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Article

Faber Polynomial Coefficient Estimates of Bi-Close-to-Convex Functions Associated with Generalized Hypergeometric Functions

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.
Mathematics 2022, 10(17), 3073; https://doi.org/10.3390/math10173073
Submission received: 3 August 2022 / Revised: 20 August 2022 / Accepted: 23 August 2022 / Published: 25 August 2022

Abstract

:
A new subclass of bi-close-to-convex functions associated with the generalized hypergeometric functions defined in ∆ = { z C : | z | < 1 } is introduced. The estimates for the general Taylor–Maclaurin coefficients of the functions in the introduced subclass are obtained by making use of Faber polynomial expansions. In particular, several previous results are generalized.

1. Introduction

Denote by A the class of analytic functions in ∆ : = { z C : | z | < 1 } of the form:
f ( z ) = z + n = 2 a n z n ( z ) .
Likewise, denote by S ( A ) the class of analytic functions that are univalent in ∆.
For the functions f A and h A given by
h ( z ) = z + n = 2 ψ n z n ( z ) ,
we define the Hadamard product of f and h as the following:
( f h ) ( z ) : = z + n = 2 a n ψ n z n = : ( h f ) ( z ) ( z ) .
Let f 1 and f 2 be two analytic functions in ∆. Then, the function f 1 is subordinate to the function f 2 and written as follows:
f 1 ( z ) f 2 ( z ) ,
if there is a Schwarz function u ( z ) , so that
f 1 ( z ) = f 2 u ( z ) .
Furthermore, if the function f 2 is univalent in ∆, then it follows that
f 1 ( z ) f 2 ( z ) ( z ) f 1 ( 0 ) = f 2 ( 0 ) and f 1 ( ) f 2 ( ) .
Let P denote the class of analytic functions φ having the following form:
φ ( z ) = 1 + P 1 z + P 2 z 2 + P 3 z 3 + ( P 1 > 0 )
and φ ( z ) > 0   ( z ) .
For f A and 0 α < 1 , we recall here the following well-known subclasses of the analytic function class A :
(i)
f is called to be a starlike function of the order α if
z f ( z ) f ( z ) > α ( z ) .
We denote this subclass with S * ( α ) .
(ii)
f is called to be a convex function of the order α if
1 + z f ( z ) f ( z ) > α ( z ) .
We denote this subclass with C ( α ) .
(iii)
f is called to be a close-to-convex function of the order α if
z f ( z ) g ( z ) > α ( z ) ,
where g S * ( 0 ) = : S * . We denote this subclass with K ( α ) .
For s 1 , s 2 , s 3 C , the generalized Gauss hypergeometric function 2 F 1 ( s 1 , s 2 , s 3 , k ; z ) is given here by
2 F 1 ( s 1 , s 2 , s 3 , k ; z ) = Γ ( s 3 ) Γ ( s 2 ) n = 0 ( s 1 ) n Γ ( k n + s 2 ) Γ ( k n + s 3 ) z n n ! = 1 + Γ ( s 3 ) Γ ( s 2 ) n = 2 Γ k ( n 1 ) + s 2 ( s 1 ) n 1 Γ k ( n 1 ) + s 3 ( n 1 ) ! z n 1 ,
where ( x ) n is the Pochhammer symbol, k > 0 , ( s 3 s 2 1 ) > 0 , s 3 0 , 1 , 2 , and z .
According to the generalized Gauss hypergeometric function defined in (4), Hussain et al. [1] considered the operator J ( s 1 , s 2 , s 3 , k ) as the following:
J ( s 1 , s 2 , s 3 , k ) f ( z ) = f ( z ) z 2 F 1 ( s 1 , s 2 , s 3 , k ; z ) = z + n = 2 γ n a n z n ,
where f A and
γ n = γ ( s 1 , s 2 , s 3 , k , n ) = ( s 1 ) n 1 Γ k ( n 1 ) + s 2 Γ ( s 3 ) ( n 1 ) ! Γ k ( n 1 ) + s 3 Γ ( s 2 ) .
