Next Article in Journal
A Computational Technique for Solving Three-Dimensional Mixed Volterra–Fredholm Integral Equations
Next Article in Special Issue
A Nonlinear Fractional BEM Model for Magneto-Thermo-Visco-Elastic Ultrasound Waves in Temperature-Dependent FGA Rotating Granular Plates
Previous Article in Journal
Generalized Beta Models and Population Growth: So Many Routes to Chaos
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Article

Certain Sharp Coefficient Results on a Subclass of Starlike Functions Defined by the Quotient of Analytic Functions

1
School of Mathematics and Statistics, Anyang Normal University, Anyang 455002, China
2
Department of Mathematics, Abdul Wali khan University Mardan, Mardan 23200, Pakistan
*
Author to whom correspondence should be addressed.
Fractal Fract. 2023, 7(2), 195; https://doi.org/10.3390/fractalfract7020195
Submission received: 16 January 2023 / Revised: 10 February 2023 / Accepted: 14 February 2023 / Published: 15 February 2023
(This article belongs to the Special Issue Nonlinear Functional Analysis and Applications)

Abstract

:
In the present paper, we consider a subclass of starlike functions G 3 / 2 defined by the ratio of analytic representations of convex and starlike functions. The main aim is to determine the bounds of Fekete–Szegö-type inequalities and Hankel determinants for functions in this class. It is proved that max H 3 , 1 ( f ) : f G 3 / 2 is equal to 1 81 . The bounds for f G 3 / 2 are sharp.

1. Introduction and Definitions

Let A denote the normalized analytic functions defined in the open unit disc D = z C : z < 1 with the series expansion of the form
f ( z ) = z + k = 2 a k z k , z D .
Let S A be the class of univalent functions in D . Suppose that P is the Carathéodory class (see [1]) of all functions p that are analytic in D with p ( z ) > 0 and normalized by
p z = 1 + n = 1 c n z n , z D .
A function f A is said to be in the class S * of starlike functions, if, and only if,
z f ( z ) f ( z ) > 0 , z D .
For the class C of convex functions, the necessary and sufficient condition is
1 + z f z f z > 0 , z D .
It is known that if f C , then z f ( z ) S * —see [2].
Nonlinear functional analysis is an active topic and has its applications in the natural sciences, economics, and numerical analysis—see, for example, [3,4,5,6,7]. In [8], Silverman introduced and studied a new subclass of A using the quotient of 1 + z f ( z ) f ( z ) / z f ( z ) f ( z ) . For b ( 0 , 1 ] , the class G b was defined by
G b = f A : 1 + z f ( z ) f ( z ) z f ( z ) f ( z ) 1 < b , z D .
In [9], Obradović and Tuneski found that, for f A , if
1 + z f ( z ) f ( z ) z f ( z ) f ( z ) < 3 2 , z D ,
then f S * .
We say g 1 is subordinate to g 2 in D , written as g 1 g 2 , if g 1 ( z ) = g 2 ω ( z ) for some analytic function ω ( z ) with ω 0 = 0 and ω ( z ) < 1 . If g 2 in D is univalent, then g 1 g 2 is equivalent to
g 1 ( 0 ) = g 2 ( 0 ) a n d g 1 ( D ) g 2 ( D ) .
Using subordination, we can also write
G b = f A : 1 + z f ( z ) f ( z ) z f ( z ) f ( z ) 1 + b z , z D .
In [10], the upper bounds on the initial coefficients and Hankel determinants for f G b were derived. Motivated by the above results, Rǎducanu [11] investigated the class G 3 / 2 defined by
G 3 / 2 : = f A : 1 + z f ( z ) f ( z ) z f ( z ) f ( z ) < 3 2 , z D .
Clearly, G 3 / 2 is a subclass of starlike functions. With the additional restriction of f ( 0 ) = p for p [ 0 , 2 ] , Rǎducanu obtained the upper bounds of some initial coefficients and the difference of moduli of successive coefficients a 3 a 2 and a 4 a 3 for f G 3 / 2 . For other investigations on the analytic functions associated with the ratio of analytic representations of convex and starlike functions, we refer to [12,13,14].
The Hankel determinant H q , n f with q , n N and a 1 = 1 for a function f S of the series form (1) was given by Pommerenke [15,16] 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 .
This is widely used in the theory of Markov processes, of non-stationary signals, in the Hamburger moment problem, and many other issues in both pure mathematics and technical applications—see, for example, [17,18]. In recent years, many results on the upper bounds of Hankel determinant for various subclasses of univalent functions were obtained—interested readers may refer to [19,20,21,22,23,24,25] and the references.
In the present paper, we aim to investigate coefficient problems related to Fekete–Szegö-type functionals and Hankel determinants for the functions f G 3 / 2 .

