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Article

Coefficient Inequalities of Second Hankel Determinants for Some Classes of Bi-Univalent Functions

by
Rayaprolu Bharavi Sharma
1 and
Kalikota Rajya Laxmi
2,*
1
Department of Mathematics, Kakatiya University, Warangal, Telangana-506009, India
2
Department of Mathematics, SRIIT, Hyderabad, Telangana-501301, India
*
Author to whom correspondence should be addressed.
Mathematics 2016, 4(1), 9; https://doi.org/10.3390/math4010009
Submission received: 17 December 2015 / Revised: 27 January 2016 / Accepted: 2 February 2016 / Published: 25 February 2016

Abstract

:
In this paper, we investigate two sub-classes S ( θ , β ) and K ( θ , β ) of bi-univalent functions in the open unit disc Δ that are subordinate to certain analytic functions. For functions belonging to these classes, we obtain an upper bound for the second Hankel determinant H 2 ( 2 ) .

1. Introduction

Let A be the class of the functions of the form
f ( z ) = z + k = 2 a k z k ,
which are analytic in the open unit disc Δ = { z : | z | < 1 } . Further, by S we shall denote the class of all functions in A that are univalent in Δ .
Let P denote the family of functions p ( z ) , which are analytic in Δ such that p ( 0 ) = 1 , and p ( z ) > 0 ( z Δ ) of the form
P ( z ) = 1 + n = 1 c n z n .
For two functions f and g , analytic in Δ , we say that the function f is subordinate to g in Δ , and we write it as f ( z ) g ( z ) if there exists a Schwarz function ω , which is analytic in Δ with ω ( 0 ) = 0 ,    | ω ( z ) | < 1 ( z Δ ) such that
f ( z ) = g ( ω ( z ) ) .
Indeed, it is known that
f ( z ) g ( z ) f ( 0 ) = g ( 0 )  and  f ( Δ ) g ( Δ ) .
Every function f S has an inverse f 1 , which is defined by f 1 ( f ( z ) ) = z , ( z Δ )
and   f ( f 1 ( w ) ) = w ,    ( | w | < r 0 ( f ) ; r 0 ( f ) 1 4 ) .
In fact, the inverse function is given by
f 1 ( w ) = w a 2 w 2 + ( 2 a 2 2 a 3 ) w 3 ( 5 a 2 3 5 a 2 a 3 + a 4 ) w 4 + ... .
A function f A is said to be bi-univalent in Δ if both f and f 1 are univalent in Δ .
Let denote the class of bi-univalent functions defined in the unit disc Δ .
We notice that is non empty .One of the best examples of bi-univalent functions is f ( z ) = log ( 1 + z 1 z ) , which maps the unit disc univalently onto a strip | Im w | < π 2 , which in turn contains the unit disc. Other examples are z , z 1 z , log ( 1 z ) .
However, the Koebe function is not a member of because it maps unit disc univalent onto the entire complex plane minus a slit along 1 4  to  . Hence, the image domain does not contain the unit disc.
Other examples of univalent function that are not in the class are z z 2 2 , z 1 z 2 .
In 1967, Lewin [1] first introduced class of bi-univalent function and showed that | a 2 | 1.51 for every f . Subsequently, in 1967, Branan and Clunie [2] conjectured that | a 2 | 2 for bi-star like functions and | a 2 | 1 for bi-convex functions. Only the last estimate is sharp; equality occurs only for f ( z ) = z 1 z or its rotation.
Later, Netanyahu [3] proved that max f | a 2 | = 4 3 . In 1985, Kedzierawski [4] proved Brannan and Clunie’s conjecture for bi-starlike functions. In 1985, Tan [5] obtained that | a 2 | < 1.485 , which is the best known estimate for bi-univalent functions. Since then, various subclasses of the bi-univalent function classes were introduced, and non-sharp estimates on the first two coefficients | a 2 | and | a 3 | in the Taylor Maclaurin’s series expansion were found in several investigations. The coefficient estimate problem for each of | a n | ( n N { 2 , 3 } ) is still an open problem.
