Next Article in Journal
Statistical Inferences about Parameters of the Pseudo Lindley Distribution with Acceptance Sampling Plans
Next Article in Special Issue
On the Relative Φ-Growth of Hadamard Compositions of Dirichlet Series
Previous Article in Journal
On the Impact of Some Fixed Point Theorems on Dynamic Programming and RLC Circuit Models in R-Modular b-Metric-like Spaces
Previous Article in Special Issue
Coefficient Inequalities for q-Convex Functions with Respect to q-Analogue of the Exponential Function
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Article

Sharp Coefficient Bounds for Starlike Functions Associated with Cosine Function †

1
Department of Mathematics, Government College University Faisalabad, Faisalabad 38000, Pakistan
2
Faculty of Mathematics and Computer Science, Babeş-Bolyai University, 400084 Cluj-Napoca, Romania
*
Author to whom correspondence should be addressed.
Dedicated to the memory of Professor Lawrence Allen Zalcman (1943–2022).
These authors contributed equally to this work.
Axioms 2024, 13(7), 442; https://doi.org/10.3390/axioms13070442
Submission received: 31 May 2024 / Revised: 24 June 2024 / Accepted: 27 June 2024 / Published: 29 June 2024
(This article belongs to the Special Issue Recent Advances in Complex Analysis and Related Topics)

Abstract

:
Let S cos * denote the class of normalized analytic functions f in the open unit disk D satisfying the subordination z f ( z ) f ( z ) cos z . In the first result of this article, we find the sharp upper bounds for the initial coefficients a 3 , a 4 and a 5 and the sharp upper bound for module of the Hankel determinant | H 2 , 3 ( f ) | for the functions from the class S cos * . The next section deals with the sharp upper bounds of the logarithmic coefficients γ 3 and γ 4 . Then, in addition, we found the sharp upper bound for H 2 , 2 F f / 2 . To obtain these results we utilized the very useful and appropriate Lemma 2.4 of N.E. Cho et al., which gave a most accurate description for the first five coefficients of the functions from the Carathéodory’s functions class, and provided a technique for finding the maximum value of a three-variable function on a closed cuboid. All the maximum found values were checked by using MAPLE™ computer software, and we also found the extremal functions in each case. All of our most recent results are the best ones and give sharp versions of those recently published by Hacet.

1. Introduction and Preliminaries

Let A denote the class of all analytic and normalized functions f having the Maclaurin series expansion as follows
f ( z ) = z + m = 2 a m z m , z D ,
where D : = { z C : | z | < 1 } represents the open unit disk in the complex plane C and we consider a subclass of S A containing all the univalent functions of A .
The subclass of A defined by
S * : = f A : Re z f ( z ) f ( z ) > 0 , z D
is called the class of starlike functions (with respect to the origin) in D and it is well-known that S * S . Let B denote the family of functions w, which are analytic in D , such that w ( 0 ) = 0 and | w ( z ) | < 1 for z D . Such functions are referred to as Schwarz functions.
Let us consider two analytic functions, f and g in D . We say that f is subordinated to g, written as f ( z ) g ( z ) if there exists a Schwarz function w such that f ( z ) = g ( w ( z ) ) for z D . If  f ( z ) g ( z ) , then f ( 0 ) = g ( 0 ) and f ( D ) g ( D ) , and if g is univalent in D , then f ( z ) g ( z ) if and only if f ( 0 ) = g ( 0 ) and f ( D ) g ( D ) .
Based on the geometric properties of the image of D , by some analytic functions, the functions can be categorized from this point of view into different families. Thus, in 1992, Ma and Minda [1] introduced a generalized subclass of S * denoted by S * ( ϕ ) , which is defined in terms of the subordination as follows
S * ( ϕ ) : = f A : z f ( z ) f ( z ) ϕ ( z ) ,
where ϕ satisfies the conditions ϕ ( 0 ) = 1 and Re ϕ ( z ) > 0 in D and ϕ maps the unit disk D onto a star-shaped domain. Several subclasses of S * can be obtained by varying the function ϕ . For example, if we choose ϕ ( z ) = 1 + L z 1 + M z , 1 M < L 1 , then we get the class S * [ L , M ] : = S * 1 + L z 1 + M z , which is called the Janowski starlike functions class and was investigated in [2]. Sokól and Stankiewicz [3] defined and studied the class S L * : = S * 1 + z , where the function ϕ ( z ) = 1 + z maps D onto the image domain bounded by w 2 1 < 1 (the square functions are considered at the main branch, i.e., those branches with 1 = 1 or log 1 = 0 ). The class S C * : = S * 1 + 4 3 z + 2 3 z 2 was studied by Sharma [4] and is related to the cardioid function.
In the case of ϕ ( z ) = cosh z , the class S cosh * was defined and thoroughly examined in [5], whereas the class S e * : = S * e z was presented and studied in [6] by Mendiratta et al. For  ϕ ( z ) = 1 + sin z , the class S sin * was introduced and investigated in [7,8], while if ϕ ( z ) = 1 + tanh z , the class S t a n h * was defined and studied in [9]. Recently, the class S cos * , defined by
S cos * : = f A : z f ( z ) f ( z ) cos z ,
was introduced and investigated in [10], and determining sharp results connected with those of [11] represents the main goal of the present paper.
The following part of this section is necessary to understand the motivation of this work. In 1916, Bieberbach presented the well-known Bieberbach conjecture, which was proved by de Branges [12] in 1985. Prior to de Branges proof of this conjecture, numerous mathematicians exerted considerable effort to prove it, leading to the establishment of coefficient bounds for some remarkable subclasses of the class S . They also developed several new inequalities related to the coefficient bounds for some subclasses of univalent functions, and those related to the Fekete-Szego functional, that is, a 3 λ a 2 2 is one of those inequalities. Another coefficient problem closely related to the Fekete–Szego functional is the Hankel determinant, as we will see below.
As we could see in Pommerenke’s paper [13], for a function f A , the Hankel determinant H m , n ( f ) is as follows
H m , n ( f ) : = a n a n + 1 a n + m 1 a n + 1 a n + 2 a n + m a n + m 1 a n + m a n + 2 m 2 ,
where m , n 1 . We remark that
H 2 , 1 ( f ) = a 3 a 2 2 , H 2 , 2 ( f ) = a 2 a 4 a 3 2 , H 2 , 3 ( f ) = a 3 a 5 a 4 2 ,
H 3 , 1 ( f ) = 2 a 2 a 3 a 4 a 4 2 a 3 3 a 2 2 a 5 + a 3 a 5 ,
where | H 2 , 1 ( f ) | is the classical Fekete–Szego functional obtained for λ = 1 . Several authors have determined the maximum value of | H 2 , 1 ( f ) | and the upper bound for | H 2 , 2 ( f ) | for various subclasses of A ; see, for example, [14,15,16]. Many results regarding the second Hankel determinant H 2 , 3 ( f ) could also be found in recent papers like [17,18,19]. The determinant H 2 , 3 ( f ) has not been studied much in the literature: Babalola [20] studied, for the first time, non-sharp bounds for the determinant H 3 , 1 ( f ) for various subclasses of S , while in 2017, Zaprawa [21] improved the results of Babalola by using a new technique. We mention that the sharp bounds of the modulus of H 3 , 1 ( f ) for the class S * were recently obtained by Kowalczyk et al. [22], whereas for the class C and bounded turning functions, sharp bounds were obtained in [23,24], respectively. For sharp inequalities results for the determinant H 3 , 1 ( f ) for some subclasses of S * , we refer to [18,25,26,27,28].
Very recently, Marimuthu et al. [11] have determined the coefficient bounds, the upper bounds for the second, third, and fourth-order Hankel determinants for the functions of the class S cos * , but most of the results presented in this paper are not sharp.
Motivated by the above-mentioned study, in this paper, we have established the sharp results for the upper bounds of the coefficients and the logarithmic coefficients of the functions of the class S cos * . We have also developed the sharp upper bounds for the modulus of the second- and third-order Hankel determinants for the functions of this class.
The well-known Carathéodory class  P is the family of holomorphic functions h in D , which satisfy the condition Re h ( z ) > 0 , z D , with the power series expansion of the form
h ( z ) = 1 + n = 1 c n z n , z D .
The study of some coefficient problems in different classes of analytic functions revolves around the idea of expressing function coefficients in a given class by function coefficients that have a positive real part. Thus, the known inequalities for the class P can be used to study coefficient functionals. We require the following results on the class P for our next proofs.
We will recall the well-known Carathéodory lemma [29] (see also [30] (Corollary 2.3, p. 41),  [31] (Carathéodory’s Lemma, p. 41)):
Lemma 1.
If h P has the form (4), then
| c n |     2 , n 1 .
The inequality holds for all n 1 if and only if h ( z ) = 1 + λ z 1 λ z , | λ | = 1 .
The next result represents the relations (2.7), (2.8), and (2.9) of Lemma 2.4 from [32]:
Lemma 2.
([32] (Lemma 2.4)). Let D ¯ : = { z C : | z | 1 } be the closed unit disk, and  h P be given by (4). Then,
c 1 = 2 t 1 , c 2 = 2 t 1 2 + 2 1     | t 1 | 2 t 2 , c 3 = 2 t 1 3 + 4 1     | t 1 | 2 t 1 t 2 2 1     | t 1 | 2 t 1 ¯ t 2 2 + 2 1     | t 1 | 2 1     | t 2 | 2 t 3 ,
for some t k D ¯ and k { 1 , 2 , 3 } .
Note that the extension of this lemma for the coefficients c 4 and c 5 may also be found in Lemma 2.1 of [33].
The next lemma represents the first part of the result from [1] (Remark p. 162).
Lemma 3.
If h P is given by (4), then
c 2 ν c 1 2 2 ν c 1 2 , 0 < ν 1 2 .
The main novelty is found in the tools we used, that is, Lemma 2, which offers the best known estimate regarding the first five coefficients of the functions of the class P . Combining with the technique for determining the extremal values of a three-variable function on a compact cuboid, we found the best upper bounds of | a 3 | , | a 4 | , | a 5 | and of the Hankel determinants | H 3 , 1 ( f ) | , | H 2 , 3 ( f ) | . In addition, the sharp upper bounds of the logarithmic coefficients | γ 3 | and | γ 4 | , combined with those of H 2 , 2 F f / 2 , are presented in Section 3.
The main strong point is the fact that all the results are the best possible, and we gave the extremal function where the equalities are obtained. Since Lemma 2 deals only with the first five coefficients of the class P , we believe that the importance of this lemma is remarkable for results involving these coefficients. Unfortunately, it is our opinion that it is hard to find similar results for higher index coefficients because of the computational difficulties, at least in the first steps of the proofs. Thus, the limitations of the below methods include the fact that the order of the Hankel determinant and the indexes of the coefficients or logarithmical coefficients cannot be higher than the present ones. Definitively, our results do not represent general investigation methods for these types of problems.

