Journal of Inequalities and Applications Volume 2008, Article ID 263413,10pages doi:10.1155/2008/263413
Research Article
On Harmonic Functions Defined by
Derivative Operator
K. Al-Shaqsi and M. Darus
School of Mathematical Sciences, Faculty of Science and Technology, Universiti Kebangsaan Malaysia, Bangi 43600 Selangor D. Ehsan, Malaysia
Correspondence should be addressed to M. Darus,[email protected]
Received 16 September 2007; Revised 20 November 2007; Accepted 26 November 2007
Recommended by Vijay Gupta
Let SH denote the class of functions f h
––
g that are harmonic univalent and sense-preserv-ing in the unit disk U {z : |z| < 1}, where hz z∞k2akzk, gz k∞1bkzk|b1| <
1. In this paper, we introduce the classMHn, λ, αof functionsfh
––
gwhich are harmonic inU.
A sufficient coefficient of this class is determined. It is shown that this coefficient bound is also nec-essary for the classM––
Hn, λ, αiffnz h
––
gn∈MHn, λ, α, wherehz z−∞k2|ak|zk, gnz
−1n∞
k1|bk|zkandn ∈ N0. Coefficient conditions, such as distortion bounds, convolution
con-ditions, convex combination, extreme points, and neighborhood for the classM––
Hn, λ, α, are
ob-tained.
Copyrightq2008 K. Al-Shaqsi and M. Darus. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
1. Introduction
A continuous functionf uivis a complex-valued harmonic function in a complex domain Cif bothuandvare real harmonic inC. In any simply connected domainD ⊂C, we can write
f hg, wherehandgare analytic inD. We callhthe analytic part andgthe coanalytic part off. A necessary and sufficient condition forf to be locally univalent and sense-preserving in Dis that|hz|>|gz|inD; see2.
Denote bySH the class of functionsf hg that are harmonic, univalent, and
sense-preserving in the unit diskU {z : |z| < 1}for whichf0 h0 fz0−1 0. Then for
f hg ∈ SH, we may express the analytic functionshandgas
hz z∞
k2
akzk, gz
∞
k1
Observe thatSHreduces toS, the class of normalized univalent analytic functions, if the
coan-alytic part offis zero. Also, denote byS∗H the subclasses ofSH consisting of functionsf that
mapUonto starlike domain.
Forf hg given by 1.1, we define the derivative operator introduced by authors
see1offas
Dn
λfz Dnλhz −1nDnλgz, n, λ∈N0 N∪ {0}, z∈U, 1.2
whereDnλhz z∞k2knCλ, kakzk, Dnλgz ∞k1knCλ, kbkzk, andCλ, k kλλ−1.
We letMHn, λ, αdenote the family of harmonic functionsfof the form1.1such that
Re
Dn1
λ fz
Dn
λfz
> α, 0≤α <1, 1.3
whereDnλfis defined by1.2.
If the coanalytic part off hgis identically zero, then the classMHn, λ, αturns out
to be the classRnλαintroduced by Al-Shaqsi and Darus1for the analytic case.
LetMHn, λ, αdenote that the subclass ofMHn, λ, αconsists of harmonic functions
fnhgnsuch thathandgnare of the form
hz z−∞
k2
akzk, g
nz −1n
∞
k1
bkzk. 1.4
It is clear that the class MHn, λ, αincludes a variety of well-known subclasses of SH. For
example,MH0,0, α≡ S∗Hαis the class of sense-preserving, harmonic, univalent functions
f which are starlike of order α in U, that is, ∂/∂θargfreiθ > α, and MH1,0, α ≡
MH0,1, α≡ HKαis the class of sense-preserving, harmonic, univalent functionsf which are convex of order α in U, that is, ∂/∂θarg∂/∂θfreiθ > α. Note that the classes
S∗
H and HKαwere introduced and studied by Jahangiri3. Also we notice that the class
MHn,0, αis the class of Salagean-type harmonic univalent functions introduced by Jahangiri et al.4; andMH0, λ, αis the class of Ruscheweyh-type harmonic univalent functions stud-ied by Murugusundaramoorthy and Vijaya5.
In 1984, Clunie and Sheil-Small2investigated the classSHas well as its geometric
sub-classes and obtained some coefficient bounds. Since then, there has been several related papers onSHand its subclasses such that Silverman6, Silverman and Silvia7, and Jahangiri3,8
studied the harmonic univalent functions. Jahangiri and Silverman 9 prove the following theorem.
Theorem 1.1. Letf hg given by1.1. If
∞
k2
k akbk≤1−b1, 1.5
thenfis sense-preserving, harmonic, and univalent inUandf ∈S∗Hconsists of functions inSHwhich
are starlike inU.
The condition1.5is also necessary iff∈ TH ≡MH0,0,0.
also necessary for functions in the classMHn, λ, α. Also, we obtain distortion theorems and characterize the extreme points for functions inMHn, λ, α. Closure theorems and application of neighborhood are also obtained.