In 1976, Noonan and Thomas [6] defined q t h Hankel determinant of f for q 1 and n 1 , which is stated by
H q ( n ) = | 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 | .
These determinants are useful, for example, in showing that a function of bounded characteristic in Δ , i.e., a function that is a ratio of two bounded analytic functions with its Laurent series around the origin having integral coefficient is rational.
The Hankel determinant plays an important role in the study of singularities (for instance, see [7] Denies, p.329 and Edrei [8]).A Hankel determinant plays an important role in the study of power series with integral coefficients. In 1966, Pommerenke [9] investigated the Hankel determinants of areally mean p-valent functions, univalent functions as well as of starlike functions, and, in 1967 [10], he proved that the Hankel determinants of univalent functions satisfy H q ( n ) < K n ( 1 2 + β ) q + 3 2       ( n = 1 , 2 , ... , q = 2 , 3 , ... ) where β > 1 4000 and K depend only on q . Later, Hayman [11] proved that H 2 ( n ) < A n 1 2       ( n = 1 , 2 , ... ; A  an absolute constant ) for areally mean univalent functions. The estimates for the Hankel determinant of areally mean p-valent functions have been investigated [12,13,14]. Elhosh [15,16] obtained bounds for Hankel determinants of univalent functions with a positive Hayman index α and k-fold symmetric and close to convex functions. Noor [9] determined the rate of growth of H q ( n ) as n for the functions in S with bounded boundary. Ehrenborg [17] studied the Hankel determinant of exponential polynomials. The Hankel transform of an integer sequence and some of its properties were discussed by Layman [18].
One can easily observe that the Fekete-Szego functional | a 3 a 2 2 | = H 2 ( 1 ) . This function was further generalized with μ real as well as complex. Fekete-Szego gave a sharp estimate of | a 3 μ a 2 2 | for μ real. The well-known results due to them is
| a 3 μ a 2 2 | { 4 μ 3 μ 1 1 + 2 exp ( 2 μ 1 μ ) 0 μ 1 3 4 μ μ 0 .
On the other hand, Zaprawa [19,20] extended the study on Fekete-Szego problem to some classes of bi-univalent functions. Ali [21] found sharp bounds on the first four coefficients and a sharp estimate for the Fekete-Szego functional | γ 3 t γ 2 2 | , where t is real, for the inverse function of f defined as f 1 ( w ) = w + k = 2 γ k w k to the class of strongly starlike functions of order α ( 0 < α 1 ) .
Recently S.K. Lee et al. [22] obtained the second Hankel determinant H 2 ( 2 ) = a 2 a 4 a 3 2 for functions belonging to subclasses of Ma-Minda starlike and convex functions. T. Ram Reddy [23] obtained the Hankel determinants for starlike and convex functions with respect to symmetric points. T. Ram Reddy et al. [24,25] also obtained the second Hankel determinant for subclasses of p-valent functions and p-valent starlike and convex function of order α .
Janteng [26] has obtained sharp estimates for the second Hankel determinant for functions whose derivative has a positive real part.Afaf Abubaker [27] studied sharp upper bound of the second Hankel determinant of subclasses of analytic functions involving a generalized linear differential operator. In 2015, the second Hankel determinant for bi-starlike and bi-convex function of order β was obtained by Erhan Deniz [28].