2. Initial Coefficients Sharp Upper Bounds

The next main results give us the sharp upper bounds for the initial coefficients of the functions from the class S cos * .
Theorem 1.
Let f S cos * be given by (1). Then,
| a 3 |   1 4 , | a 4 |   2 27 3 , | a 5 | 1 8 ,
and these bounds are sharp.
Proof. 
If f S cos * , then by the definition of subordination there exists a Schwarz function w that is analytic in D and satisfies the condition w ( 0 ) = 0 and | w ( z ) | < 1 for all z D , such that
z f ( z ) f ( z ) = cos w ( z ) , z D .
Therefore, the function h defined by
h ( z ) = 1 + w ( z ) 1 w ( z ) = 1 + c 1 z + c 2 z 2 + , z D ,
which has the property h P .
Using the relations (6) and (7) and by equating the first four coefficients, we get
a 2 = 0 , a 3 = 1 16 c 1 2 , a 4 = 1 24 c 1 3 1 12 c 1 c 2 ,
a 5 = 1 48 c 1 4 1 32 c 2 2 + 3 32 c 1 2 c 2 1 16 c 1 c 3 .
(i) From the second relation of (8), according to the inequality (5), it follows that
| a 3 |   1 4 ,
and this inequality is attained for the function f * from Remark 2.2 of [11]. Thus, the above upper bound is sharp, which is the best possible.
(ii) To find the upper bound of | a 4 | , we see that the third equality of (8) could be written in the form
a 4 = c 1 12 c 2 c 1 2 2 ,
and using Lemma 3 for ν = 1 2 we obtain
| a 4 |   c 1 12 2 c 1 2 2 .
Denoting c : = c 1 , from Lemma 1 we have 0 c 2 , hence
| a 4 |   c 12 2 c 2 2 = : F ( c ) , c [ 0 , 2 ] .
It is easy to check that the function F attained the maximum value at c = 2 3 ; then, according to the above inequality, we get
| a 4 |   F 2 3 = 2 27 3 .
To prove the sharpness of this upper bound, let t ^ = 2 3 , h 1 ( z ) = 1 z 2 1 t ^ z + z 2 and
w 1 z = h 1 ( z ) 1 h 1 ( z ) + 1 = z ( 3 z 3 ) 3 z 3 , z D ,
thus, w 1 0 = 0 . To show that w 1 z < 1 in D , we remark that the function w 1 could be written in the form w 1 ( z ) = z φ ( z ) , where
φ ( z ) = 3 z 3 3 z 3 , z D .
Since | φ ( z ) | < 1 , z D , if and only if Re H ( z ) > 0 for all z D , where
H ( z ) : = 1 φ ( z ) 1 + φ ( z ) = 3 3 z + 1 3 + 3 z 1 , z D ,
is a circular transform. It is easy to check that
H ( 0 ) = 3 3 3 + 3 > 0 , H ( 1 ) = 0 , H ( i ) = 3 3 i 3 + 3 , H ( i ) = 3 3 i 3 + 3 .
Using the fact that every circular transform maps the circles (in the large sense, circles or lines) of C : = C { } into circles of C , from the above values of H it follows that Re H ( z ) > 0 for all z D , which implies | φ ( z ) | < 1 in D , hence
| w 1 ( z ) | = | z | | φ ( z ) | < 1 , z D .
Therefore, the function
f 1 ( z ) : = z exp 0 z cos w 1 ( t ) 1 t d t = z 1 12 z 3 + 2 27 3 z 4 + , z D ,
belongs to the class S cos * ; hence, | a 4 |   = 2 27 3 for the above function f 1 , which proves the sharpness of the second inequality of this theorem.
(iii) To determine the upper bound of | a 5 | , by using the relation (9) combined with Lemma 2, we obtain
a 5 = 1 96 4 t 1 4 + 24 | t 1 | 2 t 2 2 1     | t 1 | 2 12 t 2 2 1     | t 1 | 2 2 24 t 1 1     | t 1 | 2 1     | t 2 | 2 t 3 .
Setting x : =   | t 1 |   [ 0 , 1 ] , y : =   | t 2 |   [ 0 , 1 ] and u : =   | t 3 |   [ 0 , 1 ] , from the triangle inequality we obtain
| a 5 | 1 24 x 4 + 6 x 2 1 x 2 y 2 + 3 1 x 2 2 y 2 + 6 x 1 x 2 1 y 2 u = 1 24 F ( x , y , u ) , x , y , u [ 0 , 1 ] ,
where
F ( x , y , u ) : = x 4 + 6 x 2 1 x 2 y 2 + 3 1 x 2 2 y 2 + 6 x 1 x 2 1 y 2 u .
Denoting by Ω : = [ 0 , 1 ] × [ 0 , 1 ] × [ 0 , 1 ] the closed unit cuboid, we will find the maximum value of F in Ω .
I. First, let us consider that ( x , y , u ) belongs to the interior of Ω , denoted by int Ω . Differentiating (13) with respect to u, we obtain
F ( x , y , u ) u = 6 x 1 x 2 1 y 2 0 , ( x , y , u ) int Ω ,
therefore, the function F has no extremal values in int Ω .
II. Next, we will discuss the existence of the maximum value for F on the open six faces of Ω , as follows.
(i) On the face x = 0 , the next inequality holds
F ( 0 , y , u ) = 3 y 2 < 3 , y , u ( 0 , 1 ) .
(ii) On the face x = 1 , we have the equality
F ( 1 , y , u ) = 1 , y , u ( 0 , 1 ) .
(iii) On the plane y = 0 , let us denote
κ 1 ( x , u ) : = F ( x , 0 , u ) = x 4 + 6 1 x 2 x u , x , u ( 0 , 1 ) ,
and because
κ 1 ( x , u ) u = 6 x 1 x 2 0 , x ( 0 , 1 ) ,
it follows that the function κ 1 has no extremal values on ( 0 , 1 ) × ( 0 , 1 ) .
(iv) On the open face y = 1 , the function F reduces to
s 1 ( x ) : = F ( x , 1 , u ) = x 4 + 6 x 2 1 x 2 + 3 1 x 2 2 , x ( 0 , 1 ) .
Since s 1 ( x ) = 8 x 3 < 0 , x ( 0 , 1 ) , therefore s 1 is a strictly decreasing function on ( 0 , 1 ) ,
F ( x , 1 , u ) < 3 , x , u ( 0 , 1 ) .
(v) For the open face u = 0 , we get
κ 2 ( x , y ) : = F ( x , y , 0 ) = x 4 + 6 x 2 1 x 2 y 2 + 3 1 x 2 2 y 2 , x , y ( 0 , 1 ) ,
therefore,
κ 2 ( x , y ) x = 4 x 3 3 y 2 1 , κ 2 ( x , y ) y = 6 x 1 x + 1 y x 2 + 1 ,
hence the system of equations κ 2 ( x , y ) x = 0 and κ 2 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
(vi) On the open face u = 1 , the function F becomes
κ 3 ( x , y ) : = x 4 + 6 x 2 1 x 2 y 2 + 3 y 2 1 x 2 2 + 6 x 1 x 2 1 y 2 , x , y ( 0 , 1 ) ,
and it is easy to check that the system of equations κ 3 ( x , y ) x = 0 and κ 3 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
III. Now we will investigate the existence of the maximum of F on the edges of Ω .
(i) From (13), we obtain
F ( x , 0 , 0 ) = x 4 1 , x [ 0 , 1 ] .
(ii) Also, from (16) we get s 2 ( x ) : = F ( x , 0 , 1 ) = x 4 + 6 x 1 x 2 . We may easily see that the zero of s 2 in [ 0 , 1 ] given by x 0 = 0.621924 satisfies s 2 ( x 0 ) < 0 , consequently
F ( x , 0 , 1 ) F ( x 0 , 0 , 1 ) = 2.437828 , x [ 0 , 1 ] .
(iii) Putting x = 0 in (16) we have
F ( 0 , 0 , u ) = 0 , u [ 0 , 1 ] .
(iv) Since (17) is independent of u, similar to the inequality (18), we deduce
F ( x , 1 , 1 ) = F ( x , 1 , 0 ) 3 , x [ 0 , 1 ] ,
and putting x = 0 in (17), we obtain
F ( 0 , 1 , u ) = 3 , u [ 0 , 1 ] .
(v) The function given by (15) is independent of the variables y and u, thus,
F ( 1 , y , 0 ) = F ( 1 , y , 1 ) = F ( 1 , 0 , u ) = F ( 1 , 1 , u ) = 1 , y , u [ 0 , 1 ] .
(vi) Since the function defined by (14) is independent of the variable u, we have
F ( 0 , y , 0 ) = F ( 0 , y , 1 ) 3 , y [ 0 , 1 ] .
For all the above reasons, we conclude that
max F ( x , y , u ) : ( x , y , u ) Ω = F ( 0 , 1 , u ) = 3 ,
and, according to (12), we finally obtain that | a 5 |   1 8 . This upper bound for | a 5 | is sharp for the function
f 2 ( z ) : = z exp 0 z cos t 2 1 t d t = z 1 8 z 5 + , z D ,
which completes our proof.    □
Remark 1.
1. In [11] it was proved that | a 4 |   1 3 and | a 5 |   11 24 , and the authors gave in Remark 2.2 a function of the class S cos * , for which | a 4 |   = 0 and | a 5 |   = 1 24 . In the above theorem, all the results are sharp and we gave the best upper bounds.
2. The maximum value of the function F defined by (13) could be easily found using the MAPLE™ 2016 software with the code
            [> maximize(F,x=0..1,y=0..1,u=0..1,location=true),
          
