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Article

Sharp Coefficient and Hankel Problems Related to a Symmetric Domain

1
School of Mathematics and Computer Sciences, Chifeng University, Chifeng 024000, China
2
Department of Mathematics and Statistics, Hazara University Mansehra, Mansehra 21120, Pakistan
3
Department of Mathematics, COMSATS University Islamabad, Abbottabad Campus, Abbottabad 22060, Pakistan
4
Department of Basic Sciences, Preparatory Year Deanship, King Faisal University, Al Ahsa 31982, Saudi Arabia
*
Authors to whom correspondence should be addressed.
These authors contributed equally to this work.
Symmetry 2023, 15(10), 1865; https://doi.org/10.3390/sym15101865
Submission received: 24 July 2023 / Revised: 4 September 2023 / Accepted: 22 September 2023 / Published: 4 October 2023
(This article belongs to the Special Issue Symmetry in Pure Mathematics and Real and Complex Analysis)

Abstract

:
In the current article, we utilize the concept of subordination to establish a new subclass of analytic functions associated with a bounded domain that is symmetric about the real axis. By applying the convolution technique, we derive the necessary and sufficient condition, the radius of convexity for this recently introduced class. Furthermore, we prove the sharp upper bounds for the second-order Hankel determinants | H 2 , 1 ξ | , | H 2 , 2 ξ | and third-order Hankel determinant | H 3 , 1 ξ | for the functions ξ belonging to the newly defined class.

1. Introduction

Let A denote the class of all of analytic functions ξ ( μ ) defined in the open unit disk U = { μ : μ C and μ < 1 } , whose normalized Maclaurin series representation is given as:
ξ μ = μ + t = 2 a t μ t , μ U ,
with normalization conditions ξ ( 0 ) = 0 and ξ ( 0 ) = 1 . A function is said to be univalent if it never takes the same value twice. By S , we mean the subclass of A containing all the functions which are univalent in U . Subordination is an important tool used to investigate various inclusion and radii problems for certain classes of analytic functions.
A function ξ is subordinate to g in U written as ξ g if there exists a Schwarz function χ , which is analytic in U and χ ( 0 ) = 0 with χ ( μ ) < 1 , such that ξ μ = g ( χ μ ) . In addition, if the function g is univalent in U , then we have
ξ 0 = g 0 and ξ U g U .
By S , C , K and R , we mean the well known subclasses of S consisting of starlike, convex, close-to-convex and functions with bounded turnings, respectively.
The convolution of two regular functions ξ and ς in U , with the series representation of ξ given in (1) and ς = μ + t = 2 b t μ t , is defined as
ξ ς μ = μ + t = 2 a t b t μ t , μ U .
In 1985, Padmanabhan et al. [1] defined the integrated families of starlike and convex functions by using the theory of convolution along with the function μ 1 μ a , where a R . Shanmugam [2] generalized the idea of [1] and introduced the general form of functions class S h ( ϕ ) by considering an analytic function ϕ ( μ ) with ϕ ( 0 ) = 1 , and h μ A , as:
S h ( ϕ ) = ξ A : μ ( ξ h ) ( ξ h ) ϕ ( μ ) , μ U .
By taking h μ = μ 1 μ or μ 1 μ 2 , we obtain the well known classes S ( ϕ ) and C ( ϕ ) of the Ma and Minda types of starlike and convex function defined in [3]. Further, by choosing ϕ ( μ ) = 1 + μ 1 μ , the classes S ( ϕ ) and C ( ϕ ) reduce to S and C classes.
In the recent past, a large number of researchers have defined and studied several interesting subclasses of analytic and univalent functions by restricting ϕ ( μ ) in the general form of S ( ϕ ) and C ( ϕ ) . Here we highlight some of them:
(i)
Let ϕ ( μ ) = 1 + F μ 1 + G μ ,   1 G < F 1 . Geometrically, ϕ ( μ ) maps the open unit disc onto a domain whose center lies on the real axis and is also symmetric about the real axis. For function value ϕ ( μ ) , we get S [ F , G ] = S 1 + F μ 1 + G μ , the class of Janowski starlike functions; see [4].
(ii)
For ϕ ( μ ) = cos μ , the class S cos μ was studied by Bano et al. [5], while for ϕ ( μ ) = cosh μ , the function class S cosh μ was introduced and studied by Alotaibi et al. [6].
(iii)
For ϕ ( μ ) = e μ , the class S e was defined and studied by Mendiratta [7].
(iv)
For ϕ ( μ ) = 1 + sin μ , the class S ϕ reduces to S sin , which was introduced and investigated by Cho et al. [8].
(v)
For ϕ ( μ ) = 1 + μ 1 3 μ 3 , we obtain the class S n e p investigated by Wani and Swaminathan [9].
(vi)
For ϕ ( μ ) = 1 + sinh 1 μ , the class S ϕ was introduced and investigated by Kumar et al. [10].
(vii)
For ϕ ( μ ) = 2 1 + e μ , the class S ϕ reduces to S s i g ; see [11].
(viii)
For ϕ ( μ ) = 1 + μ , we get S 1 + μ = S L investigated by Sokol et al. [12].
(ix)
For ϕ ( μ ) = 1 + tanh μ , the class becomes S tanh μ , which was introduced by Khalil et al. [13]; see also [14].
By taking inspiration and motivation from above cited work, we introduce the following subclass of analytic functions.
Definition 1. 
Let ξ A be given in (1). Then, ξ CV T if the following condition holds true:
μ ξ ( μ ) ξ ( μ ) 1 + tanh μ , μ U .
Geometrically, the class CV T contains all the functions ξ that lie within the image domain of 1 + tanh μ for a specified radius. It can be easily seen that the image of unit disc under 1 + tanh μ has an appealing geometry which is symmetric about the real axis.
Let ξ A , and for given values of n ,   q 1 the q t h Hankel determinant H q , n ξ was defined in [15] as follows:
H q , n ξ = a n a n + 1 . . . a n + q 1 a n + 1 . . . . . . . . . . . . . . . . . . . . . . . a n + q 1 . . . . a n + 2 q 1 .
Finding the sharp upper bounds of Hankel determinants H q , n for different subfamilies and certain values of n and q has become the most attractive and important problem in the theory of analytic functions.
In [16], Hayman proved that for ξ S the best sharp inequality is
H 2 , n ( ξ ) λ n ,
where λ > 0 . Similarly, Janteng et al. [17] estimated the sharp bounds for the second Hankel determinant for the classes of K , S and R as:
H 2 , 2 ( ξ ) 1 8 , ξ K , 1 , ξ S , 4 9 , ξ R .
In 2010 , Babalola [18] calculated the upper bounds of H 3 , 1 ( ξ ) for S and C . Later, many authors have estimated H 3 , 1 ( ξ ) for different subfamilies of analytic functions, see [8,19] and the references cited therein. Zaprawa [20] amended Babalola’s [18] results and claimed that they are still not the best possible, and gives the estimated value as:
H 3 , 1 ( ξ ) 49 540 , ξ K , 1 , ξ S , 41 60 , ξ R .
Furthermore, Kwon et al. [21] improved this bound as H 3 , 1 ( ξ ) 8 / 9 for ξ S . Furthermore, Zaprawa et al. [22] extend their work by estimating H 3 , 1 ( ξ ) 5 / 9 for ξ S . Working in a similar direction, the authors of [23,24,25,26] contributed by extending this work for various subfamilies of univalent functions. In the recent past, Arif et al. [27] calculated the sharpness of H 3 , 1 ( ξ ) and the coefficient bounds for a subfamily of starlike functions related to sigmoid functions, while, Shi et al. [28] estimated the sharp third Hankel determinant for functions with bounded turning along with logarithmic coefficients connected to a petal-shaped domain, whereas Ponnusamy et al. [29] defined these logarithmic coefficients for the families of inverse, starlike and convex univalent functions. The coefficient estimates help us to study the area and arc length problems.
The main objective of this study is to determine the sharp bounds for the second and third Hankel determinants, as well as the sharp upper bounds of the coefficient inequalities for functions belonging to CV T .

