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Article

Sharp Coefficient Bounds for a Subclass of Bounded Turning Functions with a Cardioid Domain

1
School of Mathematics and Statistics, Anyang Normal University, Anyang 455002, China
2
Department of Mathematics and Statistics, University of Victoria, Victoria, BC V8W 3R4, Canada
3
Department of Medical Research, China Medical University Hospital, China Medical University, Taichung 40402, Taiwan
4
Department of Mathematics and Informatics, Azerbaijan University, 71 Jeyhun Hajibeyli Street, Baku AZ1007, Azerbaijan
5
Section of Mathematics, International Telematic University Uninettuno, 00186 Rome, Italy
6
Department of Applied Mathematics, Pukyong National University, Busan 48513, Republic of Korea
7
Department of Mathematics, Abdul Wali khan University Mardan, Mardan 23200, Pakistan
*
Author to whom correspondence should be addressed.
Axioms 2023, 12(8), 775; https://doi.org/10.3390/axioms12080775
Submission received: 1 July 2023 / Revised: 5 August 2023 / Accepted: 8 August 2023 / Published: 10 August 2023
(This article belongs to the Special Issue Recent Advances in Complex Analysis and Applications)

Abstract

:
In the present paper, we give a new simple proof on the sharp bounds of coefficient functionals related to the Carathéodory functions and make a correction on the extremal functions. The result is further used to investigate some initial coefficient bounds on a subclass of bounded turning functions R associated with a cardioid domain. For functions in this class, we calculate the bounds of the Fekete–Szegö-type inequality and the second- and third-order Hankel determinants. All the results are proved to be sharp.

1. Introduction and Definitions

Let H D represent the family of functions which are analytic in the unit disc D = z C : z < 1 . Let A denote the subfamily of H D consisting of functions in the form of
f ( z ) = z + k = 2 a k z k , z D .
Suppose that P indicates the class of the class of all functions p that are analytic in D with p ( z ) > 0 and
p z = 1 + n = 1 c n z n , z D .
If p P , it is a Carathéodory function. Assume that the set S A contains all univalent functions in D . Using the Koebe theorem, it is known that for each univalent function f S , there exist an inverse function f 1 defined at least on a disc of radius 1 / 4 with the Taylor’s series of the form
f 1 w : = w + n = 2 B n w n , w < 1 4 .
For two functions F 1 , F 2 H D , we say F 1 is subordinate to F 2 , written by F 1 F 2 , if there exists a function u which is analytic in D with u 0 = 0 and u ( z ) < 1 , such that F 1 ( z ) = F 2 u ( z ) , z D . The function u is called a Schwarz function. In the case of F 2 being univalent in D , then we have the relation
F 1 z F 2 z z D F 1 ( 0 ) = F 2 ( 0 ) and F 1 ( D ) F 2 ( D ) .
In geometric function theory, the most basic and important subfamilies of the set S are the family S of starlike functions, the family C of convex functions and the family R of bounded turning functions. The interested readers are referred to [1], (Chapter II). In 1994, Ma and Minda [2] introduced a class of analytic univalent functions φ z , which maps D onto the starlike domain with respect to φ ( 0 ) = 1 in the right half plane and is symmetric about the real axis. The Ma and Minda classes of C φ , S φ and R φ are characterized, respectively, as
C φ : = f A : z f ( z ) f ( z ) φ ( z ) , S φ : = f A : z f ( z ) f ( z ) φ ( z ) , R φ : = f A : f ( z ) φ ( z ) ,
see [3,4]. By considering different image domains φ ( D ) , various classes C φ , S φ and R φ of univalent functions were considered in recent years. For example, setting φ ( z ) = 1 + z , we obtain the class S L = S 1 + z , which represents the collection of functions in the class A that z f ( z ) f ( z ) lies in the domain bounded by the lemniscate of Bernoulli w 2 1 = 1 , see [5]. Choosing φ ˜ = 1 + 2 π 2 log 1 + z 1 z 2 , S p = S ( φ ˜ ) is the class of parabolic starlike functions. For functions f S p , its image of z f ( z ) f ( z ) under D is the parabolic domain given by w C : w > w 1 , see [6]. The class S c = S 1 + 4 3 z + 2 3 z 2 is a collection of starlike functions f A where z f ( z ) f ( z ) lies in the domain bounded by the cardiod Ω c = u + i v : 9 u 2 + 9 v 2 18 u + 5 2 16 9 u 2 + 9 v 2 6 u + 1 = 0 ; for further reading we refer to [7]. In [8], Wani and Swaminathan investigated the class S N e = S 1 + z 1 3 z 3 , consisting of functions associated with a nephroid domain. For other related works, see, for instance, [9,10,11]. Recently, S. Sivaprasad Kumar et al. [12] introduced and studied a class of starlike functions defined by
S C : = f A : z f ( z ) f ( z ) 1 + z e z = : ( z ) , z D ,
where ( z ) maps the unit disk onto a cardioid domain.
Motivated by the above works, we now consider a subfamily R of bounded turning functions defined by
R : = f A : f ( z ) 1 + z e z , z D .
For given parameters q , n N = 1 , 2 , , the Hankel determinant H q , n f was defined by Pommerenke [13,14] for a function f S of the form (1) as
H q , n f = a n a n + 1 a n + q 1 a n + 1 a n + 2 a n + q a n + q 1 a n + q a n + 2 q 2 , a 1 = 1 .
The upper bounds of H q , n f have been investigated for different subclasses of univalent functions. By applying Schwarz Lemma [15,16], Selin Aydinoğlua and Bülent Nafi Örnek [17] determined the sharp bounds of Hankel determinant H 2 , 1 ( f ) = a 3 a 2 2 for the class M α , defined by the condition f A and z f ( z ) 2 f ( z ) α < 1 , where α C . Of note, the Hankel determinant H 2 , 1 ( f ) is also known as Fekete–Szegö inequality. The absolute sharp bounds of the functional H 2 , 2 f = a 2 a 4 a 3 2 were found in [18,19] for each of the sets C , S and R . The Hankel determinant of order three is given as
H 3 , 1 f = 1 a 2 a 3 a 2 a 3 a 4 a 3 a 4 a 5 = a 5 a 2 2 + 2 a 2 a 3 a 4 a 3 3 + a 5 a 3 a 4 2 .
The estimation of the determinant H 3 , 1 f seems a little harder compared to the bound of H 2 , 2 f , see [20,21,22]. In 2010, Babalola [23] obtained the upper bound of H 3 , 1 f for the families of S , C and R . Later on, many authors obtained non-sharp bounds on H 3 , 1 f for different subfamilies of univalent functions, see, for example, [24,25,26]. The sharp bound of the third Hankel determinant for convex functions C was obtained in [27]. For f S , the upper bound of H 3 , 1 f was finally proved to be 4 9 by Kowalczyk et al. [28]. For the bounded turning functions R , the sharp upper bound of third Hankel determinant was calculated to be 1 4 in [29]. For some subclasses of convex functions, starlike functions and bounded turning functions, some sharp bounds of third Hankel determinant were also obtained in [30,31,32,33].
In the current article, our main goal is to calculate the sharp bounds on some initial coefficients for the class R of bounded turning functions linked with a cardioid domain. We also obtain the Fekete–Szegö inequality, and the sharp bounds of the second- and third-order Hankel determinants for this class. In proof of our results, we give a new simple proof of an estimation for the Carathéodory function and correct an error on the extremal function in Lemma 2.1 of [34].

