1 2 w 2 1 4 w 1 2 z 2 + .
Also, we have
1 + A h ( z ) 1 + B h ( z ) = 1 + 1 2 ( A B ) w 1 z + 1 2 ( A B ) w 2 1 4 ( B + 1 ) ( A B ) w 1 2 z 2 + .
Therefore, we obtain
a 2 = A B 2 ( q + β ) ψ 1 w 1 , a 3 = A B 2 ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 w 2 1 2 ( B + 1 ) 1 + β q q + β ( A B ) w 1 2 .
Now, we can find that
| a 3 μ a 2 2 | = A B 2 ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 w 2 1 2 ( B + 1 ) 1 + β q q + β ( A B ) w 1 2 μ ( A B ) 2 4 ( q + β ) 2 ψ 1 2 w 1 2 = A B 2 ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 w 2 1 2 ( B + 1 ) ( 1 + β q ) ( q + β ) ψ 1 2 + μ ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 ( q + β ) 2 ψ 1 2 ( A B ) w 1 2 = A B 2 ( 1 + q ) [ q + ( q 2 + 1 ) β ] ψ 2 | { w 2 k 1 ( q ) w 1 2 } | ,
where
k 1 ( q ) = ( q + β ) [ ( q + β ) ( B + 1 ) ( 1 + β q ) ( A B ) ] ψ 1 2 + μ ( 1 + q ) [ q + ( q 2 + 1 ) β ] ( A B ) ψ 2 2 ( q + β ) 2 ψ 1 2 .
Applying Lemma 1 in (35), we get the desired results. The proof of Theorem 3 is completed. □
For λ = 1 , β = 0 , and q 1 , we get a result of the class 𝒮 [ A , B ] that was considered by Janowski [28].
Corollary 2.
Let a function f 𝒮 [ A , B ] be of the form given by ( 1 ) . Then,
| a 3 μ a 2 2 | A B 2 [ ( A 2 B ) μ ( A B ) ] μ < A 2 B 1 2 ( A B ) A B 2 A 2 B 1 2 ( A B ) μ A 2 B + 1 2 ( A B ) B A 2 [ ( A 2 B ) μ ( A B ) ] μ > A 2 B + 1 2 ( A B ) .
Theorem 4.
Let a function f I Σ q [ ϕ , λ , β ] be of the form given by ( 1 ) . Then,
| a 3 μ a 2 2 | | cos α 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 0 | h ( μ ) | | cos α 1 | 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 4 | h ( μ ) | | h ( μ ) | | cos α 1 | 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 ,
where μ is real and
h ( μ ) = ( 1 μ ) ( cos α 1 ) 2 2 { 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 .
Proof. 
From (30), we have
a 3 μ a 2 2 = ( 1 μ ) a 2 2 + l 1 ( s 2 t 2 ) 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 .
Using (28) and (37), we get
a 3 μ a 2 2 = ( cos α 1 ) ( s 2 t 2 ) 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 + ( 1 μ ) ( cos α 1 ) 2 ( s 2 + t 2 ) 2 { 2 [ 2 ] q [ q + β ( q 2 + 1 ) ] ( cos α 1 ) ψ 2 ( q + β ) [ 2 ( 1 + β q ) ( cos α 1 ) + ( q + β ) ( 3 cos α 1 ) ] ψ 1 2 } = h ( μ ) + cos α 1 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 s 2 + h ( μ ) cos α 1 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 t 2 ,
where h ( μ ) is given by (36).
Taking the modulus of each side in (38), we get
| a 3 μ a 2 2 | | cos α 1 | [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 0 | h ( μ ) | | cos α 1 | 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 4 | h ( μ ) | | h ( μ ) | | cos α 1 | 4 [ 2 ] q [ q + β ( q 2 + 1 ) ] ψ 2 .
This proves Theorem 4. □

3. Conclusions

In our present investigation, we have used the q-derivative (or the q-difference) operator D q , as well as the Legendre polynomials P n ( x ) to introduce and study two new subclasses of the class of q-starlike functions and the class of analytic and bi-univalent functions. For each of these subclasses, we have derived a number of coefficient estimates and Fekete–Szegö-type inequalities. The results derived in this article are also shown to extend and generalize those in some earlier works. For motivation and incentive for further research, the reader’s attention is drawn toward some of the related recent developments in [16,17,18,19] dealing with the coefficient inequalities and coefficient estimates of various subclasses of analytic, univalent, and bi-univalent functions involving the second, third, and fourth Hankel determinants, and the Fekete–Szegö functional.
In concluding this article, we choose to discourage the current trend of some amateurish-type publications in which there are falsely-claimed “generalizations" of known q-theory and known q-results by forcing-in an obviously superfluous (or redundant) parameter p. In this connection, the reader should refer to [32] (p. 340) and [33] (pp. 1511–1512) for a detailed exposition and demonstration, where it is stated clearly that the current trend of trivially and inconsequentially translating known q-results into the corresponding ( p , q ) -results leads to no more than a straightforward and shallow publication involving an additional forced-in parameter p that is obviously redundant (or superfluous).