2. Set of Lemmas

Let P denote the class of analytic functions p such that p ( 0 ) = 1 and
p ( μ ) > 0 , μ U and having the series of the form:
p μ = 1 + t = 1 c t μ t , μ U .
The following lemmas will be helpful in our subsequent work.
Lemma 1
([15]). Let p P given by (6). Then, the following hold
c t 2 f o r t 1 ,
c t + k λ c t c k < 2 f o r 0 λ 1 ,
c t + 2 k λ c t c k 2 2 ( 1 + 2 λ ) , f o r λ R ,
and
c 2 c 1 2 2 2 c 1 2 2 .
Lemma 2. 
Let p P , given by (6). Then there exist k , δ and ρ with k 1 , δ 1 , and ρ 1 such that
c 2 = 1 2 c 1 2 + k 4 c 1 2 ,
c 3 = 1 4 c 1 3 + 2 c 1 k 4 c 1 2 4 c 1 2 c 1 k 2 + 2 4 c 1 2 1 k 2 δ ,
c 4 = 1 8 c 1 4 + k 4 c 1 2 ( 4 k + ( k 2 3 k + 3 ) c 1 2 ) 4 4 c 1 2 1 k 2 ( c ( k 1 ) δ ρ 1 δ 2 + δ 2 k ˜ ) .
The inequalities given in (11), (12) and (13) are due to [15], [30] and [31], respectively.
Lemma 3
([30]). If p P is given by (6), then for 0 B 1 and
B 2 B 1 D B we have
c 3 2 B c 1 c 2 + D c 1 3 2 .