2. A Set of Lemmas

To prove our main results, we require the following lemmas.
Lemma 1.
(see [26]). Let p P be the form of (2). Then,
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 x , δ , ρ D ¯ : = z C : z 1 .
Lemma 2.
(see [27]). Let μ C . If p P is represented as (2), then
c n + k μ c n c k 2 max 1 , 2 μ 1 .
Lemma 3.
For all ( c , t ) [ 0 , 2 ) × 1 3 , 1 , we have
17 2 + c 2 2 c t 2 + 2 2 + c 23 c 2 + 116 c 162 t + 29 c 3 290 c 2 + 512 0 .
Proof. 
Let
F 1 ( c , t ) : = 17 2 + c 2 2 c t 2 + 2 2 + c 23 c 2 + 116 c 162 t + 29 c 3 290 c 2 + 512 .
It is noted that
F 1 ( c , t ) = 2 + c F 2 ( c , t ) + 29 c 3 290 c 2 + 512 ,
where
F 2 ( c , t ) = 17 4 c 2 t 2 + 2 23 c 2 + 116 c 162 t .
Let c ^ 0 = 7090 58 23 1.1392 be the only positive root of the equation 23 c 2 + 116 c 162 = 0 . If c c ^ 0 , we have 23 c 2 + 116 c 162 0 and thus F 2 ( c , t ) F 2 c , 1 3 . Then
F 1 ( c , t ) 2 + c F 2 c , 1 3 + 29 c 3 290 c 2 + 512 = : s 1 ( c ) , c c ^ 0 , 2 .
In light of
s 1 ( c ) = 2 9 191 c 3 836 c 2 + 244 c + 1400
and s 1 ( c ) 0 on c ^ 0 , 2 , we get that s 1 ( c ) s 1 ( 2 ) = 16 . Hence, we obtain that F 1 ( c , t ) 0 on c ^ 0 , 2 × [ 0 , 1 ] .
For c < c ^ 0 , we note that the symmetric axis of F 2 is defined by
t 0 = 23 c 2 116 c + 162 17 4 c 2 > 0 .
Let c ^ 1 = 982 29 3 0.7790 be the only positive root of the equation 6 c 2 + 116 c 94 = 0 . If c c ^ 1 , we have t 0 1 . Then F 2 ( c , t ) F 2 ( c , 1 ) , which leads to
F 1 ( c , t ) 2 + c F 1 ( c , 1 ) + 29 c 3 290 c 2 + 512 = 2 c 104 + 29 c 2 0 .
If c c ^ 1 , c ^ 0 , it is simple to observe that
F 1 ( c , t ) 17 2 + c 2 2 c · 1 9 + 2 2 + c 23 c 2 + 116 c 162 · 1 + 29 c 3 290 c 2 + 512 = 2 9 329 c 3 + 136 c 2 + 664 c 544 > 0
on c ^ 1 , c ^ 0 . Hence, F 1 ( c , t ) 0 for all ( c , t ) 0 , c ^ 0 × 1 3 , 1 . Therefore, we deduce that F 1 ( c , t ) 0 on [ 0 , 2 ) × 1 3 , 1 . The assertion in Lemma 3 thus follows. □
Lemma 4.
For all ( c , t ) [ 0 , 2 ) × 1 3 , 1 , we have
17 1 + c 4 c 2 t 2 + 46 c 3 + 162 c 2 + 140 c 324 t + 29 c 3 145 c 2 + 256 0 .
Proof. 
Define
F 3 ( c , t ) : = 17 1 + c 4 c 2 t 2 + 46 c 3 + 162 c 2 + 140 c 324 t + 29 c 3 145 c 2 + 256 .
It is observed that
F 3 ( c , t ) F 1 ( c , t ) = 17 4 c 2 t 2 + 162 2 c 2 t + 145 c 2 256 17 4 c 2 t + 162 2 c 2 t + 145 c 2 256 = ( 256 145 c 2 ) 1 t .
For c 2 256 145 , it is clear that F 3 ( c , t ) F 1 ( c , t ) 0 . If c 2 > 256 145 , then 46 c 3 + 162 c 2 + 140 c 324 > 0 and it follows that F 3 ( c , t ) F 3 c , 1 3 > 0 . Hence, we have F 3 ( c , t ) 0 on 0 , 2 × 1 3 , 1 , which leads to the assertion in Lemma 4. □

