EUROPEAN JOURNAL OF PURE AND APPLIED MATHEMATICS Vol. 10, No. 2, 2017, 348-362 ISSN 1307-5543 – www.ejpam.com Published by New York Business Global New Subclasses of Analytic Function Associated with q-Difference Operator C. Ramachandran 1, T. Soupramanien2, B.A. Frasin3,∗ 1 Department of Mathematics, University College of Engineering Villupuram, Anna Univer- sity, Villupuram, Tamilnadu, India. 2 Department of Mathematics, IFET College of Engineering, Gangarampalayam, Villupu- ram, Tamilnadu, India. 3 Department of Mathematics, Faculty of Science, Al al-Bayt University, Mafraq, Jordan. Abstract. The aim of this paper is to establish the coefficient bounds for certain classes of ana- lytic functions associated with q-difference operator. Certain applications of these results for the functions defined through convolution are also obtained. 2010 Mathematics Subject Classifications: Primary 30C45; Secondary 30C50 Key Words and Phrases: Univalent function, Schwarz function, q-starlike function, q-convex function, q-derivative operator, subordination, Fekete-Szego inequality. 1. Introduction Recently, the area of q-analysis has attracted the serious attention of researchers. The q-difference calculus or quantum calculus was initiated at the beginning of 19th century, that was initiated by Jackson [6, 7]. He was the first to develop q-integral and q-derivative in a systematic way. The fractional q-difference calculus had its origin in the works by Al.Salam [2] and Agarwal [1]. This great interest is due to its application in various branches of mathematics and physics, as for example, in the areas of ordinary fractional calculus, optimal control problems, q-difference and q-integral equations and in q-transform analysis. The generalization q-Taylor’s formula in fractional q-calculus was introduced by Purohit and Raina [18]. Mohammed and Darus [12] studied approximation and geometric properties of these q-operators in some subclasses of analytic functions in compact disk. Purohit and Raina recently in [18, 16] have used the fractional q-calculus operators in investigating certain classes of functions which are analytic in the open disk and Purohit [17] also studied these q-operators are defined by using convolution of normalized analytic ∗Corresponding author. Email addresses: crjsp2004@yahoo.com (C. Ramachandran), soupramani@gmail.com (T. Soupramanien), bafrasin@yahoo.com (B.A. Frasin) http://www.ejpam.com 348 c© 2017 EJPAM All rights reserved. C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 349 functions and q-hypergeometric functions. A comprehensive study on applications of q- calculus in operator theory may be found in[4]. Ramachandran et. al. [19] have used the fractional q-calculus operators in investigating certain bound for q-starlike and q-convex functions with respect to symmetric points. Let A denote the class of all analytic functions f(z) of the form f(z) = z + ∞∑ n=2 anz n, (1) defined on the open unit disk U = {z : z ∈ C : |z| < 1}. If the functions f(z) and g(z) are analytic in U, we say that the