3. Main Results

Theorem 1. 
Let ξ CV T , given in (1). Then
1 μ ξ μ M μ 2 L μ 1 μ 3 0 ,
where
M = 2 + tanh e i θ and L = tanh e i θ .
Proof. 
As ξ CV T is analytic in U , 1 μ ξ μ 0 for all μ in U . Then, by using the definition of subordination and (4), we have
μ ξ ( μ ) ξ ( μ ) = 1 + tanh χ μ ,
where, χ μ is the Schwarz function. Let χ μ = e i θ , π θ π . Then (17) becomes
μ ξ μ ξ μ tanh e i θ ,
which implies
μ 2 ξ μ μ ξ μ tanh e i θ 0 .
It can be easily seen that
μ 2 ξ μ + μ ξ μ = ξ μ μ 1 + μ 1 μ 3 and μ ξ μ = ξ μ μ 1 μ 2 .
Using (19) in (18) we get
ξ μ M μ 2 L μ 1 μ 3 0 .
From (20), we will obtain (15), where M and L are given in (16). □
Theorem 2. 
Let ξ A . Then, ξ CV T if
n = 2 M L n n 1 n n + 1 2 a n μ n 1 1 0 ,
where M and L are given in (16).
Proof. 
If ξ CV T , then from Theorem 1, we have
1 μ ξ μ M μ 2 L μ 1 μ 3 0 ,
which is equivalent to
1 μ ξ μ M μ 2 1 μ 3 ξ μ L μ 1 μ 3 0 .
Since μ 2 = μ 1 + μ μ , we have
1 μ M ξ μ μ 1 + μ 1 μ 3 ξ μ μ 1 μ 3 L ξ μ μ 1 μ 3 0 .
Now, applying (19) and some properties of convolution, (22), reduces to
1 μ M μ 2 ξ μ L 1 2 μ 2 ξ μ + μ ξ μ 0 .
Using (1) and after some simplification, we obtain (21). □
Theorem 3. 
Let ξ A be given in (1). Then, ξ CV T if
n = 2 4 + n n 3 tanh e i θ a n < 2 tanh e i θ .
Proof. 
To prove our required result, we use relation (21) as
1 n = 2 4 + n n 3 tanh e i θ 2 tanh e i θ a n μ n 1 > 1 n = 2 4 + n n 3 tanh e i θ 2 tanh e i θ a n μ n 1 .
From (23), we have
1 n = 2 4 + n n 3 tanh e i θ 2 tanh e i θ a n > 0 .
From (24), (25) and using Theorem 2, we have the desired result. □
Theorem 4. 
Let ξ CV T . Then, ξ is convex of order α ,   0 α < 1 and μ < r 1 , where
r 1 = inf n 2 4 + n n 3 tanh e i θ 2 tanh e i θ 1 α n n α 1 n 1 .
Proof. 
It is sufficient to show that
μ ξ ( μ ) ξ ( μ ) 1 1 α .
From (1), we have
μ ξ μ ξ μ n = 2 n n 1 a n μ n 1 1 n = 2 n a n μ n 1 .
(28) is bounded above by 1 α if
n = 2 n n 1 + n 1 α 1 α a n μ n 1 1 .
As ξ CV T , from Theorem 1 and for some fixed n , we have
a n 2 tanh e i θ 4 + n n 3 tanh e i θ .
From (29) and (30), we can obtain (26). □
Theorem 5. 
Let ξ CV T . Then
a 2 1 2 , a 3 1 6 and a 4 1 12 .
The first two inequalities are sharp for ξ 1 , and the third inequality is sharp for ξ 3 :
ξ 1 = 0 μ exp 0 t tanh x x d x d t = μ + 1 2 μ 2 + 1 6 μ 3 + 1 72 μ 4 . . . .
ξ 3 = 0 μ exp 0 t tanh x 3 x d x d t = μ + μ 4 12 + μ 7 126 + . . . .
Proof. 
As ξ CV T ,
μ ξ ( μ ) ξ ( μ ) 1 + tan h μ ,
which implies
μ ξ ( μ ) ξ ( μ ) = 1 + tan h χ μ .
From (1), we have
μ ξ ( μ ) ξ ( μ ) = 1 + 2 a 2 μ + 6 a 3 4 a 2 2 μ 2 + 12 a 4 18 a 2 a 3 + 8 a 2 3 μ 3 + 20 a 5 32 a 2 a 4 18 a 3 2 + 48 a 3 a 2 2 16 a 2 4 μ 4 + . . . .
Let p P , then we have
p μ = 1 + χ μ 1 χ μ = 1 + c 1 μ + c 2 μ 2 + c 3 μ 3 + c 4 μ 4 + .
This implies that
χ μ = 1 2 c 1 μ + 1 2 c 2 1 4 c 1 2 μ 2 + 1 8 c 1 3 1 2 c 1 c 2 + 1 2 c 3 μ 3 + 1 2 c 4 1 2 c 1 c 3 1 4 c 2 2 1 16 c 1 4 + 3 8 c 1 2 c 2 μ 4 + .
Then
1 + tanh χ μ = 1 + 1 2 c 1 μ + 1 2 c 2 1 4 c 1 2 μ 2 + 1 12 c 1 3 1 2 c 1 c 2 + 1 2 c 3 μ 3 + 1 2 c 4 + 1 4 c 1 2 c 2 1 2 c 1 c 3 1 4 c 2 2 μ 4 + .
From (34) and (35), we have
a 2 = 1 4 c 1 ,
a 3 = 1 12 c 2 ,
a 4 = 1 12 1 24 c 1 3 1 8 c 2 c 1 + 1 2 c 3 ,
a 5 = 1 20 5 144 c 1 4 1 12 c 1 2 c 2 1 6 c 3 c 1 1 8 c 2 2 + 1 2 c 4 .
Then, from Lemma 1 we have
a 2 1 2 , a 3 1 6 .
From (38), we have
a 4 = 1 24 c 3 1 4 c 1 c 2 1 12 c 1 3 ,
by using Lemma 3 we have
a 4 1 12 .
Theorem 6. 
Let ξ CV T , then
H 2 , 1 ξ = a 3 a 2 2 1 6 .
The result is sharp for the function