2. Preliminaries

Motivated by above work, in this paper, we introduce certain subclasses of bi-univalent functions and obtained an upper bound to the coefficient functional a 2 a 4 a 3 2 for the function f in these classes defined as follows:
Definition 2.1.: A function f A is said to be in the class S ( θ , β ) if it satisfies the following conditions:
{ e i θ { z f ( z ) f ( z ) } } > β cos θ    ( z Δ )
{ e i θ { w g ( w ) g ( w ) } } > β cos θ    ( w Δ )
where g is an extension of f 1 to Δ .
Note: 1. For θ = 0 , the class S ( θ , β ) reduces to the class S σ ( β ) , and, for this class, coefficient inequalities of the second Hankel determinant were studied by Deniz et al [28].
2. For θ = 0 and β = 0 , the class S ( θ , β ) reduces to the class S σ , and, for this class, coefficient inequalities of the second Hankel determinant were studied by Deniz et al [28].
Definition 2.2.: A function f A is said to be in the class K ( θ , β ) if it satisfies the following conditions:
{ e i θ { 1 + z f ( z ) f ( z ) } } > β cos θ     ( z Δ )
{ e i θ { 1 + w g ( w ) g ( w ) } } > β cos θ     ( w Δ )
where g is an extension of f 1 in Δ .
Note: 1. For θ = 0 , the class K ( θ , β ) reduces to the class K σ ( β ) , and, for this class, coefficient inequalities ofthe second Hankel determinantwere studied by Deniz et al [28].
2. For θ = 0 and β = 0 the class K ( θ , β ) reduces to the class K σ , and, for this class, coefficient inequalities ofthe second Hankel determinantwere studied by Deniz et al [28].
To prove our results, we require the following Lemmas:
Lemma 2.1. [14] Let the function p P be given by the following series:
p ( z ) = 1 + c 1 z + c 2 z 2 + c 3 z 3 + ....                ( z Δ ) .
Then the sharp estimate is given by | c n | 2       ( n N ) .
Lemma 2.2. [29] The power series for the function p P is given (10) converges in the unit disc Δ to a function in P if and only if Toeplitz determinants
D n = | 2 c 1 c 2 c n c 1 2 c 1 c n 1 c n c n + 1 c n + 2 2 | ,     n N
and c k = c ¯ k are all non-negative. These are strictly positive except for p ( z ) = k = 1 m ρ k P 0 ( e i t k z ) ,     ρ k > 0 ,     t k   real   and   t k t j for k j , where P 0 ( z ) = ( 1 + z 1 z ) ; in this case, D n > 0 for n < ( m 1 ) and D n = 0   for   n m .
This necessary and sufficient condition found in the literature [29] is due to Caratheodary and Toeplitz. We may assume without any restriction that c 1 > 0 . On using Lemma (2.2) for n = 2 and n = 3 respectively, we get
D 2 = | 2 c 1 c 2 c ¯ 1 2 c 1 c ¯ 2 c ¯ 1 2 | = [ 8 + 2 Re { c 1 2 c 2 } 2 | c 2 | 2 4 c 1 2 ] 0 .
It is equivalent to
2 c 2 = { c 1 2 + x ( 4 c 1 2 ) } ,  for some  x ,     | x | 1
D 3 = | 2 c 1 c 2 c 3 c ¯ 1 2 c 1 c 2 c ¯ 2 c ¯ 1 2 c 1 c ¯ 3 c ¯ 2 c ¯ 1 2 | 0 .
Then D 3 0 is equivalent to
| ( 4 c 3 4 c 1 c 2 + c 1 3 ) ( 4 c 1 2 ) + c 1 ( 2 c 2 c 1 2 ) 2 | 2 ( 4 c 1 2 ) 2 2 | ( 2 c 2 c 1 2 ) | 2 .
From the relations (2.6) and (2.7), after simplifying, we get
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 ) z ,
for some x , z with
| x | 1 and  | z | 1.

