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Article

Analytic Functions Related to a Balloon-Shaped Domain

1
Department of Mathematics and Statistics, Hazara University Mansehra, Mansehra 21120, Pakistan
2
Department of Mathematical Sciences, United Arab Emirates University, Al Ain 15551, United Arab Emirates
3
Department of Mathematics, Faculty of Science, The University of Jordan, Amman 11942, Jordan
4
Department of Mathematics, COMSATS University Islamabad, Abbottabad 22060, Pakistan
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Fractal Fract. 2023, 7(12), 865; https://doi.org/10.3390/fractalfract7120865
Submission received: 4 September 2023 / Revised: 27 November 2023 / Accepted: 29 November 2023 / Published: 5 December 2023
(This article belongs to the Special Issue Fractional Calculus and Hypergeometric Functions in Complex Analysis)

Abstract

:
One of the fundamental parts of Geometric Function Theory is the study of analytic functions in different domains with critical geometrical interpretations. This article defines a new generalized domain obtained based on the quotient of two analytic functions. We derive various properties of the new class of normalized analytic functions X defined in the new domain, including the sharp estimates for the coefficients a 2 , a 3 , and a 4 , and for three second-order and third-order Hankel determinants, H 2 , 1 X , H 2 , 2 X , and H 3 , 1 X . The optimality of each obtained estimate is given as well.

1. Introduction

Let A be the class of all analytic functions X defined in the open unit disc U = { z C : z < 1 } with X 0 = 0 and X 0 = 1 . Thus, each analytic function in A has the following Taylor series representation
X z = z + t = 2 a t z t .
Let S be the subclass of all analytic functions in A that are univalent in U .
An analytic function X is said to be subordinate to an analytic function g in U , denoted as X g , if there exists a Schwarz function ξ that is analytic in U with ξ ( 0 ) = 0 and ξ ( z ) < 1, such that X z = g ( ξ ( z ) ) . In particular (see [1]), if g is univalent in U , then X g if and only if
X 0 = g 0 and X U g U .
Using the concept of subordination, many subclasses have been defined and studied, such as S , C , K and R of starlike, convex, close to convex, and functions with bounded turnings, respectively. See [2,3,4,5,6] for the new results about more subclasses.
For two analytic functions X and ζ in A with the series representation of X given in (1) and ζ ( z ) = z + t = 2 b t z t the convolution (Hadamard product) X ζ is defined by
X ζ ( z ) = z + t = 2 a t b t z t = ζ X ( z ) .
Shanmugam [7] generalized the idea of Padmanabhan et al. [8] and introduced the general form of function class S h ( φ ) as follows
S h ( φ ) = X A : z ( X h ) ( z ) ( X h ) ( z ) φ ( z ) , z U ,
where h is a fixed function in A and φ is a convex univalent function on U with φ ( 0 ) = 1 and R e ( φ ( z ) ) > 0 .
Ma and Minda [9] defined a more general form of function class S ( φ ) by applying for some restrictions h z = z 1 z (and hence X h = X ) with φ ( 0 ) = 1 and φ ( 0 ) > 0 . The generic form of Ma and Minda-type class of starlike functions is defined as
S ( φ ) = X A : z X z X z φ ( z ) , z U .
In recent years, many authors have established important subfamilies of analytic functions by varying φ ( z ) in S ( φ ) , and they proved significant geometric properties of those subfamilies. For details, see [10,11,12,13,14].
We discuss the following two classes that have some interesting geometric properties.
(i)
For φ 1 ( z ) = 1 + z , the class S ( φ ) becomes S L , which was introduced by Sokol and Stankiewicz [15], and it contains those functions X A such that z X z X z lies in the region bounded by the right half of the lemniscate of Bernoulli defined by z 2 1 < 1 .
(ii)
For φ 2 ( z ) = 2 1 + e z , the class S ( φ ) becomes S s i g , which was defined and investigated by Geol et al. [16]. Geometrically, a function X S s i g if and only if z X z X z lies in the region defined by w C : log w 2 w < 1 .
By taking inspiration from all of the previous works mentioned, we introduce the following new class of analytic functions by using the quotient of φ 1 ( z ) = 1 + z and φ 2 ( z ) = 2 1 + e z .
Definition 1.
Let X A , given in (1). We say X R s l if it satisfies the following condition
X ( z ) 2 1 + z 1 + e z , z U .
Geometrically, each X R s l maps the open unit disc into a balloon-shaped domain, which is symmetric about the real axis, as shown in the following Figure 1.
For X A and n , k 0 , Pommerenke [17] defined the k t h order Hankel determinant H k , n by
H k , n X = a n a n + 1 . . . a n + k 1 a n + 1 a n + 2 . . . a n + k . . . . . . . . . . . . . . . . . . a n + k 1 a n + k . . . a n + 2 k 1 .
Recently, finding the sharp upper bounds of the Hankel determinants H k , n X for certain n and k for various subfamilies of analytic functions has been identified as an interesting and important problem. Many researchers have observed sharp upper bounds of Hankel determinants for many subfamilies of analytic functions. In particular, the upper bounds of second and third-order Hankel determinants have been estimated in [18,19,20,21,22,23] for several subclasses of normalized analytic function.
Hayman [24] was the first to give the sharp inequality for X S , and subsequently proved that H 2 , n ( X ) λ n , where λ > 0 . This inequality is further explained in [25] and showed that H 2 , 2 ( X ) λ , where 1 λ 11 3 .
Janteng et al. [26] determined the sharp bounds of H 2 , 2 ( X ) for the subfamilies of K , S , and R . Babalola [27] studied a third-order Hankel determinant for the subclasses of S and C , while Zaprawa [28] amended Babalola’s results and gave the following estimates, which it is believed may not be the best possible results.
H 3 , 1 ( X ) 49 540 X K , 1 X S , 41 60 X R .
Kwon et al. [29] improved this determinant for starlike functions as H 3 , 1 ( X ) 8 9 . Zaprawa et al. [30] extended his work by estimating H 3 , 1 ( X ) 5 9 for X S .
Arif et al. [31] calculated the sharpness of the bounds of the coefficients and H 3 , 1 ( X ) for a subfamily of starlike functions related to sigmoid functions; see [32] for the modified sigmoid functions. Orhan et al. [33] estimated the sharp Hankel determinants for a subfamily of analytic functions associated with the lemniscate of Bernoulli. Moreover, Shi et al. [34,35] estimated the sharpness of Hankel determinants for the functions with bounded turning associated with a petal-shaped domain and inverse functions, respectively.
Moreover, the estimation of various bounds can be considered for many classes of functions; for example, see [36,37,38].
It is natural to ask what the upper bounds for the analytic functions in the newly defined class R s l related to the coefficients of the Taylor series representation (1) and Hankel determinants are.
The aim and novelty of this article are the sharp upper bounds of the modulus of the coefficients a 2 , a 3 , and a 4 and the second-order and third-order Hankel determinants, H 2 , 1 X , H 2 , 2 X , and H 3 , 1 X , for the analytic functions in the new class R s l .