2. A Set of Lemmas

The key to the proof of our results is the following lemmas.
Lemma 1 
([35]). Let p P be given by (2). Then, we have
2 c 2 = c 1 2 + x 4 c 1 2 ,
4 c 3 = c 1 3 + 2 4 c 1 2 c 1 x c 1 4 c 1 2 x 2 + 2 4 c 1 2 1 x 2 δ , 8 c 4 = c 1 4 + 4 c 1 2 x c 1 2 x 2 3 x + 3 + 4 x 4 4 c 1 2 1 x 2
· c 1 x 1 δ + x ¯ δ 2 1 δ 2 ρ
for some complex numbers x, δ and ρ, such that x 1 , δ 1 and ρ 1 .
Lemma 2 
([36]). If p P has the form (2), then
c n 2 for n 1 .
Lemma 3 
([37]). For any complex number μ and p P ,
c n + k μ c n c k 2 max 1 , 2 μ 1 .
Lemma 4 
([38]). Let ω ( z ) = n = 1 w k z k be a Schwarz function. Then, for real numbers μ and ν, we have the following sharp estimate given by
Ψ ( ω ) = w 3 + μ w 1 w 2 + ν w 1 3 Φ ( μ , ν ) ,
where Φ ( μ , ν ) is defined by
Φ ( μ , ν ) = 1 , ( μ , ν ) D 1 D 2 2 , 1 , ν , ( μ , ν ) k = 3 7 D k , 2 3 μ + 1 μ + 1 3 ( μ + 1 + ν ) , ( μ , ν ) D 8 D 9 , 1 3 ν μ 2 4 μ 2 4 ν μ 2 4 3 ν 1 , ( μ , ν ) D 10 D 11 2 , 1 , 2 3 ν 1 μ 1 3 μ 1 ν , ( μ , ν ) D 12 ,
and
D 1 = ( μ , ν ) : μ 1 2 , 1 ν 1 , D 2 = ( μ , ν ) : 1 2 μ 2 , 4 27 μ + 1 3 μ + 1 ν 1 , D 3 = ( μ , ν ) : μ 1 2 , ν 1 , D 4 = ( μ , ν ) : μ 1 2 , ν 2 3 μ + 1 , D 5 = ( μ , ν ) : μ 2 , ν 1 , D 6 = ( μ , ν ) : 2 μ 4 , ν 1 12 μ 2 + 8 , D 7 = ( μ , ν ) : μ 4 , ν 2 3 μ 1 , D 8 = ( μ , ν ) : 1 2 μ 2 , 2 3 μ + 1 ν 4 27 μ + 1 3 μ + 1 , D 9 = ( μ , ν ) : μ 2 , 2 3 μ + 1 ν 2 μ μ + 1 μ 2 + 2 μ + 4 , D 10 = ( μ , ν ) : 2 μ 4 , 2 μ μ + 1 μ 2 + 2 μ + 4 ν 1 12 μ 2 + 8 , D 11 = ( μ , ν ) : μ 4 , 2 μ μ + 1 μ 2 + 2 μ + 4 ν 2 μ μ 1 μ 2 2 μ + 4 , D 12 = ( μ , ν ) : μ 4 , 2 μ μ 1 μ 2 2 μ + 4 ν 2 3 μ 1 .
The following Lemma was obtained by Virendra Kumar et al. [34] in 2019. As the authors point out, it is of independent interest as well. Unfortunately, there are some minor mistakes on the extremal function. Next, we will give a new more simple proof of this result using Lemma 4.
Lemma 5. 
Let p ( z ) = 1 + p 1 z + p 2 z 2 + p 3 z 3 + P . Then, for any real number σ,
σ p 3 p 1 3 2 σ 4 , σ < 4 3 , 2 σ σ σ 1 , σ 4 3 .
The above estimate is sharp.
Proof. 
Let p P and
p ( z ) = 1 + p 1 z + p 2 z 2 + p 3 z 3 + , z D .
Suppose that ω ( z ) = p ( z ) 1 p ( z ) + 1 . Clearly, ω ( 0 ) = 0 . Since p ( z ) lies in the right half plane and z 1 z + 1 maps the right half plane to the unit disk, we know ω ( z ) < 1 . Thus, ω is a Schwarz function. Assume that
ω ( z ) = w 1 z + w 2 z 2 + w 3 z 3 + w 4 z 4 + , z D .
From the fact that
p ( z ) = 1 + ω ( z ) 1 ω ( z ) = 1 + 2 w 1 z + 2 w 1 2 + 2 w 2 z 2 + 2 w 1 3 + 4 w 2 w 1 + 2 w 3 z 3 + ,
we have p 1 = 2 w 1 , p 2 = 2 w 2 + w 1 2 and p 3 = 2 w 3 + 2 w 2 w 1 + w 1 3 . It follows that
σ p 3 p 1 3 = 2 σ w 3 + 4 σ w 1 w 2 + 2 σ 8 w 1 3 .
As σ = 0 the proof is trivial, we assume that σ 0 in the following. Then, we obtain
σ p 3 p 1 3 = 2 σ w 3 + 2 w 1 w 2 + σ 4 σ w 1 3 .
Let μ = 2 , ν = σ 4 σ . Clearly, μ , ν is only possible to lie in the disk D 4 , D 5 , D 6 , D 8 and D 9 , which can be further specified as
D 4 = ( μ , ν ) : μ 1 2 , ν 2 , D 5 = ( μ , ν ) : μ 2 , ν 1 , D 6 = ( μ , ν ) : 2 μ 4 , ν 1 , D 8 = ( μ , ν ) : 1 2 μ 2 , 2 ν 1 , D 9 = ( μ , ν ) : μ 2 , 2 ν 1 .
For σ < 0 , it is observed that ν > 1 and ( μ , ν ) D 5 D 6 . Thus, we have
w 3 + 2 w 1 w 2 + σ 4 σ w 1 3 ν = σ 4 σ .
For 0 < σ < 4 3 , we see ν < 2 and ( μ , ν ) D 4 . Thus,
w 3 + 2 w 1 w 2 + σ 4 σ w 1 3 ν = σ 4 σ .
For σ 4 3 , we know 2 ν < 1 and ( μ , ν ) D 8 D 9 . Then we deduce that
w 3 + 2 w 1 w 2 + σ 4 σ w 1 3 2 3 μ + 1 μ + 1 3 ( μ + 1 + ν ) = σ σ 1 .
Combining (15)–(18), the result of Lemma 5 follows. □
Remark 1. 
In [34], the authors gave an extremal function f given by
f ( z ) = 1 z 2 1 2 σ σ 1 z + z 2 , σ > 4 3 .
Let q = σ σ 1 . It is seen that
f ( z ) = 1 + 2 q z + 2 2 q 2 1 z 2 + 2 q 4 q 2 3 z 3 + 2 8 q 4 8 q 2 + 1 z 4 + , z D .
We know f P because c 1 = 2 q > 2 . Hence, the extremal function is not correct, since it is not a Carathéodory function. Indeed, the extremal function f ^ for σ > 4 3 can be defined by taking
f ^ ( z ) = 1 + p ^ 1 z + p ^ 2 z 2 + p ^ 3 z 3 + , z D ,
where p ^ 1 = σ σ 1 , p ^ 2 = σ 2 σ 1 and p ^ 3 = 2 σ 3 σ σ σ 1 3 .