3. Main Results

We now prove our main result for the function f in the class S ( θ , β ) .
Theorem 3.1. Let the function f given by (1.1) be in the class S ( θ , β ) . Then
| a 2 a 4 a 3 2 | { 16 ( 1 β ) 4 cos 4 θ 3 + 4 3 ( 1 β ) 2 cos 2 θ ,        β [ 0 , 1 1 2 2 cos θ ] 3 ( 1 β ) 2 cos 2 θ 2 [ 1 2 ( 1 β ) 2 cos 2 θ ] ,          β ( 1 1 2 2 cos θ , 1 ) .
Proof: Let f S ( θ , β ; h ) and g = f 1 . From (6) and (7) it follows that
e i θ { z f ( z ) f ( z ) } = [ ( 1 β ) p ( z ) + β ] ] cos θ + i sin θ
e i θ { w g ( w ) g ( w ) } = [ ( 1 β ) q ( w ) + β ] ] cos θ + i sin θ
where p ( z ) = 1 + c 1 z + c 2 z 2 + c 3 z 3 + ....                P , ( z Δ ) and q ( w ) = 1 + d 1 w + d 2 w 2 + d 3 w 3 + ....                P ,    ( w Δ ) . Now, equating the coefficients in (14) and (15), we have
e i θ a 2 = c 1 ( 1 β ) cos θ
e i θ ( 2 a 3 a 2 2 ) = c 2 ( 1 β ) cos θ
e i θ ( 3 a 4 3 a 2 a 3 + a 2 3 ) = c 3 ( 1 β ) cos θ
and
e i θ a 2 = d 1 ( 1 β ) cos θ
e i θ ( 3 a 2 2 2 a 3 ) = d 2 ( 1 β ) cos θ
e i θ ( 3 a 4 + 12 a 2 a 3 10 a 2 3 ) = d 3 ( 1 β ) cos θ
Now from (16) and (19) we get
c 1 = d 1
and
c 2 = e i θ p 1 ( 1 β ) cos θ .
Now, from (17) and (20), we get
a 3 = e 2 i θ c 1 2 ( 1 β ) 2 cos 2 θ + e i θ ( 1 β ) cos θ ( c 2 d 2 ) 4 .
Additionally, from (18) and (21), we get
a 4 = 2 3 e 3 i θ c 1 3 ( 1 β ) 3 cos 3 θ + 5 8 e 2 i θ c 1 ( c 2 d 2 ) ( 1 β ) 2 cos 2 θ + 1 6 e i θ ( c 3 d 3 ) ( 1 β ) cos θ .
Thus, we can easily obtain
| a 2 a 4 a 3 2 | = | 1 3 e 4 i θ c 1 4 ( 1 β ) 4 cos 4 θ + 1 8 e 3 i θ c 1 2 ( c 2 d 2 ) ( 1 β ) 3 cos 3 θ +                1 6 e 2 i θ c 1 ( c 3 d 3 ) ( 1 β ) 2 cos 2 θ 1 16 e 2 i θ ( c 2 d 2 ) 2 ( 1 β ) 2 cos 2 θ | .
According to Lemma (2.2) and Equation (22), we get
2 c 2 = c 1 2 + x ( 4 c 1 2 ) 2 d 2 = d 1 2 + x ( 4 d 1 2 ) } c 2 d 2 = 0
and
c 3 d 3 = c 1 3 2 c 1 ( 4 c 1 2 ) x c 1 ( 4 c 1 2 ) x 2 2
| a 2 a 4 a 3 2 | = | 1 3 e 4 i θ c 1 4 ( 1 β ) 4 cos 4 θ + 1 12 e 2 i θ c 1 4 ( 1 β ) 2 cos 2 θ                                 1 6 e 2 i θ c 1 2 ( 4 c 1 2 ) x ( 1 β ) 2 cos 2 θ 1 12 e 2 i θ c 1 2 ( 4 c 1 2 ) x 2 ( 1 β ) 2 cos 2 θ | .
Since p P , so | c 1 | 2 . Letting c 1 = c , we may assume without any restriction that c [ 0 , 2 ] . Thus, applying the triangle inequality on the right-hand side of Equation (29), with μ = | x | 1 , we obtain