2. A Set of Lemmas

Let P represent the class of analytic functions p, such that p ( 0 ) = 1 , R e ( p ( z ) ) > 0 for z U , which has the following Taylor series form,
p z = 1 + t = 1 c t z t .
The subsequent Lemmas 1–4 will help to demonstrate our main findings, where c t , c t + k , and c t + 2 k for t , k N are coefficients of the Taylor series (6).
Lemma 1.
([17]). Let p P . Then, the following inequalities hold true
c t 2 for t 1 ,
c t + k ρ c t c k < 2 for 0 ρ 1 ,
c t + 2 k ρ c t c k 2 2 ( 1 + 2 ρ ) , for 0 ρ 1 ,
and
c 2 c 1 2 2 2 c 1 2 2 .
Lemma 2.
Let p P . Then there exists q , γ , and μ C with q 1 , γ 1 , and μ 1 such that
c 2 = 1 2 c 1 2 + q 4 c 1 2 ,
c 3 = 1 4 c 1 3 + 2 c 1 q 4 c 1 2 4 c 1 2 c 1 q 2 + 2 4 c 1 2 1 q 2 γ ,
and
c 4 = 1 8 c 1 4 + q 4 c 1 2 ( 4 q + ( q 2 3 q + 3 ) c 1 2 ) 4 4 c 1 2 1 q 2 ( c ( q 1 ) γ μ 1 γ 2 + q ¯ γ 2 ) .
The inequalities given in (11)–(13) are due to [17,39,40], respectively.
Lemma 3.
([39]). If p P , 0 R 1 , and R 2 R 1 S R , then the following inequality holds true
c 3 2 R c 1 c 2 + S c 1 3 2 .
Lemma 4.
([41]). Let α , β , γ , and λ satisfying the conditions 0 < α < 1 ,
0 < λ < 1 , and
8 λ 1 λ α β 2 γ 2 + α λ + α β 2 + α 1 α β 2 λ α 2 4 α 2 1 α 2 λ 1 λ .
Let p P be given in (6), then the following inequality holds true
γ c 1 4 + λ c 2 2 + 2 α c 1 c 3 3 2 β c 1 2 c 2 c 4 2 .