ξ 2 = 0 μ exp 0 t tanh x 2 x d x d t = μ + μ 3 6 + μ 5 40 + . . . .
Proof. 
As ξ CV T , from (36) and (37), we have
a 3 a 2 2 = 1 12 c 2 1 16 c 1 2 = 1 12 c 2 3 4 c 1 2 ,
then from Lemma 1 we get
H 2 , 1 ξ 1 6 .
Theorem 7. 
Let ξ CV T . Then
H 2 , 2 ξ = a 2 a 4 a 3 2 1 36 .
This inequality is sharp for the function given in (41).
Proof. 
As ξ CV T , from (36)–(38), we have
a 2 a 4 a 3 2 = 1 1152 c 1 4 1 384 c 1 2 c 2 + 1 96 c 3 c 1 1 144 c 2 2 .
Using Lemma 2 we obtain
a 2 a 4 a 3 2 = 1 576 t 2 k 2 1 384 t k 2 c 1 2 + 1 2304 t k c 1 2 + 1 192 1 | k | 2 δ t c 1 1 768 c 1 4 .
From t = 4 c 1 2 , c 1 = c ,   δ 1 ,   k = b and using triangular inequality, we have
a 2 a 4 a 3 2 1 2304 4 ( 4 c 2 ) 2 b 2 + 6 ( 4 c 2 ) b 2 c 2 + ( 4 c 2 ) b c 2 + 12 ( 1 b 2 ) ( 4 c 2 ) c + 3 c 4 .
Consider
ξ ( c , b ) = 4 ( 4 c 2 ) 2 b 2 + 6 ( 4 c 2 ) b 2 c 2 + ( 4 c 2 ) b c 2 + 12 ( 1 b 2 ) ( 4 c 2 ) c + 3 c 4 .
To find the maximum value of ξ ( c , b ) , let
ξ b = 4 c 2 32 b + 4 b c 2 24 b c + c 2 0 ,
which implies
ξ ( c , b ) ξ ( c , 1 ) .
Putting b = 1 , we get
a 2 a 4 a 3 2 1 2304 4 ( 4 c 2 ) 2 + 6 ( 4 c 2 ) c 2 + ( 4 c 2 ) c 2 + 3 c 4 .
Now let
G ( c ) = 4 ( 4 c 2 ) 2 + 7 ( 4 c 2 ) c 2 + 3 c 4 ,
which implies
G c = 8 c 0 for all c 0 , 2 ,
which shows that G ( c ) is the decreasing function, so the maximum value occurs at c = 0 , so (43) becomes
H 2 , 2 ξ 1 36 .
Theorem 8. 
Let ξ CV T . Then
H 3 , 1 ξ 1 144 .
This result is sharp for the function given in (32).
Proof. 
From (5), we have
H 3 , 1 ξ = 2 a 2 a 3 a 4 a 2 2 a 5 a 3 3 + a 3 a 5 a 4 2 .
Using (36)–(39) with c 1 = c , we have
H 3 , 1 ξ = 1 414720 50 c 6 207 c 2 c 2 2 456 c 2 3 720 c 3 2 + 864 c 2 c 4 648 c 2 c 4 + 336 c 3 c 3 + 78 c 4 c 2 + 792 c c 2 c 3 .
From Lemma 3, with 4 c 2 = t , we can simplify terms occurring in (45) as
207 c 2 c 2 2 = 207 4 c 6 + 207 2 c 4 t k + 207 4 c 2 t 2 k 2 , 456 c 2 3 = 57 t 3 k 3 + 171 t 2 k 2 c 2 + 171 t k c 4 + 57 c 6 , 720 c 3 2 = 45 c 6 90 c 4 t k 2 + 180 c 4 t k + 180 c 3 1 k 2 t δ + 45 c 2 t 2 k 4 180 c 2 t 2 k 3 + 180 c 2 t 2 k 2 180 c 1 k 2 t 2 k 2 δ + 360 c 1 k 2 t 2 k δ + 180 1 k 2 2 t 2 δ 2 , 864 c 2 c 4 = 54 c 6 + 54 c 4 t k 3 162 c 4 t k 2 + 216 c 4 t k 216 1 k 2 c 3 t k δ + 216 1 k 2 c 3 t δ + 54 c 2 t 2 k 4 162 c 2 t 2 k 3 + 162 c 2 t 2 k 2 + 216 c 2 t k 2 216 1 k 2 c 2 t k δ 2 + 216 1 k 2 1 δ 2 ρ c 2 t 216 1 k 2 c t 2 k 2 δ + 216 1 k 2 c t 2 k δ + 216 t 2 k 3 216 1 k 2 t 2 k 2 δ 2 + 216 1 k 2 1 δ 2 ρ t 2 k , 648 c 2 c 4 = 81 c 6 + 81 t c 4 k 3 243 t c 4 k 2 + 243 t c 4 k 324 1 k 2 t c 3 k δ + 324 1 k 2 t c 3 δ + 324 t c 2 k 2 324 1 k 2 t c 2 k δ 2 + 324 1 k 2 t 1 δ 2 ρ c 2 , 336 c 3 c 3 = 84 c 6 84 t c 4 k 2 + 168 t c 4 k + 168 1 k 2 t δ c 3 , 78 c 4 c 2 = 39 c 6 + 39 t k c 4 , 792 c c 2 c 3 = 99 c 6 99 c 4 t k 2 + 297 c 4 t k + 198 1 k 2 δ c 3 t 99 c 2 t 2 k 3 + 198 c 2 t 2 k 2 + 198 1 k 2 δ c t 2 k .
Putting above values in (45), we have
H 3 , 1 ξ = 1 414720 35 4 c 6 27 c 4 t k 3 12 c 4 t k 2 + 45 2 c 4 t k + 108 c 3 1 k 2 t k δ + 78 c 3 1 k 2 t δ + 108 c 2 1 k 2 t k δ 2 108 1 δ 2 ρ c 2 1 k 2 t + 9 c 2 t 2 k 4 81 c 2 t 2 k 3 171 4 c 2 t 2 k 2 108 c 2 t k 2 36 c 1 k 2 t 2 k 2 δ + 54 c 1 k 2 t 2 k δ 180 1 k 2 2 t 2 δ 2 216 1 k 2 t 2 k 2 δ 2 + 216 1 δ 2 ρ 1 k 2 t 2 k 57 t 3 k 3 + 216 t 2 k 3 .
Since t = 4 c 2 , it follows that
H 3 , 1 ξ ( μ ) = 1 414720 u 1 ( c , k ) + u 2 ( c , k ) δ + u 3 ( c , k ) δ 2 + ϕ ( c , k , δ ) ρ ,
where