It is well-known that a function g S has its inverse g 1 , which meets the following equality:
g ( g 1 ( ζ ) ) = ζ | ζ | < r 0 ( g ) ; r 0 ( g ) 1 4 .
We say that a function g S is bi-univalent in ∆ if g and g 1 are univalent in ∆, and we denote the subclass with Σ ( S ) . A history of the functions in Σ can be found in [2,3]. Lewin considered the class Σ in [4] and obtained that | a 2 | < 1.51 . In [5], Brannan and Clunie proved that | a 2 | < 2 . In [6], Netanyahu improved the results above to | a 2 | < 4 3 .
Some elements of functions in the class Σ are presented below (see [2]):
f 1 ( z ) = z 1 z , f 2 ( z ) = log ( 1 z ) and f 3 ( z ) = 1 2 log 1 + z 1 z ,
and their corresponding inverses are given by
f 1 1 ( ω ) = ω 1 + ω , f 2 1 ( ω ) = e ω 1 e ω and f 3 1 ( ω ) = e 2 ω 1 e 2 ω + 1 .
Certain subclasses of the bi-univalent function class Σ , considered by Brannan and Taha [7], are similar to the subclasses S * ( α ) and C ( α ) (see [8]). The authors of [7] introduced the subclasses S Σ * ( α ) of bi-starlike functions of the order α , and C Σ * ( α ) of bi-convex functions of the order α , as presented below:
S Σ * ( α ) : = f : f Σ , arg z f ( z ) f ( z ) < α π 2 ( z ) and arg ω F ( ω ) F ( ω ) < α π 2 ( ω )
and
C Σ * ( α ) : = f : f Σ , arg 1 + z f ( z ) f ( z ) < α π 2 ( z ) and arg 1 + ω F ( ω ) F ( ω ) < α π 2 ( ω ) ,
where
F ( ω ) : = f 1 ( ω ) = ω a 2 ω 2 + ( 2 a 2 2 a 3 ) ω 3 ( 5 a 2 3 5 a 2 a 3 + a 4 ) ω 4 + = ω + n = 2 A n ω n .
For each of the above bi-univalent function subclasses, S Σ * ( α ) and C Σ * ( α ) , non-sharp bounds of the first two coefficients | a 2 | and | a 3 | are given in [7]. The widely cited paper by Srivastava et al. [3] not only represents one of the most important studies of bi-univalent functions, but it also resuscitated the study of bi-univalent functions in recent years. Many subsequent papers investigated the problems concerned with bi-univalent functions, such as [9,10,11,12].
Next, we introduce a new subclass, K Σ ( β , γ n ) , of bi-close-to-convex functions.
Definition 1.
For 0 β 1 and γ n given by (6), a function f Σ is said to be in the class K Σ ( β , γ n ) if there exists a function g S * and if it satisfies the following subordination conditions:
z J ( s 1 , s 2 , s 3 , k ) f ( z ) + β z 2 J ( s 1 , s 2 , s 3 , k ) f ( z ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) g ( z ) + β z J ( s 1 , s 2 , s 3 , k ) g ( z ) φ ( z ) ( z )
and
ω J ( s 1 , s 2 , s 3 , k ) F ( ω ) + β ω 2 J ( s 1 , s 2 , s 3 , k ) F ( ω ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) G ( ω ) + β ω J ( s 1 , s 2 , s 3 , k ) G ( ω ) φ ( ω ) ( ω ) ,
where φ P , the function F given by (7) is the analytic extension of f 1 , and the function G is an extension of g 1 as the following:
G ( ω ) = ω b 2 ω 2 + ( 2 b 2 2 b 3 ) ω 3 ( 5 b 2 3 5 b 2 b 3 + b 4 ) ω 4 + ( ω ) .
By setting b n = a n ( n N \ { 1 } ) , we can define the bi-starlike function class S Σ ( β , γ n ) given below:
z J ( s 1 , s 2 , s 3 , k ) f ( z ) + β z 2 J ( s 1 , s 2 , s 3 , k ) f ( z ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) f ( z ) + β z J ( s 1 , s 2 , s 3 , k ) f ( z ) φ ( z ) ( z )
and
ω J ( s 1 , s 2 , s 3 , k ) F ( ω ) + β ω 2 J ( s 1 , s 2 , s 3 , k ) F ( ω ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) F ( ω ) + β ω J ( s 1 , s 2 , s 3 , k ) F ( ω ) φ ( ω ) ( ω ) .
Remark 1.
If we set φ ( z ) = 1 + ( 1 2 η ) z 1 z   ( 0 η < 1 ) and replace J ( s 1 , s 2 , s 3 , k ) by B ( λ , α , β ) in (8), (9), (11), and (12), where
B ( λ , α , β ) f ( z ) = z + n = 2 Γ ( 1 + ( n 1 ) λ ) [ ( n 1 ) λ ] n 2 e ( n 1 ) λ ( n 1 ) ! E α , β ( ( n 1 ) λ ) Γ ( β + α ( n 1 ) ) a n z n = z + n = 2 ϕ n a n z n ( 0 < λ 1 ; α C , Re ( α ) > 0 ; β C \ Z 0 ) ,
E α , β ( z ) = z + n = 2 Γ ( β ) Γ ( β + α ( n 1 ) ) z n
and
ϕ n = Γ ( 1 + ( n 1 ) λ ) [ ( n 1 ) λ ] n 2 e ( n 1 ) λ ( n 1 ) ! E α , β ( ( n 1 ) λ ) Γ ( β + α ( n 1 ) ) ,
then we obtain the function classes U Σ α , β , λ ( η , ν ) and P Σ α , β , λ ( η , ν ) given by Srivastava et al. [11].
Applying Faber polynomial expansions to f A , we get the coefficient expansion of the inverse mapping, as follows (see [13]; also see the recent developments [14,15,16,17,18], each of which is based upon the Faber polynomial expansions):
F ( ω ) = f 1 ( ω ) = ω + n = 2 1 n K n 1 n ( a 2 , a 3 , ) ω n = ω + n = 2 A n ω n ,
where
K n 1 n ( a 2 , a 3 , ) = ( n ) ! ( 2 n + 1 ) ! ( n 1 ) ! a 2 n 1 + ( n ) ! ( 2 ( n + 1 ) ) ! ( n 3 ) ! a 2 n 3 a 3 + ( n ) ! ( 2 n + 3 ) ! ( n 4 ) ! a 2 n 4 a 4 + ( n ) ! ( 2 ( n + 2 ) ) ! ( n 5 ) ! a 2 n 5 [ ( n + 2 ) a 3 2 + a 5 ] + ( n ) ! ( 2 n + 5 ) ! ( n 6 ) ! a 2 n 6 [ ( 2 n + 5 ) a 3 a 4 + a 6 ] + j 7 a 2 n j U j .
In this paper, an expression such as ( n ) ! is to be symbolically explained by
( n ) ! : = ( n ) ( n 1 ) ( n 2 ) = Γ ( 1 n ) ( n N 0 ) ,
and U j   ( 7 j n ) is a homogeneous polynomial of a 2 , a 3 , , a n .
In particular, K 1 2 = 2 a 2 , K 2 3 = 3 ( 2 a 2 2 a 3 ) , and K 3 4 = 4 ( 5 a 2 2 5 a 2 a 3 + a 4 ) . In general, an expansion of K n p is as follows (see [2]):
K n p = p a n + p ( p 1 ) 2 D n 2 + p ! ( p 3 ) ! 3 ! D n 3 + + p ! ( p n ) ! n ! D n n ,
where
D n p = D n p ( a 2 , a 3 , ) ,
and (see [19])
D n m ( a 1 , a 2 , , a n ) = n = 1 m ! i 1 ! i n ! a 1 i 1 a n i n .
While a 1 = 1 , the above sum is taken over by the non-negative integers i 1 , , i n satisfying
i 1 + 2 i 2 + + n i n = n i 1 + i 2 + + i n = m .
Finally, we get
D n n ( a 1 , a 2 , , a n ) = a 1 n .
Lemma 1
(see [20]). Let the function s ( z ) given by
s ( z ) = n = 1 s n z n A ( | z | < 1 )
be a Schwarz function, then | s n |   1 . Moreover, if ϑ 0 , then
| s 2 + ϑ s 1 2 | 1 + ( ϑ 1 ) | s 1 | 2 .
In the investigation of bi-univalent functions, estimates for the first two coefficients are usually obtained. Furthermore, bounds of the first three Taylor–Maclaurin coefficients are given in [21]. Essentially motivated by some recent works (for example, see [11,21,22,23]), in this paper, we investigate the estimates for the Taylor–Maclaurin coefficients of the functions in K Σ ( β , γ n ) and S Σ ( β , γ n ) . Several previous results are generalized.