3. Main Results

For the class of analytic univalent functions, Fekete Szegö studied the maximum value of a 3 ζ a 2 when ζ is real. After that, the upper bound for the functional a 3 ζ a 2 were investigated extensively for various subclasses of univalent functions. For some recent works, see, for example, [28,29,30,31]. We begin by finding the Fekete–Szegö-type inequalities for f G 3 / 2 .
Theorem 1.
Let γ C . If f G 3 / 2 is of the form (1), then
a 3 γ a 2 2 1 4 max 1 , 3 4 γ .
The inequality is sharp.
Proof. 
Let f G 3 / 2 . Then there exists a function p P such that
3 z f ( z ) f z 2 1 + z f ( z ) f ( z ) = p ( z ) z f ( z ) f ( z ) , z D .
Assuming that
p z = 1 + c 1 z + c 2 z 2 + c 3 z 3 + c 4 z 4 + , z D .
Using (1), it follows that
z f z f z = 1 + a 2 z + 2 a 3 a 2 2 z 2 + a 2 3 3 a 2 a 3 + 3 a 4 z 3 + 4 a 5 a 2 4 + 4 a 2 2 a 3 4 a 2 a 4 2 a 3 2 z 4 +
and
1 + z f z f z = 1 + 2 a 2 z + 6 a 3 4 a 2 2 z 2 + 8 a 2 3 18 a 2 a 3 + 12 a 4 z 3 + 20 a 5 16 a 2 4 + 48 a 2 2 a 3 32 a 2 a 4 18 a 3 2 z 4 + .
Combining (26)–(29), we obtain
a 2 = 1 2 c 1 ,
a 3 = 1 8 c 2 2 c 1 2 ,
a 4 = 1 144 8 c 3 21 c 1 c 2 + 18 c 1 3 ,
a 5 = 1 1152 36 c 4 27 c 2 2 80 c 1 c 3 + 138 c 1 2 c 2 72 c 1 4 .
Employing (30) and (31), we have
a 3 γ a 2 2 = 1 8 c 2 2 1 γ c 1 2 .
An application of Lemma 2 leads to the assertion in Theorem 1. The equality can be attained by the functions f 1 and f 2 given, respectively, by the equations
3 z f ( z ) f z 2 1 + z f ( z ) f ( z ) = 1 z 1 + z · z f ( z ) f ( z ) , z D ,
3 z f ( z ) f z 2 1 + z f ( z ) f ( z ) = 1 z 2 1 + z 2 · z f ( z ) f ( z ) , z D .
Using series expansions, f 1 and f 2 are in the form of
f 1 ( z ) = z + z 2 + 3 4 z 3 + 19 36 z 4 + 101 288 z 5 + , z D ,
f 2 ( z ) = z + 1 4 z 3 + 1 32 z 5 + , z D .
The second Hankel determinant is known as the functional H 2 , 2 ( f ) = a 2 a 4 a 3 2 . In recent years, many results on the upper bounds of second Hankel determinant for certain subclass of univalent functions were obtained, see [32,33,34,35]. Now, we provide the sharp bound of H 2 , 2 ( f ) for f G 3 / 2 .
Theorem 2.
If f G 3 / 2 , then
H 2 , 2 f = a 2 a 4 a 3 2 1 16 .
The bound is sharp.
Proof. 
From (30) to (32), we have
H 2 , 2 f = a 2 a 4 a 3 2 = 1 64 c 2 2 1 96 c 1 2 c 2 + 1 36 c 1 c 3 .
Let f G 3 / 2 and f θ ( z ) = e i θ f e i θ z , θ R . We know f θ ( z ) G 3 / 2 for all θ R and H 2 , 2 f θ = H 2 , 2 f . Since the class G 3 / 2 and the functional H 2 , 2 ( f ) are rotation-invariant, we can assume that a 2 of f is real and, thus, c 1 : = c 0 , 2 . Using (11) and (12) to express c 2 and c 3 , we obtain
H 2 , 2 f = 5 2304 c 4 + 1 1152 c 2 4 c 2 x 1 2304 36 + 7 c 2 4 c 2 x 2 + 1 72 c 4 c 2 1 x 2 δ .
Let x : = t . From δ 1 , we get
H 2 , 2 f 5 2304 c 4 + 1 1152 c 2 4 c 2 t + 1 2304 36 + 7 c 2 4 c 2 t 2 + 1 72 c 4 c 2 1 t 2 = : G c , t .
As 7 c 2 32 c + 36 0 on [ 0 , 2 ] , it is noted that
G t = 1 1152 4 c 2 7 c 2 32 c + 36 t + c 2 0 .