2. Coefficient bounds
We begin with a sufficient coefficient condition for functions inMHn, λ, α. Theorem 2.1. Letf hg be given by1.1. If
∞
k1
k−αak kαbkknCλ, k≤21−α, 2.1
wherea1 1, n, λ ∈ N0, Cλ, k kλλ−1, and0 ≤ α < 1, thenf is sense-preserving, harmonic,
univalent inU, andf ∈MHn, λ, α.
Proof. Ifz1/z2, then
f z1
−f z2
h z1
−h z2
≥1−g z1
−g z2
h z1
−h z2
1−
∞
k1bk zk1−z k 2
z1−z2
∞k2ak zk1−zk2
>1−
∞
k1kbk 1−∞k2kak
≥1−
∞
k1 kαknCλ, k/1−αbk
1−∞k2 k−αknCλ, k/1−αak ≥0,
2.2
which proves univalence. Note thatf is sense-preserving inU. This is because
hz≥1−∞
k2
kak|z|k−1
>1−
∞
k2
k−αknCλ, k
1−α ak
≥∞
k1
kαknCλ, k
1−α bk
>∞
k1
kαknCλ, k
1−α bk|z|
k−1≥∞
k1
kbk|z|k−1≥gz.
2.3
Using the fact that Rew > αif and only if|1−αw| ≥ |1α−w|, it suffices to show that
1−αDn
SubstitutingDnλfzin2.4yields, by2.1, we obtain
1−αDn
λfz Dnλ1fz−1αDλnfz− Dλn1fz
2−αz
∞
k2
k1−αknCλ, kakzk−−1n
∞
k1
k−1αknCλ, kbkzk
−−αz∞
k2
k−1−αknCλ, kakzk −−1n
∞
k1
k1αknCλ, kbkzk
≥21−α|z|
1−∞
k2
k−αknCλ, k
1−α ak|z|
k−1∞
k1
kαknCλ, k
1−α bk|z|
k−1
≥21−α
1−
∞
k2
k−αknCλ, k
1−α ak−
∞
k1
kαknCλ, k
1−α bk
.
2.5
This last expression is nonnegative by2.1, and so the proof is complete.
The harmonic function
fz z∞
k2
1−α
k−αknCλ, kxkzk
∞
k1
1−α
kαknCλ, kykzk, 2.6
wheren, λ∈ N0and∞k2|xk|
∞
k1|yk| 1 show that the coefficient bound given by2.1is sharp. The functions of the form2.6are inMHn, λ, αbecause
∞
k1
k−α
1−αak
kα
1−αbk
knCλ, k 1
∞
k2
xk∞
k1
yk2. 2.7
In the following theorem, it is shown that the condition 2.1is also necessary for functions
fnhgn, wherehandgnare of the form1.4.
Theorem 2.2. Letfnhgnbe given by1.4. Thenfn∈MHn, λ, αif and only if
∞
k1
k−αak kαbkknCλ, k≤21−α, 2.8
wherea11, n, λ∈N0, Cλ, k kλλ−1, and0≤α <1.
Proof. SinceMHn, λ, α⊂ MHn, λ, α, we only need to prove the “if and only if” part of the
theorem. To this end, for functions fn of the form1.4, we notice that the condition 1.3is
equivalent to
Re
1−αz−∞k2k−αknCλ, kakzk−−12n∞k1kαknCλ, kbkzk
z−∞k2knCλ, kakzk −12n
∞
k1knCλ, kbkzk
The above required condition2.9must hold for all values ofzinU. Upon choosing the values ofzon the positive real axis, where 0≤zr <1, we must have
1−α−∞k2k−αknCλ, kakrk−1−
∞
k1kαknCλ, kbkrk−1 1−∞k2knCλ, kakrk−1
∞
k1knCλ, kbkrk−1
≥0. 2.10
If the condition2.8does not hold, then the numerator in2.10is negative forr sufficiently close to 1. Hence there exist z0 r0 in0,1for which the quotient in2.8is negative. This contradicts the required condition forfn∈MHn, λ, αand so the proof is complete.
3. Distortion bounds
In this section, we will obtain distortion bounds for functions inMHn, λ, α.
Theorem 3.1. Letfn∈MHn, λ, α. Then for|z|r <1, one has
fnz≤ 1b1r 1 2nλ1
1−α 2−α−
1α 2−αb1
r2,
fnz≥ 1−b1r− 1 2nλ1
1−α 2−α−
1α 2−αb1
r2.
3.1
Proof. We only prove the left-hand inequality. The proof for the right-hand inequality is similar
and will be omitted. Letfn∈MHn, λ, α. Taking the absolute value offn, we obtain
fnz
z−
∞
k2
akzk −1n
∞
k1
bkzk
≥ 1−b1r−
∞
k2
akbkrk
≥ 1−b1r−r2
∞
k2
akbk
≥ 1−b1r− 1−
α
2−α2nλ1
∞
k2
2−α2nλ1
1−α ak
2−α2nλ1
1−α bk
r2
≥ 1−b1r− 1−
α
2−α2nλ1
∞
k2
k−αknCλ, k
1−α ak
kαknCλ, k
1−α bk
r2
≥ 1−b1r−
1−α
2−α2nλ1
1−1α 1−αb1
r2.