2. Main Results

In this section, we find estimates for the Taylor–Maclaurin coefficients of the functions in K Σ ( β , γ n ) by using the Faber polynomial expansion method.
Theorem 1.
Let 0 β 1 and f K Σ ( β , γ n ) . If a k = 0 and b k = 0 for 2 k n 1 , then
| a n |   1 + P 1 n [ 1 + ( n 1 ) β ] | γ n | .
Proof. 
Suppose that f K Σ ( β , γ n ) , then we have a function g ( z ) = z + n = 2 b n z n S * , such that
z J ( s 1 , s 2 , s 3 , k ) f ( z ) + β z 2 J ( s 1 , s 2 , s 3 , k ) f ( z ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) g ( z ) + β z J ( s 1 , s 2 , s 3 , k ) g ( z ) φ ( z ) ( z ) .
According to the Faber polynomial expansion, we get
z J ( s 1 , s 2 , s 3 , k ) f ( z ) + β z 2 J ( s 1 , s 2 , s 3 , k ) f ( z ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) g ( z ) + β z J ( s 1 , s 2 , s 3 , k ) g ( z ) = 1 + n = 2 ( [ 1 + β ( n 1 ) ] γ n ( n a n b n ) + t = 1 n 2 γ n t [ 1 + ( n t 1 ) β ] · K t 1 [ ( 1 + β ) γ 2 b 2 , ( 1 + 2 β ) γ 3 b 3 , , ( 1 + t β ) γ t + 1 b t + 1 ] · [ ( n t ) a n t b n t ] z n 1 .
Moreover, for the function F = f 1 , we have a function G ( ω ) = ω + n = 2 B n ω n S * , such that
ω J ( s 1 , s 2 , s 3 , k ) F ( ω ) + β ω 2 J ( s 1 , s 2 , s 3 , k ) F ( ω ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) G ( ω ) + β ω J ( s 1 , s 2 , s 3 , k ) G ( ω ) φ ( ω ) ( ω ) .
Since
F ( ω ) = ω + n = 2 A n ω n ,
we get
ω J ( s 1 , s 2 , s 3 , k ) F ( ω ) + β ω 2 J ( s 1 , s 2 , s 3 , k ) F ( ω ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) G ( ω ) + β ω J ( s 1 , s 2 , s 3 , k ) G ( ω ) = 1 + n = 2 ( [ 1 + β ( n 1 ) ] γ n ( n A n B n ) + t = 1 n 2 γ n t [ 1 + ( n t 1 ) β ] · K t 1 [ ( 1 + β ) γ 2 B 2 , ( 1 + 2 β ) γ 3 B 3 , , ( 1 + t β ) γ t + 1 B t + 1 ] · [ ( n t ) A n t B n t ] ω n 1 .
Since both f and F = f 1 are in K Σ ( β , γ n ) , there exist the following two Schwarz functions:
u ( z ) = n = 1 c n z n
and
ν ( ω ) = n = 1 d n ω n ,
so that
z J ( s 1 , s 2 , s 3 , k ) f ( z ) + β z 2 J ( s 1 , s 2 , s 3 , k ) f ( z ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) g ( z ) + β z J ( s 1 , s 2 , s 3 , k ) g ( z ) = φ ( u ( z ) ) = 1 + P 1 c 1 z + ( P 1 c 2 + P 2 c 1 2 ) z 2 + = 1 + n = 1 k = 1 n P k D n k ( c 1 , c 2 , , c n ) z n
and
ω J ( s 1 , s 2 , s 3 , k ) F ( ω ) + β ω 2 J ( s 1 , s 2 , s 3 , k ) F ( ω ) ( 1 β ) J ( s 1 , s 2 , s 3 , k ) G ( ω ) + β ω J ( s 1 , s 2 , s 3 , k ) G ( ω ) = φ ( ν ( ω ) ) = 1 + P 1 d 1 ω + ( P 1 d 2 + P 2 d 1 2 ) ω 2 + = 1 + n = 1 k = 1 n P k D n k ( d 1 , d 2 , , d n ) ω n .
Then, from (15) and (17), we obtain
k = 1 n 1 P k D n 1 k ( c 1 , c 2 , , c n 1 ) = ( [ 1 + β ( n 1 ) ] γ n ( n a n b n ) + t = 1 n 2 γ n t [ 1 + ( n t 1 ) β ] · K t 1 [ ( 1 + β ) γ 2 b 2 , ( 1 + 2 β ) γ 3 b 3 , , ( 1 + t β ) γ t + 1 b t + 1 ] · [ ( n t ) a n t b n t ] .
Under the assumption that a k = 0 and b k = 0 for 2 k n 1 , we have
[ 1 + β ( n 1 ) ] γ n ( n a n b n ) = P 1 c n 1 .