Thus we have G c , t G c , 1 . Putting t = 1 leads to
H 2 , 2 f 1 16 1 576 c 4 1 16 .
The bound is achieved by the function f 2 given by Equation (36). □
It is not easy to find the sharp bound of the third Hankel determinant for a certain subclass of univalent functions. For instance, Kowalczyk et al. [36] proved that H 3 , 1 f 4 9 for f S * . Before it was solved, there are many works investigated this problem—for details, we refer to [37,38]. Now, we give the sharp bound of H 3 , 1 f for f G 3 / 2 .
Theorem 3.
Suppose that f G 3 / 2 . Then,
H 3 , 1 f 1 81 .
The result is the best possible.
Proof. 
From the definition, we know
H 3 , 1 f = 2 a 2 a 3 a 4 a 4 2 a 2 2 a 5 a 3 3 + a 3 a 5 .
Let f G 3 / 2 and f θ ( z ) = e i θ f e i θ z , θ R . It is observed that f θ ( z ) G 3 / 2 for all θ R and H 3 , 1 f θ = H 3 , 1 f . As the class G 3 / 2 and the functional H 3 , 1 ( f ) are invariant under the rotations, we may assume that a 2 of f is real and, thus, c 1 : = c 0 , 2 . Substituting (30)–(33) into (44), we have
H 3 , 1 f = 1 82944 81 c 2 3 + 48 c c 2 c 3 + 324 c 2 c 4 256 c 3 2 + 18 c 2 c 2 2 .
Let b = 4 c 2 . By applying Lemma 1 and inserting the formulae of c 2 , c 3 and c 4 into (45), we obtain
H 3 , 1 f = 1 663552 37 c 6 81 x 3 b 3 + 648 x 3 b 2 + 648 c 2 x 2 b 278 c 4 x 2 b + 162 c 4 x 3 b 137 c 2 x 2 b 2 22 c 2 x 3 b 2 + 34 c 2 x 4 b 2 + 109 c 4 x b + 232 c 3 b 1 x 2 δ 648 x 2 b 2 1 x 2 δ 2 512 b 2 1 x 2 2 δ 2 136 c x 2 b 2 ( 1 x 2 ) δ 648 c 2 x ¯ b ( 1 x 2 ) δ 2 280 c x b 2 1 x 2 δ 648 c 3 x b ( 1 x 2 ) δ + 648 c 2 b 1 x 2 1 δ 2 ρ + 648 x b 2 1 x 2 1 δ 2 ρ ,
where x , δ , ρ D ¯ . By suitable rearrangements, it is observed that H 3 , 1 f can be written as
H 3 , 1 f = 1 663552 u 1 c , x + u 2 c , x δ + u 3 c , x δ 2 + Φ c , x , δ ρ ,
where
u 1 c , x = 37 c 6 + 4 c 2 x 34 c 2 4 c 2 x 3 + 103 c 4 88 c 2 + 1296 x 2 + c 2 100 141 c 2 x + 109 c 4 , u 2 c , x = 8 ( 4 c 2 ) 1 x 2 c 17 4 c 2 x 2 46 c 2 + 140 x + 29 c 2 , u 3 c , x = 8 ( 4 c 2 ) 1 x 2 4 c 2 17 x 2 64 81 c 2 x ¯ , Φ c , x , δ = 648 ( 4 c 2 ) 1 x 2 1 δ 2 4 c 2 x + c 2 .
Let x = : t and δ = : y . By observing ρ 1 , it follows that
H 3 , 1 f 1 663552 u 1 c , x + u 2 c , x y + u 3 c , x y 2 + Φ c , x , δ 1 663552 Γ c , t , y ,
where
Γ c , t , y = σ 1 c , t + σ 2 c , t y + σ 3 c , t y 2 + σ 4 c , t 1 y 2 ,
with
σ 1 c , t = 37 c 6 + ( 4 c 2 ) 34 c 2 4 c 2 t 4 + 103 c 4 88 c 2 + 1296 t 3 + c 2 100 + 141 c 2 t 2 + 109 c 4 t , σ 2 c , t = 8 ( 4 c 2 ) 1 t 2 c 17 4 c 2 t 2 + 46 c 2 + 140 t + 29 c 2 , σ 3 c , t = 8 ( 4 c 2 ) 1 t 2 4 c 2 17 t 2 + 64 + 81 c 2 t , σ 4 c , t = 648 ( 4 c 2 ) 1 t 2 4 c 2 t + c 2 .
The inequality (47) comes from the fact that u j ( c , x ) σ j ( c , t ) for j = 1 , 2 , 3 and Φ c , x , δ σ 4 ( c , t ) 1 δ 2 . Here, u 1 ( c , x ) σ 1 ( c , t ) follows from 4 c 2 0 and 103 c 4 88 c 2 + 1296 0 on [ 0 , 2 ] .