| a 2 a 4 a 3 2 | 1 3 c 4 ( 1 β ) 4 cos 4 θ + 1 12 c 4 ( 1 β ) 2 cos 2 θ + 1 6 c 2 ( 4 c 2 ) μ ( 1 β ) 2 cos 2 θ                          + 1 12 c 2 ( 4 c 2 ) μ 2 ( 1 β ) 2 cos 2 θ = F ( μ ) .
Differentiating F ( μ ) , we get
F ( μ ) = c 2 ( 4 c 2 ) ( 1 β ) 2 cos 2 θ + c 2 ( 4 c 2 ) μ ( 1 β ) 2 cos 2 θ 6 .
Using elementary calculus, one can show that F ( μ ) > 0 for μ > 0 . This implies that F is an increasing function, and it therefore cannot have a maximum value at any point in the interior of the closed region [ 0 , 2 ] × [ 0 , 1 ] . Further, the upper bound for F ( μ ) corresponds to μ = 1 , in which case F ( μ ) F ( 1 )
1 3 c 4 ( 1 β ) 4 cos 4 θ + 1 12 c 4 ( 1 β ) 2 cos 2 θ + 1 4 c 2 ( 4 c 2 ) ( 1 β ) 2 cos 2 θ = G ( c ) .
Then
G ( c ) = 2 3 c ( 1 β ) 2 cos 2 θ [ ( 2 ( 1 β ) 2 cos 2 θ 1 ) c 2 + 1 ] .
Setting G ( c ) = 0 , the real critical points are c 01 = 0 , c 02 = 3 1 2 ( 1 β ) 2 cos 2 θ .
After some calculations we obtain the following cases:
Case 1: When β [ 0 , 1 1 2 2 cos θ ] , we observe that c 02 2 , that is c 02 , is out of the interval ( 0 , 2 ) . Therefore, the maximum value of G ( c ) occurs at c 01 = 0 or c = c 02 , which contradicts our assumption of having a maximum value at the interior point of c [ 0 , 2 ] . Since G is an increasing function, the maximum point of G must be on the boundary of c [ 0 , 2 ] , that is c = 2 . Thus, we have
max 0 c 2 G ( c ) = G ( 2 ) = 16 ( 1 β ) 4 cos 4 θ 3 + 4 3 ( 1 β ) 2 cos 2 θ .
Case 2: When β ( 1 1 2 2 cos θ , 1 ) , we observe that c 02 < 2 , that is c 02 , is interior of the interval [ 0 , 2 ] . Since G ( c 02 ) < 0 , the maximum value of G ( c ) occurs at c = c 02 . Thus, we have
max 0 c 2 G ( c ) = G ( c 02 ) = G ( 1 1 3 2 3 ( 1 β ) 2 cos 2 θ ) = 3 ( 1 β ) 2 cos 2 θ 2 [ 1 2 ( 1 β ) 2 cos 2 θ ] .
This completes the proof of the theorem.
Corollary 1: Let f given by (1.1) be in the class S σ ( β ) . Then
| a 2 a 4 a 3 2 | { 16 ( 1 β ) 4 3 + 4 3 ( 1 β ) 2 ,        β [ 0 , ( 1 1 2 2 ) ] 3 ( 1 β ) 2 2 [ 1 2 ( 1 β ) 2 ] ,                    β ( 1 1 2 2 , 1 ) .
Corollary 2: Let f given by (1.1) be in the class S σ . Then
| a 2 a 4 a 3 2 | 20 3 .
These two corollaries coincide with the results of Deniz et al. [28].
Remark 3.1: It is observed that for θ = 0 , we get the Hankel determinant | a 2 a 4 a 3 2 | for the class S σ ( β ) and the Hankel determinant of this class was studied by Deniz et al. [28].