Similarly, by using (16) and (18), we obtain
k = 1 n 1 P k D n 1 k ( d 1 , d 2 , , d n 1 ) = ( [ 1 + β ( n 1 ) ] γ n ( n A n B n ) + t = 1 n 2 γ n t [ 1 + ( n t 1 ) β ] · K t 1 [ ( 1 + β ) γ 2 B 2 , ( 1 + 2 β ) γ 3 B 3 , , ( 1 + t β ) γ t + 1 B t + 1 ] · [ ( n t ) A n t B n t ] .
Applying the hypothesis, we have A n = a n . Thus,
[ 1 + β ( n 1 ) ] γ n ( n a n B n ) = P 1 d n 1 .
By making moduli of each member in (20) and (22) for | B n |   n and | b n |   n , and using Lemma 1, we find that
| a n |   1 + P 1 n [ 1 + ( n 1 ) β ] | γ n | .
Now, the proof of Theorem 1 is completed. □
Setting
φ ( z ) = 1 + ( 1 2 η ) z 1 z ( 0 η < 1 ) and γ n = ϕ n
in Theorem 1, we get the following corollary.
Corollary 1.
Let 0 < λ 1 , 0 β 1 , α C , ( α ) > 0 and β C \ Z 0 . In addition, let f U Σ α , β , λ ( η , ν ) . If a k = 0 and b k = 0 for 2 k n 1 , then
| a n |   1 + 2 ( 1 η ) n [ 1 + ( n 1 ) β ] | ϕ k | .
Theorem 2.
Let 0 β 1 and f S Σ ( β , γ n ) . Suppose that P 2 = α P 1 ( 0 < α 1 ) . Then,
| a 2 |   P 1 ( 1 + β ) | γ 2 | P 1 ( 1 + β ) 2 | γ 2 | 2 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | P 1 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | 0 < P 1 ( 1 + β ) 2 | γ 2 | 2 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 |
and
| a 3 |   P 1 ( 1 + P 1 ) 2 ( 1 + 2 β ) | γ 3 | P 1 ( 1 + β ) 2 | γ 2 | 2 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | P 1 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | 0 < P 1 ( 1 + β ) 2 | γ 2 | 2 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | .
Proof. 
Setting n = 2 and n = 3 in (19) and (21), one can see that
( 1 + β ) γ 2 a 2 = P 1 c 1 ,
2 ( 1 + 2 β ) γ 3 a 3 ( 1 + β ) 2 γ 2 2 a 2 2 = P 1 c 2 + α P 1 c 1 2 ,
( 1 + β ) γ 2 a 2 = P 1 d 1
and
2 ( 1 + 2 β ) γ 3 a 3 + { 4 ( 1 + 2 β ) γ 3 ( 1 + β ) 2 γ 2 2 } a 2 2 = P 1 d 2 + α P 1 d 1 2 .
From (25), (26), and Lemma 1, we have
| a 2 | = P 1 | c 1 | ( 1 + β ) | γ 2 | = P 1 | d 1 | ( 1 + β ) | γ 2 | P 1 ( 1 + β ) | γ 2 | .
Now, by adding (26)–(28), we obtain
{ 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 } a 2 2 = P 1 [ ( c 2 + α c 1 2 ) + ( d 2 + α d 1 2 ) ]
such that
a 2 2 = P 1 [ ( c 2 + α c 1 2 ) + ( d 2 + α d 1 2 ) ] 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 .
By using Lemma 1, we obtain
| a 2 2 | P 1 [ 1 + ( α 1 ) | c 1 | 2 + 1 + ( α 1 ) | d 1 | 2 ] | 4 ( 1 + 2 β ) | γ 3 | 2 ( 1 + β ) 2 | γ 2 | 2 | P 1 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | .
Therefore, we have
| a 2 |   P 1 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | .
Combining (29) and (31), we derive the estimate on | a 2 | as presented in (28).
By subtracting (28) from (26), we get
4 ( 1 + 2 β ) γ 3 ( a 3 a 2 2 ) = P 1 [ ( c 2 + α c 1 2 ) ( d 2 + α d 1 2 ) ] ,
so that
a 3 = a 2 2 + P 1 [ ( c 2 + α c 1 2 ) ( d 2 + α d 1 2 ) ] 4 ( 1 + 2 β ) γ 3 .
Plugging (30) into (32) and using Lemma 1, we have
| a 3 |   P 1 | 2 ( 1 + 2 β ) | γ 3 | ( 1 + β ) 2 | γ 2 | 2 | .