function f(z) is subordinate to g(z), written as f ≺ g in U or f(z) ≺ g(z) (z ∈ U), if there exists a Schwarz function w(z), in U with w(0) = 0 and |w(z)| < 1 (z ∈ U) such that f(z) = g(w(z)). Furthermore, if the function g(z) is univalent in U, the above subordination is equivalence holds (see [11] and [5]) f(z) ≺ g(z) ⇐⇒ f(0) = g(0), and f(U) ⊂ g(U). For function f ∈ A given by (1) and 0 < q < 1, the q-derivative of a function f is defined by (see [6, 7]) Dqf(z) = f(qz)− f(z) (q − 1)z (z 6= 0), (2) Dqf(0) = f ′(0) and D2 qf(z) = Dq(Dqf(z)). From (2), we deduce that Dqf(z) = 1 + ∞∑ k=2 [k]q akz k−1, (3) where [k]q = 1− qk 1− q . (4) As q → 1−, [k]q → k. For a function h(z) = zk, we observe that Dq(h(z)) = Dq ( zk ) = 1− qk 1− q zk−1 = [k]q z k−1, lim q→1− (Dq(h(z))) = lim q→1− ( [k]qz k−1 ) = kzk−1 = h′(z), where h′ is the ordinary derivative. As a right inverse, Jackson [7] introduced the q-integral∫ z 0 f(t)dqt = z(1− q) ∞∑ k=0 qkf ( zqk ) , C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 350 provided that the series converges. For a function h(z) = zk, we observe that∫ z 0 h(t)dqt = ∫ z 0 tkdqt = zk+1 [k + 1]q (k 6= −1) lim q→1− ∫ z 0 h(t)dqt = lim q→1− zk+1 [k + 1]q = zk+1 k + 1 = ∫ z 0 h(t)dt, where ∫ z 0 h(t)dt is the ordinary integral. Making use of the q-derivative Dqf(z), the subclasses S∗q (α) and Cq(α) of the class A for 0 ≤ α ≤ 1 are introduced by S∗q (α) = { f ∈ A : Re ( zDqf(z) f(z) ) ≥ α, z ∈ U } (5) Cq(α) = { f ∈ A : Re ( Dq(zDqf(z)) Dqf(z) ) ≥ α, z ∈ U } . (6) We note that f ∈ Cq(α)⇔ zDqf ∈ S∗q (α), (7) and lim q→1− S∗q (α) = { f ∈ A : lim q→1− Re ( zDqf(z) f(z) ) ≥ α, z ∈ U } = S∗(α), lim q→1− Cq(α) = { f ∈ A : lim q→1− Re ( Dq(zDqf(z)) Dqf(z) ) ≥ α, z ∈ U } = C(α), where S∗(α) and C(α) are respectively, the classes of starlike of order α and convex of order α in U (see Robertson [23]). Kanas and Rǎducanu in [8] used the Ruscheweyh q- differential operator to introduce and study some properties of (q, k) uniformly starlike functions of order α. It is clear that Dqf(z)→ f ′(z) as q → 1−. This difference operator helps us to generalize the class of starlike functions S∗ analytically. By making use of the q-derivative of a function f ∈ A and the principle of subordina- tion, we now introduce the following classes Definition 1. Let φ(z) be a univalent starlike function with respect to 1, which maps the open unit disk U onto a region in the right half-plane and is symmetric with respect to the real axis, with φ(0) = 1 and φ′(0) ≥ 0. A function f ∈ A is said to be in the class Mq,α,β,λ(φ) if( zDqf(z) f(z) )α [ (1− λ) ( zDqf(z) f(z) ) + λ ( Dq(zDqf(z)) Dqf(z) )]β ≺ φ(z) (8) where 0 ≤ β ≤ 1; 0 ≤ α ≤ 1; 0 ≤ λ ≤ 1. C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 351 We note that (i) lim q→1− Mq,α,β,λ(φ) =Mα,β,λ(φ) (C. Ramachandran et al. [20]) (ii) lim q→1− Mq,0,1,λ(φ) =M(λ, φ) (Ali et al. [3]) (iii) lim q→1− Mq,α,β,1(φ) =Mα,β(φ) (V. Ravichandran et al. [21]) (iv) lim q→1− Mq,0,1,0(φ) = lim q→1− Mq,1,0,λ(φ) = S∗(φ) and lim q→1− Mq,0,1,1(φ) = C(φ) (Ma and Minda [9]) 2. Preliminary Results In