which gives the same result as above.
In the following two theorems, we determined the sharp upper bounds for the Hankel determinants | H 3 , 1 | and | H 2 , 3 | , respectively, over the class S cos * .
Theorem 2.
If f S cos * is given by (1), then
| H 3 , 1 ( f ) |   3115 164,268 + 671 657,072 1342 = 0.018446 ,
and this result is sharp.
Proof. 
Using the relations (8) and (9) in (3), we obtain
H 3 , 1 ( f ) = 7 36,864 c 1 6 + 5 4608 c 1 4 c 2 + 1 256 c 1 3 c 3 23 4608 c 1 2 c 2 2 ,
and replacing all the variables of the above relation with those of Lemma 2, it follows that
H 3 , 1 ( f ) = 1 576 [ 3 t 1 6 36 t 1 2 | t 1 | 2 t 2 2 1 | t 1 | 2 46 t 1 2 t 2 2 1 | t 1 | 2 2 + 36 t 1 3 1 | t 1 | 2 1 | t 2 | 2 t 3 ] .
If we set x : =   | t 1 |   [ 0 , 1 ] , y : =   | t 2 |   [ 0 , 1 ] and u : =   | t 3 |   [ 0 , 1 ] , using the above relation and the triangle inequality, we get
| H 3 , 1 ( f ) | 1 576 3 x 6 + 36 x 4 1 x 2 y 2 + 46 x 2 1 x 2 2 y 2 + 36 x 3 1 x 2 1 y 2 u = 1 576 F ( x , y , u ) , x , y , u [ 0 , 1 ] ,
where
F ( x , y , u ) : = 3 x 6 + 36 x 4 1 x 2 y 2 + 46 x 2 1 x 2 2 y 2 + 36 x 3 1 x 2 1 y 2 u .
With the same notations and method as in the proof of Theorem 1, next we will find the maximum value of F in Ω .
I. If we consider that ( x , y , u ) int Ω , differentiating (21) with respect to u, we obtain
F ( x , y , u ) u = 36 x 3 1 x 2 1 y 2 0 , ( x , y , u ) int Ω ,
hence, it follows that the function F has no maximum value in int Ω .
II. In the sequel, we will study the existence of the maximum value of F in the interior of six faces of Ω .
(i) On the face x = 0 , we have
F ( 0 , y , u ) = 0 , y , u ( 0 , 1 ) .
(ii) On the face x = 1 , we get
F ( 1 , y , u ) = 3 , y , u ( 0 , 1 ) .
(iii) On the plane y = 0 , the function F can be written as
κ 1 ( x , u ) : = F ( x , 0 , u ) = 3 x 6 + 36 x 3 1 x 2 u , x , u ( 0 , 1 ) .
Since
κ 1 ( x , u ) u = 36 x 3 1 x 2 0 , x ( 0 , 1 ) ,
it implies that the function κ 1 has no maximum points in the face of Ω .
(iv) On y = 1 the function F reduces to
s 1 ( x ) : = F ( x , 1 , u ) = 3 x 6 + 36 x 4 1 x 2 + 46 x 2 1 x 2 2 , x ( 0 , 1 ) .
Since s 1 ( x ) = 78 x 5 224 x 3 + 92 x , x ( 0 , 1 ) , it follows that s 1 ( x ) = 0 has the zero x 0 = 2184 39 1342 39 = 0.704685 ( 0 , 1 ) that satisfy the inequality s 1 ( x 0 ) < 0 . Therefore, we obtain
F ( x , 1 , u ) 49,840 4563 + 2684 4563 1342 = 10.625427 , x , u ( 0 , 1 ) .
(v) On the face u = 0 , the function F becomes
κ 2 ( x , y ) : = F ( x , y , 0 ) = 3 x 6 + 36 x 4 ( 1 x 2 ) y 2 + 46 x 2 ( 1 x 2 ) 2 y 2 , x , y ( 0 , 1 ) ,
thus,
κ 2 ( x , y ) x = 60 y 2 + 18 x 5 224 x 3 y 2 + 92 x 2 , κ 2 ( x , y ) y = 4 x 2 y 5 x 4 28 x 2 + 23 .
It is easy to see that the system of equations κ 2 ( x , y ) x = 0 and κ 2 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
(vi) On u = 1 the function F takes the form
κ 3 ( x , y ) = 3 x 6 + 36 x 4 ( 1 x 2 ) y 2 + 46 x 2 ( 1 x 2 ) 2 y 2 + 36 x 3 ( 1 x 2 ) ( 1 y 2 ) , x , y ( 0 , 1 ) .
Similarly, the system of equations κ 3 ( x , y ) x = 0 and κ 3 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
III. Now we will investigate the existence of the maximum of F on the edges of Ω .
(i) From (24) we obtain
F ( x , 0 , 0 ) = 3 x 6 3 , x [ 0 , 1 ] .
(ii) The relation (24) at u = 1 becomes s 2 ( x ) : = F ( x , 0 , 1 ) = 3 x 6 + 36 x 3 ( 1 x 2 ) , x [ 0 , 1 ] . The solution of s 2 ( x ) = 18 x 2 x 3 10 x 2 + 6 = 0 is x 0 = 0.807920 [ 0 , 1 ] and satisfies s 2 ( x 0 ) < 0 , hence
F ( x , 0 , 1 ) F ( x 0 , 0 , 1 ) = 7.427102 , x [ 0 , 1 ] .
(iii) Putting x = 0 in (24), we have
F ( 0 , 0 , u ) = 0 , u [ 0 , 1 ]
(iv) Since (25) is independent of u, similarly as above, we obtain
F ( x , 1 , 1 ) = F ( x , 1 , 0 ) 49,840 4563 + 2684 4563 1342 , x [ 0 , 1 ] ,
while if we take x = 0 in (25) it follows
F ( 0 , 1 , u ) = 0 , u [ 0 , 1 ] .
(v) The relation (23) is independent of the variables y , u [ 0 , 1 ] , hence
F ( 1 , y , 0 ) = F ( 1 , y , 1 ) = F ( 1 , 0 , u ) = F ( 1 , 1 , u ) = 3 , y , u [ 0 , 1 ] .
(vi) Finally, since (22) is independent of the variable u [ 0 , 1 ] , we have
F ( 0 , y , 0 ) = F ( 0 , y , 1 ) = 0 , y [ 0 , 1 ] .
All the inequalities we obtained above show that
max F ( x , y , u ) : ( x , y , u ) Ω = F 2184 39 1342 39 , 1 , u = 49,840 4563 + 2684 4563 1342 = 10.625427 ,
and using (20), our inequality is proved.
For proving the sharpness of this inequality, let us consider t ˜ = 2184 39 1342 39 , h 3 ( z ) = 1 + 1 + i t ˜ z + i z 2 1 1 i t ˜ z i z 2 and
w 3 ( z ) = h 2 ( z ) 1 h 2 ( z ) + 1 = z 2184 39 1342 + 39 i z 39 + 2184 39 1342 i z , z D .
We can see that w 3 ( 0 ) = 0 , and let us write the function w 3 as w 3 ( z ) = z ψ ( z ) , where
ψ ( z ) = 2184 39 1342 + 39 i z 39 + 2184 39 1342 i z , z D .
For the same reasons regarding the circular transforms as in the proof of the sharpness of Theorem 1 item (ii), we will show that | ψ ( z ) | < 1 in D by proving that Re H ( z ) > 0 , z D , where
H ( z ) : = 1 ψ ( z ) 1 + ψ ( z ) = 2184 39 1342 39 z + i 2184 39 1342 + 39 z + i , z D ,
is a circular transform. Since
H ( 0 ) = 2184 39 1342 + 39 2184 39 1342 + 39 = 0.173236 > 0 , H ( i ) = 0 , H ( 1 ) = 2184 39 1342 39 i 2184 39 1342 + 39 , H ( 1 ) = 2184 39 1342 39 i 2184 39 1342 + 39 ,
as in the above-mentioned proof, these values of H lead us to Re H ( z ) > 0 , z D , which implies | ψ ( z ) | < 1 in D ; therefore,
| w 3 ( z ) |   = | z | | ψ ( z ) | < 1 , z D .
Thus, the function
f 3 ( z ) = z exp 0 z cos w 3 ( t ) 1 t d t = z + 14 39 + 1342 156 z 3 1 4563 17 + 1342 2184 39 1342 z 4 + 23,135 36,504 163 1342 9126 z 5 + , z D ,
belongs to the class S cos * , with the initial coefficients
a 2 = 0 , a 3 = 14 39 + 1342 156 , a 4 = 1 4563 17 + 1342 2184 39 1342 i , a 5 = 23,135 36,504 163 1342 9126 .
From the relation (3), we get H 3 , 1 ( f 3 ) = 3115 164,268 + 671 657,072 1342 = 0.018446 and the proof is complete. □
Remark 2.
In [11], it is proved that | H 3 , 1 ( f ) |   139 576 = 0.241319 for all f S cos * , but that result was not the best possible. If we compare the upper bounds of | H 3 , 1 ( f ) | for f S cos * , obtained here with those of [11], the result of Theorem 2 is a significant improvement of the previous one. Moreover, the inequality obtained in above theorem is sharp, thus the found upper bound for | H 3 , 1 ( f ) | if f S cos * cannot be improved.
