A Comprehensive Subclass of Bi-Univalent Functions Associated with

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Sep 25, 2018 - 1,2Department of Mathematics, The University of Jordan, Amman 11942, Jordan. 3School ..... of complex order, Afrika Matematika (2018) 1–7.
arXiv:1809.09365v1 [math.CV] 25 Sep 2018

A Comprehensive Subclass of Bi-Univalent Functions Associated with Chebyshev Polynomials of the Second Kind Feras Yousef1,∗ , Somaia Alroud2 , Mohamed Illafe3 1,2 3

Department of Mathematics, The University of Jordan, Amman 11942, Jordan.

School of Engineering, Math, & Technology, Navajo Technical University, Crownpoint, NM 87313, USA. e-mail: 1 [email protected], 2 [email protected], 3 [email protected]

Abstract — Our objective in this paper is to introduce and investigate a newly-constructed subclass of normalized analytic and bi-univalent functions by means of the Chebyshev polynomials of the second kind. Upper bounds for the second and third Taylor-Maclaurin coefficients, and also Fekete-Szego¨ inequalities of functions belonging to this subclass are founded. Several connections to some of the earlier known results are also pointed out.

Keywords: Analytic functions; Univalent and bi-univalent functions; Taylor-Maclaurin series; Fekete-Szego¨ problem; Chebyshev polynomials; Coefficient bounds; Subordination. 2010 Mathematics Subject Classification. Primary 30C45; Secondary 30C50.

1.

Introduction, Definitions and Notations

Let A denote the class of all analytic functions f defined in the open unit disk U = {z ∈ C : |z| < 1} and normalized by the condition f (0) = f ′ (0) − 1 = 0. Thus each f ∈ A has a Taylor-Maclaurin series expansion of the form: ∞ X an zn , (z ∈ U). (1.1) f (z) = z + n=2

Further, let S denote the class of all functions f ∈ A which are univalent in U (for details, see [15]; see also some of the recent investigations [3–7]). Given two functions f and 1 in A. The function f is said to be subordinate to 1 in U, written as f (z) ≺ 1(z), if there exists a Schwarz function ω(z), analytic in U, with ω(0) = 0 and |ω(z)| < 1 for all z ∈ U, such that f (z) = 1 (ω(z)) for all z ∈ U. Furthermore, if the function 1 is univalent in U, then we have the following equivalence (see [21] and [28]): f (z) ≺ 1(z) ⇔ f (0) = 1(0) and f (U) ⊂ 1(U). ∗

Corresponding author.

1

Two of the important and well-investigated subclasses of the analytic and univalent function class S are the class S∗ (α) of starlike functions of order α in U and the class K(α) of convex functions of order α in U. By definition, we have ∗

S (α) := and K(α) :=

(

(

) z f ′ (z) > α, f : f ∈ S and Re f (z) (

) z f ′′ (z) f : f ∈ S and Re 1 + ′ > α, f (z) (

) (z ∈ U; 0 ≤ α < 1) , ) (z ∈ U; 0 ≤ α < 1) .

(1.2)

(1.3)

It is clear from the definitions (1.2) and (1.3) that K(α) ⊂ S∗ (α). Also we have f (z) ∈ K(α) iff z f ′ (z) ∈ S∗ (α), and ∗

f (z) ∈ S (α) iff

Z

z 0

f (t) dt = F(z) ∈ K(α). t

It is well-known [15] that every function f ∈ S has an inverse map f −1 that satisfies the following conditions: f −1 ( f (z)) = z (z ∈ U), and   f f −1 (w) = w

  |w| < r0 ( f ); r0 ( f ) ≥ 41 .

In fact, the inverse function is given by f −1 (w) = w − a2 w2 + (2a22 − a3 )w3 − (5a32 − 5a2 a3 + a4 )w4 + · · · .