3. Main Results

Theorem 1.
Let X R s l . Then, the following inequalities for the coefficients in (1) are true.
a 2 1 2 , a 3 1 3 , a 4 1 4 , and a 5 1 5 .
The sharpness of these inequalities can be obtained using the function
X n ( z ) = 2 1 + z n 1 + e z n , n N .
In particular, if n = 1 , 2 , 3 , and 4, then we have
X 1 = 0 z 2 1 + t 1 + e t d t = z + 1 2 z 2 + 1 24 z 3 1 96 z 4 11 1920 z 5 ,
X 2 = 0 z 2 1 + t 2 1 + e t 2 d t = z + 1 3 z 3 + 1 40 z 5 1 168 z 7 ,
X 3 = 0 z 2 1 + t 3 1 + e t 3 d t = z + 1 4 z 4 + 1 56 z 7 ,
X 4 = 0 z 2 1 + t 4 1 + e t 4 d t = z + 1 5 z 5 .
Proof. 
As X R l s , from (4), we obtain
X z = 2 1 + ξ ( z ) 1 + e ξ ( z ) .
Then, (1) gives
X z = 1 + 2 a 2 z + 3 a 3 z 2 + 4 a 4 z 3 + 5 a 5 z 4 . . . .
Let p P be written by
p z = 1 + ξ ( z ) 1 ξ ( z ) = 1 + c 1 z + c 2 z 2 + c 3 z 3 + c 4 z 4 + .
This implies that
ξ ( z ) = 1 2 c 1 z + 1 2 c 2 1 4 c 1 2 z 2 + 1 8 c 1 3 1 2 c 1 c 2 + 1 2 c 3 z 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 z 4 + .
Then,
2 1 + ξ ( z ) 1 + e ξ ( z ) = 1 + 1 2 c 1 z + 1 2 c 2 7 32 c 1 2 z 2 + 1 2 c 3 7 16 c 1 c 2 + 17 192 c 1 3 z 3 + 203 6144 c 1 4 + 17 64 c 1 2 c 2 7 16 c 1 c 3 7 32 c 2 2 + 1 2 c 4 z 4 + . . . .
It follows from (21) and (22) that
a 2 = 1 4 c 1 ,
a 3 = 1 6 c 2 7 96 c 1 2 ,
a 4 = 17 768 c 1 3 7 64 c 1 c 2 + 1 8 c 3 ,
a 5 = 203 30720 c 1 4 + 17 320 c 1 2 c 2 7 80 c 1 c 3 7 160 c 2 2 + 1 10 c 4 .
Using Lemma 1, (23) and (24) imply
a 2 1 2 and a 3 1 3 .
By (25),
a 4 = 1 8 c 3 7 8 c 1 c 2 + 17 96 c 1 3 .
Using Lemma 3, we obtain
a 4 1 4 .
From (26), we have
a 5 = 1 10 203 3072 c 1 4 + 7 16 c 2 2 + 2 7 16 c 1 c 3 17 32 c 1 2 c 2 c 4 .
By applying Lemma 4,
a 5 1 5 .
Theorem 2.
Let X R l s . Then, the sharp upper bound for the following second-order Hankel determinant is given by
H 2 , 1 X 1 3 .
The function (17) gives the sharpness of the inequality (27).
Proof. 
Applying to the identities (23) and (24),
a 3 a 2 2 = 1 6 c 2 13 16 c 1 2 .
Using Lemma 1, we obtain
H 2 , 1 X 1 3 .
It is easy to verify that the function ((17).) gives the sharpness of the inequality (27). □
Theorem 3.
Let X R l s . Then, the sharp upper bound for the following second-order Hankel determinant is given by
H 2 , 2 X 1 9 .
The function (17) gives the sharpness of the inequality (28).
Proof. 
By the identities (23)–(25),
a 2 a 4 a 3 2 = 1 4608 c 1 4 7 2304 c 1 2 c 2 + 1 32 c 3 c 1 1 36 c 2 2 .
Now, using Lemma 2, we have
a 2 a 4 a 3 2 = 1 4608 32 t 2 q 2 36 t q 2 c 1 2 72 γ t c 1 1 q 2 + t q c 1 2 2 c 1 4 .
Using the triangular inequality by taking c 1 = c 0 , 2 , t = 4 c 2 , γ 1 , and q = b [ 0 , 1 ] .
a 2 a 4 a 3 2 1 4608 32 4 c 2 2 b 2 + 36 4 c 2 b 2 c 2 + 72 c 4 c 2 1 b 2 + 4 c 2 b c 2 + 2 c 4 .
Let
F b , c = 1 4608 32 4 c 2 2 b 2 + 36 4 c 2 b 2 c 2 + 72 c 4 c 2 1 b 2 + 4 c 2 b c 2 + 2 c 4 .
Then
F b = 1 4608 4 c 2 256 b + 8 b c 2 144 b c + c 2 0 ,
which shows that F b , c is an increasing function for all b [ 0 , 1 ] and c 0 , 2 . Thus, the maximum value occurs at b = 1 . Consequently,
F b , c F 1 , c = 1 4608 32 4 c 2 2 + 36 4 c 2 c 2 + 4 c 2 c 2 + 2 c 4 .
Let
G c = 32 4 c 2 2 + 36 4 c 2 c 2 + 4 c 2 c 2 + 2 c 4 ,
which implies
G c = 12 c c 2 + 18 0 ,
this shows that G c is a decreasing function for all c [ 0 , 2 ] , and the maximum value occurs at c = 0 . By referring to (29), we can deduce the required inequality,
H 2 , 2 X = a 2 a 4 a 3 2 1 9 .
It is also easy to verify that the function (17) provides the sharpness of the inequality (28). □
Theorem 4.
Let X R l s . Then, we have the sharp upper bound for the following third-order Hankel determinant.