Theorem 3.
If f S cos * has the form (1), then
| H 2 , 3 ( f ) |   77 15,552 + 29 15,552 58 = 0.019152 ,
and the result is sharp.
Proof. 
Replacing in (2) the values of a 2 , a 3 , a 2 , and a 5 given by (8) and (9), we obtain
H 2 , 3 ( f ) = 1 2304 c 1 6 + 5 4608 c 1 4 c 2 + 1 256 c 1 3 c 3 23 4608 c 1 2 c 2 2 .
According to Lemma 2, from the above relation we deduce that
H 2 , 3 ( f ) = 1 288 [ 3 t 1 6 18 t 1 2 | t 1 | 2 t 2 2 1 | t 1 | 2 23 t 1 2 t 2 2 1 | t 1 | 2 2 + 18 t 1 3 1 | t 1 | 2 1 | t 2 | 2 t 3 ] .
Setting x : =   | t 1 |   [ 0 , 1 ] , y : =   | t 2 |   [ 0 , 1 ] and u : =   | t 3 |   [ 0 , 1 ] , then, using the triangle’s inequality, the above relation leads us to
| H 2 , 3 ( f ) | 1 288 3 x 6 + 18 x 4 1 x 2 y 2 + 23 x 2 1 x 2 2 y 2 + 18 x 3 1 x 2 1 y 2 u = 1 288 F ( x , y , u ) , x , y , u [ 0 , 1 ] ,
where
F ( x , y , u ) : = 3 x 6 + 18 x 4 1 x 2 y 2 + 23 x 2 1 x 2 2 y 2 + 18 x 3 1 x 2 1 y 2 u .
With the same notations as those in the proofs of the two previous theorems, we have to find the maximum value of F on int Ω , on the six faces, and on the twelve edges of Ω .
I. First, we consider the arbitrary interior point ( x , y , u ) int Ω . Differentiating (28) with respect to u, we obtain
F ( x , y , u ) u = 18 x 3 1 x 2 1 y 2 0 , ( x , y , u ) int Ω ,
therefore, we have no maximum value of F in int Ω .
II. Next, we will study the existence of the maximum value of the function F in the interior of six faces of Ω .
(i) On the face x = 0 , the function F reduces to
F ( 0 , y , u ) = 0 , y , u ( 0 , 1 ) .
(ii) On the face x = 1 , it takes the form
F ( 1 , y , u ) = 3 , y , u ( 0 , 1 ) .
(iii) On y = 0 , the function F can be written as
κ 1 ( x , u ) : = F ( x , 0 , u ) = 3 x 6 + 18 x 3 1 x 2 u , x , u ( 0 , 1 ) .
Since
κ 1 ( x , u ) u = 18 x 3 1 x 2 0 , x ( 0 , 1 ) ,
it follows that κ 1 has no maximum point in this face of Ω .
(iv) On y = 1 , the function F reduces to
s 1 ( x ) : = F ( x , 1 , u ) = 3 x 6 + 18 x 4 1 x 2 + 23 x 2 1 x 2 2 , x ( 0 , 1 ) ,
thus,
s 1 ( x ) = 48 x 5 112 x 3 + 46 x , x ( 0 , 1 ) .
Hence s 1 ( x ) = 0 has the zero x 0 = 42 3 58 6 = 0.729396 ( 0 , 1 ) and s 1 ( x 0 ) < 0 . Therefore,
F ( x , 1 , u ) F ( x 0 , 1 , u ) = 77 54 + 29 54 58 = 5.515878 , x , u ( 0 , 1 ) .
(v) On the face u = 0 , the function F becomes
κ 2 ( x , y ) : = F ( x , y , 0 ) = 3 x 6 + 18 x 4 1 x 2 y 2 + 23 x 2 1 x 2 2 y 2 , x , y ( 0 , 1 ) .
Therefore,
κ 2 ( x , y ) x = 2 x 15 x 4 y 2 + 9 x 4 56 x 2 y 2 + 23 y 2 , κ 2 ( x , y ) y = 2 x 2 y 5 x 4 28 x 2 + 23 ,
and the system of equations κ 2 ( x , y ) x = 0 and κ 2 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
(vi) On u = 1 , the function F takes the form
κ 3 ( x , y ) = 3 x 6 + 18 x 4 1 x 2 y 2 + 23 x 2 1 x 2 2 y 2 + 18 x 3 1 x 2 1 y 2 , x , y ( 0 , 1 ) ,
hence,
κ 3 ( x , y ) x = 6 5 y 2 + 3 x 5 90 1 y 2 x 4 112 x 3 y 2 + 54 1 y 2 x 2 + 46 x y 2 , κ 3 ( x , y ) y = 10 x 1 2 x + 1 y x + 23 5 x 2 .
Therefore, the system of equations κ 3 ( x , y ) x = 0 and κ 3 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
III. Now we investigate the maximum of F on the edges of Ω .
(i) From (31), we obtain
F ( x , 0 , 0 ) = 3 x 6 3 , x [ 0 , 1 ] .
(ii) Also, from (31) at u = 1 we get s 2 ( x ) : = F ( x , 0 , 1 ) = 3 x 6 + 18 x 3 1 x 2 . The solution in [ 0 , 1 ] of the equation s 2 ( x ) = 18 x 5 90 x 4 + 54 x 2 = 0 for which s 2 ( x ) < 0 is x 0 = 0.850256 [ 0 , 1 ] , thus
F ( x , 0 , 1 ) F ( x 0 , 0 , 1 ) = 4.199005 , x [ 0 , 1 ] .
(iii) Putting x = 0 in (31) we have
F ( 0 , 0 , u ) = 0 , u [ 0 , 1 ] .
(iv) Since (32) is independent of u, according to (33), we obtain
F ( x , 1 , 1 ) = F ( x , 1 , 0 ) 77 54 + 29 54 58 , x [ 0 , 1 ] .
(v) If we take x = 0 in (32), we get
F ( 0 , 1 , u ) = 0 , u [ 0 , 1 ] .
Using the fact that the relation (30) is independent of the variables y and u, we deduce
F ( 1 , y , 0 ) = F ( 1 , y , 1 ) = F ( 1 , 0 , u ) = F ( 1 , 1 , u ) = 3 , y , u [ 0 , 1 ] .
(vi) Since the relation (29) is independent of the variable u, we have
F ( 0 , y , 0 ) = F ( 0 , y , 1 ) = 0 , y [ 0 , 1 ] .
Consequently, for the above reasons, we conclude that
max F ( x , y , u ) : ( x , y , u ) Ω = F 42 3 58 6 , 1 , u = 77 54 + 29 54 58 = 5.515878 ,
and, combining with (27), it follows that
H 2 , 3 ( f ) 77 15,552 + 29 15,552 58 = 0.019152 .
To prove the sharpness of the above result, let us consider t * = 1 3 42 3 58 , h 4 ( z ) = 1 + t * z + z 2 1 z 2 and
w 4 ( z ) = h 4 ( z ) 1 h 4 ( z ) + 1 = z 42 3 58 + 6 z 6 + 42 3 58 z , z D .
First, w 4 ( 0 ) = 0 and we will denote w 4 ( z ) = z χ ( z ) , where
χ ( z ) = 42 3 58 + 6 z 6 + 42 3 58 z , z D .
Using the same property of the circular transforms as in the proof of the sharpness of Theorem 1 item (ii) and Theorem 2, we will show that | χ ( z ) | < 1 in D by proving that Re H ( z ) > 0 , z D , where
H ( z ) : = 1 χ ( z ) 1 + χ ( z ) = 42 3 58 6 ( z 1 ) 42 3 58 + 6 ( z + 1 ) ,
is a circular transform. Computing the below values
H ( 0 ) = 42 3 58 6 42 3 58 + 6 = 0.156472 > 0 , H ( 1 ) = 0 , H ( i ) = 42 3 58 6 i 42 3 58 + 6 , H ( i ) = 42 3 58 6 i 42 3 58 + 6 ,
for similar reasons as in the above-mentioned proofs, these values of H impliy Re H ( z ) > 0 , z D , which yields | χ ( z ) | < 1 in D , therefore
| w 4 ( z ) |   = | z | | χ ( z ) | < 1 , z D .
Consequently, the function
f 4 ( z ) = z exp 0 z cos w 4 ( t ) 1 t d t = z + 7 24 + 1 48 58 z 3        1 216 2 + 58 42 3 58 z 4 + 7 54 + 5 216 58 z 5 + , z D ,
belongs to the class S cos * . In the above power series expansion, we have a 3 = 7 24 + 1 48 58 , a 4 = 1 216 2 + 58 42 3 58 and a 5 = 7 54 + 5 216 58 , hence
H 2 , 3 ( f 4 ) = a 3 a 5 a 4 2 = 77 15,552 + 29 15,552 58 ,
which completes our proof. □
Remark 3.
The maximum values of the functions F defined by (21) and (28) could be also found by using the MAPLE™ computer software codes like in the Remark 1 item 2, and we obtain the same values as in both of the above two theorems.