3. Coefficient Bounds for the Family R

We begin this section by finding the bounds on some initial coefficients for functions in the class R .
Theorem 1. 
If f R has the series representation of the form (1), then
a 2 1 2 , a 3 1 3 , a 4 14 14 0.2673 .
These bounds are best possible.
Proof. 
Let f R . Then (5) can be written by Schwarz function as
f z = 1 + ω ( z ) e ω z , z D .
Assuming that
ω z = w 1 z + w 2 z 2 + w 3 z 3 + , z D ,
and
p z = 1 + ω z 1 ω z = 1 + c 1 z + c 2 z 2 + c 3 z 3 + c 4 z 4 + , z D .
It is seen that p P and
ω z = p z 1 p z + 1 = c 1 z + c 2 z 2 + c 3 z 3 + c 4 z 4 + 2 + c 1 z + c 2 z 2 + c 3 z 3 + c 4 z 4 + , z D .
From (1) we obtain
f z = 1 + 2 a 2 z + 3 a 3 z 2 + 4 a 4 z 3 + 5 a 5 z 4 + .
By simplifications and using the series expansion of (23), we obtain
1 + ω ( z ) e ω z = 1 + 1 2 c 1 z + 1 2 c 2 z 2 + 1 16 c 1 3 + 1 2 c 3 z 3 + 1 24 c 1 4 3 16 c 1 2 c 2 + 1 2 c 4 z 4 + .
Comparing (24) and (25), we have
a 2 = 1 4 c 1 ,
a 3 = 1 6 c 2 ,
a 4 = 1 8 1 8 c 1 3 + c 3 ,
a 5 = 1 10 1 12 c 1 4 3 8 c 1 2 c 2 + c 4 .
For a 2 and a 3 , implementing Lemma 2, we obtain a 2 1 2 and a 3 1 3 . For a 4 , an application of Lemma 5 leads us to a 4 1 4 8 7 = 14 14 . The equality of a 2 and a 3 are achieved by the functions f 1 and f 2 given, respectively, by
f 1 z = 0 z 1 + t e t d t = z + 1 2 z 2 + 1 3 z 3 + 1 8 z 4 + 1 30 z 5 + , z D ,
f 2 z = 0 z 1 + t 2 e t 2 d t = z + 1 3 z 3 + 1 5 z 5 + 1 14 z 7 + 1 54 z 9 + , z D .
The equality on the bounds of a 4 is obtained by f 3 defined by
f 3 z = 0 z 1 + ω ( t ) e ω ( t ) d t , z D ,
where ω ( z ) = p ( z ) 1 p ( z ) + 1 and
p ( z ) = 1 + 56 7 z 6 7 z 2 26 14 49 z 3 + , z D .
It is verified that
f 3 ( z ) = z + 14 14 z 2 1 7 z 3 14 14 z 4 + , z D .
The proof of Theorem 1 is thus completed. □
Theorem 2. 
If f is of the form (1) belonging to R , then
a 3 γ a 2 2 max 1 3 , 3 γ 4 12 , γ C .
This inequality is sharp.
Proof. 
Employing (26) and (27), we may write
a 3 γ a 2 2 = 1 6 c 2 3 8 γ c 1 2 .
An application of (12) leads us to
a 3 γ a 2 2 max 1 3 , 3 γ 4 12 .
This result is sharp for the functions f 1 and f 2 given by (30) and (31). □
Theorem 3. 
Let f R . Then
a 2 a 3 a 4 1 4 .
This inequality is sharp with the extremal function f 4 given by
f 4 z = 0 z 1 + t 3 e t 3 d t = z + 1 4 z 4 + 1 7 z 7 + 1 20 z 10 + 1 78 z 13 + , z D .
Proof. 
Using (26)–(28), we have
a 2 a 3 a 4 = 1 8 c 3 1 3 c 1 c 2 1 8 c 1 3 .
From (21) and (22), it is noted that
c 1 = 2 w 1 ,
c 2 = 2 w 2 + w 1 2 ,
c 3 = 2 w 3 + 2 w 1 w 2 + w 1 3 .
Hence, we obtain
a 2 a 3 a 4 = 1 4 w 3 + 4 3 w 1 w 2 1 6 w 1 3 .
Taking μ = 4 3 and ν = 1 6 , we know ( μ , ν ) D 2 . Using Lemma 4, we easily obtain
a 2 a 3 a 4 1 4 .
Clearly, the bound is sharp with the extremal function given by (35). □
Theorem 4. 
If f R , then
H 2 , 2 f = a 2 a 4 a 3 2 1 9 .
The inequality is sharp with the extremal function given by (31).
Proof. 
From (26)–(28), we have
H 2 , 2 f = 1 256 c 1 4 + 1 32 c 1 c 3 1 36 c 2 2 .
