On Certain Subclass of Analytic Functions Based on Convolution of Ruscheweyh and Generalized Salagean Differential Operator ()

1. Introduction and Definitions
Let
denote the class of analytic functions of the form
(1)
which are analytic in the open unit disk
and normalized by
. Let S be the subclass of
consisting of analytic univalent function of the form (1.1).
The study of normalised analytic univalent functions is enhanced by the used of operators, mostly, differential and integral operators. In this study, we have implored the used of convulation of well known differential operators to defined our class. For more works on operators see [1] [2] [3] .
Definition 1
Let T denotes the subclass of S consisting of functions of the form
(2)
Further we define the class
by
(3)
Definition 2 ( [4] )
For
and
of the form (1.1)
and
, the operator
is defined by
i.e.
(4)
Definition 2 [3] Let
, the operator
is defined by
Thus it is obvious to see from above that
(5)
where
Thus by convolution as earlier defined by [5] we have
(6)
We now defined a class
, which consist of functions
such that the following inequality is satisfy
Motivated here by the works of [1] [6] , we characterize our class using well know existing geometric properties.
2. Properties of the Class
2.1. Coefficient Inequality
Theorem 2.1.
let
. Then
if and only if
(7)
where
Proof:
Supposed the inequality (7) holds true and
, then we have
But by maximun modullus principle,
establishing our desired result.
Conversely,
Let
, then
(8)
Then
Recall that
, thus we have
(9)
Choose z on the real axis and let
. Then we have
(10)
This yields;
(11)
This establishes our proof.
Corollary 2.1.
If
then
(12)
equality is attained for
(13)
We shall state the growth and distortion theorems for the class
The results of which follow easily on applying Theorem 2.1, therefore, we deem it necessary to omit the trivial proofs.
2.2. Growth and Distortion Theorems
Theorem 2.2.
Let the function
then for
Theorem 2.3.
Let the function
then for
When
we obtain a sharp result.
2.3. Radii of Close-to-Convexity, Starlikeness and Convexity
Theorem 2.4.
Let the function
, then
is close-to-convex of order
in
where
The result obtained is sharp.
Proof.
It is sufficient to show that
for
Thus we can write
Therefore
if
(14)
But we have from theorem 2.1. that
(15)
Relating (14) and (15) we have our desired result.
Theorem.2.5.
Let the function
, then
is starlike of order
,
in
where
The result obtain here is sharp.
Proof.
We must show that
for
. Equivalently, we have
(16)
But we have from theorem 2.1. that
(17)
Relating (16) and (17) will have our desired result.
Theorem 2.6.
Let the function
, then
is convex of order
,
in
where
The result obtain here is sharp.
Proof.
By using the technique of theorem 2.5 we easily show that
this holds for
. The analogous details of theorem 2.5 are thus omitted, hence the proof.
3. Integral Operator
Theorem 3.1.
Let the function
defined by (2) be in the class
and let
be a real number such that
. Then the function defined by
(18)
also belong to the class
Proof.
From the representation and definition of
we have that
(19)
where
(20)
Thus we have
(21)
(22)
since
. By theorem 1.1
. This establishes our proof.