3. Logarithmic Coefficients Sharp Upper Bounds

The logarithmic coefficients γ n : = γ n ( f ) , n N for the function f S are defined by
F f ( z ) : = log f ( z ) z = 2 n = 1 γ n z n , z D .
Since the function ϕ ( z ) : = cos z has a positive real part in D , and moreover
Re ( cos z ) > 1 2 , z D ,
it follows that S cos * S * S (see [11], p. 610). Therefore, it is possible to define the logarithmic coefficients for the functions f S cos * .
In this section, we give the sharp upper bounds estimates for the third and fourth logarithmic coefficients of the functions that belong to the class S cos * .
Theorem 4.
If f S cos * is given by (1), then
| γ 3 |   3 27 , | γ 4 | 1 16 .
These bounds are sharp.
Proof. 
If f S cos * has the form (1), then
log f ( z ) z = a 2 z + a 2 2 2 + a 3 z 2 + a 2 a 3 + a 4 + a 2 3 3 z 3 + , z D .
And, equating the first four coefficients of (34) with those of (35), we get
γ 1 = a 2 2 , γ 2 = 1 4 2 a 3 a 2 2 , γ 3 = 1 6 a 2 3 3 a 2 a 3 + 3 a 4 ,
γ 4 = 1 8 a 2 4 + 4 a 2 2 a 3 4 a 2 a 4 2 a 3 2 + 4 a 5 .
With the same notation as in the proof of Theorem 1, replacing in (36) and (37) the values of a 2 , a 3 , a 4 and a 5 from the relations (8) and (9), we obtain
γ 1 = 0 , γ 2 = 1 32 c 1 2 , γ 3 = 1 48 c 1 3 1 24 c 1 c 2 ,
γ 4 = 35 3072 c 1 4 1 64 c 2 2 + 3 64 c 1 2 c 2 1 32 c 1 c 3
For the upper bound of | γ 3 | , using (38), we write
γ 3 = c 1 24 c 2 c 1 2 2 ,
and according to Lemma 3 for ν = 1 2 , we obtain
| γ 3 |   c 1 24 2 c 1 2 2 .
Denoting c : = c 1 , from Lemma 1, we have
| γ 3 |   c 24 2 c 2 2 = F ( c ) , c [ 0 , 2 ] .
Using the result we got for the computation of the maximum F given by (10) we get | γ 3 |   3 27 .
To prove the sharpness of this bound, let us consider the function f 1 given by (11), were a 1 = 1 , a 2 = 0 , a 3 = 1 12 and a 4 = 2 27 3 . Therefore, for this function, by using the last of the relations from (36), we obtain γ 3 = 3 27 .
To find the upper bound of | γ 4 | , from (37) combined with Lemma 2, we can write
γ 4 = 1 192 t 1 4 + 24 | t 1 | 2 t 2 2 1     | t 1 | 2 12 t 2 2 1     | t 1 | 2 2 24 t 1 1     | t 1 | 2 1     | t 2 | 2 t 3 ,
and setting x : =   | t 1 |   [ 0 , 1 ] , y : =   | t 2 |   [ 0 , 1 ] and u : =   | t 3 |   [ 0 , 1 ] , using the triangle’s inequality, we obtain
| γ 4 | 1 192 x 4 + 24 x 2 1 x 2 y 2 + 12 1 x 2 2 y 2 + 24 x 1 x 2 1 y 2 u = 1 192 F ( x , y , u ) , x , y , u [ 0 , 1 ] ,
where
F ( x , y , u ) : = x 4 + 24 x 2 1 x 2 y 2 + 12 1 x 2 2 y 2 + 24 x 1 x 2 1 y 2 u .
Using the notations and the technique from the proofs of the previous theorems, we will determine the maximum of F on Ω as follows.
I. In the points ( x , y , u ) int Ω , differentiating (41) with respect to u, we obtain
F ( x , y , u ) u = 24 x 1 x 2 1 y 2 0 , ( x , y , u ) int Ω ,
therefore, the function F does not attain its maximum value in int Ω .
II. In the next items, we will discuss the existence of the maximum value of F in the interior of six faces of Ω .
(i) On the face x = 0 , we get
F ( 0 , y , u ) = 12 y 2 12 , y , u ( 0 , 1 ) .
(ii) On the face x = 1 , the function F takes the form
F ( 1 , y , u ) = 1 , y , u ( 0 , 1 ) .
(iii) On y = 0 , the function can be written as
κ 1 ( x , u ) : = F ( x , 0 , u ) = x 4 + 24 x 1 x 2 u , x , u ( 0 , 1 ) ,
and because
κ 1 ( x , u ) u = 24 x 1 x 2 0 , x ( 0 , 1 ) ,
it implies that the function κ 1 has no maximum in ( 0 , 1 ) × ( 0 , 1 ) .
(iv) On y = 1 , the function F reduces to
s 1 ( x ) : = F ( x , 1 , u ) = 11 x 4 + 12 , x ( 0 , 1 ) .
Since s 1 ( x ) = 44 x 3 < 0 , x ( 0 , 1 ) , the function s 1 is strictly decreasing on ( 0 , 1 ) , hence
F ( x , 1 , u ) F ( 0 , 1 , u ) = 12 , x , u ( 0 , 1 ) .
(v) On the face u = 0 , the function F will have the form
κ 2 ( x , y ) : = F ( x , y , 0 ) = x 4 + 24 x 2 1 x 2 y 2 + 12 1 x 2 2 y 2 , x , y ( 0 , 1 ) .
Therefore,
κ 2 ( x , y ) x = 4 x 3 12 y 2 1 , κ 2 ( x , y ) y = 24 y x 1 x + 1 x 2 + 1 ,
thus, the system of equations κ 2 ( x , y ) x = 0 and κ 2 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
(vi) On u = 1 , the function F will be
κ 3 ( x , y ) : = 12 x 4 y 2 + 24 x 3 y 2 + x 4 24 x 3 24 x y 2 + 12 y 2 + 24 x , x , y ( 0 , 1 ) .
Similarly, it is easy to check that the system of equations κ 3 ( x , y ) x = 0 and κ 3 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
III. Now we will investigate the existence of the maximum of F on the edges of Ω .
(i) From (44) at u = 0 , we have
F ( x , 0 , 0 ) = x 4 1 , x [ 0 , 1 ] .
(ii) Using (44) at u = 1 , we get s 2 ( x ) : = F ( x , 0 , 1 ) = x x 3 24 x 2 + 24 , hence, s 2 ( x ) = 4 x 3 72 x 2 + 24 . The solution of s 2 ( x ) = 0 in [ 0 , 1 ] is x 0 = 0.587000 [ 0 , 1 ] and s 2 ( x 0 ) < 0 ; it follows that
F ( x , 0 , 1 ) F ( x 0 , 0 , 1 ) = 9.352439 , x [ 0 , 1 ] .
(iii) Putting x = 0 in (44), we get
F ( 0 , 0 , u ) = 0 , u [ 0 , 1 ] ,
(iv) Since (45) is independent of u, we obtain
F ( x , 1 , 1 ) = F ( x , 1 , 0 ) 12 , x [ 0 , 1 ] ,
while for x = 0 in (45), we get
F ( 0 , 1 , u ) = 12 .
(v) The relation (43) is independent with respect to the variables y and u, thus
F ( 1 , y , 0 ) = F ( 1 , y , 1 ) = F ( 1 , 0 , u ) = F ( 1 , 1 , u ) = 1 , y , u [ 0 , 1 ] .
(vi) Finally, since (42) is independent of the variable u, we have
F ( 0 , y , 0 ) = F ( 0 , y , 1 ) 1 , z [ 0 , 1 ] .
The above computations lead to
max F ( x , y , u ) : ( x , y , u ) Ω = F ( 0 , 1 , u ) = 12 ,
and from (40) we conclude that | γ 4 |   1 16 .
For proving the sharpness of the above inequality, we consider the function f 2 given by (19). In this case, a 1 = 1 , a 2 = a 3 = a 4 = 0 and a 5 = 1 8 , and from (37) we get | γ 4 |   = 1 16 , which completes our proof. □
Remark 4.
In [11] it is proved that | γ 3 |   1 6 and | γ 4 |   85 384 , while our above results are sharp and give the best upper bounds for these coefficients.
Theorem 5.
Let f S cos * be given by (1). Then, for the function F f given by (34), the next inequality holds
H 2 , 2 F f / 2 10,577 1,028,376 + 1549 4,113,504 1549 = 0.015678 ,
and this result is sharp.
Proof. 
Replacing the values of (38) and (39) in the relation (2), we obtain