Let f R and f θ ( z ) = e i θ f ( e i θ z ) , θ R . We have H 2 , 2 ( f θ ) = H 2 , 2 ( f ) for all θ R . Hence, when estimating the upper bounds of H 2 , 2 ( f ) , we may assume a 2 of f to be real, and thus c 1 : = c [ 0 , 2 ] . Using (8) and (9) to express c 2 and c 3 in terms of c 1 = c , we obtain
H 2 , 2 f = 7 2304 c 4 + 1 576 c 2 4 c 2 x 1 1152 4 c 2 c 2 + 32 x 2 + 1 64 c 4 c 2 1 x 2 δ .
With the aid of the triangle inequality, replacing δ 1 , x = t 1 and taking c 0 , 2 , we obtain
H 2 , 2 f 7 2304 c 4 + 1 576 c 2 4 c 2 t + 1 1152 4 c 2 c 2 + 32 t 2 + 1 64 c 4 c 2 1 t 2 = : K c , t .
It is noted that
K t = 1 576 c 2 ( 4 c 2 ) + 1 576 4 c 2 c 2 18 c + 32 t 0
for t 0 , 1 , thus K c , t K c , 1 . Putting t = 1 gives
H 2 , 2 f 7 2304 c 4 + 1 576 c 2 4 c 2 + 1 1152 4 c 2 c 2 + 32 = : χ ( c ) .
Since χ ( c ) = 1 2304 c 4 40 c 2 + 256 and χ c 0 on [ 0 , 2 ] , we know χ is decreasing for c [ 0 , 2 ] and
H 2 , 2 f χ ( 0 ) = 1 9 .
The equality is obtained by the extremal function defined by (31). This completes the proof of Theorem 4. □
Theorem 5. 
If f R has the form (1), then
H 3 , 1 f 1 16 .
This inequality is sharp with the extremal function f 4 given by (35).
Proof. 
From the definition, H 3 , 1 f can be written as
H 3 , 1 f = 2 a 2 a 3 a 4 a 3 3 a 4 2 + a 3 a 5 a 2 2 a 5 .
Let c 1 = c . By putting (26)–(29) into (41), we obtain
H 3 , 1 f = 1 552 , 960 423 c 6 + 1344 c 4 c 2 + 2160 c 3 c 3 3456 c 2 c 2 2 3456 c 2 c 4 + 5760 c c 2 c 3 2560 c 2 3 + 9216 c 2 c 4 8640 c 3 2 .
Let f R and f θ = e i θ f e i θ z , θ R . Note that H 3 , 1 ( f θ ) = H 3 , 1 ( f ) for all θ R , we may also assume that c [ 0 , 2 ] . Suppose that b = 4 c 2 . Using (8)–(10), we obtain
H 3 , 1 f = 1 552 , 960 71 c 6 + 2304 b 2 x 3 320 b 3 x 3 + 576 c 2 b x 2 + 144 c 4 b x 3 612 c 4 b x 2 + 72 c 4 b x + 36 c 2 b 2 x 4 288 c 2 b 2 x 3 816 c 2 b 2 x 2 2160 b 2 1 x 2 2 δ 2 + 576 c 2 b 1 x 2 1 δ 2 ρ 576 c 3 b x 1 x 2 δ 576 c 2 b x ¯ 1 x 2 δ 2 + 936 c 3 b 1 x 2 δ 144 c b 2 x 2 1 x 2 δ 2304 b 2 x 2 1 x 2 δ 2 576 c b 2 x 1 x 2 δ + 2304 b 2 x 1 x 2 1 δ 2 ρ ,
where ρ , x , δ D ¯ : = z : z 1 . Observing that H 3 , 1 f can be written as
H 3 , 1 f = 1 552 , 960 d 1 c , x + d 2 c , x δ + d 3 c , x δ 2 + Φ c , x , δ ρ ,
with
d 1 c , x = 71 c 6 + 4 c 2 4 c 2 1024 x 3 + 32 c 2 x 3 + 36 c 2 x 4 816 c 2 x 2 + 576 c 2 x 2 612 c 4 x 2 + 144 c 4 x 3 + 72 c 4 x , d 2 c , x = 72 4 c 2 1 x 2 4 c 2 2 c x 2 32 c x + 13 c 3 , d 3 c , x = 144 4 c 2 1 x 2 4 c 2 x 2 15 4 c 2 x ¯ , Φ c , x , δ = 576 4 c 2 1 x 2 1 δ 2 c 2 + 4 x 4 c 2 .
Taking x = t , δ = y and utilizing the fact ρ 1 , we obtain
H 3 , 1 f 1 552 , 960 d 1 c , x + d 2 c , x y + d 3 c , x y 2 + Φ c , x , δ . 1 552 , 960 Γ c , t , y ,
where
Γ c , t , y = h 1 c , t + h 2 c , t y + h 3 c , t y 2 + h 4 c , t 1 y 2 ,
with
h 1 c , t = 71 c 6 + 4 c 2 4 c 2 1024 t 3 + 32 c 2 t 3 + 36 c 2 t 4 + 816 c 2 t 2 + 576 c 2 t 2 + 144 c 4 t 3 + 612 c 4 t 2 + 72 c 4 t , h 2 c , t = 72 4 c 2 1 t 2 4 c 2 2 c t 2 + 13 c 3 + 32 c t , h 3 c , t = 144 4 c 2 1 t 2 4 c 2 t 2 + 15 + 4 c 2 t , h 4 c , t = 576 4 c 2 1 t 2 c 2 + 4 t 4 c 2 .