Author Contributions

Every author’s contribution is equal. All authors have read and agreed to the published version of the manuscript.

Funding

This work was supported by the National Natural Science Foundation of China (Grant No. 11571299).

Data Availability Statement

Not applicable.

Acknowledgments

The authors would like to express their sincere thanks to the referees for their careful reading and suggestions, which has helped us to improve the presentation of this paper.

Conflicts of Interest

The authors declare no conflict of interest.

References

  1. Jackson, F.H. On q-functions and a certain difference operator. Trans. R. Soc. Edinb. 1908, 46, 64–72. [Google Scholar] [CrossRef]
  2. Jackson, F.H. On q-definite integrals. Quart. J. Pure Appl. Math. 1910, 41, 193–203. [Google Scholar]
  3. Jackson, F.H. q-difference equations. Am. J. Math. 1910, 32, 305–314. [Google Scholar] [CrossRef]
  4. Jackson, F.H. The application of basic numbers to Bessel’s and Legendre’s functions. Proc. Lond. Math. Soc. 1905, 3, 1–23. [Google Scholar] [CrossRef]
  5. Srivastava, H.M.; Ahmad, Q.Z.; Khan, N.; Khan, N.; Khan, B. Hankel and Toeplitz determinants for a subclass of q-starlike funtions associated with a general conic domain. Mathematics 2019, 7, 181. [Google Scholar] [CrossRef] [Green Version]
  6. Ahuja, O.P.; Cetinkaya, A.; Polatoğlu, Y. Bieberbach-de Branges and Fekete-Szegö inequalities for certain families of q-convex and q-close-to-convex functions. J. Comput. Anal. Appl. 2019, 26, 639–649. [Google Scholar]
  7. Aouf, M.K.; Mostafa, A.O.; Al-Quhali, F.Y. Properties for class of bi-uniformly univalent functions defined by Sălăgean type q-difference operator. Int. J. Open Probl. Complex Anal. 2019, 11, 1–16. [Google Scholar]
  8. Khan, N.; Ahmad, Q.Z.; Khalid, T. Results on spirallike p-valent functions. AIMS Math. 2017, 3, 12–20. [Google Scholar] [CrossRef]
  9. Khan, S.; Hussain, S.; Darus, M. Inclusion relations of q-Bessel functions associated with generalized conic domain. AIMS Math. 2021, 6, 3624–3640. [Google Scholar] [CrossRef]
  10. Pommerenke, C. Univalent Functions; Vandenhoeck & Ruprecht: Göttingen, Germany, 1975. [Google Scholar]
  11. Rehman, M.S.U.; Ahmad, Q.Z.; Srivastava, H.M.; Khan, N.; Darus, M.; Khan, B. Applications of higher-order q-derivatives to the subclass of q-starlike functions associated with the Janowski functions. AIMS Math. 2021, 6, 1110–1125. [Google Scholar] [CrossRef]
  12. Srivastava, H.M.; Tahir, M.; Khan, B.; Ahmad, Q.Z.; Khan, N. Some general families of q-starlike functions associated with the Janowski functions. Filomat 2019, 33, 2613–2626. [Google Scholar] [CrossRef]
  13. Rogosinski, W. On the coefficients of subordinate functions. Proc. Lond. Math. Soc. 1943, 48, 48–82. [Google Scholar] [CrossRef]
  14. Srivastava, H.M.; Tahir, M.; Khan, B.; Ahmad, Q.Z.; Khan, N. Some general classes of q-starlike functions associated with the Janowski functions. Symmetry 2019, 11, 292. [Google Scholar] [CrossRef]
  15. Güney, H.Ö.; Oros, G.I.; Owa, S. An application of Sălăgean operator concerning starlike functions. Axioms 2022, 11, 50. [Google Scholar] [CrossRef]
  16. Srivastava, H.M.; Kaur, G.; Singh, G. Estimates of the fourth Hankel determinant for a class of analytic functions with bounded turnings involving cardioid domains. J. Nonlinear Convex Anal. 2021, 22, 511–526. [Google Scholar]
  17. Srivastava, H.M.; Shaba, T.G.; Murugusundaramoorthy, G.; Wanas, A.K.; Oros, G.I. The Fekete-Szegö functional and the Hankel determinant for a certain class of analytic functions involving the Hohlov operator. AIMS Math. 2022, 8, 340–360. [Google Scholar] [CrossRef]
  18. Srivastava, H.M.; Murugusundaramoorthy, G.; Bulboacă, T. The second Hankel determinant for subclasses of bi-univalent functions associated with a nephroid domain. Rev. Real Acad. Cienc. Exactas Fís. Natur. Ser. A Mat. (RACSAM) 2022, 116, 145. [Google Scholar] [CrossRef]