order to prove the main results we need the following lemmas. Lemma 1. [9] If p(z) = 1 + c1z+ c2z 2 + · · · is an analytic function with positive real part in U, then ∣∣c2 − νc21∣∣ ≤  −4ν + 2 if ν ≤ 0 2 if 0 ≤ ν ≤ 1 4ν + 2 if ν ≥ 1. When ν < 0 or ν > 1, the equality holds if and only if p(z) = 1 + z 1− z or one of its rotations. If 0 < ν < 1, then the equality holds true if and only if p(z) = 1 + z2 1− z2 or one of its rotations. If ν = 0, the equality holds if and only if p(z) = ( 1 2 + 1 2 η ) 1 + z 1− z + ( 1 2 − 1 2 η ) 1− z 1 + z , (0 ≤ η ≤ 1) or one of its rotations. If ν = 1, the equality holds true if and only if p(z) is the reciprocal of one of the functions such that the equality holds true in the case when ν = 0. Although the above upper bound is sharp, in the case when 0 < ν < 1, it can be further improved as follows: |c2 − νc21|+ ν|c1|2 ≤ 2 ( 0 < ν ≤ 1 2 ) and |c2 − νc21|+ (1− ν)|c1|2 ≤ 2 ( 1 2 < ν ≤ 1 ) . We also need the following result in our investigation. Lemma 2. [22] If p1(z) = 1 + c1z + c2z 2 + · · · is a function with positive real part in U, then |c2 − νc21| ≤ 2 max{1, |2ν − 1|}. The result is sharp for the function p1(z) = 1 + z2 1− z2 and p1(z) = 1 + z 1− z . C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 352 3. Main Results Unless otherwise mentioned, we assume throughout this paper that the function 0 < q < 1, φ ∈ P, [k]q is given by (4) and z ∈ U. By making use of Lemma 1, we first prove the Fekete-Szegö type inequalities asserted by Theorem 1 below. Theorem 1. Let 0 ≤ µ ≤ 1, 0 ≤ α ≤ 1, 0 ≤ β ≤ 1 and 0 ≤ λ ≤ 1. Also let φ(z) = 1 +B1z +B2z 2 +B3z 3 + . . . , where the coefficients Bn are real with B1 > 0 and B2 ≥ 0. If f(z) given by (1) belongs to the function class Mq,α,β,λ(φ), then |a3 − µa22| ≤  1 2ξ ( 2B2 − ( ρ2 + 2µξ − τ ρ2 ) B2 1 ) if µ ≤ σ1, B1 ξ if σ1 ≤ µ ≤ σ2, 1 2ξ ( −2B2 + ( ρ2 + 2µξ − τ ρ2 ) B2 1 ) if µ ≥ σ2, (9) where, for convenience, σ1 := 2ρ2(B2 −B1)− (ρ2 − τ)B2 1 2ξB2 1 , (10) σ2 := 2ρ2(B2 +B1)− (ρ2 − τ)B2 1 2ξB2 1 , (11) σ3 := 2ρ2B2 − (ρ2 − τ)B2 1 2ξB2 1 . (12) ρ = ([2]q − 1)α+ ([2]q − 1 + λ)β, (13) ξ = ([3]q − 1)α+ ([3]q − 1 + λ ([3]q ([2]q − 1) + 1))β, (14) τ = ( [2]2q − 1 ) α+ ( [2]2q − 1 + 2[2]2qλ+ λ2 ) β. (15) If σ1 ≤ µ ≤ σ3, then |a3 − µa22|+ ρ2 ξB1 ( 1− B2 B1 + ( ρ2 + 2µξ − τ 2ρ2 ) B1 ) |a2|2 ≤ B1 ξ . (16) Furthermore, if σ3 ≤ µ ≤ σ2, then |a3 − µa22|+ ρ2 ξB1 ( 1 + B2 B1 − ( ρ2 + 2µξ − τ 2ρ2 ) B1 ) |a2|2 ≤ B1 ξ . (17) Each of these results is sharp. C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 353 Proof. If f(z) ∈Mq,α,β,λ(φ), then there exists a Schwarz function w(z), analytic in U with w(0) = 0 and |w(z)| < 1 (z ∈ U), such that( zDqf(z) f(z) )α [ (1− λ) ( zDqf(z) f(z) ) + λ ( Dq(zDqf(z)) Dqf(z) )]β = φ (w(z)) . (18) Define the function p1(z) by p1(z) = 1 + w(z) 1− w(z) = 1 + c1z + c2z 2 + · · · . (19) Since w(z) is a Schwarz function, we see that <(p1(z)) > 0 (z ∈ U) and p1(0) = 1. Now, defining the function p(z) by p(z) := ( zDqf(z) f(z) )α [ (1− λ) ( zDqf(z) f(z) ) + λ ( Dq(zDqf(z)) Dqf(z) )]β = 1 + b1z + b2z 2 + · · · , (20) we find from (18) and (19) that p(z) = φ ( p1(z)− 1 p1(z) + 1 ) . (21) Thus, by using (19) and (21), we obtain b1 = 1 2 B1c1 and b2 = 1 2 B1 ( c2 − 1 2 c21 ) + 1 4 B2c 2 1. An easy computation would show that( zDqf(z) f(z) )α [ (1− λ) ( zDqf(z) f(z) ) + λ ( Dq(zDqf(z)) Dqf(z) )]β = 1 + [([2]q − 1)α+ ([2]q − 1 + λ)β] a2z + [([3]q − 1)α+ ([3]q − 1 + λ ([3]q ([2]q − 1) + 1))β] a3z 2 +[ α 2 ([2]q − 1) ((α− 1) ([2]q − 1)− 2) + β (β − 1) 2 ([2]q − 1 + λ)2 + α ([2]q − 1)β ([2]q − 1 + λ)− (([2]q − 1) + ([2]q ([2]q − 1) + 1)λ)β] a22z 2 + · · · which, in view of (20), yields b1 = [([2]q − 1)α+ ([2]q − 1 + λ)β] a2 C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 354 and b2 = [([3]q − 1)α+ ([3]q − 1 + λ ([3]q ([2]q − 1) + 1))β] a3 +[ α 2 ([2]q − 1) ((α− 1) ([2]q − 1)− 2) + β (β − 1) 2 ([2]q − 1 + λ)2 + α ([2]q − 1)β ([2]q − 1 + λ)− (([2]q − 1) + ([2]q ([2]q − 1) + 1)λ)β] a22. Equivalently, we have a2 = B1c1 2 [([2]q − 1)α+ ([2]q − 1 + λ)β] and a3 = B1 2 [([3]q − 1)α+ ([3]q − 1 + λ ([3]q ([2]q − 1) + 1))β] [ c2 − 1 2 ( 1− B2 B1 + Λ0B1 ) c21 ] where Λ0 = 1 [([2]q − 1)α+ ([2]q − 1 + λ)β]2 [α 2 ([2]q − 1) ((α− 1) ([2]q − 1)− 2) + β (β − 1) 2 ([2]q − 1 + λ)2 + α ([2]q − 1)β ([2]q − 1 + λ)− (([2]q − 1) + ([2]q ([2]q − 1) + 1)λ)β] . Therefore, we obtain a3 − µa22 = B1 2 [([3]q − 1)α+ ([3]q − 1 + λ ([3]q ([2]q − 1) + 1))β] ( c2 − νc21 ) (22) where ν = 1 2 ( 1− B2 B1 + B1 2 [([2]q − 1)α+ ([2]q − 1 + λ)β]2 [ (([2]q − 1)α+ ([2]q − 1 + λ)β)2 +2µ (([3]q − 1)α+ ([3]q − 1 + λ ([3]q ([2]q − 1) + 1))β)−(( [2]2q − 1 ) α+ ( [2]2q − 1 + 2[2]2qλ+ λ2 ) β )]) . The assertion of Theorem 1 now follows by an application of Lemma 1. To show that the bounds asserted by Theorem 1 are sharp, we define the following functions: Kφn(z) (n ∈ N\{1};N := {1, 2, 3, · · · }), with Kφn(0) = 0 = K′φn(0)− 1, by ( zK′φn(z) Kφn(z) )α [ (1− λ) ( zK′φn(z) Kφn(z) ) + λ ( K′φn(zK′φn(z)) K′φn(z) )]β = φ(zn−1), C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 355 and the functions Fη and Gη (0 ≤ η ≤ 1) with Fη(0) = 0 = F ′η(0)− 1 and Gη(0) = 0 = G′η(0)− 1 by ( zF ′η(z) Fη(z) )α [ (1− λ) ( zF ′η(z) Fη(z) ) + λ (F ′η(zF ′η(z)) F ′η(z) )]β = φ ( z(z + η) 1 + ηz ) and ( zG′η(z) Gη(z) )α [ (1− λ) ( zG′η(z) Gη(z) ) + λ (G′η(zG′η(z)) G′η(z) )]β = φ ( −z(z + η) 1 + ηz ) respectively. Then, clearly, the functions Kφn , Fη, Gη ∈Mq,α,β,λ(φ). Also we write Kφ := Kφ2 . If µ < σ1 or µ > σ2, then the equality in Theorem 1 holds true if and only if f is Kφ or one of its rotations. When σ1 ≤ µ ≤ σ2, then the equality holds true if and only if f is Kφ3 or one of its rotations. If µ = σ1, then the equality holds true if and only if f is Fη or one of its rotations. If µ = σ2 , then the equality holds true if and only if f is Gη or one of its rotations. By making use of Lemma 2, we immediately obtain the following Fekete-Szegö type inequality. Theorem 2. Let 0 ≤ µ ≤ 1, 0 ≤ α ≤ 1, 0 ≤ β ≤ 1 and 0 ≤ λ ≤ 1. Also let φ(z) = 1 +B1z +B2z 2 +B3z 3 + . . . , where the coefficients Bn are real with B1 > 0 and B2 ≥ 0. If f(z) given by (1) belongs to the function class Mq,α,β,λ(φ), then |a3 − µa22| ≤ B1 ξ max { 1, ∣∣∣∣−B2 B1 + ( ρ2 + 2µξ − τ 2ρ2 ) B1 ∣∣∣∣} (µ ∈ C), where ρ, ξ and τ are defined by (13), (14) and (15). The result is sharp. Remark 1. The coefficient bounds for |a2| and |a3| are special cases of those asserted by Theorem 1. Remark 2. In its special case when lim q→1− , Theorem 1 reduces to the result obtained in [20]. Note that there were few typographical errors in the assertion of [20, Theorem 1] and the following result is the corrected one: Corollary 1. [20, Theorem 1] Let 0 ≤ µ ≤ 1, 0 ≤ α ≤ 1, 0 ≤ β ≤ 1 and 0 ≤ λ ≤ 1. Also let φ(z) = 1 + B1z + B2z 2 + B3z 3 + . . . , where the coefficients Bn are real with B1 > 0 and B2 ≥ 0. C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 356 If f(z) given by (1) belongs to the function class Mα,β,λ(φ), then |a3 − µa22| ≤  1 4ξ ( 2B2 − ( ρ2 + 4µξ − τ ρ2 ) B2 1 ) if µ ≤ σ1, B1 2ξ if σ1 ≤ µ ≤ σ2, 1 4ξ ( −B2 + ( ρ2 + 4µξ − τ ρ2 ) B2 1 ) if µ ≥ σ2, where, for convenience, σ1 := 2ρ2(B2 −B1)− (ρ2 − τ)B2 1 4ξB2 1 , σ2 := 2ρ2(B2 +B1)− (ρ2 − τ)B2 1 4ξB2 1 , σ3 := 2ρ2B2 − (ρ2 − τ)B2 1 4ξB2 1 . ρ = α+ (1 + λ)β, ξ = α+ (1 + 2λ)β, τ = (3)α+ ( 3 + 8λ+ λ2 ) β. If σ1 ≤ µ ≤ σ3, then |a3 − µa22|+ ρ2 2ξB1 ( 1− B2 B1 + ( ρ2 + 4µξ − τ 2ρ2 ) B1 ) |a2|2 ≤ B1 2ξ . Furthermore, if σ3 ≤ µ ≤ σ2, then |a3 − µa22|+ ρ2 2ξB1 ( 1 + B2 B1 − ( ρ2 + 4µξ − τ 2ρ2 ) B1 ) |a2|2 ≤ B1 2ξ . Each of these results is sharp. Remark 3. When lim q→1− Mq,α,β,1(φ) =Mα,β(φ), Theorem 1 reduces to the result obtained by V. Ravichandran et al. [21]. Remark 4. Special case if Mq,0,1,0(φ) = Mq,1,0,λ(φ) = S∗q (φ) Theorem 1 reduces to starlike function with q-difference operator and Mq,0,1,1(φ) = Cq(φ), Theorem 1 reduces to convex function with q-difference operator which was obtained by Seoudy et al. [24]. C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 357 Remark 5. Special case if lim q→1− Mq,0,1,0(φ) = lim q→1− Mq,1,0,λ(φ) = S∗(φ) Theorem 1 re- duces to starlike function and lim q→1− Mq,0,1,1(φ) = C(φ), Theorem 1 reduces to convex function which was obtained by Ma and Minda [9]. 4. Applications to analytic functions defined by using fractional calculus operators and convolution During the past three decades, the subject of fractional calculus (that is, calculus of integrals and derivatives of any arbitrary real or complex order) has gained considerable popularity and importance. There are two most recent works on this subject of widespread investigations, namely rather comprehensive treatises on the theory, applications of frac- tional differential equations by Podlubny [15] and Kilbas et al. [10]. For the applications of the results given in the preceding sections, we first introduce the class Mδ q,α,β,λ(φ), which is defined by means of the Hadamard product (or convolution) and a certain operator of fractional calculus, known as the Owa-Srivastava operator (see, for details, [25] and [27]; see also [13], [14], and [26]). Definition 2. The fractional integral of order δ is defined, for a function f(z), by D−δz f(z) = 1 Γ(δ) z∫ 0 f(ζ) (z − ζ)1−δ dζ (δ > 0), (23) where the function f(z) be analytic in a