Moreover, if we substitute the value of a 2 2 from (26) into (27), we obtain
a 3 = P 1 [ ( c 2 + α c 1 2 + P 1 c 1 2 ] 2 ( 1 + 2 β ) γ 3 .
Thus, based on Lemma 1, we find that
| a 3 |   P 1 ( 1 + P 1 ) 2 ( 1 + 2 β ) | γ 3 | .
From (33) and (34), we get the estimate on | a 3 | , as presented in (24). This proves Theorem 2. □
Putting
φ ( z ) = 1 + ( 1 2 η ) z 1 z ( 0 η < 1 ) and γ n = ϕ n
in Theorem 2, we get the following corollary.
Corollary 2.
Let 0 < λ 1 , 0 β 1 , α C , ( α ) > 0 and β C \ Z 0 . Additionally, let f P Σ α , β , λ ( η , ν ) . Then,
| a 2 |   2 ( 1 η ) ( 1 + β ) | ϕ 2 | 0 η < 1 ( 1 + β ) 2 | ϕ 2 | 2 2 | 2 ( 1 + 2 β ) | ϕ 3 | ( 1 + β ) 2 | ϕ 2 | 2 | 2 ( 1 η ) | 2 ( 1 + 2 β ) | ϕ 3 | ( 1 + β ) 2 | ϕ 2 | 2 | 1 ( 1 + β ) 2 | ϕ 2 | 2 2 | 2 ( 1 + 2 β ) | ϕ 3 | ( 1 + β ) 2 | ϕ 2 | 2 | η < 1
and
| a 3 |   ( 1 η ) ( 1 + 2 ( 1 η ) ) ( 1 + 2 β ) | ϕ 3 | 0 η < 1 ( 1 + β ) 2 | ϕ 2 | 2 2 | 2 ( 1 + 2 β ) | ϕ 3 | ( 1 + β ) 2 | ϕ 2 | 2 | 2 ( 1 η ) | 2 ( 1 + 2 β ) | ϕ 3 | ( 1 + β ) 2 | ϕ 2 | 2 | 1 ( 1 + β ) 2 | ϕ 2 | 2 2 | 2 ( 1 + 2 β ) | ϕ 3 | ( 1 + β ) 2 | ϕ 2 | 2 | η < 1 .
Theorem 3. 
Let 0 β 1 and f S Σ ( β , γ n ) . Moreover, let P 2 = α P 1 (   0 < α 1 ) . Then,
| a 3 μ a 2 2 |   P 1 2 ( 1 + 2 β ) | γ 3 | 0 | y ( μ ) | P 1 4 ( 1 + 2 β ) | γ 3 | 2 | y ( μ ) | | y ( μ ) | P 1 4 ( 1 + 2 β ) | γ 3 | ,
where
y ( μ ) = ( 1 μ ) P 1 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 ( μ C ) .
Proof. 
According to (30) and (32), we have
a 3 μ a 2 2 = ( 1 μ ) P 1 [ ( c 2 + α c 1 2 ) + ( d 2 + α d 1 2 ) ] 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 + P 1 [ ( c 2 + α c 1 2 ) ( d 2 + α d 1 2 ) ] 4 ( 1 + 2 β ) γ 3 ,
so that
a 3 μ a 2 2 = ( 1 μ ) P 1 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 + P 1 4 ( 1 + 2 β ) γ 3 ( c 2 + α c 1 2 ) + ( 1 μ ) P 1 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 P 1 4 ( 1 + 2 β ) γ 3 ( d 2 + α d 1 2 ) ,
that is, that
a 3 μ a 2 2 = y ( μ ) + P 1 4 ( 1 + 2 β ) γ 3 ( c 2 + α c 1 2 ) + y ( μ ) P 1 4 ( 1 + 2 β ) γ 3 ( d 2 + α d 1 2 ) ,
where
y ( μ ) = ( 1 μ ) P 1 4 ( 1 + 2 β ) γ 3 2 ( 1 + β ) 2 γ 2 2 .
Taking the moduli of each member of (36), we have
| a 3 μ a 2 2 |   P 1 2 ( 1 + 2 β ) | γ 3 | 0 | y ( μ ) | P 1 4 ( 1 + 2 β ) | γ 3 | 2 | y ( μ ) | | y ( μ ) | P 1 4 ( 1 + 2 β ) | γ 3 | .
This completes the proof of Theorem 3. □
Setting
φ ( z ) = 1 + ( 1 2 η ) z 1 z ( 0 η < 1 ) and γ n = ϕ n
in Theorem 3, we get the following corollary.
Corollary 3.
Let 0 < λ 1 , 0 β 1 , α C , ( α ) > 0 and β C \ Z 0 . Furthermore, let f P Σ α , β , λ ( η , ν ) . Then,
| a 3 μ a 2 2 |   ( 1 η ) ( 1 + 2 β ) | ϕ 3 | 0 | h ( μ ) | ( 1 η ) 2 ( 1 + 2 β ) | ϕ 3 | 2 | y ( μ ) | | h ( μ ) | ( 1 η ) 2 ( 1 + 2 β ) | ϕ 3 | ,
where
h ( μ ) = ( 1 μ ) ( 1 η ) 2 ( 1 + 2 β ) ϕ 3 ( 1 + β ) 2 ϕ 2 2 .
By taking μ = 1 in Theorem 3, we have the following corollary.
Corollary 4.
Let 0 β 1 and f S Σ ( β , γ n ) . Then,
| a 3 a 2 2 |   P 1 2 ( 1 + 2 β ) | γ 3 | .