Now, we have to maximize Γ in the closed cuboid Θ : = 0 , 2 × 0 , 1 × 0 , 1 . It is not hard to see that Γ ( 0 , 0 , 1 ) = 34 , 560 . Thus, we have max ( c , t , y ) Θ Γ ( c , t , y ) 34 , 560 . We aim to prove that the maximum values of Γ with ( c , t , y ) Θ is simply equal to 34,560. For this, we first show that the maximum value of Γ is obtained on the face y = 1 of Θ .
On the face t = 1 , it reduces to Γ ( c , 1 , y ) = r 1 ( c ) = 127 c 6 3312 c 4 + 8256 c 2 + 16 , 384 . Then,
r 1 c = 6 c 127 c 4 2208 c 2 + 2752 c .
Putting r 1 c = 0 , we obtain the only critical point c ^ 0 = 1104 136 47 127 1.1625 for c ( 0 , 2 ) . Therefore, max r 1 ( c ) 21 , 805.95 with the maximum value attained on c = c ^ 0 . Thus, we assume that t < 1 . Furthermore, for the points on the face c = 2 , Γ ( 2 , t , y ) 4544 for all ( t , y ) [ 0 , 1 ] × [ 0 , 1 ] . Hence, we further assume that c < 2 .
Let c , t , y 0 , 2 × 0 , 1 × 0 , 1 . By differentiating Γ partially with respect to y, we obtain
Γ y = h 2 ( c , t ) + 2 h 3 ( c , t ) h 4 ( c , t ) y .
Obviously, we have
H y y = 0 = h 2 ( c , t ) 0 .
Let
H y y = 1 = h 2 ( c , t ) + 2 h 3 ( c , t ) h 4 ( c , t ) = : ζ 1 ( c , t ) .
It is noted that
ζ 1 ( c , t ) = 72 ( 4 c 2 ) ( 1 t 2 ) ζ 2 ( c , t ) ,
where
ζ 2 ( c , t ) = ( 4 c 2 ) ( 2 c t 2 + 4 t 2 + 60 64 t ) + 13 c 3 + 32 c t + 16 c 2 t 16 c 2 .
Clearly, we have
ζ 2 ( c , t ) ( 4 c 2 ) ( 4 t 2 + 60 64 t ) + 13 c 3 + 16 c 2 t 16 c 2 = : η ( c , t ) .
Suppose that η ( c , t ) = η 0 + η 1 t + η 2 t 2 , where η 0 = 240 76 c 2 + 13 c 3 , η 1 = 80 c 2 256 and η 2 = 16 4 c 2 . Taking η as a polynomial of degree 2 with respect to t, we know η 2 > 0 and the symmetric axis t 0 is defined as
t 0 = η 1 2 η 2 = 2 ( 16 5 c 2 ) 4 c 2 .
Let c ˜ 0 = 4 5 . For c [ c ˜ 0 , 2 ) , it is observed that t 0 0 . Then, the minimum value of η is achieved on t = 0 . We thus have
η ( c , t ) η ( c , 0 ) = η 0 40 > 0 , c [ c ˜ 0 , 2 ) .
Let c ¯ 0 = 2 7 3 . It is seen that t 0 1 for c [ 0 , c ¯ 0 ] . It follows that
η ( c , t ) η ( c , 1 ) = η 0 + η 1 + η 2 = 13 c 3 0 , c 0 , c ¯ 0 .
Assume that c ( c ¯ 0 , c ˜ 0 ) . Then t 0 ( 0 , 1 ) . Hence, the minimum value of η is obtained on t = t 0 . This leads to
η ( c , t ) η c , t 0 = η 0 η 1 2 4 η 2 = ι ( c ) 4 c 2 ,
where
ι ( c ) = 13 c 5 324 c 4 + 52 c 3 + 2016 c 2 3136 , c ( c ¯ 0 , c ˜ 0 ) .
It is calculated that ι achieves its minimum value of about 56.9731 on c = c ˜ 0 , thus we know
η ( c , t ) > 0 , c ( c ¯ 0 , c ˜ 0 ) .
Combining (45)–(47), we have η ( c , t ) 0 on 0 , 2 × [ 0 , 1 ) , which leads to ζ 1 ( c , t ) 0 for all ( c , t ) [ 0 , 2 ) × 0 , 1 . Therefore, we have Γ y y = 1 0 . As Γ y is a linear continuous function with respect to y, we have
Γ y min Γ y y = 0 , Γ y y = 1 0 , y [ 0 , 1 ] .
Hence, Γ ( c , t , y ) Γ ( c , t , 1 ) for all ( c , t , y ) [ 0 , 2 ) × [ 0 , 1 ) × [ 0 , 1 ] . Based on the above discussions, it reduces to find the global maximum value of Γ on the face y = 1 of Θ . On the face y = 1 , we have
Γ ( c , t , 1 ) = 71 c 6 + 4 c 2 2 36 ( c 2 4 c 4 ) t 4 + 32 ( c 2 + 32 ) t 3 + 48 ( 17 c 2 + 3 c 42 ) t 2 + 2160 + ( 4 c 2 ) 144 c ( c 3 4 c 16 ) t 3 + 36 c 2 ( 17 c 2 26 c + 16 ) t 2 + 72 c ( c 3 + 8 c + 32 ) t + 936 c 3 = : Λ ( c , t ) .