Now the problem reduces to find the maximum value of Γ in the closed cuboid Ω : = [ 0 , 2 ] × [ 0 , 1 ] × [ 0 , 1 ] . By noting that Γ 0 , 0 , 1 = 8192 , we have max ( c , t , y ) Ω Γ ( c , t , y ) 8192 . In the following, we show that max ( c , t , y ) Ω Γ ( c , t , y ) = 8192 .
On the face, c = 2 ,   Γ ( 2 , t , y ) 2368 . For t = 1 , we have
Γ ( c , 1 , y ) = 282 c 6 + 1128 c 4 704 c 2 + 5184 = : r 1 ( c ) .
Since r 1 ( c ) = 0 has two positive roots c ˜ 1 = 4 3 20 141 141 0.6007 and c ˜ 2 = 4 3 + 20 141 141 1.5185 , r 1 attains its maximum value about 6100.85 on c = c ˜ 2 for c [ 0 , 2 ] . Thus, we may only consider the cases of c < 2 and t < 1 .
First we suppose that c , t , y 0 , 2 × 0 , 1 × 0 , 1 . By differentiating partially Γ with respect to y, we obtain
Γ y = σ 2 ( c , t ) + 2 σ 3 ( c , t ) σ 4 ( c , t ) y .
Taking Γ y = 0 , we obtain
y = 17 c 4 c 2 t 2 + 46 c 3 + 140 c t + 29 c 3 2 ( 1 t ) 17 4 c 2 t + 145 c 2 256 = : y 0 .
For y 0 0 , 1 , it is possible only if
17 2 + c 2 2 c t 2 + 2 2 + c 23 c 2 + 116 c 162 t + 29 c 3 290 c 2 + 512 < 0
and
c 2 > 4 64 17 t 145 17 t .
Now we have to obtain the solutions that satisfy both inequalities (52) and (53) for the existence of critical points with y ( 0 , 1 ) . From Lemma 3, we know (52) is impossible to hold for t 1 3 , 1 .
Let c ˜ , t ˜ , y ˜ be a critical point of Γ lies in [ 0 , 2 ) × [ 0 , 1 ) × ( 0 , 1 ) . From the above discussions, we know t ˜ < 1 3 . Assume that g ( t ) = 4 64 17 t 145 17 t . As g ( t ) < 0 in 0 , 1 ,   g ( t ) is decreasing over 0 , 1 . Hence, c ˜ 2 350 209 . Under the conditions that t 0 , 1 3 , c 350 209 , 2 and y ( 0 , 1 ) , we find that
σ 1 c , t σ 1 c , 1 3 = : τ 1 ( c )
and
σ j c , x 9 8 σ j c , 1 3 = : τ j ( c ) , j = 2 , 3 , 4 .
Therefore, we have
Γ c , t , y τ 1 c + τ 2 ( c ) y + τ 3 c y 2 + τ 4 c 1 y 2 = : Ξ ( c , y ) .
Since Ξ y = τ 2 ( c ) + 2 τ 3 ( c ) τ 4 ( c ) y , we have
Ξ y | y = 1 = τ 2 ( c ) + 2 τ 3 ( c ) τ 4 ( c ) = 16 9 ( 4 c 2 ) r 2 ( c ) ,
where r 2 ( c ) = 191 c 3 836 c 2 + 244 c + 1400 . It is easy to get that r 2 ( c ) 0 for c [ 0 , 2 ] . Thus, we have Ξ y | y = 1 0 . As Ξ y | y = 0 = τ 2 ( c ) 0 and Ξ y is a continuous linear function with respect to y, we deduce that
Ξ y min Ξ y | y = 0 , Ξ y | y = 1 0 , y ( 0 , 1 ) .
Thus,
Ξ ( c , y ) Ξ ( c , 1 ) = τ 1 ( c ) + τ 2 ( c ) + τ 3 ( c ) = : r 3 ( c ) .
By numerical calculation, we know r 3 has a maximum value about 7391.58 on c = 350 209 1.2941 for c 350 209 , 2 . Therefore, we have Γ ( c , t , y ) < 8192 on ( c , t , y ) 350 209 , 2 × 0 , 1 3 × ( 0 , 1 ) . Hence, Γ c ˜ , t ˜ , y ˜ < 8192 . Thus, any critical point which lies in Ω with y ( 0 , 1 ) , has a maximum value less than Γ ( 0 , 0 , 1 ) . Then it is sufficient to consider the face y = 0 and y = 1 of Ω to get the maximum value of Γ .
Since
Γ ( c , t , 0 ) = σ 1 ( c , t ) + σ 4 ( c , t )
and
Γ ( c , t , 1 ) = σ 1 ( c , t ) + σ 2 ( c , t ) + σ 3 ( c , t ) ,
we note that
Γ ( c , t , 1 ) Γ ( c , t , 0 ) = σ 2 ( c , t ) + σ 3 ( c , t ) σ 4 ( c , t ) = : 8 4 c 2 1 t 2 Θ ( c , t ) ,
where
Θ ( c , t ) = 17 1 + c 4 c 2 t 2 + 46 c 3 + 162 c 2 + 140 c 324 t + 29 c 3 145 c 2 + 256 .
From Lemma 4, we know Θ ( c , t ) 0 on 0 , 2 × 1 3 , 1 ; thus, we have
Γ ( c , t , 0 ) Γ ( c , t , 1 ) , ( c , t ) 0 , 2 × 1 3 , 1 .
If t < 1 3 , from (54) and (55), we obtain
Γ ( c , t , 0 ) τ 1 ( c ) + τ 4 ( c ) = : r 4 ( c ) .
Since
r 4 ( c ) = 2 81 745 c 6 8908 c 4 + 34592 c 2 + 147744
has a maximum value about 4376.24 attained on c 1.2707 and Γ ( 0 , 0 , 1 ) = 8192 , we have
Γ ( c , t , 0 ) < Γ ( 0 , 0 , 1 ) , ( c , t ) 0 , 2 × 0 , 1 3 .
Combining (62) and (65), it remains to find the maximum value of Γ on the face of y = 1 .
On the face y = 1 , it is noted that
Γ ( c , t , 1 ) = 37 c 6 + 4 c 2 λ 4 t 4 + λ 3 t 3 + λ 2 t 2 + λ 1 t + λ 0 = : Q ( c , t ) ,
where
λ 4 = 34 ( 4 c 2 ) c 2 4 c 4 , λ 3 = 103 c 4 368 c 3 736 c 2 1120 c + 1296 , λ 2 = 141 c 4 368 c 3 + 476 c 2 + 544 c 1504 , λ 1 = 109 c 4 + 368 c 3 + 648 c 2 + 1120 c , λ 0 = 232 c 3 512 c 2 + 2048 .
In virtue of c 2 4 c 4 0 on [ 0 , 2 ] , we have λ 4 0 and thus
Q ( c , t ) 37 c 6 + 4 c 2 λ 3 t 3 + λ 2 t 2 + λ 1 t + λ 0 = : W ( c , t ) .
Now we need to find the maximum value of W on [ 0 , 2 ] × [ 0 , 1 ] . On the vertices ( 0 , 0 ) , ( 2 , 0 ) , ( 0 , 1 ) and ( 2 , 1 ) , we have W ( 0 , 0 ) = 8192 , W ( 2 , 0 ) = W ( 2 , 1 ) = 2368 and W ( 0 , 1 ) = 7360 . On the sides of [ 0 , 2 ] × [ 0 , 1 ] , if c = 0 , we have
W ( 0 , t ) = 5184 t 3 6016 t 2 + 8192 = : r 5 ( t ) .
Since r 5 ( t ) = 0 has only one positive root t ˜ 1 = 188 243 0.7737 , we see the maximum value of r 5 is 8192 attained on t = 0 . If c = 2 , then W ( 2 , t ) 2368 for all t [ 0 , 1 ] . It is left to discuss the case of ( c , t ) ( 0 , 2 ) × ( 0 , 1 ) . Solving the system of equations
W t = ( 4 c 2 ) 3 λ 3 t 2 + 2 λ 2 t + λ 1 = 0
and
W c = μ 3 ( c ) t 3 + μ 2 ( c ) t 2 + μ 1 ( c ) t + μ 0 = 0 ,
where
μ 3 = 618 c 5 + 1840 c 4 + 4592 c 3 1056 c 2 8480 c 4480 , μ 2 = 846 c 5 + 1840 c 4 + 352 c 3 6048 c 2 + 6816 c + 2176 , μ 1 = 654 c 5 1840 c 4 848 c 3 + 1056 c 2 + 5184 c + 4480 , μ 0 = 2 c 111 c 4 580 c 3 + 1024 c 2 + 1392 c 4096 ,
it is found that all the three critical points lie in ( 0 , 2 ) × ( 0 , 1 ) are c ¯ 1 , t ¯ 1 0.4480 , 0.4137 , c ¯ 2 , t ¯ 2 1.0708 , 0.7129 and c ¯ 3 , t ¯ 3 0.4973 , 0.9759 . As W c ¯ 1 , t ¯ 1 7913.01 , W c ¯ 2 , t ¯ 2 8167.95 and W c ¯ 3 , t ¯ 3 7823.08 , we see the maximum value of W is less than 8192 in ( 0 , 2 ) × ( 0 , 1 ) . In conclusion, we obtain that W ( c , t ) 8192 on [ 0 , 2 ] × [ 0 , 1 ] , which leads to Γ c , t , y 8192 for all ( c , t , y ) 0 , 2 × 0 , 1 × 0 , 1 . Hence, we obtain
H 3 , 1 f 8192 663552 = 1 81 .
For the sharpness, we consider the function f 3 satisfying the equation
3 z f ( z ) f z 2 1 + z f ( z ) f ( z ) = 1 z 3 1 + z 3 · z f ( z ) f ( z ) , z D .
The series expansion of f 3 is given by
f 3 ( z ) = z 1 2 z 2 + 1 4 z 3 1 72 z 4 11 144 z 5 + , z D .
This completes the proof Theorem 3. □