H 3 , 1 X 1 16 .
The sharpness of this inequality can occur according to the function given in (18).
Proof. 
From (5), we have
H 3 , 1 X = 2 a 2 a 3 a 4 a 2 2 a 5 a 3 3 + a 3 a 5 a 4 2 .
Taking c 1 = c in the identities (23)–(26), we have
H 3 , 1 X = 1 1105920 16 c 6 309 c 4 c 2 + 1944 c 3 c 3 246 c 2 c 2 2 14976 c 2 c 4 13184 c 2 3 + 18432 c 2 c 4 17280 c 3 2 + 25632 c c 2 c 3 .
Also, taking 4 c 2 = t in Lemma 2, we can simplify the terms in (32).
309 c 4 c 2 = 309 2 c 6 309 2 t q c 4 , 1944 c 3 c 3 = 486 c 6 486 t c 4 q 2 + 972 t c 4 q + 972 1 q 2 t γ c 3 , 246 c 2 c 2 2 = 123 2 c 6 123 c 4 t q 123 2 c 2 t 2 q 2 , 14976 c 2 c 4 = 1872 c 6 1872 t c 4 q 3 + 5616 t c 4 q 2 5616 t c 4 q + 7488 1 q 2 t c 3 q γ 7488 1 q 2 t c 3 γ 7488 t c 2 q 2 + 7488 1 q 2 t c 2 q γ 2 7488 1 q 2 t 1 γ 2 μ c 2 , 13184 c 2 3 = 1648 c 6 4944 c 4 t q 4944 c 2 t 2 q 2 1648 t 3 q 3 , 18432 c 2 c 4 = 1152 c 6 + 1152 c 4 t q 3 3456 c 4 t q 2 + 4608 c 4 t q 4608 1 q 2 c 3 t q γ + 4608 1 q 2 c 3 t γ + 1152 c 2 t 2 q 4 3456 c 2 t 2 q 3 + 3456 c 2 t 2 q 2 + 4608 c 2 t q 2 4608 1 q 2 c 2 t q γ 2 + 4608 1 q 2 1 γ 2 μ c 2 t 4608 1 q 2 c t 2 q 2 γ + 4608 1 q 2 c t 2 q γ + 4608 t 2 q 3 4608 1 q 2 t 2 q 2 γ 2 + 4608 1 q 2 1 γ 2 μ t 2 q , 17280 c 3 2 = 1080 c 6 + 2160 c 4 t q 2 4320 c 4 t q 4320 c 3 1 q 2 t γ 1080 c 2 t 2 q 4 + 4320 c 2 t 2 q 3 4320 c 2 t 2 q 2 + 4320 c 1 q 2 t 2 q 2 γ 8640 c 1 q 2 t 2 q γ 4320 1 q 2 2 t 2 γ 2 , 25632 c c 2 c 3 = 3204 c 6 3204 c 4 t q 2 + 9612 c 4 t q + 6408 1 q 2 γ c 3 t 3204 c 2 t 2 q 3 + 6408 c 2 t 2 q 2 + 6408 1 q 2 γ c t 2 q .
Substituting the simplified terms into (32),
H 3 , 1 X = 1 1105920 26 c 6 720 c 4 t q 3 + 630 c 4 t q 2 + 69 2 c 4 t q + 2880 c 3 1 q 2 t q γ + 180 c 3 1 q 2 t γ + 2880 c 2 1 q 2 t q γ 2 288 c 1 q 2 t 2 q 2 γ 2880 c 2 1 γ 2 1 q 2 μ t 2340 c 2 t 2 q 3 + 1077 2 c 2 t 2 q 2 2880 c 2 t q 2 + 2376 c 1 q 2 t 2 q γ 4320 1 q 2 2 t 2 γ 2 4608 1 q 2 t 2 q 2 γ 2 + 72 c 2 t 2 q 4 + 4608 1 γ 2 1 q 2 t 2 q 1648 t 3 q 3 + 4608 t 2 q 3 .
Since t = 4 c 2 ,
H 3 , 1 X = 1 1105920 m 1 c , q + m 2 c , q γ + m 3 c , q γ 2 + φ c , q , γ μ ,
where
m 1 c , q = 26 c 6 1 2 4 c 2 q 4 c 2 q 1384 c 2 q 144 c 2 q 2 1077 c 2 + 3968 q + 5760 c 2 q 1260 c 4 q + 1440 c 4 q 2 69 c 4 , m 2 c , q = 36 c 4 c 2 1 q 2 2 4 c 2 q 4 q 33 80 c 2 q 5 c 2 , m 3 c , q = 288 4 c 2 1 q 2 4 c 2 q 2 + 15 10 c 2 q , φ c , q , γ = 576 4 c 2 1 q 2 1 γ 2 8 4 c 2 q 5 c 2 .
Let γ = y and μ 1 , then
H 3 , 1 X 1 1105920 m 1 c , q + m 2 c , q y + m 3 c , q y 2 + φ c , q , γ 1 1105920 G c , q , y ,
where
G c , q , y = n 1 c , q + n 2 c , q y + n 3 c , q y 2 + n 4 c , q 1 y 2 ,
with
n 1 c , q = 26 c 6 + 1 2 4 c 2 q 4 c 2 q 1384 c 2 q + 144 c 2 q 2 + 1077 c 2 + 3968 q + 5760 c 2 q + 1260 c 4 q + 1440 c 4 q 2 + 69 c 4 , n 2 c , q = 36 c 4 c 2 1 q 2 4 c 2 q 8 q + 66 + 80 c 2 q + 5 c 2 , n 3 c , q = 288 4 c 2 1 q 2 4 c 2 q 2 + 15 + 10 c 2 q , n 4 c , q = 576 4 c 2 1 q 2 8 q 4 c 2 + 5 c 2 .
To find the maximum values of the function G c , q , y within the closed cuboid = 0 , 2 × 0 , 1 × 0 , 1 , we need to examine the function G c , q , y inside the cuboid, on its faces and along its edges. Let us divide the analysis into the following three cases.
I. 
Interior points of cuboid
Now, we find the maximum value of G c , q , y within the cuboid’s interior.
Let c , q , y 0 , 2 × 0 , 1 × 0 , 1 . By differentiating G c , q , y with respect to y, we obtain
G y = 36 c 4 c 2 1 q 2 4 c 2 q 8 q + 66 + 5 c 2 16 q + 1 + 576 y 4 c 2 1 q 2 4 c 2 q 15 + 10 c 2 q 1 .