4. Hankel Determinants for the Class of Functions K ( θ , β ; h )

We now estimate an upper bound a 2 a 4 a 3 2 for the function f ( z ) in the class K ( θ , β ; h ) .
Theorem 4.1. Let the f ( z ) given by (1.1) be in the class K ( θ , β ; h ) . Then
| a 2 a 4 a 3 2 | { 1 6 ( 1 β ) 4 cos 4 θ + 1 6 ( 1 β ) 2 cos 2 θ ,        β [ 0 , 1 1 2 cos θ ] 3 ( 1 β ) 2 cos 2 θ 8 [ 2 ( 1 β ) 2 cos 2 θ ] ,          β ( 1 1 2 cos θ , 1 ) .
Proof: Let f K ( θ , β ; h ) and g = f 1 . From (8) and (9) we have
e i θ { 1 + z f ( z ) f ( z ) } = [ ( 1 β ) p ( z ) + β ] ] cos θ + i sin θ
e i θ { 1 + w g ( w ) g ( w ) } = [ ( 1 β ) p ( w ) + β ] ] cos θ + i sin θ
where p ( z ) = 1 + c 1 z + c 2 z 2 + c 3 z 3 + ....                ,    ( z Δ ) and q ( w ) = 1 + d 1 w + d 2 w 2 + d 3 w 3 + ....                ,    ( w Δ ) .
Now, equating the coefficients in (33) and (34), we have
2 e i θ a 2 = c 1 ( 1 β ) cos θ
e i θ ( 6 a 3 4 a 2 2 ) = c 2 ( 1 β ) cos θ
e i θ ( 12 a 4 18 a 2 a 3 + 8 a 2 3 ) = c 3 ( 1 β ) cos θ
and
2 e i θ a 2 = d 1 ( 1 β ) cos θ
e i θ ( 8 a 2 2 6 a 3 ) = d 2 ( 1 β ) cos θ
e i θ ( 32 a 2 3 + 42 a 2 a 3 12 a 4 ) = d 3 ( 1 β ) cos θ .
Now from (35) and (38), we get
c 1 = d 1
and
a 2 = e i θ c 1 ( 1 β ) cos θ 2 .
Now, from (36) and (39), we get
a 3 = e 2 i θ c 1 2 ( 1 ρ ) 2 cos 2 θ 4 + e i θ ( c 2 d 2 ) ( 1 ρ ) cos θ 12 .
Additionally, from (37) and (40), we get
a 4 = 5 48 e 3 i θ c 1 3 ( 1 β ) 3 cos 3 θ + 5 48 e 2 i θ c 1 ( c 2 d 2 ) ( 1 β ) 2 cos 2 θ + 1 24 e i θ ( c 3 d 3 ) ( 1 β ) cos θ .
Thus, we can easily obtain
| a 2 a 4 a 3 2 | = | c 1 4 96 e 4 i θ ( 1 β ) 4 cos 4 θ + c 1 2 96 e 3 i θ ( c 2 d 2 ) ( 1 β ) 3 cos 3 θ +                              c 1 48 e 2 i θ ( c 3 d 3 ) ( 1 β ) 3 cos 3 θ e 2 i θ ( c 2 d 2 ) 2 ( 1 β ) 2 cos 2 θ 144 | .
According to Lemma (2.2), and from Equation (41), we get
2 c 2 = c 1 2 + x ( 4 c 1 2 ) 2 d 2 = d 1 2 + x ( 4 d 1 2 ) } c 2 d 2 = 0
and
c 3 d 3 = c 1 3 2 c 1 ( 4 c 1 2 ) x c 1 ( 4 c 1 2 ) x 2 2
| a 2 a 4 a 3 2 | = | c 1 4 96 e 4 i θ ( 1 β ) 4 cos 4 θ + c 1 4 96 e 2 i θ ( 1 β ) 2 cos 2 θ                            e 2 i θ c 1 2 ( 4 c 1 2 ) x ( 1 β ) 2 cos 2 θ 48 e 2 i θ c 1 2 ( 4 c 1 2 ) x 2 ( 1 β ) 2 cos 2 θ 96 | .
Since p P , | c 1 | 2 . Letting c 1 = c , we may assume without any restriction that c [ 0 , 2 ] . Thus, applying the triangle inequality on the right-hand side of Equation (4.16), with μ = | x | 1 , we obtain