4. Conclusions

In this paper, we investigated some coefficient-related problems for the class G 3 / 2 , which is defined by the ratio of analytic representations of convex and starlike functions. Fekete–Szegö-type inequalities and upper bounds for the second and third Hankel determinant were obtained. The calculation is based on the relationship between the coefficients of functions in the considered class and the coefficients for the corresponding Carathéodory class. The results may inspire further investigations on getting more sharp bounds related with functional such as a 3 a 5 a 4 2 , a 4 a 2 a 3 and a 5 a 3 2 . By making use of the concept of q-calculus, it is also interesting to investigate a more general class of this type.

Author Contributions

The idea of the present paper comes from M.A. L.S. writes and completes the calculations. M.A. checks all the results. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

Not applicable.

Acknowledgments

The authors would like to express their gratitude for the referees’ valuable suggestions which truly improve the present work.

Conflicts of Interest

The authors declare that they have no conflict of interest.

References

  1. Carathéodory, C. Über den Variabilitatsbereich der Koeffizienten von Potenzreihen, die gegebene werte nicht annehmen. Math. Ann. 1907, 64, 95–115. [Google Scholar] [CrossRef] [Green Version]
  2. Goodman, A.W. Univalent Functions; Mariner: Tampa, FL, USA, 1983. [Google Scholar]
  3. Ji, E.K.; Kwang, H.S. A regularity of split-biquaternionic-valued functions in Clifford analysis. J. Nonlinear Sci. Appl. 2016, 9, 6302–6311. [Google Scholar]
  4. Ji, E.K.; Kwang, H.S. Hyper-conjugate harmonic function of conic regular functions in conic quaternions. East Asian Math. J. 2015, 31, 127–134. [Google Scholar]
  5. Liu, Q.; Dai, B.; Katib, I.; Alhamami, M.A. Financial accounting measurement model based on numerical analysis of rigid normal differential equation and rigid generalised functional equation. Appl. Math. Nonlinear Sci. 2022, 7, 541–548. [Google Scholar] [CrossRef]
  6. Sun, R.; Sharaf, S.; Ali, B. Human gait modelling and tracking based on motion functionalisation. Appl. Math. Nonlinear Sci. 2022, 7, 21–30. [Google Scholar] [CrossRef]
  7. An, X.; Yang, R.; Alghazzawi, D.; Joseph, N. Mathematical function data model analysis and synthesis system based on short-term human movement. Appl. Math. Nonlinear Sci. 2022, 7, 49–58. [Google Scholar] [CrossRef]
  8. Silverman, H. Convex and starlike criteria. Int. J. Math. Math. Sci. 1999, 22, 75–79. [Google Scholar] [CrossRef] [Green Version]
  9. Obradović, M.; Tuneski, N. On the starlike criteria defined by Silverman. Zesz. Nauk. Politech. Rzesz. Mat. 2000, 24, 59–64. [Google Scholar]
  10. Park, J.H.; Kumar, V.; Cho, N.E. Sharp coefficient bounds for the quotient of analytic functions. Kyungpook Math. J. 2018, 58, 231–242. [Google Scholar] [CrossRef]
  11. Rǎducanu, D. Coefficient estimates for a subclass of starlike functions. Mathematics 2020, 8, 1646. [Google Scholar] [CrossRef]
  12. Tuneski, N. On the quotient of the representations of convexity and starlikeness. Math. Nachrichten 2003, 248, 200–203. [Google Scholar] [CrossRef]
  13. Tuneski, N. On a criteria for starlikeness of analytic functions. Integral Transform. Spec. Funct. 2003, 14, 263–270. [Google Scholar] [CrossRef]
  14. Singh, V.; Nikola, T. On criteria for starlikeness and convexity of analytic functions. Acta Math. Sci. 2004, 24, 597–602. [Google Scholar] [CrossRef]
  15. Pommerenke, C. On the coefficients and Hankel determinants of univalent functions. J. Lond. Math. Soc. 1966, 1, 111–122. [Google Scholar] [CrossRef]
  16. Pommerenke, C. On the Hankel determinants of univalent functions. Mathematika 1967, 14, 108–112. [Google Scholar] [CrossRef]
  17. Dienes, P. The Taylor Series: An Introduction to the Theory of Functions of a Complex Variable; Dover: New York, NY, USA, 1957. [Google Scholar]
  18. Srivastava, H.M.; Kaur, G.; Singh, G. Estimates of the fourth Hankel determinant for a class of analytic functions with bounded turnings involving cardioid domains. J. Nonlinear Convex Anal. 2021, 22, 511–526. [Google Scholar]