Putting G y = 0 , gives
y = c 2 q 4 c 2 4 q + 33 + 5 c 2 16 q + 1 16 4 c 2 15 q 10 c 2 q 1 = y 1 .
If y 1 is a critical point inside , then y 1 0 , 1 , which is possible only if
5 c 3 16 q + 1 + 2 c q 4 c 2 4 q + 33 + 16 4 c 2 15 q 1 q < 160 1 q c 2 ,
and
c 2 > 4 15 q 25 q .
To identify the critical point, we need to find a solution that satisfies the inequalities (34) and (35). Let g q = 4 15 q 25 q with g q = 40 25 q 2 < 0 , which shows that g q is a decreasing function, so
c 2 > 7 3 .
It follows from the simple calculations that (34) is not held for q 15 32 , 1 . As a result, it can be concluded that the function G c , q , y does not possess any critical points within the interior of the cuboid 0 , 2 × 15 32 , 1 × 0 , 1 .
Suppose c , q , y is a critical point of G in the interior of the cuboid, satisfying the conditions q 0 , 15 32 and y 0 , 1 which leads us to c 2 > g 15 32 = 372 157 . It can also be observed that
n 1 c , q n 1 c , 15 32 = ϑ 1 c .
Since 1 q 2 1 and 0 < q < 15 32 , we have
n 2 c , q 36 4 c 2 4 c 2 8 c 15 32 2 + 66 c 15 32 + 5 16 15 32 + 1 c 3 , = 1024 799 n 2 c , 15 32 = ϑ 2 c .
Similarly, we obtain
n j c , q 1024 799 n j c , 15 32 = ϑ j c j = 3 , 4 .
It follows that
G c , q , y ϑ 1 c + ϑ 4 c + ϑ 2 c y + ϑ 3 c ϑ 4 c y 2 = Ψ c , y .
Differentiating with regard to “y”, we have
Ψ y = ϑ 2 c + 2 ϑ 3 c ϑ 4 c y .
Consider
ϑ 3 c ϑ 4 c = 288 4 c 2 7905 256 13 345 1024 c 2 0 , c 372 157 , 2 .
Then, for all c 372 157 , 2 and y 0 , 1 , we have
Ψ y = ϑ 2 c + 2 ϑ 3 c ϑ 4 c y ϑ 2 c + 2 ϑ 3 c ϑ 4 c = 36 4 c 2 1255 128 c 3 13345 64 c 2 + 4185 32 c + 7905 16 0 .
Thus, we obtain
Ψ c , y Ψ c , 1 = ϑ 1 c + ϑ 2 c + ϑ 3 c = ζ c ,
where
ζ c = 1269383 131 072 c 6 11295 32 c 5 + 32362695 16 384 c 4 13185 4 c 3 210375495 8192 c 2 + 37665 2 c + 2348865 32 .
It can be seen that ζ c 0 , for any c 372 157 , 2 . Also, ζ c is a decreasing function and its maximum value occurs at c 1.53928554 , which is 37,437.
II. 
On the six faces of the cuboid
Next, we proceed to examine the maximum value of the function G c , q , y on all six faces of the cuboid .
i On the face c = 0 : G 0 , q , y becomes
h 1 q , y = 31744 q 3 + 4608 q 1 q 15 y 2 + 73728 q 1 q 2 ,
then
h 1 y = 9216 y q 2 1 q 1 q 15 0 for y 0 , 1 ,
which implies that h 1 does not have any optimal points within the interval 0 , 1 × 0 , 1 .
ii On the face c = 2 , we have
G 2 , q , y = 1664
iii On the face q = 0 , G c , 0 , y becomes
h 2 c , y = 26 c 6 + 180 c 3 y 4 c 2 + 7200 c 4 y 2 2880 c 4 46080 c 2 y 2 + 11520 c 2 + 69120 y 2 ,
then h 2 y = 0 gives
y = c 3 16 5 c 2 12 = y 0 .
For the provided range of y , y 0 0 , 1 , if c > c 0 1.5491933 .
Also, h 2 c = 0 gives
12 c 13 c 4 75 c 3 y + 2400 c 2 y 2 960 c 2 + 180 c y 7680 y 2 + 1920 = 0 .
Putting (37) in (38), we obtain
14925 c 9 1222920 c 7 + 7916976 c 5 17694720 c 3 + 13271040 c = 0 .
Solving for c within the range 0 , 2 , we find that c 1.4228 . This indicates that there is no optimal solution for G c , 0 , y .
iv On the face q = 1 : G c , 1 , y becomes
h 3 c , y = 820 c 6 + 334 c 4 + 4264 c 2 + 31744 ,
then h 3 c = 0 gives a critical point c 1.208 , where h 3 attains its maximum value; that is,
h 3 c , y 36129 .
v On the face y = 0 : G c , q , 0 becomes
h 4 c , q = 72 c 6 q 4 28 c 6 q 3 183 2 c 6 q 2 69 2 c 6 q + 26 c 6 576 c 4 q 4 5280 c 4 q 3 1788 c 4 q 2 + 4746 c 4 q 2880 c 4 + 1152 c 2 q 4 + 32064 c 2 q 3 + 8616 c 2 q 2 36864 c 2 q + 11520 c 2 41984 q 3 + 73728 q .
Thus,
h 4 c = 432 c 5 q 4 168 c 5 q 3 549 c 5 q 2 207 c 5 q + 156 c 5 2304 c 3 q 4 21 120 c 3 q 3 7152 c 3 q 2 + 18984 c 3 q 11520 c 3 + 2304 c q 4 + 64128 c q 3 + 17232 c q 2 73728 c q + 23040 c ,