| a 2 a 4 a 3 2 | c 4 96 e 4 i θ ( 1 β ) 4 cos 4 θ + c 4 96 e 2 i θ ( 1 β ) 2 cos 2 θ                             e 2 i θ c 2 ( 4 c 2 ) μ ( 1 β ) 2 cos 2 θ 48 + e 2 i θ c 2 ( 4 c 2 ) μ 2 ( 1 β ) 2 cos 2 θ 96                            = F ( μ ) .
Differentiating F ( μ ) , we get
F ( μ ) = e 2 i θ c 2 ( 4 c 2 ) ( 1 β ) 2 cos 2 θ 48 + e 2 i θ c 2 ( 4 c 2 ) μ ( 1 β ) 2 cos 2 θ 48 .
Using elementary calculus, one can show that F ( μ ) > 0 for μ > 0 . It implies that F is an increasing function and it hence cannot have a maximum value at any point in the interior of the closed region [ 0 , 2 ] × [ 0 , 1 ] . Further, the upper bound for F ( μ ) corresponds to μ = 1 , in which case
F ( μ ) F ( 1 ) c 4 96 ( 1 β ) 4 cos 4 θ + c 4 96 ( 1 β ) 2 cos 2 θ + c 2 ( 4 c 2 ) ( 1 β ) 2 cos 2 θ 48      + c 2 ( 4 c 2 ) ( 1 β ) 2 cos 2 θ 96 = G ( c )    ( say ) .
Then
G ( c ) = c 3 24 ( 1 β ) 4 cos 4 θ + c 3 24 ( 1 β ) 2 cos 2 θ + [ 8 c 4 c 3 ] ( 1 β ) 2 cos 2 θ 32 .
Setting G ( c ) = 0 , the real critical points are c 01 = 0 , c 02 = 6 [ 2 ( 1 β ) 2 cos 2 θ ] .
After some calculations we obtain the following cases:
Case 1: When β [ 0 , 1 1 2 cos θ ] , we observe that c 02 2 , that is c 02 , is out of the interval ( 0 , 2 ) . Therefore, the maximum value of G ( c ) occurs at c 01 = 0 or c = c 02 , which contradicts our assumption of having the maximum value at the interior point of c [ 0 , 2 ] . Since G is an increasing function, the maximum point of G must be on the boundary of c [ 0 , 2 ] , that is c = 2 . Thus, we have
max 0 c 2 G ( c ) = G ( 2 ) = 1 6 ( 1 β ) 4 cos 4 θ + 1 6 ( 1 β ) 2 cos 2 θ .
Case 2: When β ( 1 1 2 cos θ , 1 ) , we observe that c 02 < 2 , that is c 02 , is interior of the interval [ 0 , 2 ] . Since G ( c 02 ) < 0 , the maximum value of G ( c ) occurs at c = c 02 . Thus, we have
max 0 c 2 G ( c ) = G ( c 02 ) = G ( 6 [ 2 ( 1 β ) 2 cos 2 θ ] )                                          = 3 ( 1 β ) 2 cos 2 θ 8 [ 2 ( 1 β ) 2 cos 2 θ ] .
This completes the proof of the theorem.
Corollary 1: Let f given by (1) be in the class K σ ( β ) . Then
| a 2 a 4 a 3 2 | { ( 1 β ) 4 6 + ( 1 β ) 2 6 ,        β [ 0 , ( 1 1 2 ) ] 3 ( 1 β ) 2 8 [ 2 ( 1 β ) 2 ] ,                    β ( 1 1 2 , 1 ) .
Corollary 2: Let f given by (1) be in the class K σ . Then
| a 2 a 4 a 3 2 | 1 3 .
These two corollaries coincide with the results of Deniz et al. [28].