u 1 ( c , k ) = 35 4 c 6 3 4 ( 4 c 2 ) k ( 4 c 2 ) k 57 c 2 12 c 2 k 2 + 32 c 2 k + 16 k + 144 c 2 k + 16 c 4 k + 36 c 4 k 2 30 c 4 , u 2 ( c , k ) = 6 c ( 1 k 2 ) ( 4 c 2 ) 6 k 2 9 k ( 4 c 2 ) 18 c 2 k 13 c 2 , u 3 ( c , k ) = 36 ( 1 k 2 ) ( 4 c 2 ) k 2 + 5 ( 4 c 2 ) 3 c 2 k , ϕ ( c , k , δ ) = 108 ( 1 k 2 ) ( 4 c 2 ) 2 ( 4 c 2 ) k c 2 ( 1 δ 2 ) .
k = k and δ = y , are replaced with ρ 1 , such that
H 3 , 1 ξ = 1 414720 u 1 ( c , k ) + u 2 ( c , k ) y + u 3 ( c , k ) y 2 + ϕ ( c , k , δ ) , 1 414720 ψ ( c , k , y ) .
where
ψ ( c , k , y ) = v 1 ( c , k ) + v 2 ( c , k ) y + v 3 ( c , k ) y 2 + v 4 ( c , k ) ( 1 y 2 ) ,
with
v 1 ( c , k ) = 35 4 c 6 + 3 4 ( 4 c 2 ) k k 57 c 2 + 12 c 2 k 2 + 32 c 2 k + 16 k ( 4 c 2 ) + 144 c 2 k + 16 c 4 k + 36 c 4 k 2 + 30 c 4 , v 2 ( c , k ) = 6 c ( 1 k 2 ) ( 4 c 2 ) 6 k 2 + 9 k ( 4 c 2 ) + 18 c 2 k + 13 c 2 , v 3 ( c , k ) = 36 ( 1 k 2 ) ( 4 c 2 ) k 2 + 5 ( 4 c 2 ) + 3 c 2 k , v 4 ( c , k ) = 108 ( 1 k 2 ) ( 4 c 2 ) 2 k ( 4 c 2 ) + c 2 .
To maximize the function ψ ( c , k , y ) in the cuboid, Δ = 0 , 2 × 0 , 1 × 0 , 1 , we need to discuss the maximum values of ψ ( c , k , y ) inside on the six faces as well as on edges of Δ .
1. Interior points of the cuboid
First, we check the maximum value in the interior of the cuboid; for this, let ψ c , k , y 0 , 2 × 0 , 1 × 0 , 1 and consider
ψ y = 6 c ( 1 k 2 ) ( 4 c 2 ) 6 k 2 + 9 k ( 4 c 2 ) + 18 c 2 k + 13 c 2 + 72 ( 1 k 2 ) ( 4 c 2 ) 4 c 2 k 5 + 3 c 2 k 1 y ,
for critical point in Δ , ψ y = 0 , which gives
y = c 3 k ( 4 c 2 ) 2 k + 3 + c 2 18 k + 13 12 4 c 2 5 k 36 c 2 k 1 = y 1 ,
since y 1 0 , 1 ,
c 3 k ( 4 c 2 ) 2 k + 3 + c 2 18 k + 13 + 12 4 c 2 5 k 1 k 36 c 2 1 k
and
c 2 4 5 k 8 k .
In order to show the existence of the critical points, we must find solutions that meet the inequalities in (49) and (50). For this let h ( k ) = 4 5 k 8 k , and calculations show that h ( k ) < 0 , that is a decreasing function on 0 , 1 , so
c 2 16 7 .
Simple calculation shows that inequality (49) does not hold true for k 0 , 1 , which means in the interior of the cuboid, there are no critical points.
2. On the six faces of the cuboid
We will now examine the interior of each of the six faces of Δ to find the maximum of ψ c , k , y .
i On the face c = 0 , we have
p 1 k , y = ψ ( 0 , k , y ) = 192 k 3 + 3456 k + 576 y 2 k 1 k 5 1 k 2 ,
for critical points, let
p 1 y = 1152 y k 2 1 k 1 k 5 0 ,
which indicates that p 1 has no optimum points in 0 , 1 × 0 , 1 .
ii On the face c = 2 , we have
ψ ( 2 , k , y ) = 560 .
iii On the face k = 0
p 2 c , y = ψ ( c , 0 , y ) = 35 4 c 6 + 78 c 3 y 4 c 2 + 288 c 4 y 2 108 c 4 1872 c 2 y 2 + 432 c 2 + 2880 y 2 .
For the critical point, let
p 2 y = 6 4 c 2 13 c 3 96 y c 2 + 240 y ,
putting p 2 y = 0 gives
y = 13 c 3 48 2 c 2 5 = y 0 .
For the specified range of y ,   y 0 0 , 1 , if c > c 0 1.5811388 .
Further p 2 c = 0 gives
3 2 c 35 c 4 260 c 3 y + 768 c 2 y 2 288 c 2 + 624 c y 2496 y 2 + 576 = 0 .
Putting the value of (52) in (53), we get
333 c 9 8070 c 7 + 48564 c 5 112320 c 3 + 86400 c = 0 .
Now solving for c 0 , 2 , we get c 1.2691 , which shows that no optimal solution exists.
iv On the face k = 1
p 3 c , y = ψ ( c , 1 , y ) = 23 c 6 456 c 4 + 1548 c 2 + 192 ,
for critical points, let
p 3 c = 138 c 5 1824 c 3 + 3096 c .
Putting p 3 c = 0 , we obtained c 1.4142 , at which p 3 attains its maximum value, which is
p 3 c , y 1648 .
v On the face y = 0