H 2 , 2 F f / 2 = γ 2 γ 4 γ 3 2 = 23 294,912 c 1 6 + 5 18,432 c 1 4 c 2 + 1 1024 c 1 3 c 3 23 18,432 c 1 2 c 2 2 .
Using the Lemma 2, we obtain
H 2 , 2 F f / 2 = 1 4608 [ 3 t 1 6 72 t 1 2 | t 1 | 2 t 2 2 1 | t 1 | 2 92 t 1 2 t 2 2 1 | t 1 | 2 2 + 72 t 1 3 1 | t 1 | 2 1 | t 2 | 2 t 3 ] ,
and denoting x : =   | t 1 |   [ 0 , 1 ] , y : =   | t 2 |   [ 0 , 1 ] , u : =   | t 3 |   [ 0 , 1 ] , by using the triangle’s inequality, the above relation leads us to
H 2 , 2 F f / 2 1 4608 [ 3 x 6 + 72 x 4 1 x 2 y 2 + 92 x 2 1 x 2 2 y 2 + 72 x 3 1 x 2 1 y 2 u ] = 1 4608 F ( x , y , u ) , x , y , u [ 0 , 1 ] ,
where
F ( x , y , u ) : = 3 x 6 + 72 x 4 1 x 2 y 2 + 92 x 2 1 x 2 2 y 2 + 72 x 3 1 x 2 1 y 2 u .
With the notations used in the proofs of the previous three theorems, we will determine the maximum value of F in Ω .
I. For all the interior points ( x , y , u ) int Ω , differentiating (48) with respect to u, we obtain
F ( x , y , u ) u = 72 x 3 1 x 2 1 y 2 0 , ( x , y , u ) int Ω ,
hence, the function does not get its maximum value in int Ω .
II. Next, we will study whether it is possible to obtain the maximum value of F in the interior of six faces of Ω .
(i) On the face x = 0 , we have
F ( 0 , y , u ) = 0 , y , u ( 0 , 1 ) .
(ii) On the face x = 1 , the function F takes the form
F ( 1 , y , u ) = 3 , y , u ( 0 , 1 ) .
(iii) On y = 0 , the function F can be written as
κ 1 ( x , u ) : = F ( x , 0 , u ) = 3 x 6 + 72 x 3 1 x 2 u , x , u ( 0 , 1 ) .
Since
κ 1 ( x , u ) u = 72 x 3 1 x 2 0 , x ( 0 , 1 ) ,
it follows that the function κ 1 has no maximum value in ( 0 , 1 ) × ( 0 , 1 ) .
(iv) On y = 1 , the function F becomes
s 1 ( x ) : = F ( x , 1 , u ) = 3 x 6 + 72 x 4 1 x 2 + 92 x 2 1 x 2 2 , x ( 0 , 1 ) .
Since s 1 ( x ) = 138 x 5 448 x 3 + 184 x = 0 has on ( 0 , 1 ) the root x 0 = 7728 138 1549 69 = 0.694547 ( 0 , 1 ) and s 1 ( x 0 ) < 0 , we deduce that
F ( x , 1 , u ) F ( x 0 , 1 , u ) = 676,928 14,283 + 24,784 14,283 1549 = 20.899268 , x ( 0 , 1 ) .
(v) On the face u = 0 , the function F reduces to
κ 2 ( x , y ) : = F ( x , y , 0 ) = 3 x 6 + 72 x 4 1 x 2 y 2 + 92 x 2 1 x 2 2 y 2 , x , y ( 0 , 1 ) ,
therefore,
κ 2 ( x , y ) x = 2 x 60 x 4 y 2 + 9 x 4 224 x 2 y 2 + 92 y 2 , κ 2 y = 8 x 2 x 2 1 y 5 x 2 23 .
Thus, the system of equations κ 2 ( x , y ) x = 0 and κ 2 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
(vi) On u = 1 , the function F takes the form
κ 3 ( x , y ) : = F ( x , y , 1 ) = 3 x 6 + 72 x 4 1 x 2 y 2 + 92 x 2 1 x 2 2 y 2 + 72 x 3 1 x 2 1 y 2 , x , y ( 0 , 1 ) .
We get
κ 3 ( x , y ) x = 120 y 2 + 18 x 5 + 360 y 2 360 x 4 448 x 3 y 2 + 216 y 2 + 216 x 2 + 184 x y 2 ,
and
κ 3 y = 8 y x 2 5 x + 23 x + 1 x 1 2 ,
hence, the system of equations κ 3 ( x , y ) x = 0 and κ 3 ( x , y ) y = 0 has no solutions in ( 0 , 1 ) × ( 0 , 1 ) .
III. Now we will investigate the maximum of F on the edges of Ω .
(i) From (51) for u = 0 we have
F ( x , 0 , 0 ) = 3 x 6 3 , x [ 0 , 1 ] .
(ii) From (51) for u = 1 , let s 2 ( x ) : = F ( x , 0 , 1 ) = 3 x 6 72 x 5 + 72 x 3 . The solutions in [ 0 , 1 ] of the equation s 2 ( x ) = 18 x 5 360 x 4 + 216 x 2 = 0 are x 0 = 0.790371 [ 0 , 1 ] and x 1 = 0 . Since s 2 ( x 0 ) < 0 and s 2 ( 0 ) = 0 we deduce that
F ( x , 0 , 1 ) F ( x 0 , 0 , 1 ) = 14.073287 , x [ 0 , 1 ] .
(iii) Putting x = 0 in (51) we have
F ( 0 , 0 , u ) = 0 , u [ 0 , 1 ] .
(iv) Since the relation (52) is independent on u, from (53) we obtain
F ( x , 1 , 1 ) = F ( x , 1 , 0 ) 676,928 14,283 + 24,784 14,283 1549 , x [ 0 , 1 ] .
(v) If we take x = 0 in (52), we obtain
F ( 0 , 1 , u ) = 0 , u [ 0 , 1 ]
(vi) The relation (50) is independent of the variables y and u, hence
F ( 1 , y , 0 ) = F ( 1 , y , 1 ) = F ( 1 , 0 , u ) = F ( 1 , 1 , u ) = 3 , y , u [ 0 , 1 ] .
Similarly, since the Formula (49) is independent of the variable u, we have
F ( 0 , y , 0 ) = F ( 0 , y , 1 ) = 0 , y [ 0 , 1 ] .
For the above reasons, it follows that
max F ( x , y , u ) : ( x , y , u ) Ω = F ( x 0 , 1 , u ) = 676,928 14,283 + 24,784 14,283 1549 ,
and using (47), we conclude that
H 2 , 2 F f / 2 10,577 1,028,376 + 1549 4,113,504 1549 = 0.015678 .
To prove the sharpness of the above inequality, we denote t = 2 69 7728 138 1549 and h 5 ( z ) = 1 + t z + z 2 1 z 2 such that
w 5 ( z ) = h 5 ( z ) 1 h 5 ( z ) + 1 = z ( 7728 138 1549 + 69 z ) 69 + 7728 138 1549 z , z D .
It is easy to see that w 7 ( 0 ) = 0 , and to prove that | w 7 ( z ) | < 1 in D , we will define the function w 5 as w 5 ( z ) = z ρ ( z ) , where
ρ ( z ) = 7728 138 1549 + 69 z 69 + 7728 138 1549 z , z D .
According to the same reasons regarding the circular transforms as in the proofs of the sharpness of Theorem 1 item (ii) and Theorem 2, we will show that | ρ ( z ) | < 1 , z D , by proving that Re H ( z ) > 0 , z D , where
H ( z ) : = 1 ρ ( z ) 1 + ρ ( z ) = 7728 138 1549 69 z 1 7728 138 1549 + 69 z + 1 , z D ,
is a circular transform. It is easy to compute
H ( 0 ) = 7728 138 1549 69 7728 138 1549 + 69 = 0.1802561912 > 0 , H ( 1 ) = 0 , H ( i ) = 7728 138 1549 69 i 7728 138 1549 + 69 , H ( i ) = 7728 138 1549 69 i 7728 138 1549 + 69 ,
and these values of the circular transform H imply that Re H ( z ) > 0 for all z D , which leads us to | ρ ( z ) | < 1 in D , hence
| w 5 ( z ) |   = | z | | ρ ( z ) | < 1 , z D .
Consequently, the function
f 5 ( z ) = z exp 0 z cos w 5 ( t ) 1 t d t = z + 28 69 + 1 138 1549 z 3 1 14 , 283 43 + 2 1549 7728 138 1549 z 4 + 71 , 467 114 , 264 + 241 14 , 283 1549 z 5 + , z D ,
belongs to the class S cos * . The initial coefficients of f 5 are
a 3 = 28 69 + 1 138 1549 , a 4 = 1 14 , 283 43 + 2 1549 7728 138 1549 , a 5 = 71 , 467 114 , 264 + 241 14 , 283 1549 ,
and from (36) and (37), we obtain
γ 2 = 14 69 + 1 276 1549 , γ 3 = ( 43 + 2 1549 ) 7728 138 1549 28 , 566 , γ 4 = 42 , 761 114 , 264 + 283 28 , 566 1549 .
Hence,
H 2 , 2 F f 5 / 2 = γ 2 γ 4 γ 3 2 = 10,577 1,028,376 + 1549 4,113,504 1549 ,
which proves the sharpness of our estimation. □
Remark 5.
As we already mentioned in Remark 3, the same maximum values of the functions F defined by (41) and (48) could also be found by using the MAPLE™ computer software codes as in Remark 1 item 2.