5. Conclusion

For specific values of α and β , the results obtained in this paper will generalize and unify the results of the earlier researchers in this direction.
Interested researchers can work upon finding an upper bound for | a 2 a 4 μ a 3 2 | and | a n | for a real or complex μ .

Acknowledgments

The authors are very much thankful to T. Ram Reddy for his valuable guidance in preparing this paper.

Author Contributions

Both authors has read and approved the final paper.

Conflicts of Interest

The authors declare that there are no conflicts of interest regarding the publication of this paper.

References

  1. Lewin, M. On a Coefficient problem for bi-univalent functions. Proc. Am. Math. Soc. 1967, 18, 63–68. [Google Scholar] [CrossRef]
  2. Brannan, D.A.; Clunie, J.G. (Eds.) Aspects of Contemporary Complex Analysis. In Proceedings of the NATO Advanced Study Institute, University of Durham, Durham, UK, 1–20 July 1979; Academic Press: New York, NY, USA; London, UK, 1980.
  3. Netanyahu, E. The minimal distance of the image boundary from the origin and the second coefficient of a univalent function in | Z | < 1 . Arch. Ration. Mech. Anal. 1969, 32, 100–112. [Google Scholar]
  4. Kedzierawski, A.W. Some remarks on bi-univalent functions. Ann. Univ. Mariae Curie Skłodowska Sect. A 1985, 39, 77–81. [Google Scholar]
  5. Tan, D.L. Coefficient estimates for bi-univalent functions. Chinese Ann. Math. Ser. A 1984, 5, 559–568. [Google Scholar]
  6. Noonan, J.W.; Thomas, D.K. On the second Hankel determinant of a really mean p-valent functions. Trans. Am. Math. Soc. 1976, 223, 337–346. [Google Scholar]
  7. Dienes, P. The Taylor Series; Dover: New York, NY, USA, 1957. [Google Scholar]
  8. Edrei, A. Sur les determinants recurrents et less singularities d’une fonction donee por son develepment de Taylor. Compos. Math. 1940, 7, 20–88. [Google Scholar]
  9. Pommerenke, C. On the coefficients and Hankel determinants of univalent functions. J. Lond. Math. Soc. 1966, 41, 111–122. [Google Scholar] [CrossRef]
  10. Pommerenke, C. On the Hankel determinants of univalent functions. Mathematika 1967, 14, 108–112. [Google Scholar] [CrossRef]
  11. Hayman, W.K. On the second Hankel determinant of mean univalent functions. Proc. Lond. Math. Soc. 1968, 18, 77–94. [Google Scholar] [CrossRef]
  12. Noonan, J.W.; Thomas, D.K. On the Hankel determinants of a really mean p-valent functions. Proc. Lond. Math. Soc. 1972, 25, 503–524. [Google Scholar] [CrossRef]
  13. Noonan, J.W. Coefficient differences and Hankel determinants of a really mean p-valent functions. Proc. Am. Math. Soc. 1974, 46, 29–37. [Google Scholar]
  14. Pommerenke, C. Univalent Functions; Vandenhoeck and Rupercht: Gotingen, Germany, 1975. [Google Scholar]
  15. Elhosh, M.M. On the second Hankel determinant of close-to-convex functions. Bull. Malays. Math. Soc. 1986, 9, 67–68. [Google Scholar]
  16. Elhosh, M.M. On the second Hankel determinant of univalent functions. Bull. Malays. Math. Soc. 1986, 9, 23–25. [Google Scholar]
  17. Ehrenborg, R. The Hankel determinant of exponential polynomials. Am. Math. Mon. 2000, 107, 557–560. [Google Scholar] [CrossRef]
  18. Layman, J.W. The Hankel transform and some of its properties. J. Integer Seq. 2001, 4, 1–11. [Google Scholar]
  19. Cantor, D.G. Power series with integral coefficients. Bull. Am. Math. Soc. 1963, 69, 362–366. [Google Scholar] [CrossRef]
  20. Zaprawa, P. Estimates of initial coefficients for bi-univalent functions. Abstr. Appl. Anal. 2014, 2014, 357480. [Google Scholar] [CrossRef]
  21. Ali, R.M. Coefficients of the inverse of strongly starlike functions. Bull. Malays. Math. Sci. Soc. 2003, 26, 63–71. [Google Scholar]
  22. Lee, S.K.; Ravichandran, V.; Supramaniam, S. Bounds for the second Hankel determinant of certain univalent functions. J. Inequal. Appl. 2013, 2013, 281. [Google Scholar] [CrossRef]
  23. RamReddy, T.; Vamshee Krishna, D. Hankel determinant for starlike and convex functions with respect to symmetric points. J. Indian Math. Soc. 2012, 79, 161–171. [Google Scholar]
  24. RamReddy, T.; Vamshee Krishna, D. Hankel determinant for p-valent starlike and convex functions of order α. Novi Sad J. Math. 2012, 42, 89–96. [Google Scholar]
  25. RamReddy, T.; Vamshee Krishna, D. Certain inequality for certain subclass of p-valent functions. Palest. J. Math. 2015, 4, 223–228. [Google Scholar]
  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, 1–5. [Google Scholar]
  27. Abubaker, A.; Darus, M. Hankel determinant for a class of analytic functions involving a generalized linear differential operator. Int. J. Pure Appl. Math. 2011, 69, 429–435. [Google Scholar]
  28. Deniz, E.; Çağlar, M.; Orhan, H. Second hankel determinant for bi-starlike and bi-convex functions of order β. Appl. Math. Comput. 2015, 271, 301–307. [Google Scholar] [CrossRef]
  29. Grenander, U.; Szego, G. Toeplitz Forms and Their Applications; University of Californi Press: Berkeley, CA, USA, 1958. [Google Scholar]

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Bharavi Sharma, R.; Rajya Laxmi, K. Coefficient Inequalities of Second Hankel Determinants for Some Classes of Bi-Univalent Functions. Mathematics 2016, 4, 9. https://doi.org/10.3390/math4010009

AMA Style

Bharavi Sharma R, Rajya Laxmi K. Coefficient Inequalities of Second Hankel Determinants for Some Classes of Bi-Univalent Functions. Mathematics. 2016; 4(1):9. https://doi.org/10.3390/math4010009

Chicago/Turabian Style

Bharavi Sharma, Rayaprolu, and Kalikota Rajya Laxmi. 2016. "Coefficient Inequalities of Second Hankel Determinants for Some Classes of Bi-Univalent Functions" Mathematics 4, no. 1: 9. https://doi.org/10.3390/math4010009

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