(1.4)

A function f ∈ A is said to be bi-univalent in U if both f (z) and f −1 (z) are univalent in U. Let Σ denote the class of bi-univalent functions in U given by (1.1). For a brief history and some interesting examples of functions and characterization of the class Σ, see Srivastava et al. [26], Frasin and Aouf [16], and Magesh and Yamini [19]. In 1967, Lewin [17] investigated the bi-univalent function class √ Σ and showed that |a2 | < 1.51. Subsequently, Brannan and Clunie [9] conjectured that |a2 | ≤ 2. Later, Netanyahu [22] showed that max |a2 | = 43 if f ∈ Σ. Brannan and Taha [13] introduced certain subclasses of a bi-univalent function class Σ similar to the familiar subclasses S∗ (α) and K(α) of starlike and convex functions of order α (0 ≤ α < 1), respectively (see [8]). Thus, following the works of Brannan and Taha [13], for 0 ≤ α < 1, a function f ∈ Σ is in the class S∗Σ (α) of bi-starlike functions of order α; or KΣ (α) of bi-convex functions of order α if both f and f −1 are respectively starlike or convex functions of order α. Recently, many researchers have introduced and investigated several interesting subclasses of the bi-univalent function class Σ and they have found non-sharp estimates on the first two TaylorMaclaurin coefficients |a2 | and |a3 |. In fact, the aforecited work of Srivastava et al. [26] essentially revived the investigation of various subclasses of the bi-univalent function class Σ in recent years; it was followed by such works as those by Frasin and Aouf [16], Xu et al. [27], C ¸ aglar ˘ et al. [14], and others (see, for example, [1, 18, 23, 24] and [25]). The coefficient estimate problem for each of the following Taylor-Maclaurin coefficients |an | (n ∈ N\{1, 2}) for each f ∈ Σ given by (1.1) is still an open problem. 2

The Chebyshev polynomials are a sequence of orthogonal polynomials that are related to De Moivre’s formula and which can be defined recursively. They have abundant properties, which make them useful in many areas in applied mathematics, numerical analysis and approximation theory. There are four kinds of Chebyshev polynomials, see for details Doha [12] and Mason [20]. The Chebyshev polynomials of degree n of the second kind, which are denoted Un (t), are defined for t ∈ [−1, 1] by the following three-terms recurrence relation: U0 (t) = 1, U1 (t) = 2t, Un+1 (t) := 2tUn (t) − Un−1 (t). The first few of the Chebyshev polynomials of the second kind are U2 (t) = 4t2 − 1, U3 (t) = 8t3 − 4t, U4 (t) = 16t4 − 12t2 + 1, · · · .

(1.5)

The generating function for the Chebyshev polynomials of the second kind, Un (t), is given by: ∞

X 1 Un (t)zn (z ∈ U). = H(z, t) = 2 1 − 2tz + z n=0 µ

Yousef et al. [29] introduced the following class BΣ (β, λ, δ) of analytic and bi-univalent functions defined as follows: Definition 1.1. For λ ≥ 1, µ ≥ 0, δ ≥ 0 and 0 ≤ β < 1, a function f ∈ Σ given by (1.1) is said to be in the µ class BΣ (β, λ, δ) if the following conditions hold for all z, w ∈ U:

and

  !µ !µ−1   f (z) f (z) Re (1 − λ) + λ f ′ (z) + ξδz f ′′ (z) > β z z   !µ !µ−1   1(w) 1(w) + λ1′ (w) + ξδw1′′ (w) > β, Re (1 − λ) w w

where the function 1(w) = f −1 (w) is defined by (1.4) and ξ =

(1.6)

(1.7)

2λ+µ 2λ+1 .

This work is concerned with the coefficient bounds for the Taylor-Maclaurin coefficients |a2 | and µ |a3 | and the Fekete-Szego¨ inequality for functions belonging to the class BΣ (λ, δ, t) defined as follows:   Definition 1.2. For λ ≥ 1, µ ≥ 0, δ ≥ 0 and t ∈ 12 , 1 , a function f ∈ Σ given by (1.1) is said to be in the µ class BΣ (λ, δ, t) if the following subordinations hold for all z, w ∈ U: f (z) (1 − λ) z and 1(w) (1 − λ) w





f (z) + λ f (z) z ′

1(w) + λ1 (w) w ′

!µ−1

!µ−1

+ ξδz f ′′ (z) ≺ H(z, t) :=

+ ξδw1′′ (w) ≺ H(w, t) :=

where the function 1(w) = f −1 (w) is defined by (1.4) and ξ = 3

2λ+µ 2λ+1 .