  19. Arif, M.; Barukab, O.M.; Khan, S.A.; Abbas, M. The sharp bounds of Hankel determinants for the families of three-leaf-type analytic functions. Fractal Fract. 2022, 6, 291. [Google Scholar] [CrossRef]
  20. 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]
  21. 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]
  22. Shi, L.; Shutaywi, M.; Alreshidi, N.; Arif, M.; Ghufran, M.S. The sharp bounds of the third-order Hankel determinant for certain analytic functions associated with an eight-shaped domain. Fractal Fract. 2022, 6, 223. [Google Scholar] [CrossRef]
  23. Shi, L.; Srivastava, H.M.; Rafiq, A.; Arif, M.; Ihsan, M. Results on Hankel determinants for the inverse of certain analytic functions subordinated to the exponential function. Mathematics 2022, 10, 3429. [Google Scholar] [CrossRef]
  24. 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. Fractal Fract. 2022, 6, 658. [Google Scholar] [CrossRef]
  25. Wang, Z.-G.; Raza, M.; Arif, M.; Ahmad, K. On the third and fourth Hankel determinants of a subclass of analytic functions. Bull. Malays. Math. Sci. Soc. 2022, 45, 323–359. [Google Scholar] [CrossRef]
  26. 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]
  27. 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]
  28. Seoudy, T.; Aouf, M.K. Fekete-Szegö problem for certain subclass of analytic functions with complex order defined by q-analogue of Ruscheweyh Operator. Constr. Math. Anal. 2020, 3, 36–44. [Google Scholar] [CrossRef]
  29. Baksa, V.; Bandura, A.; Skaskiv, O. Growth estimates for analytic vector-valued functions in the unit ball having bounded L-index in joint variables. Constr. Math. Anal. 2020, 3, 9–19. [Google Scholar]
  30. Aouf, M.K.; Seoudy, T. Certain class of bi-Bazilevic functions with bounded boundary rotation involving Salăgeăn Operator. Constr. Math. Anal. 2020, 3, 139–149. [Google Scholar]
  31. Srivastava, H.M.; Wanas, A.K.; Güney, H.Ö. New families of bi-univalent functions associated with the Bazilevič functions and the λ-pseudo-starlike functions. Iran. J. Sci. Technol. Trans. A Sci. 2021, 45, 1799–1804. [Google Scholar] [CrossRef]
  32. Kowalczyk, B.; Lecko, A. Second Hankel determinant of logarithmic coefficients of convex and starlike functions. Bull. Aust. Math. Soc. 2022, 105, 458–467. [Google Scholar] [CrossRef]
  33. Sunthrayuth, P.; Aldawish, I.; Arif, M.; Abbas, M.; El-Deeb, S. Estimation of the second-order Hankel determinant of logarithmic coefficients for two subclasses of starlike functions. Symmetry 2022, 14, 2039. [Google Scholar] [CrossRef]
  34. Sümer Eker, S.; Şeker, B.; Çekiç, B.; Acu, M. Sharp bounds for the second Hankel determinant of logarithmic coefficients for strongly starlike and strongly convex functions. Axioms 2022, 11, 369. [Google Scholar] [CrossRef]
  35. Sim, Y.J.; Lecko, A.; Thomas, D.K. The second Hankel determinant for strongly convex and Ozaki close-to-convex functions. Ann. Mat. Pura Appl. (1923-) 2021, 200, 2515–2533. [Google Scholar] [CrossRef]
  36. 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]
  37. 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]
  38. Zaprawa, P.; Obradović, M.; Tuneski, N. Third Hankel determinant for univalent starlike functions. Rev. Real Acad. Cienc. Exactas Fis. Nat. Ser. A Mat. 2021, 115, 1–6. [Google Scholar] [CrossRef]
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content.

Share and Cite

MDPI and ACS Style

Shi, L.; Arif, M. Certain Sharp Coefficient Results on a Subclass of Starlike Functions Defined by the Quotient of Analytic Functions. Fractal Fract. 2023, 7, 195. https://doi.org/10.3390/fractalfract7020195

AMA Style

Shi L, Arif M. Certain Sharp Coefficient Results on a Subclass of Starlike Functions Defined by the Quotient of Analytic Functions. Fractal and Fractional. 2023; 7(2):195. https://doi.org/10.3390/fractalfract7020195

Chicago/Turabian Style

Shi, Lei, and Muhammad Arif. 2023. "Certain Sharp Coefficient Results on a Subclass of Starlike Functions Defined by the Quotient of Analytic Functions" Fractal and Fractional 7, no. 2: 195. https://doi.org/10.3390/fractalfract7020195

Article Metrics

Back to TopTop