p 4 c , k = ψ ( c , k , 0 ) = 9 c 6 k 4 3 c 6 k 3 + 123 4 c 6 k 2 45 2 c 6 k + 35 4 c 6 72 c 4 k 4 288 c 4 k 3 294 c 4 k 2 + 306 c 4 k 108 c 4 + 144 c 2 k 4 + 2016 c 2 k 3 + 684 c 2 k 2 1728 c 2 k + 432 c 2 3264 k 3 + 3456 k ,
for critical points inside 0 , 2 × 0 , 1 , let
p 4 c = 54 c 5 k 4 18 c 5 k 3 + 369 2 c 5 k 2 135 c 5 k + 105 2 c 5 288 c 3 k 4 1152 c 3 k 3 1176 c 3 k 2 + 1224 c 3 k 432 c 3 + 288 c k 4 + 4032 c k 3 + 1368 c k 2 3456 c k + 864 c
and
p 4 k = 36 c 6 k 3 9 c 6 k 2 + 123 2 c 6 k 45 2 c 6 288 c 4 k 3 864 c 4 k 2 588 c 4 k + 306 c 4 + 576 c 2 k 3 + 6048 c 2 k 2 + 1368 c 2 k 1728 c 2 9792 k 2 + 3456 .
Computation shows that these systems of equations p 4 c = 0 and p 4 k = 0 do not have a solution in 0 , 2 × 0 , 1 .
vi On the face y = 1
p 5 c , k = ψ ( c , k , 1 ) = 9 c 6 k 4 3 c 6 k 3 + 123 4 c 6 k 2 45 2 c 6 k + 35 4 c 6 36 c 5 k 4 + 54 c 5 k 3 + 114 c 5 k 2 54 c 5 k 78 c 5 108 c 4 k 4 + 36 c 4 k 3 546 c 4 k 2 18 c 4 k + 180 c 4 + 288 c 3 k 4 600 c 3 k 2 + 312 c 3 + 432 c 2 k 4 144 c 2 k 3 + 2268 c 2 k 2 + 432 c 2 k 1440 c 2 576 c k 4 864 c k 3 + 576 c k 2 + 864 c k 576 k 4 + 192 k 3 2304 k 2 + 2880 .
Now, for the critical point, let
p 5 c = 54 c 5 k 4 18 c 5 k 3 + 369 2 c 5 k 2 135 c 5 k + 105 2 c 5 180 c 4 k 4 + 270 c 4 k 3 + 570 c 4 k 2 270 c 4 k 390 c 4 432 c 3 k 4 + 144 c 3 k 3 2184 c 3 k 2 72 c 3 k + 720 c 3 + 864 c 2 k 4 1800 c 2 k 2 + 936 c 2 + 864 c k 4 288 c k 3 + 4536 c k 2 + 864 c k 2880 c 576 k 4 864 k 3 + 576 k 2 + 864 k
and
p 5 k = 36 c 6 k 3 9 c 6 k 2 + 123 2 c 6 k 45 2 c 6 144 c 5 k 3 + 162 c 5 k 2 + 228 c 5 k 54 c 5 432 c 4 k 3 + 108 c 4 k 2 1092 c 4 k 18 c 4 + 1152 c 3 k 3 1200 c 3 k + 1728 c 2 k 3 432 c 2 k 2 + 4536 c 2 k + 432 c 2 2304 c k 3 2592 c k 2 + 1152 c k + 864 c 2304 k 3 + 576 k 2 4608 k .
Computation indicates that the solution to the system of equation p 5 c = 0 and p 5 k = 0 does not exist in 0 , 2 × 0 , 1 .
3. On the twelve edges of the cuboid
Now, to find the maximum of ψ c , k , y on the twelve edges of the cuboid
i On k = 0 and y = 0
p 6 c = ψ ( c , 0 , 0 ) = 35 4 c 6 108 c 4 + 432 c 2 ,
putting p 6 c = 0 , gives the critical value c 1.8516 , at which we have
ψ ( c , 0 , 0 ) 564 .
ii On k = 0 and y = 1
p 7 c = ψ ( c , 0 , 1 ) = 35 4 c 6 78 c 5 + 180 c 4 + 312 c 3 1440 c 2 + 2880 .
Differentiating w . r . t c”, we have
p 7 c = 105 2 c 5 390 c 4 + 720 c 3 + 936 c 2 2880 c 0 ,
for all c [ 0 , 2 ] ; thus, the maximum occurs at c = 0
ψ ( c , 0 , 1 ) 2880 .
iii On k = 0 and c = 0 , we obtain
p 8 ( y ) = ψ ( 0 , 0 , y ) = 2880 y 2 .
Clearly, p 8 y > 0 for y [ 0 , 1 ] , which shows that the function is increasing, so the maximum value occurs at y = 1
p 8 ( y ) 2880 .
As the terms ψ ( c , 1 , 0 ) and ψ ( c , 1 , 1 ) are free from k, that is
p 9 c = ψ ( c , 1 , 0 ) = ψ ( c , 1 , 1 ) = 23 c 6 456 c 4 + 1548 c 2 + 192 .
Putting p 9 c = 0 and solving, we obtained c 1.4142 , at which p 9 attains its maximum value, which is
p 9 c 1648 .
iv On c = 0 and k = 1
p 10 y = ψ 0 , 1 , y = 192 .
v On c = 2
ψ ( 2 , k , 0 ) = ψ ( 2 , k , 1 ) = ψ ( 2 , 0 , y ) = ψ ( 2 , 1 , y ) = 560 .
vi On c = 0 and y = 0
p 11 k = ψ ( 0 , k , 0 ) = 3456 k 3264 k 3 ,
for critical points, p 11 k = 0 , and we get k 0.59409 , at which the maximum value is
p 11 k 1368 .
vii On y = 1 and c = 0 , we have
p 12 k = ψ ( 0 , k , 1 ) = 576 k 4 + 192 k 3 2304 k 2 + 2880 .
By checking p 12 k , the maximum value occurs at k = 0 , which is
p 12 k 2880 .
From all the computations, we conclude that
ψ c , k , y 2880 .
Hence, it follows from (46) that
H 3 , 1 ξ 1 144 .