1 1 − 2tz + z2 1 , 1 − 2tw + w2

(1.8)

(1.9)

The following special cases of Definitions 1.2 are worthy of note: Remark 1. Note that for λ = 1, µ = 1 and δ = 0, the class of functions BΣ1 (1, 0, t) := BΣ (t) have been introduced and studied by Altinkaya and Yalc¸in [2], for µ = 1 and δ = 0, the class of functions BΣ1 (λ, 0, t) := BΣ (λ, t) have been introduced and studied by Bulut et al. [10], for δ = 0, the class of µ µ functions BΣ (λ, 0, t) := BΣ (λ, t) have been introduced and studied by Bulut et al. [11], and for µ = 1, the class of functions BΣ1 (λ, δ, t) := BΣ (λ, δ, t) have been introduced and studied by Yousef et al. [30]. µ

Coefficient bounds for the function class BΣ(λ, δ, t)

2.

In this section, we establish coefficient bounds for the Taylor-Maclaurin coefficients |a2 | and |a3 | of the µ function f ∈ BΣ (λ, δ, t). Several corollaries of the main result are also considered. µ

Theorem 2.1. Let the function f (z) given by (1.1) be in the class BΣ (λ, δ, t). Then √ 2t 2t

|a2 | ≤ p |(λ + µ + 2ξδ)2 − 2[2(λ + µ + 2ξδ)2 − (2λ + µ)(µ + 1) − 12ξδ]t2 |

and

|a3 | ≤

2t 4t2 + . 2 2λ + µ + 6ξδ (λ + µ + 2ξδ)

(2.1)

(2.2)

µ

Proof. Let f ∈ BΣ (λ, δ, t). From (1.8) and (1.9), we have f (z) (1 − λ) z and 1(w) (1 − λ) w





!µ−1

+ ξδz f ′′ (z) = 1 + U1 (t)w(z) + U2 (t)w2 (z) + · · ·

(2.3)

!µ−1

+ ξδw1′′ (w) = 1 + U1 (t)v(w) + U2 (t)v2 (w) + · · · ,

(2.4)

f (z) + λ f (z) z ′

1(w) + λ1 (w) w ′

for some analytic functions w(z) = c1 z + c2 z2 + c3 z3 + · · ·

(z ∈ U),

v(w) = d1 w + d2 w2 + d3 w3 + · · ·

(w ∈ U),

and such that w(0) = v(0) = 0, |w(z)| < 1 (z ∈ U) and |v(w)| < 1 (w ∈ U). It follows from (2.3) and (2.4) that f (z) (1 − λ) z



f (z) + λ f (z) z ′

!µ−1

h i + ξδz f ′′ (z) = 1 + U1 (t)c1 z + U1 (t)c2 + U2 (t)c21 z2 + · · ·

and 1(w) (1 − λ) w



1(w) + λ1 (w) w ′

!µ−1

h i + ξδw1′′ (w) = 1 + U1 (t)d1 w + U1 (t)d2 + U2 (t)d21 )w2 + · · · .

4

Equating the coefficients yields  λ + µ + 2ξδ a2 = U1 (t)c1 , " !  # µ−1 2  6δ (2λ + µ) a3 = U1 (t)c2 + U2 (t)c21 , a2 + 1 + 2 2λ + 1

(2.5) (2.6)

and  − λ + µ + 2ξδ a2 = U1 (t)d1 , ! "  #  µ+3 12δ 6δ 2 a3 = U1 (t)d2 + U2 (t)d21 . + a − 1+ (2λ + µ) 2 2λ + 1 2 2λ + 1

(2.7) (2.8)

From (2.5) and (2.7), we obtain c1 = −d1 , and

   2 λ + µ + 2ξδ 2 a22 = U12 (t) c21 + d21 .

By adding (2.6) to (2.8), we get     12δ a22 = U1 (t) (c2 + d2 ) + U2 (t) c21 + d21 . (2λ + µ) 1 + µ + 2λ + 1 By using (2.10) in (2.11), we obtain     2U2 (t) λ + µ + 2ξδ 2  2  a = U1 (t) (c2 + d2 ) . (2λ + µ)(µ + 1) + 12ξδ −  2  U12 (t)

(2.9) (2.10)

(2.11)

(2.12)

It is fairly well known [15] that if |w(z)| < 1 and |v(w)| < 1, then |c j | ≤ 1 and |d j | ≤ 1 for all j ∈ N.