simply connected domain of the complex z-plane containing the origin and the multiplicity of (z−ζ)δ−1 is removed by requiring that log(z−ζ) to be real when z − ζ > 0. Definition 3. The fractional integral of order δ is defined, for a function f(z), by Dδzf(z) = 1 Γ(1− δ) z∫ 0 f(ζ) (z − ζ)δ dζ (0 ≤ δ < 1), (24) where f(z) is constrained, and the multiplicity of (z− ζ)−δ is removed, as in Definition 2. Definition 4. Under the hypotheses of Definition 3, the fractional derivative of order n+δ is defined, for a function f(z), by Dn+δz f(z) = dn dzn ( Dδzf(z) ) (0 ≤ δ < 1; n ∈ N0 = N ∪ {0}). (25) Using Definitions 2, 3 and 4 of fractional derivatives and fractional integrals, Owa and Srivatsava [14] introduced what is popularly referred to in the current literature as the Owa-Srivastava operator Ωδ : A → A defined by (Ωδf)(z) := Γ(2− δ)zδDδzf(z), (δ 6= 2, 3, 4 · · · ). (26) C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 358 In terms of the Owa-Srivastava operator Ωδ defined by (26), we now introduce the function class Mδ q,α,β,λ(φ) in the following way: Mδ q,α,β,λ(φ) := {f : f ∈ A and Ωδf ∈Mq,α,β,λ(φ)}. (27) It is easily seen that the function class Mδ q,α,β,λ(φ) is a special case of the function class Mg q,α,β,λ(φ)when g(z) = z + ∞∑ n=2 Γ (n+ 1) Γ (2− δ) Γ (n+ 1− δ) zn. (28) Suppose now that g(z) = z + ∞∑ n=2 gnz n (gn > 0). Then, since f(z) = z + ∞∑ n=2 anz n ∈Mg q,α,β,λ(φ)⇐⇒ (f ∗ g)(z) = z + ∞∑ n=2 gnanz n ∈Mq,α,β,λ(φ) (29) we can obtain the coefficient estimates for functions in the class Mg q,α,β,λ(φ) from the corresponding estimates for functions in the classMq,α,β,λ(φ). By applying Theorem 1 to the following Hadamard product (or convolution): (f ∗ g)(z) = z + g2a2z 2 + g3a3z 3 + · · · , we get Theorem 3 below after an obvious change of the parameter µ. Theorem 3. Let 0 ≤ µ ≤ 1, 0 ≤ α ≤ 1, 0 ≤ β ≤ 1 and 0 ≤ λ ≤ 1. Also let φ(z) = 1 +B1z +B2z 2 +B3z 3 + . . . , where the coefficients Bn are real with B1 > 0, B2 ≥ 0 and Bn > 0 (n ∈ N\{1, 2}). If f(z) given by (1) belongs to the function class Mg q,α,β,λ(φ), then |a3 − µa22| ≤  1 2ξg3 ( 2B2 − B2 1 ρ2 γ2 ) if µ ≤ σ4, B1 ξg3 if σ4 ≤ µ ≤ σ5, 1 2ξg3 ( −2B2 + B2 1 ρ2 γ2 ) if µ ≥ σ5, where, for convenience, σ4 := g3 g22 ( 2ρ2(B2 −B1)− (ρ2 − τ)B2 1 2ξB2 1 ) , C. Ramachandran, T. Soupramanien, B.A. Frasin / Eur. J. Pure Appl. Math, 10 (2) (2017), 348-362 359 σ5 := g3 g22 ( 2ρ2(B2 +B1)− (ρ2 − τ)B2 1 2ξB2 1 ) , and γ2 := ( ρ2 + 2µξg3 g22 − τ ) (30) and ρ, ξ and τ are defined as in (13), (14) and (15), respectively. These results are sharp. Since, by (1) and the definition 4, (Ωδf)(z) = z + ∞∑ n=2 Γ (n+ 1) Γ (2− δ) Γ (n+ 1− δ) anz n, (31) we readily obtain g2 := Γ(3)Γ(2− δ) Γ(3− δ) = 2 2− δ (32) and g3 := Γ(4)Γ(2− δ) Γ(4− δ) = 6 (2− δ)(3− δ) , (33) For g2 and g3 given by (32) and (33), respectively, Theorem 3 reduces to the following interesting result. Theorem 4. Let 0 ≤ µ ≤ 1, 0 ≤ α ≤ 1, 0 ≤ β ≤ 1 and 0 ≤ λ ≤ 1. Also let φ(z) = 1 +B1z +B2z 2 +B3z 3 + . . . , where the coefficients Bn are real with B1 > 0, B2 ≥ 0. 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