By observing that c 2 4 c 4 0 and c 3 4 c 16 0 for c [ 0 , 2 ) , we have
Λ ( c , t ) 71 c 6 + 4 c 2 2 32 ( c 2 + 32 ) t 3 + 48 ( 17 c 2 + 3 c 42 ) t 2 + 2160 + ( 4 c 2 ) 36 c 2 ( 17 c 2 26 c + 16 ) t 2 + 72 c ( c 3 + 8 c + 32 ) t + 936 c 3 = : Q ( c , t ) .
Furthermore, using 17 c 2 26 c + 16 0 , t 3 t 2 t leads to
Q ( c , t ) 71 c 6 + 4 c 2 2 32 ( c 2 + 32 ) t 2 + 48 ( 17 c 2 + 3 c 42 ) t 2 + 2160 + ( 4 c 2 ) 36 c 2 ( 17 c 2 26 c + 16 ) t + 72 c ( c 3 + 8 c + 32 ) t + 936 c 3 = 4 ( 4 c 2 ) R ( c , t ) + 71 c 6 + 2160 ( 4 c 2 ) 2 + 936 ( 4 c 2 ) c 3 = : W ( c , t ) ,
where
R ( c , t ) = 4 ( 4 c 2 ) ( 53 c 2 + 9 c 62 ) t 2 + 9 c ( 19 c 3 26 c 2 + 32 c + 64 ) t .
Clearly, if c 1 , we have 53 c 2 + 9 c 62 0 and 19 c 3 26 c 2 + 32 c + 64 0 , which leads to
R ( c , t ) R ( c , 1 ) , c [ 1 , 2 ) .
Then, we obtain
W ( c , t ) 4 ( 4 c 2 ) R ( c , 1 ) + 71 c 6 + 2160 ( 4 c 2 ) 2 + 936 ( 4 c 2 ) c 3 = : ϱ 1 ( c ) , c [ 1 , 2 ) .
In virtue of ϱ 1 ( c ) = 235 c 6 + 144 c 5 4032 c 4 3456 c 3 + 8832 c 2 + 11 , 520 c + 18 , 688 obtaining its maximum value of about 32,192.46 on c 1.1053 for c [ 1 , 2 ) , we have Λ ( c , t ) < 34 , 560 on [ 1 , 2 ) × [ 0 , 1 ) . Suppose that c [ 0 , 1 ) and m ( c ) = 19 c 3 26 c 2 + 32 c + 64 . It is noted that m ( c ) = 54 c 2 52 c + 32 0 for c [ 0 , 1 ) . Thus, we have m ( c ) [ 64 , 89 ) . Since 0 < 4 c 2 4 and c 2 c , it is not hard to see that
R ( c , t ) 992 ( c 1 ) t 2 + 801 c t = : V ( c , t ) .
Let V ( c , t ) = v 1 t + v 2 t 2 , where v 1 = 801 c and v 2 = 992 ( c 1 ) . Obviously, we have v 2 < 0 . Considering V as a polynomial of degree 2 with respect to t, we obtain the symmetric axis t ¯ 0 defined by
t ¯ 0 = v 1 2 v 2 = 801 c 1984 ( 1 c ) .
For c > c ˙ 0 = 1984 2785 0.7124 , we have t ¯ 0 > 1 . Then, the maximum value of V is attained on t = 1 , which implies that V ( c , t ) V ( c , 1 ) = 1793 c 992 . Then,
W ( c , t ) 4 ( 4 c 2 ) V ( c , 1 ) + 71 c 6 + 2160 ( 4 c 2 ) 2 + 936 ( 4 c 2 ) c 3 = : ϱ 2 ( c ) , c c ˙ 0 , 1 .
It is calculated that
ϱ 2 ( c ) = 71 c 6 936 c 5 + 2160 c 4 3428 c 3 13 , 312 c 2 + 28 , 688 c + 18 , 688 , c c ˙ 0 , 1 ,
which obtains its maximum value of about 32,127.89 on c 0.8966 . Hence, we obtain
Γ ( c , t ) < 34560 , ( c , t ) [ c ˙ 0 , 1 ) × [ 0 , 1 ) .
For c [ 0 , c ˙ 0 ) , we have t 0 [ 0 , 1 ) . Then, we obtain
V ( c , t ) v 1 2 4 v 2 = 801 2 3968 · c 2 1 c 162 c 2 1 c 162 c 2 ,
which yields to
W ( c , t ) 648 ( 4 c 2 ) c 2 + 71 c 6 + 2160 ( 4 c 2 ) 2 + 936 ( 4 c 2 ) c 3 = : ϱ 3 ( c ) , c [ 0 , c ˙ 0 ) .
In light of
ϱ 3 ( c ) = 71 c 6 936 c 5 + 1512 c 4 + 3744 c 3 14 , 688 c 2 + 34 , 560 , c [ 0 , c ˙ 0 ) ,
it is not hard to see that ϱ 3 achieves its maximum value 34,560 on c = 0 . Therefore, we conclude that
Λ ( c , t ) 34 , 560 , ( c , t ) [ 0 , 2 ) × [ 0 , 1 ) .
From the above cases, we obtain
Γ c , t , y 34 , 560 on 0 , 2 × 0 , 1 × 0 , 1 .
Using (43), it follows that
H 3 , 1 f 1 552 , 960 Γ c , t , y 1 16 = 0.0625 .
The proof of Theorem 5 is thus completed. □