(2.13)

By considering (1.5) and (2.13), we get from (2.12) the desired inequality (2.1). Next, by subtracting (2.8) from (2.6), we have       6δ 6δ a3 − 2(2λ + µ) 1 + a22 = U1 (t) (c2 − d2 ) + U2 (t) c21 − d21 . 2(2λ + µ) 1 + 2λ + 1 2λ + 1

(2.14)

Further, in view of (2.9), it follows from (2.14) that a3 = a22 +

U1 (t) (c2 − d2 ) . 2(2λ + µ + 6ξδ)

(2.15)

By considering (2.10) and (2.13), we get from (2.15) the desired inequality (2.2). This completes the proof of Theorem 2.1. Taking λ = 1, µ = 1 and δ = 0 in Theorem 2.1, we get the following consequence. Corollary 2.2. [10] Let the function f (z) given by (1.1) be in the class BΣ (t). Then √ t 2t , |a2 | ≤ √ 1 − t2 and

2 |a3 | ≤ t2 + t. 3 5

Taking µ = 1 and δ = 0 in Theorem 2.1, we get the following consequence. Corollary 2.3. [10] Let the function f (z) given by (1.1) be in the class BΣ (λ, t). Then √ 2t 2t

|a2 | ≤ p |(λ + 1)2 − 4λ2 t2 |

and

|a3 | ≤

2t 4t2 . + 2 2λ + 1 (λ + 1)

Taking δ = 0 in Theorem 2.1, we get the following consequence. µ

Corollary 2.4. [11] Let the function f (z) given by (1.1) be in the class BΣ (λ, t). Then √ 2t 2t

|a2 | ≤ p |(λ + µ)2 − 2[2(λ + µ)2 − (2λ + µ)(µ + 1)]t2 |

and

|a3 | ≤

2t 4t2 . + 2 2λ +µ (λ + µ)

Taking µ = 1 in Theorem 2.1, we get the following consequence. Corollary 2.5. [30] Let the function f (z) given by (1.1) be in the class BΣ (λ, δ, t). Then √ 2t 2t |a2 | ≤ q   (1 + λ + 2δ)2 − 4 (λ + 2δ)2 − 2δ t2 and

|a3 | ≤

3.

2t 4t2 + . 2 1 + 2λ + 6δ (1 + λ + 2δ) µ

Fekete-Szego¨ problem for the function class BΣ(λ, δ, t) µ

Now, we are ready to find the sharp bounds of Fekete-Szego¨ functional a3 − ηa22 defined for BΣ (λ, δ, t) given by (1.1). The results presented in this section improve or generalize the earlier results of Bulut et al. [11], Yousef et al. [30], and other authors in terms of the ranges of the parameter under consideration. µ

Theorem 3.1. Let the function f (z) given by (1.1) be in the class BΣ (λ, δ, t). Then for some η ∈ R,

where

      2 |a3 − ηa2 | ≤      M :=

2t 2λ+µ+6ξδ ,

|η − 1| ≤ M

8|η−1|t3 2 −2 2(λ+µ+2ξδ)2 −((2λ+µ)(µ+1)+12ξδ) t2 , (λ+µ+2ξδ) | [ ] |

h i (λ + µ + 2ξδ)2 − 2 2(λ + µ + 2ξδ)2 − ((2λ + µ)(µ + 1) + 12ξδ) t2 4(2λ + µ + 2ξδ)t2

6

(3.1)

|η − 1| ≥ M

.