4. Conclusions

In the present investigation, we studied a new subclass of analytic functions related to a bounded, symmetric domain. We focused our attention on deriving sharp coefficient bounds, second and third Hankel determinants and the radius problem for functions belonging to this class. This study can be extended to the classes of meromorphic and harmonic functions and can be related to q-calculus as well.

Author Contributions

Methodology, H.T.; Writing—original draft, A.A. (Adeel Ahmad) and A.R.; Writing—review and editing, A.A. (Asad Ali) and S.H.; Conceptualization, A.A. (Adeel Ahmad) and S.H.; Validation, S.N. All authors have read and agreed to the published version of the manuscript.

Funding

The following funding organizations provided assistance to the first author in this work: (i) the Natural Science Foundation of the People’s Republic of China under Grant 11561001 and the Natural Science Foundation of Inner Mongolia of the People’s Republic of China under Grant 2022MS01004; (ii) the program for young Talents of Science and Technology in Universities of Inner Mongolia Autonomous Region under Grant NJYT-18-A14 and the Higher School Foundation of Inner Mongolia of the People’s Republic of China under Grant NJZY22168 and (iii) the program for Key Laboratory Construction of Chifeng University (no. CFXYZD202004) and the Research and Innovation Team of Complex Analysis and Nonlinear Dynamic Systems of Chifeng University (no. cfxykycxtd202005).

Data Availability Statement

No data were used to support this study.

Acknowledgments

The authors would like to thank the editor and the anonymous reviewers for their constructive comments and suggestions, which helped us to improve the manuscript. This work was supported by the Deanship of Scientific Research, the Vice Presidency for Graduate Studies and Scientific Research, King Faisal University, Saudi Arabia (Grant no. 4312).

Conflicts of Interest

The authors declare no conflict of interest.