Author Contributions

The idea was proposed by L.S. and improved by H.M.S., L.S., N.E.C. and M.A. wrote and completed the calculations. H.M.S. and M.A. checked all the results. All authors read and approved the final 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 gratitude for the referees’ valuable suggestions which truly improved the present work.

Conflicts of Interest

The authors declare no conflict of interest.

References

  1. Duren, P. Univalent Functions; Grundlehren der Mathematischen Wissenschaften 259, New York, Berlin, Heidelberg, Tokyo; Springer: Berlin/Heidelberg, Germany, 1983. [Google Scholar]
  2. Ma, W.C.; Minda, D. A unified treatment of some special classes of univalent functions. In Proceedings of the Conference on Complex Analysis, Tianjin, China, 19–23 June 1992; pp. 157–169. [Google Scholar]
  3. Cho, N.E.; Kwon, O.S.; Lecko, A.; Sim, Y.J. Sharp estimates of generalized zalcman functional of early coefficients for Ma-Minda type functions. Filomat 2018, 32, 6267–6280. [Google Scholar] [CrossRef] [Green Version]
  4. Sharma, P.; Raina, R.K.; Sokół, J. Certain Ma-Minda type classes of analytic functions associated with the crescent-shaped region. Anal. Math. Phys. 2019, 9, 1887–1903. [Google Scholar] [CrossRef]
  5. Madaan, V.; Kumar, A.; Ravichandran, V. Starlikeness associated with lemniscate of Bernoulli. Filomat 2019, 33, 1937–1955. [Google Scholar] [CrossRef] [Green Version]
  6. Ali, R.M.; Ravichandran, V. Uniformly convex and uniformly starlike functions. Ramanujan Math. Newsl. 2011, 355, 16–30. [Google Scholar]
  7. Sharma, K.; Jain, N.K.; Ravichandran, V. Starlike functions associated with a cardioid. Afr. Mat. 2016, 27, 923–939. [Google Scholar] [CrossRef]
  8. Wani, L.A.; Swaminathan, A. Starlike and convex functions associated with a nephroid domain. Bull. Malays. Math. Sci. Soc. 2021, 44, 79–104. [Google Scholar] [CrossRef]
  9. 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]
  10. Goel, P.; Sivaprasad Kumar, S. Certain class of starlike functions associated with modified sigmoid function. Bull. Malays. Math. Sci. Soc. 2020, 43, 957–991. [Google Scholar] [CrossRef]
  11. Gandhi, S. Radius estimates for three leaf function and convex combination of starlike functions. In Mathematical Analysis 1: Approximation Theory ICRAPAM; Deo, N., Gupta, V., Acu, A., Agrawal, P., Eds.; Springer: Singapore, 2018; Volume 306. [Google Scholar]
  12. Sivaprasad Kumar, S.; Kamaljeet, G. A cardioid domain and starlike functions. Anal. Math. Phys. 2021, 11, 54. [Google Scholar] [CrossRef]
  13. Pommerenke, C. On the coefficients and Hankel determinants of univalent functions. J. Lond. Math. Soc. 1966, 1, 111–122. [Google Scholar] [CrossRef]
  14. Pommerenke, C. On the Hankel determinants of univalent functions. Mathematika 1967, 14, 108–112. [Google Scholar] [CrossRef]
  15. Mateljević, M. Schwarz lemma and Kobayashi metrics for harmonic and holomorphic functions. J. Math. Anal. Appl. 2018, 464, 78–100. [Google Scholar] [CrossRef]
  16. Mateljević, M.; Mutavdžic, N.; Örnek, B.N. Note on some classes of holomorphic functions related to Jack’s and Schwarz’s lemma. Appl. Anal. Discret. Math. 2022, 16, 111–131. [Google Scholar] [CrossRef]
  17. Aydinoğlua, S.; Örnek, B.N. Estimates concerned with Hankel determinant for (α) class. Filomat 2022, 36, 3679–3688. [Google Scholar] [CrossRef]
  18. Janteng, A.; Halim, S.A.; Darus, M. Coefficient inequality for a function whose derivative has a positive real part. J. Inequalities Pure Appl. Math. 2006, 7, 1–5. [Google Scholar]
  19. Janteng, A.; Halim, S.A.; Darus, M. Hankel determinant for starlike and convex functions. Int. J. Math. 2007, 1, 619–625. [Google Scholar]
  20. Cho, N.E.; Kowalczyk, B.; Kwon, O.S.; Lecko, A.; Sim, Y.J. The bounds of some determinants for starlike functions of order alpha. Bull. Malays. Math. Sci. Soc. 2018, 41, 523–535. [Google Scholar] [CrossRef]