µ

Proof. Let f ∈ BΣ (λ, δ, t). By using (2.12) and (2.15) for some η ∈ R, we get    a3 − ηa22 = 1 − η 

 U13 (t) (c2 + d2 )   + U1 (t) (c2 − d2 )  2  2(2λ + µ + 6ξδ) 2 (2λ + µ)(µ + 1) + 12ξδ U1 (t) − 2(λ + µ + 2ξδ) U2 (t)

! ! # 1 1 c2 + h(η) − d2 , = U1 (t) h(η) + 2(2λ + µ + 6ξδ) 2(2λ + µ + 6ξδ)

where

"

 U12 (t) 1 − η h(η) = .  (2λ + µ)(µ + 1) + 12ξδ U12 (t) − 2(λ + µ + 2ξδ)2 U2 (t)

Then, in view of (1.5), we easily conclude that

 1 2t   2λ+µ+6ξδ , |h(η)| ≤ 2(2λ+µ+6ξδ)    |a3 − ηa22 | ≤    1   4|h(η)|t, |h(η)| ≥ 2(2λ+µ+6ξδ)

This proves Theorem 3.1.

We end this section with some corollaries concerning the sharp bounds of Fekete-Szego¨ functional µ a3 − ηa22 defined for f ∈ BΣ (λ, δ, t) given by (1.1). Taking η = 1 in Theorem 3.1, we get the following corollary.

µ

Corollary 3.2. Let the function f (z) given by (1.1) be in the class BΣ (λ, δ, t). Then |a3 − a22 | ≤

2t . 2λ + µ + 6ξδ

Taking λ = 1, µ = 1 and δ = 0 in Theorem 3.1, we get the following corollary. Corollary 3.3. [11] Let the function f (z) given by (1.1) be in the class BΣ (t). Then for some η ∈ R,  2 2   |η − 1| ≤ 1−t  2 3 t, 3t   |a3 − ηa22 | ≤    2  2|η−1|t3  , |η − 1| ≥ 1−t 1−t2 3t2 Taking η = 1 in Corollary 3.3, we get the following corollary.

Corollary 3.4. [30] Let the function f (z) given be (1.1) be in the class BΣ (t). Then 2 |a3 − a22 | ≤ t. 3 Taking µ = 1 and δ = 0 in Theorem 3.1, we get the following corollary. Corollary 3.5. [11] Let the function f (z) given by (1.1) be in the class BΣ (λ, t). Then for some η ∈ R,  |(1+λ)2 −4λ2 t2 |  2t  , |η − 1| ≤ 4(1+2λ)t2   1+2λ   (3.2) |a3 − ηa22 | ≤    8|η−1|t3  |(1+λ)2 −4λ2 t2 |   (1+λ)2 −4λ2 t2 , |η − 1| ≥ 4(1+2λ)t2 | | 7

Taking η = 1 in Corollary 3.5, we get the following corollary. Corollary 3.6. [30] Let the function f (z) given by (1.1) be in the class BΣ (λ, t). Then |a3 − a22 | ≤

2t . 1 + 2λ

Taking δ = 0 in Theorem 3.1, we get the following corollary. µ

Corollary 3.7. [11] Let the function f (z) given by (1.1) be in the class BΣ (λ, t). Then for some η ∈ R,        2 |a3 − ηa2 | ≤      

2t 2λ+µ ,

|η − 1| ≤

8|η−1|t3 , |(λ+µ)2 −2[2(λ+µ)2 −(2λ+µ)(µ+1)]t2 |

|η − 1| ≥

|(λ+µ)2 −2[2(λ+µ)2 −(2λ+µ)(µ+1)]t2 | 4(2λ+µ)t2

|(λ+µ)2 −2[2(λ+µ)2 −(2λ+µ)(µ+1)]t2 |

(3.3)

4(2λ+µ)t2

Taking µ = 1 in Theorem 3.1, we get the following corollary. Corollary 3.8. [30] Let the function f (z) given by (1.1) be in the class BΣ (λ, δ, t). Then for some η ∈ R,  |(1+λ+2δ)2 −4[(λ+2δ)2 −2δ]t2 |  2t  , |η − 1| ≤   1+2λ+6δ 4(1+2λ+6δ)t2   |a3 − ηa22 | ≤  (3.4)  2 −4 (λ+2δ)2 −2δ t2  3 (1+λ+2δ)  8|η−1|t | | [ ]   (1+λ+2δ)2 −4 (λ+2δ)2 −2δ t2 , |η − 1| ≥ 4(1+2λ+6δ)t2 | [ ] |

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