References

  1. Padmanabhan, K.S.; Parvatham, R. Some applications of differential subordination. Bull. Aust. Math. Soc. 1985, 32, 321–330. [Google Scholar] [CrossRef]
  2. Shanmugam, T.N. Convolution and Differential subordination. Int. J. Math. Math. Sci. 1989, 12, 333–340. [Google Scholar] [CrossRef]
  3. Ma, W.C.; Minda, D. A unified treatment of some special classes of univalent functions. In Conference on Complex Analysis; Li, Z., Ren, F., Yang, L., Zhang, S., Eds.; International Press: New York, NY, USA, 1992; pp. 157–169. [Google Scholar]
  4. Janowski, W. Extremal problems for a family of functions with positive real part and for some related families. Ann. Polonici Math. 1971, 23, 159–177. [Google Scholar] [CrossRef]
  5. Bano, K.; Raza, M. Starlike functions associated with cosine function. Bull. Iran. Math. Soc. 2021, 47, 1513–1532. [Google Scholar] [CrossRef]
  6. Alotaibi, A.; Arif, M.; Alghamdi, M.A.; Hussain, S. Starlikness associated with cosine hyperbolic function. Mathematics 2020, 8, 1118. [Google Scholar] [CrossRef]
  7. Mendiratta, S.; Nagpal, V.; 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]
  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. 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]
  10. Kumar, S.S.; Arora, K. Starlike functions associated with a petal shaped domain. arXiv 2020, arXiv:2010.10072. [Google Scholar]
  11. Geol, P.; Kumar, S.S. Certain class of starlike functions associated with modified sigmoid function. Bull. Malays. Math. Sci. Soc. 2020, 43, 957–991. [Google Scholar] [CrossRef]
  12. Sokol, J.; Stankiewicz, J. Radius of convexity of some subclasses of strongly starlike functions. Zeszyty Naukowe Oficyna Wydawnicza al. Powstanców Warszawy 1996, 19, 101–105. [Google Scholar]
  13. Ullah, K.; Zainab, S.; Arif, M.; Darus, M.; Shutaywi, M. Radius problems for starlike functions associated with the tan hyperbolic function. J. Funct. Space 2021, 2021, 9967640. [Google Scholar] [CrossRef]
  14. 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. Ineq Appl. 2021, 2021, 1–20. [Google Scholar] [CrossRef]
  15. Pommerenke, C.; Jensen, G. Univalent Functions; Vandenhoeck and Ruprecht: Gottingen, Germany, 1975. [Google Scholar]
  16. Hayman, W.K. On second Hankel determinant of mean univalent functions. Proc. Lond. Math. Soc. 1968, 3, 77–94. [Google Scholar] [CrossRef]
  17. 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, 1–5. [Google Scholar]
  18. Babalola, K.O. On H 3(1) Hankel determinant for some classes of univalent functions. Inequal. Theory Appl. 2010, 6, 1–7. [Google Scholar]
  19. Wang, Z.-G.; Arif, M.; Liu, Z.H.; Zainab, S.; Fayyaz, R.; Ihsan, M.; Shutaywi, M. Sharp bounds of Hankel determinants for certain subclass of starlike functions. J. Appl. Anal. Comput. 2023, 13, 860–873. [Google Scholar] [CrossRef] [PubMed]
  20. Zaprawa, P. Third Hankel determinants for subclasses of univalent functions. Mediterr. J. Math. 2017, 14, 10. [Google Scholar] [CrossRef]
  21. 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]
  22. Zaprawa, P.; Obradovi, M.; Tuneski, C.N. Third Hankel determinant for univalent starlike functions. Rev. Real Acad. Cienc. Exactas Fís. Nat. Ser. A Mat. 2021, 49, 115. [Google Scholar] [CrossRef]
  23. Obradovi, M.; Tuneski, C.N. Hankel determinants of second and third order for the class S of univalent functions. Math. Slovaca 2021, 71, 649–654. [Google Scholar] [CrossRef]
  24. 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]
  25. Ullah, K.; Al-Shbeil, I.; Faisal, M.I.; Arif, M.; Alsaud, H. Results on Second-order Hankel determinants for convex functions with symmetric points. Symmetry 2023, 15, 939. [Google Scholar] [CrossRef]
  26. Shareef, Z.; Hussain, S.; Darus, M. Subclasses of analytic functions associated with k-symmetric points. Information 2015, 18, 355–364. [Google Scholar]
  27. Arif, M.; Marwa, S.; Xin, Q.; Tchier, F.; Ayaz, M.; Malik, S.N. Sharp coefficient problems of functions with bounded turning subordinated by sigmoid function. Mathematics 2022, 10, 3862. [Google Scholar] [CrossRef]
  28. Shi, L.; Arif, M.; Rafiq, A.; Abbas, M.; Iqbal, J. Sharp bounds of Hankel determinant on logarithmic coefficients for functions of bounded turning associated with petal-shaped domain. Mathematics 2022, 10, 1939. [Google Scholar] [CrossRef]
  29. Ponnusamy, S.; Sharma, N.L.; Wirths, K.J. Logarithmic coefficients problems in families related to starlike and convex functions. J. Aust. Math. Soc. 2019, 109, 230–249. [Google Scholar] [CrossRef]
  30. Libera, R.J.; Zlotkiewicz, E.J. Coefficient bounds for the inverse of a function with derivative in P. Proc. Am. Math. Soc. 1983, 87, 251–257. [Google Scholar] [CrossRef]
  31. 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]
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Tang, H.; Ahmad, A.; Rasheed, A.; Ali, A.; Hussain, S.; Noor, S. Sharp Coefficient and Hankel Problems Related to a Symmetric Domain. Symmetry 2023, 15, 1865. https://doi.org/10.3390/sym15101865

AMA Style

Tang H, Ahmad A, Rasheed A, Ali A, Hussain S, Noor S. Sharp Coefficient and Hankel Problems Related to a Symmetric Domain. Symmetry. 2023; 15(10):1865. https://doi.org/10.3390/sym15101865

Chicago/Turabian Style

Tang, Huo, Adeel Ahmad, Akhter Rasheed, Asad Ali, Saqib Hussain, and Saima Noor. 2023. "Sharp Coefficient and Hankel Problems Related to a Symmetric Domain" Symmetry 15, no. 10: 1865. https://doi.org/10.3390/sym15101865

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