4. Conclusions

In this article, we have obtained the sharp coefficient bounds for the starlike functions that are connected to the cosine function, and we have also obtained the sharp coefficient bounds for the logarithmic coefficients of such functions.
The main tools of our results were those of N.E. Cho et al. [32], which seem to be a very efficient for the estimation of the first coefficients of Carathéodory’s function. In addition, we have determined the sharp bound for the fifth coefficient. The technique of this paper can be used to determine the sharp upper bound of the initial coefficients for a variety of classes of analytic functions.
Moreover, we have used these results to determine the sharp upper bounds for the Hankel determinants up to order three, and we emphasize that all the results we obtained are the best possible, so they cannot be improved.

Author Contributions

Conceptualization, R.A., M.R. and T.B.; methodology, R.A., M.R. and T.B.; software, R.A., M.R. and T.B.; validation, R.A., M.R. and T.B.; formal analysis, R.A., M.R. and T.B.; investigation, R.A., M.R. and T.B.; resources, R.A., M.R. and T.B.; data curation, R.A., M.R. and T.B.; writing—original draft preparation, M.R. and T.B.; writing—review and editing, M.R. and T.B.; visualization, R.A., M.R. and T.B.; supervision, M.R. and T.B.; project administration, R.A., M.R. and T.B. 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.

Acknowledgments

The authors are grateful to the reviewers for the valuable remarks, comments and advice, which helped us to improve the quality of the manuscript.