h 4 q = 288 c 6 q 3 84 c 6 q 2 183 c 6 q 69 2 c 6 2304 c 4 q 3 15840 c 4 q 2 3576 c 4 q + 4746 c 4 + 4608 c 2 q 3 + 96192 c 2 q 2 + 17232 c 2 q 36864 c 2 125952 q 2 + 73728 .
Computation shows that the system of equations h 4 c = 0 and h 4 q = 0 has no solutions in 0 , 2 × 0 , 1 .
vi On the face y = 1 : G c , q , 1 , becomes
h 5 c , q = 72 c 6 q 4 28 c 6 q 3 183 2 c 6 q 2 69 2 c 6 q + 26 c 6 288 c 5 q 4 + 504 c 5 q 3 + 468 c 5 q 2 504 c 5 q 180 c 5 864 c 4 q 4 + 2208 c 4 q 3 8700 c 4 q 2 2742 c 4 q + 4320 c 4 + 2304 c 3 q 4 + 7488 c 3 q 3 3024 c 3 q 2 7488 c 3 q + 720 c 3 + 3456 c 2 q 4 16320 c 2 q 3 + 52392 c 2 q 2 + 11520 c 2 q 34560 c 2 4608 c q 4 38016 c q 3 + 4608 c q 2 + 38016 c q 4608 q 4 + 31744 q 3 64512 q 2 + 69120 .
It follows that
h 5 c = 432 c 5 q 4 168 c 5 q 3 549 c 5 q 2 207 c 5 q + 156 c 5 1440 c 4 q 4 + 2520 c 4 q 3 + 2340 c 4 q 2 2520 c 4 q 900 c 4 3456 c 3 q 4 + 8832 c 3 q 3 34 800 c 3 q 2 10 968 c 3 q + 17 280 c 3 + 6912 c 2 q 4 + 22 464 c 2 q 3 9072 c 2 q 2 22 464 c 2 q + 2160 c 2 + 6912 c q 4 32 640 c q 3 + 104 784 c q 2 + 23 040 c q 69 120 c 4608 q 4 38 016 q 3 + 4608 q 2 + 38 016 q ,
h 5 q = 288 c 6 q 3 84 c 6 q 2 183 c 6 q 69 2 c 6 1152 c 5 q 3 + 1512 c 5 q 2 + 936 c 5 q 504 c 5 3456 c 4 q 3 + 6624 c 4 q 2 17 400 c 4 q 2742 c 4 + 9216 c 3 q 3 + 22 464 c 3 q 2 6048 c 3 q 7488 c 3 + 13 824 c 2 q 3 48 960 c 2 q 2 + 104 784 c 2 q + 11 520 c 2 18 432 c q 3 114 048 c q 2 + 9216 c q + 38 016 c 18 432 q 3 + 95 232 q 2 129 024 q .
Also, the computation indicates that the system of equations h 5 c = 0 and h 5 q = 0 has no solutions in 0 , 2 × 0 , 1 .
III. 
On the twelve edges of the cuboid
Finally, we need to find the maximum values of G c , q , y along the twelve edges.
i On q = 0 and y = 0 : G c , 0 , 0 becomes
h 6 c = 26 c 6 2880 c 4 + 11520 c 2 ,
then h 6 c = 0 gives the critical point c 1.4343 , where the maximum value is obtained as follows.
h 6 c 11737 .
ii On q = 0 and y = 1 : G c , 0 , 1 becomes
h 7 c = 26 c 6 180 c 5 + 4320 c 4 + 720 c 3 34560 c 2 + 69120 .
It is clear that h 7 c 0 , for all c [ 0 , 2 ] . This indicates that h 7 c is a decreasing function and attains its maximum value at c = 0 .
h 7 c 69120 .
iii On q = 0 and c = 0 : G 0 , 0 , y becomes
h 8 y = 66816 y 2 + 2304 .
Therefore, h 8 c > 0 for the interval [ 0 , 1 ] , which shows that h 8 y is an increasing function. As a result, it attains its maximum value at y = 1 ; that is,
h 8 y 69120 .
As the terms G c , 1 , 1 and G c , 1 , 0 are free from q, that is
h 9 c = G c , 1 , 0 = G c , 1 , 1 = 56 c 6 5778 c 4 + 16488 c 2 + 31744 .
Putting h 9 c = 0 , we find a critical point c 1.1825 . At this critical point, h 9 c achieves its maximum value, which is
h 9 c 43349 .
iv On q = 1 and c = 0 : G 0 , 1 , y becomes
h 10 y = G 0 , 1 , y = 31744 .
v On c = 2 :
G 2 , 0 , y = G 2 , 1 , y = G 2 , q , 1 = G 2 , q , 0 = 1664 .
vi On c = 0 and y = 0 : G 0 , q , 0 becomes
h 11 q = 1024 q 41 q 2 72 ,
and calculation shows that h 11 q 0 for all q 0 , 1 , which means h 11 q is a decreasing function and maximum value occurs at q = 0 ; that is,
h 11 q 0 .
vii On c = 0 and y = 1 : G 0 , q , 1 becomes
h 12 q = 4608 q 4 + 31744 q 3 64512 q 2 + 69120 .
Let h 12 q = 0 , we then find a critical point q = 0 , where the function h 12 q achieves its maximum value,
h 12 q 69120 .
Therefore, we can conclude that
G c , q , y 69120 .
And hence, we reach the following inequality as described by (33),
H 3 , 1 X 1 16 .

