Applied Mathematics
Vol.5 No.7(2014), Article ID:44806,8 pages DOI:10.4236/am.2014.57099
A New Look for Starlike Logharmonic Mappings
Zayid Abdulhadi
Department of Mathematics, American University of Sharjah, Sharjah, UAE
Email: zahadi@aus.edu
Copyright © 2014 by author and Scientific Research Publishing Inc.
This work is licensed under the Creative Commons Attribution International License (CC BY).
http://creativecommons.org/licenses/by/4.0/
Received 25 November 2013; revised 25 December 2013; accepted 2 January 2014
ABSTRACT
A function f(z) defined on the unit disc U is said to be logharmonic if it is the solution of the nonlinear elliptic partial differential equation where
such that
. These mappings admit a global representation of the form
where
In this paper,we shall consider the logharmonic mappings
, where
is starlike. Distortion theorem and radius of starlikess are obtained. Moreover, we use star functions to determine the integral means for these mappings. An upper bound for the arclength is included.
Keywords:Logharmonic, Univalent, Starlike, Integral Means, Arclength
1. Introduction
Let B denote the set of all analytic functions defined on the unit disk
having the property that
for all
A logharmonic mapping defined on the unit disk
is a solution of the nonlinear elliptic partial differential equation
(1.1)
where the second dilatation function. Because
the Jacobian
is positive and hence, non-constant logharmonic mappings are sense-preserving and open on U. If f is a nonconstant logharmonic mapping of and vanishes at
but has no other zeros in U, then f admits the following representation
(1.2)
where m is a nonnegative integer, and,
and
are analytic functions in
with
and
([1] ). The exponent
in (1.2) depends only on
and can be expressed by
Note that if and only if
and that a univalent logharmonic mapping on
vanish at the origin if and only if
. Thus, a univalent logharmonic mappings on
which vanishes at the origin will be of the form
where and
and have been studied extensively in the recent years, see [1] -[7] . In this case, it follows that
are univalent harmonic mappings of the half-plane
a detail study of univalent harmonic mappings to be found in [8] -[14] . Such mappings are closely related to the theory of minimal surfaces, see [15] [16] .
Let be a univalent logharmonic mapping. We say that
is starlike logharmonic mapping if
for all. Denote by
the set of all starlike logharmonic mappings, and by
the set of all starlike analytic mappings. It was shown in [4] that
if and only if
It is rather a natural question to ask whether there exists a linkage between the starlikeness of and
In Section 2, we determine the radius of starlikeness for the logharmonic mapping where
A distortion theorem and an upper bound for the arclength of these mappings will be included.
In Section 3, we discuss the integral means for logharmonic mappings associated to starlike analytic mappings.
2. Basic Properties of Mappings from
We start this section by establishing a linkage between the starlikeness of and
Theorem 1 a) Let be a logharmonic mapping where
Then f maps the disk
, where
onto a starlike domain.
b) If. Then
maps the disk
, where
onto a starlike domain.
Proof. a) Let be a logharmonic mapping with respect to
and
Suppose that
Then
can be written in the form
(2.1)
A simple calculations leads to
where Since
and
we obtain
This gives
Thus if
Therefore, the radius of starlikeness
is the smallest positive root (less than 1) of
which is
We conclude that f is univalent in
and maps the disk
onto a starlike domain.
b) Let be a starlike logharmonic mapping defined on the unit disk
with respect to
with Then by [4]
and also,
Hence,
and then simple calculations give that
Thus if
Therefore, the radius of starlikeness
is the smallest positive root (less than 1) of
which is
We conclude that
is univalent in
and maps the disk
onto a starlike domain.
Our next result is a distortion theorem for the set of all logharmonic mappings where
Theorem 2 Let be a logharmonic mapping defined on the unit disk U where
then for
i)
ii)
iii)
Equality holds for the right hand side if and only if and
which leads to
where
Proof. i) Let be a logharmonic mapping with respect to
with
Suppose that
Then
can be written in the form
(2.2)
For we have
(2.3)
and
(2.4)
Combining (2.2), (2.3) and (2.4), we get
Equality holds for the right hand side if and only if and
which leads to
For the left hand side inequality, we have
ii) and iii) Differentiation in (2.2) with respect to
and
respectively leads to
(2.5)
and
(2.6)
The result follows from substituting from Theorem 2(i), (2.3) and (2.4) into (2.5) and (2.6).
In the next theorem we establish an upper bound for the arclength of the set of all logharmonic mappings where
Theorem 3 Let be a logharmonic mapping defined on the unit disk U where
Suppose that for
then
Proof. Let denote the closed curve which is the image of the circle
under the mapping
. Then
Now using (2.5) and (2.6) we have
Therefore,
(2.7)
(2.8)
Since is harmonic, and by the mean value theorem for harmonic functions,
Also,
is subordinate to
therefore, we have
Substituting the bounds for and
in (2.8), we get
3. Integral Means
Theorem 4 of this section is an applications of the Baerstein star functions to the class of logharmonic mappings defined on the unit disk
where
. Star function was first introduced and properties were derived by Baerstein [17] [18] , [Chapter 7]. The first application was the remarkable result, if
then
(3.1)
where,
and
If is a real
function in an annulus
then the definition of the star function of
,
is
One important property is that when is symmetric (even) re-arrangement then
(3.2)
Other properties [18] , [Chapter 7] are that the star-function is sub-additive and star respects subordination. Respect means that the star of the subordinate function is less than or equal to the star of the function. In addition, it was also shown that star-function is additive when functions are symmetric re-arrangements. Here is a lemma, quoted in [18] , [Chapter 7] which we will use later.
Lemma 1 For real and
on
the following are equivalent a) For every convex non-decreasing function
b) For every
c) For every
Our main result of this section is the following theorem.
Theorem 4 If be a logharmonic mapping defined on the unit disk U where
then for each fixed
and as a function of
Equality occurs if and only if is one of the functions of the form
,
, where
Proof. Let, then by (2.2), we have
where and
Then
(3.3)
Write where
is analytic,
and
(see [9] ).
As the star-function is sub-additive,
(3.4)
But since
each is subharmonic. is subordinate to
and
is subordinate to
Hence
and
Then,
Thus,
It follows that
(3.5)
Consequently, by combining (3.4), (3.5) and using the fact that star-functions respect subordination, it follows that
Hence, as star-functions are additive when functions are symmetric re-arrangements,
(3.6)
Now by using Theorem 4 we have Corollary 1 If be a logharmonic mapping defined on the unit disk U where
then
and
the later implies that hence
has radial limits.
Proof. Let this is non-decreasing convex function .The first integral mean can be obtained using part (a) of Lemma 1 and Theorem 4. Moreover, the choice
yields the second integral mean.
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