Conflicts of Interest

The authors declare no conflicts of interest.

References

  1. Ma, W.C.; Minda, D. A unified treatment of some special classes of univalent functions. In Proceedings of the Conference on Complex Analysis; (Tianjin, 1992); International Press: Cambridge, MA, USA, 1994; pp. 157–169. [Google Scholar]
  2. Janowski, W. Extremal problems for a family of functions with positive real part and for some related families. Ann. Pol. Math. 1970, 23, 159–177. [Google Scholar] [CrossRef]
  3. Sokół, J.; Stankiewicz, J. Radius of convexity of some subclasses of strongly starlike functions. Zesz. Nauk. Politech. Rzesz. Mat. Fiz. 1996, 19, 101–105. [Google Scholar]
  4. Sharma, K.; Jain, N.K.; Ravichandran, V. Starlike functions associated with a cardioid. Afr. Mat. 2016, 27, 923–939. [Google Scholar] [CrossRef]
  5. Alotaibi, A.; Arif, M.; Alghamdi, M.A.; Hussain, S. Starlikeness associated with cosine hyperbolic function. Mathematics 2020, 8, 1118. [Google Scholar] [CrossRef]
  6. Mendiratta, R.; Nagpal, S.; Ravichandran, V. On a subclass of strongly starlike functions associated with exponential function. Bull. Malays. Math. Sci. Soc. 2015, 38, 365–386. [Google Scholar] [CrossRef]
  7. Arif, M.; Raza, M.; Tang, H.; Hussain, S.; Khan, H. Hankel determinant of order three for familiar subsets of analytic functions related with sine function. Open Math. 2019, 17, 1615–1630. [Google Scholar] [CrossRef]
  8. Cho, N.E.; Kumar, V.; Kumar, S.S.; Ravichandran, V. Radius problems for starlike functions associated with the sine function. Bull. Iran. Math. Soc. 2019, 45, 213–232. [Google Scholar] [CrossRef]
  9. Ullah, K.; Srivastava, H.M.; Rafiq, A.; Arif, M.; Arjika, S. A study of sharp coefficient bounds for a new subfamily of starlike functions. J. Inequal. Appl. 2021, 1, 194. [Google Scholar] [CrossRef]
  10. Bano, K.; Raza, M. Starlike functions associated with cosine functions. Bull. Iran. Math. Soc. 2021, 47, 1513–1532. [Google Scholar] [CrossRef]
  11. Marimuthu, K.; Uma, J.; Bulboacă, T. Coefficient estimates for starlike and convex functions associated with cosine function. Hacet. J. Math. Stat. 2023, 52, 596–618. [Google Scholar]
  12. De Branges, L. A proof of the Bieberbach conjecture. Acta Math. 1985, 154, 137–152. [Google Scholar] [CrossRef]
  13. Pommerenke, C. On the coefficients and Hankel determinants of univalent functions. J. Lond. Math. Soc. 1966, 41, 111–122. [Google Scholar] [CrossRef]
  14. Janteng, A.; Halim, S.A.; Darus, M. Coefficient inequality for a function whose derivative has a positive real part. J. Inequal. Pure Appl. Math. 2006, 7, 50. [Google Scholar]
  15. Janteng, A.; Halim, S.A.; Darus, M. Hankel determinant for starlike and convex functions. Int. J. Math. Anal. 2007, 1, 619–625. [Google Scholar]
  16. Obradović, M.; Tuneski, N. Hankel determinants of second and third order for the class S of univalent functions. Math. Slovaca 2021, 71, 649–654. [Google Scholar] [CrossRef]
  17. Obradović, M.; Tuneski, N. Two types of the second Hankel determinant for the class U and the general class S . Acta Comment. Univ. Tartu. Math. 2023, 27, 59–67. [Google Scholar]
  18. Riaz, A.; Raza, M.; Binyamin, M.A.; Saliu, A. The second and third Hankel determinants for starlike and convex functions associated with Three-Leaf function. Heliyon 2023, 9, 12748. [Google Scholar] [CrossRef]
  19. Zaprawa, P. On Hankel determinant H2(3) for univalent functions. Results Math. 2018, 73, 89. [Google Scholar] [CrossRef]
  20. Babalola, K.O. On H3(1) Hankel determinant for some classes of univalent functions. In Inequality Theory and Applications; Cho, Y.J., Ed.; Nova Science Publishers: New York, NY, USA, 2010; Volume 6, pp. 1–7. [Google Scholar]
  21. Zaprawa, P. Third Hankel determinants for subclasses of univalent functions. Mediterr. J. Math. 2017, 14, 19. [Google Scholar] [CrossRef]
  22. Kowalczyk, B.; Lecko, A.; Thomas, D.K. The sharp bound of the third Hankel determinant for starlike functions. Forum Math. 2022, 34, 1249–1254. [Google Scholar] [CrossRef]
  23. Kowalczyk, B.; Lecko, A. The sharp bound of the third Hankel determinant for functions of bounded turning. Bol. Soc. Mat. Mex. 2021, 27, 69. [Google Scholar] [CrossRef]
  24. Kowalczyk, B.; Lecko, A.; Sim, Y.J. The sharp bound for the Hankel determinant of the third kind for convex functions. Bull. Aust. Math. Soc. 2018, 97, 435–445. [Google Scholar] [CrossRef]
  25. Banga, S.; Kumar, S.S. The sharp bounds of the second and third Hankel determinants for the class SL *. Math. Slovaca 2020, 70, 849–862. [Google Scholar] [CrossRef]
  26. Lecko, A.; Sim, Y.J.; Śmiarowska, B. The sharp bound of the Hankel determinant of the third kind for starlike functions of order 1/2. Complex Anal. Oper. Theory 2019, 13, 2231–2238. [Google Scholar] [CrossRef]
  27. Riaz, A.; Raza, M. The third Hankel determinant for starlike and convex functions associated with lune. Bull. Sci. Math. 2023, 187, 103289. [Google Scholar] [CrossRef]
  28. Riaz, A.; Raza, M.; Thomas, D.K. Hankel determinants for starlike and convex functions associated with sigmoid functions. Forum Math. 2022, 34, 137–156. [Google Scholar] [CrossRef]
  29. Carathéodory, C. Über den Variabilitätsbereich der Koeffizienten von Potenzreihen, die gegebene Werte nicht annehmen. Math. Ann. 1907, 64, 95–115. [Google Scholar] [CrossRef]
  30. Pommerenke, C. Univalent Functions; Vandenhoeck and Ruprecht: Göttingen, Germany, 1975. [Google Scholar]
  31. Duren, P.L. Univalent Functions; Grundlehren der mathematischen Wissenschaften; Springer: New York, NY, USA, 2001; Volume 259. [Google Scholar]
  32. Cho, N.E.; Kowalczyk, B.; Lecko, A. Sharp bounds of some coefficient functionals over the class of functions convex in the direction of the imaginary axis. Bull. Aust. Math. Soc. 2019, 100, 86–96. [Google Scholar] [CrossRef]
  33. Cho, N.E.; Kowalczyk, B.; Lecko, A.; Śmiarowska, B. On the Fourth and Fifth coefficients in the Carathéodory class. Filomat 2020, 34, 2061–2072. [Google Scholar] [CrossRef]
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content.

Share and Cite

MDPI and ACS Style

Ali, R.; Raza, M.; Bulboacă, T. Sharp Coefficient Bounds for Starlike Functions Associated with Cosine Function. Axioms 2024, 13, 442. https://doi.org/10.3390/axioms13070442

AMA Style

Ali R, Raza M, Bulboacă T. Sharp Coefficient Bounds for Starlike Functions Associated with Cosine Function. Axioms. 2024; 13(7):442. https://doi.org/10.3390/axioms13070442

Chicago/Turabian Style

Ali, Rashid, Mohsan Raza, and Teodor Bulboacă. 2024. "Sharp Coefficient Bounds for Starlike Functions Associated with Cosine Function" Axioms 13, no. 7: 442. https://doi.org/10.3390/axioms13070442

APA Style

Ali, R., Raza, M., & Bulboacă, T. (2024). Sharp Coefficient Bounds for Starlike Functions Associated with Cosine Function. Axioms, 13(7), 442. https://doi.org/10.3390/axioms13070442

Note that from the first issue of 2016, this journal uses article numbers instead of page numbers. See further details here.

Article Metrics

Back to TopTop