4. Conclusions

In the present article, we defined a class of analytic functions by considering the ratio of two well-known functions. We investigated the sharp upper bounds of the modulus of coefficients a 2 , a 3 , and a 4 ; and the sharp upper bounds for the modulus of three second-order and third-order Hankel determinants, H 2 , 1 X , H 2 , 2 X , and H 3 , 1 X , for the normalized analytic functions X belonging to the newly defined class. These findings contribute to the existing body of knowledge and provide valuable insights for further research in the field. This work provides a direction to define more interesting generalized domains and to extend to new subclasses of starlike and convex functions by using quantum calculus.

Author Contributions

Conceptualization, A.A. (Adeel Ahmad), J.G., I.A.-S., A.R., A.A. (Asad Ali) and S.H.; Methodology, A.A. (Adeel Ahmad), J.G., I.A.-S., A.R., A.A. (Asad Ali) and S.H.; Formal analysis, A.A. (Adeel Ahmad), J.G., I.A.-S., A.R., A.A. (Asad Ali) and S.H.; Investigation, A.A. (Adeel Ahmad), J.G., I.A.-S., A.R., A.A. (Asad Ali) and S.H.; Writing—original draft, A.A. (Adeel Ahmad), J.G., I.A.-S., A.R., A.A. (Asad Ali) and S.H.; Writing—review & editing, A.A. (Adeel Ahmad), J.G., I.A.-S., A.R., A.A. (Asad Ali) and S.H.; All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by United Arab Emirates University with UAEU Program for Advanced Research (UPAR12S127).

Data Availability Statement

No new data were created or analyzed in this study. Data sharing is not applicable to this article.

Conflicts of Interest

The authors declare no conflict of interest.