  19. Shi, L.; Srivastava, H.M.; Rafiq, A.; Arif, M.; Ihsan, M. Results on Hankel determinants for the inverse of certain analytic functions subordinated to the exponential function. Mathematics 2022, 10, 3429. [Google Scholar] [CrossRef]
  20. Srivastava, H.M.; Mishra, A.K.; Gochhayat, P. Certain subclasses of analytic and bi-univalent functions. Appl. Math. Lett. 2010, 23, 1188–1192. [Google Scholar] [CrossRef] [Green Version]
  21. Srivastava, H.M. Some families of generating functions associated with orthogonal polynomials and other higher transcendental functions. Mathematics 2022, 10, 3730. [Google Scholar] [CrossRef]
  22. Goodman, A.W. Univalent Functions; Mariner Publishing Company Incorporated: Tampa, FL, USA, 1983. [Google Scholar]
  23. Murugusundaramoorthy, G.; Cotîrlă, L.-I. Bi-univalent functions of complex order defined by Hohlov operator associated with Legendre polynomial. AIMS Math. 2022, 7, 8733–8750. [Google Scholar] [CrossRef]
  24. Kanas, S.; Răducanu, D. Some class of analytic functions related to conic domains. Math. Slov. 2014, 64, 1183–1196. [Google Scholar] [CrossRef]
  25. Srivastava, H.M.; Wanas, A.K.; Srivastava, R. Applications of the q-Srivastava-Attiya operator involving a certain family of bi-univalent functions associated with the Horadam polynomials. Symmetry 2021, 13, 1230. [Google Scholar] [CrossRef]
  26. Noor, K.I. On new classes of integral operators. J. Natur. Geom. 1999, 16, 71–80. [Google Scholar]
  27. Srivastava, H.M.; Khan, B.; Khan, N.; Ahmad, Q.Z. Coefficient inequalities for q-starlike functions associated with the Janowski functions. Hokkaido Math. J. 2019, 48, 407–425. [Google Scholar] [CrossRef]
  28. Janowski, W. Some extremal problems for certain families of analytic functions. Ann. Polon. Math. 1973, 28, 297–326. [Google Scholar] [CrossRef] [Green Version]
  29. Silverman, H. Univalent functions with negative coefficients. Proc. Amer. Math. Soc. 1975, 51, 109–116. [Google Scholar] [CrossRef]
  30. Ma, W.C.; Minda, D. A unified treatment of some special classes of univalent functions. In Proceeding of the International Conference on Complex Analysis, Tianjin, China, 19–23 June 1992; pp. 157–169. [Google Scholar]
  31. Duren, P.L. Univalent Functions (Grundlehren der Mathematischen Wissenschaften 259); Springer: New York, NY, USA; Berlin/Heidelberg, Germany; Tokyo, Japan, 1983. [Google Scholar]
  32. Srivastava, H.M. Operators of basic (or q-) calculus and fractional q-calculus and their applications in geometric function theory of complex analysis. Iran. J. Sci. Technol. Trans. A Sci. 2020, 44, 327–344. [Google Scholar] [CrossRef]
  33. Srivastava, H.M. Some parametric and argument variations of the operators of fractional calculus and related special functions and integral transformations. J. Nonlinear Convex Anal. 2021, 22, 1501–1520. [Google Scholar]
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Cheng, Y.; Srivastava, R.; Liu, J.-L. Applications of the q-Derivative Operator to New Families of Bi-Univalent Functions Related to the Legendre Polynomials. Axioms 2022, 11, 595. https://doi.org/10.3390/axioms11110595

AMA Style

Cheng Y, Srivastava R, Liu J-L. Applications of the q-Derivative Operator to New Families of Bi-Univalent Functions Related to the Legendre Polynomials. Axioms. 2022; 11(11):595. https://doi.org/10.3390/axioms11110595

Chicago/Turabian Style

Cheng, Ying, Rekha Srivastava, and Jin-Lin Liu. 2022. "Applications of the q-Derivative Operator to New Families of Bi-Univalent Functions Related to the Legendre Polynomials" Axioms 11, no. 11: 595. https://doi.org/10.3390/axioms11110595

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