  21. Shi, L.; Srivastava, H.M.; Arif, M.; Hussain, S.; Khan, H. An investigation of the third Hankel determinant problem for certain subfamilies of univalent functions involving the exponential function. Symmetry 2019, 11, 598. [Google Scholar] [CrossRef] [Green Version]
  22. Srivastava, H.M.; Khan, B.; Khan, N.; Tahir, M.; Ahmad, S.; Khan, N. Upper bound of the third Hankel determinant for a subclass of q-starlike functions associated with the q-exponential function. Bull. Sci. Math. 2021, 167, 102942. [Google Scholar] [CrossRef]
  23. Babalola, K.O. On H3(1) Hankel determinant for some classes of univalent functions. Inequal. Theory Appl. 2010, 6, 1–7. [Google Scholar]
  24. Kwon, O.S.; Lecko, A.; Sim, Y.J. The bound of the Hankel determinant of the third kind for starlike functions. Bull. Malays. Math. Sci. Soc. 2019, 42, 767–780. [Google Scholar] [CrossRef] [Green Version]
  25. Altınkaya, Ş.; Yalçın, S. Third Hankel determinant for Bazilevič functions. Adv. Math. 2016, 5, 91–96. [Google Scholar]
  26. Zaprawa, P.; Obradović, M.; Tuneski, N. Third Hankel determinant for univalent starlike functions. Revista de la Real Academia de Ciencias Exactas, Físicas y Naturales. Ser. A Mat. 2021, 115, 1–6. [Google Scholar]
  27. Kowalczyk, B.; Lecko, A.; Sim, Y.J. The sharp bound of the Hankel determinant of the third kind for convex functions. Bull. Aust. Math. Soc. 2018, 97, 435–445. [Google Scholar] [CrossRef]
  28. 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]
  29. 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]
  30. 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] [Green Version]
  31. 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]
  32. Shi, L.; Arif, M.; Ullah, K.; Alreshidi, N.; Shutaywi, M. On sharp estimate of third Hankel determinant for a subclass of starlike functions. Fractal Fract. 2022, 6, 437. [Google Scholar] [CrossRef]
  33. Wang, Z.G.; Raza, M.; Arif, M.; Ahmad, K. On the third and fourth Hankel determinants for a subclass of analytic functions. Bulletin of the Malaysian Mathematical Sciences Society 2022, 45, 323–359. [Google Scholar] [CrossRef]
  34. Kumar, V.; Cho, N.E.; Ravichandran, V.; Srivastava, H.M. A sharp coefficient bounds for starlike functions associated with the Bell numbers. Math. Slovaca 2019, 69, 1053–1064. [Google Scholar] [CrossRef]
  35. Kwon, O.S.; Lecko, A.; Sim, Y.J. On the fourth coefficient of functions in the Carathéodory class. Comput. Methods Funct. Theory 2018, 18, 307–314. [Google Scholar] [CrossRef]
  36. Pommerenke, C. Univalent Function; Vanderhoeck & Ruprecht: Göttingen, Germany, 1975. [Google Scholar]
  37. Libera, R.J.; Złotkiewicz, E.J. Coefficient bounds for the inverse of a function with derivative in P, II. Proc. Am. Math. Soc. 1984, 92, 58–60. [Google Scholar]
  38. Prokhorov, D.V.; Szynal, J. Inverse coefficients for (α,β)-convex functions. Ann. Univ. Mariae Curie-Sklodowska (Sect. A) 1981, 3, 125–143. [Google Scholar]
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Shi, L.; Srivastava, H.M.; Cho, N.E.; Arif, M. Sharp Coefficient Bounds for a Subclass of Bounded Turning Functions with a Cardioid Domain. Axioms 2023, 12, 775. https://doi.org/10.3390/axioms12080775

AMA Style

Shi L, Srivastava HM, Cho NE, Arif M. Sharp Coefficient Bounds for a Subclass of Bounded Turning Functions with a Cardioid Domain. Axioms. 2023; 12(8):775. https://doi.org/10.3390/axioms12080775

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Shi, Lei, Hari Mohan Srivastava, Nak Eun Cho, and Muhammad Arif. 2023. "Sharp Coefficient Bounds for a Subclass of Bounded Turning Functions with a Cardioid Domain" Axioms 12, no. 8: 775. https://doi.org/10.3390/axioms12080775

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