References

  1. Al-Shbeil, I.; Gong, J.; Shaba, T.G. Coefficients Inequalities for the Bi-Univalent Functions Related to q-Babalola Convolution Operator. Fractal Fract. 2023, 7, 155. [Google Scholar] [CrossRef]
  2. Khan, M.F.; Al-Shbeil, I.; Khan, S.; Khan, N.; Haq, W.U.; Gong, J. Applications of a q-Differential Operator to a Class of Harmonic Mappings Defined by q-Mittag–Leffler Functions. Symmetry 2022, 14, 1905. [Google Scholar] [CrossRef]
  3. Saliu, A.; Al-Shbeil, I.; Gong, J.; Malik, S.N.; Aloraini, N. Properties of q-Symmetric Starlike Functions of Janowski Type. Symmetry 2022, 14, 1907. [Google Scholar] [CrossRef]
  4. Ur Rehman, M.S.; Ahmad, Q.Z.; Al-Shbeil, I.; Ahmad, S.; Khan, A.; Khan, B.; Gong, J. Coefficient Inequalities for Multivalent Janowski Type q-Starlike Functions Involving Certain Conic Domains. Axioms 2022, 11, 494. [Google Scholar] [CrossRef]
  5. Murugusundaramoorthy, G. Fekete–Szegő Inequalities for Certain Subclasses of Analytic Functions Related with Nephroid Domain. J. Contemp. Math. Anal. 2022, 57, 90–101. [Google Scholar] [CrossRef]
  6. Khan, M.G.; Khan, B.; Gong, J.; Tchier, F.; Tawfiq, F.M.O. Applications of First-Order Differential Subordination for Subfamilies of Analytic Functions Related to Symmetric Image Domains. Symmetry 2023, 15, 2004. [Google Scholar] [CrossRef]
  7. Shanmugam, T.N. Convolution and Differential subordination. Int. J. Math. Math. Sci. 1989, 12, 333–340. [Google Scholar] [CrossRef]
  8. Padmanabhan, K.S.; Parvatham, R. Some applications of differential subordination. Bull. Aust. Math. Soc. 1985, 32, 321–330. [Google Scholar] [CrossRef]
  9. Ma, W.C.; Minda, D. A unified treatment of some special classes of univalent functions. In Proceedings of the 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]
  10. 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]
  11. Kumar, S.S.; Arora, K. Starlike functions associated with a petal-shaped domain. arXiv 2020, arXiv:2010.10072. [Google Scholar]
  12. 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]
  13. Mundula, M.; Kumar, S.S. On subfamily of starlike functions related to hyperbolic cosine function. J. Anal. 2023, 31, 2043–2062. [Google Scholar] [CrossRef]
  14. Sharma, K.; Jain, N.K.; Ravichandran, V. Starlike functions associated with cardioid. Afr. Mat. 2016, 27, 923–939. [Google Scholar] [CrossRef]
  15. Sokol, J.; Stankiewicz, J. Radius of convexity of some subclasses of strongly starlike functions. Zeszyty Naukowe Oficyna Wydawnicza Al. Powstańców Warszawy 1996, 19, 101–105. [Google Scholar]
  16. 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]
  17. Pommerenke, C.; Jensen, G. Univalent Functions; Vandenhoeck and Ruprecht: Gottingen, Germany, 1975. [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] [PubMed]
  19. Bansal, D.; Maharana, S.; Prajapat, J.K. Third order Hankel determinant for certain univalent functions. J. Korean Math. Soc. 2015, 52, 1139–1148. [Google Scholar] [CrossRef]
  20. Krishna, D.V.; Venkateswarlu, B.; RamReddy, T. Third Hankel determinant for bounded turning functions of order alpha. J. Niger. Math. Soc. 2015, 34, 121–127. [Google Scholar] [CrossRef]
  21. Singh, G. On the second Hankel determinant for a new subclass of analytic functions. J. Math. Sci. Appl. 2014, 2, 1–3. [Google Scholar]
  22. Al-Shbeil, I.; Gong, J.; Khan, S.; Khan, N.; Khan, A.; Khan, M.F.; Goswami, A. Hankel and Symmetric Toeplitz Determinants for a New Subclass of q-Starlike Functions. Fractals Fract. 2022, 6, 658. [Google Scholar] [CrossRef]
  23. Orhan, H.; Deniz, E.; Raducanu, D. The Fekete–Szegö problem for subclasses of analytic functions defined by a differential operator related to conic domains, Comput. Math. Appl. 2010, 59, 283–295. [Google Scholar]
  24. Hayman, W.K. On second Hankel determinant of mean univalent functions. Proc. Lond. Math. Soc. 1968, 3, 77–94. [Google Scholar] [CrossRef]
  25. Obradovi c, 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]
  26. 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]
  27. Babalola, K.O. On H3(1) Hankel determinant for some classes of univalent functions. Inequal. Theory Appl. 2010, 6, 1–7. [Google Scholar]
  28. Zaprawa, P. Third Hankel determinants for subclasses of univalent functions. Mediterr. J. Math. 2017, 14, 10. [Google Scholar] [CrossRef]
  29. 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]
  30. Zaprawa, P.; Obradović, M.; Tuneski, N. Third Hankel determinant for univalent starlike functions. Rev. R. Acad. Cienc. Exactas Fís. Nat. Ser. A Mat. 2021, 49, 115. [Google Scholar] [CrossRef]
  31. 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]
  32. Khan, M.G.; Ahmad, B.; Murugusundaramoorthy, G.; Chinram, R.; Wali Khan Mashwani, W.K. Applications of Modified Sigmoid Functions to a Class of Starlike Functions. J. Funct. Spaces 2020, 2020, 8844814. [Google Scholar] [CrossRef]
  33. Orhan, H.; ÇaĞlar, M.; Cotirla, L.-I. Third Hankel determinant for a subfamily of holomorphic functions related with lemniscate of Bernoulli. Mathematics 2023, 11, 1147. [Google Scholar] [CrossRef]
  34. 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]
  35. Shi, L.; Arif, M.; Abbas, M.; Ihsan, M. Sharp bounds of Hankel determinant for the inverse functions on a subclass of bounded turning functions. Mediterr. J. Math. 2023, 20, 156. [Google Scholar] [CrossRef]
  36. Kanas, S.; Răducanu, D. Some class of analytic functions related to conic domains. Math. Slovaca 2014, 64, 1183–1196. [Google Scholar] [CrossRef]
  37. Abd El-Hamid, H.A.H.; Rezk, M.; Ahmed, A.M.; AlNemer, G.; Zakarya, M.; El Saify, H.A. Dynamic Inequalities in Quotients with General Kernels and Measures, J. Funct. Spaces 2020, 2020, 5417084. [Google Scholar] [CrossRef]
  38. Ahmed, A.M.; Saker, S.H.; Kenawy, M.R.; Rezk, H.M. Lower Bounds on a Generalization of Cesaro Operator on Time Scales, Dyn. Contin. Discret. Impuls. Syst. Ser. A Math. Anal. 2021, 28, 345–355. [Google Scholar]
  39. 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]
  40. 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]
  41. Ravichandran, V.; Verma, S. Bound for the fifth coefficient of certain starlike functions. Comptes Rendus Math. 2015, 353, 505–510. [Google Scholar] [CrossRef]
Figure 1. The geometry of the function ϕ (z)= 2 1 + z 1 + e z .
Figure 1. The geometry of the function ϕ (z)= 2 1 + z 1 + e z .
Fractalfract 07 00865 g001
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MDPI and ACS Style

Ahmad, A.; Gong, J.; Al-Shbeil, I.; Rasheed, A.; Ali, A.; Hussain, S. Analytic Functions Related to a Balloon-Shaped Domain. Fractal Fract. 2023, 7, 865. https://doi.org/10.3390/fractalfract7120865

AMA Style

Ahmad A, Gong J, Al-Shbeil I, Rasheed A, Ali A, Hussain S. Analytic Functions Related to a Balloon-Shaped Domain. Fractal and Fractional. 2023; 7(12):865. https://doi.org/10.3390/fractalfract7120865

Chicago/Turabian Style

Ahmad, Adeel, Jianhua Gong, Isra Al-Shbeil, Akhter Rasheed, Asad Ali, and Saqib Hussain. 2023. "Analytic Functions Related to a Balloon-Shaped Domain" Fractal and Fractional 7, no. 12: 865. https://doi.org/10.3390/fractalfract7120865

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