3. Conclusions

In the investigation of bi-univalent functions, estimates of the first two coefficients are usually obtained. However, there are bounds of the first three Taylor–Maclaurin coefficients, which are given in [21]. In this paper, we introduced a new subclass of bi-close-to-convex functions associated with the generalized hypergeometric functions defined in the open unit disk. By using the Faber polynomial expansions, the estimates for the general Taylor–Maclaurin coefficients of the functions in this subclass were derived. In particular, several previous results were generalized.

Author Contributions

Writing—original draft, J.Z.; Writing—review & editing, R.S. and J.-L.L. All authors contributed equally to this work. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

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 helped us to improve the paper.

Conflicts of Interest

The authors declare no conflict of interest.

References

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Zhai, J.; Srivastava, R.; Liu, J.-L. Faber Polynomial Coefficient Estimates of Bi-Close-to-Convex Functions Associated with Generalized Hypergeometric Functions. Mathematics 2022, 10, 3073. https://doi.org/10.3390/math10173073

AMA Style

Zhai J, Srivastava R, Liu J-L. Faber Polynomial Coefficient Estimates of Bi-Close-to-Convex Functions Associated with Generalized Hypergeometric Functions. Mathematics. 2022; 10(17):3073. https://doi.org/10.3390/math10173073

Chicago/Turabian Style

Zhai, Jie, Rekha Srivastava, and Jin-Lin Liu. 2022. "Faber Polynomial Coefficient Estimates of Bi-Close-to-Convex Functions Associated with Generalized Hypergeometric Functions" Mathematics 10, no. 17: 3073. https://doi.org/10.3390/math10173073

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