3.2
The functions
fz zb1z 1 2nλ1
1−α 2−α−
1α 2−αb1
z2,
fz 1−b1z− 1 2nλ1
1−α 2−α−
1α 2−αb1
z2
3.3
The following covering result follows from the left-hand inequality inTheorem 3.1.
Corollary 3.2. If the functionfnhgn, wherehandggiven by1.4are inMHn, λ, α, then
w:|w|< 2
n1λ1−1− 2nλ1−1α
2nλ12−α −
2n1λ1−1− 2nλ1 1α 2nλ12−α b1
⊂fnU.
3.4
4. Convolution, convex combination, and extreme points
In this section, we show that the classMHn, λ, αis invariant under convolution and convex combination of its member.
For harmonic functions fnz z − k∞2akzk −1
n∞
k1bkz
k and F
nz z −
∞
k2Akzk −1
n∞
k1Bkz k
, the convolution offnandFnis given by
fn∗Fnz fnz∗Fnz z−
∞
k2
akAkzk −1n
∞
k1
bkBkzk. 4.1
Theorem 4.1. For 0 ≤ β ≤ α < 1, let fn ∈ MHn, λ, α and Fn ∈ MHn, λ, β. Then fn∗Fn
∈MHn, λ, α⊂MHn, λ, β.
Proof. We wish to show that the coefficients of fn∗Fn satisfy the required condition given in
Theorem 2.2. ForFn∈MHn, λ, β,we note that|Ak| ≤1 and|Bk| ≤1. Now, for the convolution
functionfn∗Fn, we obtain
∞
k2
k−βknCλ, k
1−β akAk
∞
k1
kβknCλ, k
1−β bkBk
≤∞
k2
k−βknCλ, k
1−β ak
∞
k1
kβknCλ, k
1−β bk
≤∞
k2
k−αknCλ, k
1−α ak
∞
k1
kαknCλ, k
1−α bk≤1,
4.2
since 0≤β≤α <1 andfn∈MHn, λ, α. Thereforefn∗Fn∈MHn, λ, α⊂MHn, λ, β.
We now examine the convex combination ofMHn, λ, α. Let the functionsfnjzbe defined, forj 1,2, . . . ,by
fnjz z−
∞
k2
ak,jzk −1n
∞
k1
bk,jzk. 4.3
Theorem 4.2. Let the functions fnjz defined by 4.3 be in the class MHn, λ, α for every j 1,2, . . . , m. Then the functionstjzdefined by
tjz m
j1
cjfnjz, 0≤cj ≤1 4.4
Proof. According to the definition oftj, we can write
tjz z−
∞
k2
m
j1
cjak,j
zk −1n∞ k1
m
j1
cjbn,j
zk. 4.5
Further, sincefnjzare inMHn, λ, αfor everyj1,2, . . ., then by2.8, we have
∞
k1
k−α
m
j1
cjak,j
kα m
j1
cjbk,j
knCλ, k
m
j1
cj
∞
k1
k−αan,j kαbn,jknCλ, k
≤m
j1
cj21−α≤21−α.
4.6
Hence the theorem follows.
Corollary 4.3. The classMHn, λ, αis closed under convex linear combination.
Proof. Let the functionsfnjz j 1,2defined by4.1be in the classMHn, λ, α. Then the
functionΨzdefined by
Ψz μfn1z 1−μfn2z, 0≤μ≤1 4.7
is in the classMHn, λ, α. Also, by takingm 2,t1 μ, andt2 1−μinTheorem 4.1, we have the corollary.
Next we determine the extreme points of closed convex hulls ofMHn, λ, αdenoted by clcoMHn, λ, α.
Theorem 4.4. Letfnbe given by1.4. Thenfn∈MHn, λ, αif and only if
fnz
∞
k1
Xkhkz Ykgnkz
, 4.8
where h1z z, hkz z − 1 − α/k − αknCλ, kzk, k 2,3, . . . , gnkz z
−1n1−α/kαknCλ, kzk, k 1,2,3, . . . ,and ∞k1 Xk Yk
1, Xk ≥ 0, Yk ≥ 0. In
particular, the extreme points ofMHn, λ, αarehkandgnk
.
Proof. For the functionsfnof the form4.8, we have
fnz
∞
k1
Xkhkz Ykgnkz
∞
k1
XkYkz−
∞
k2
1−α
k−αknCλ, kXkzk −1n
∞
k1
1−α
kαknCλ, kYkzk.
4.9
Then
∞
k2
k−αknCλ, k
1−α ak
∞
k1
kαknCλ, k
1−α bk
∞
k2
Xk
∞
k1
and sofn∈clcoMHn, λ, α.
Conversely, suppose thatfn∈clcoMHn, λ, α. Setting
Xk k−αk
nCλ, k
1−α ak, 0≤Xk ≤1, k 2,3, . . . ,
Yk kαk
nCλ, k
1−α bk, 0≤Yk ≤1, k1,2,3, . . . ,
4.11
andX11−∞k2Xk−
∞
k1Yk. Therefore,fncan be written as
fnz z−
∞
k2
akzk −1n
∞
k1
bkzk
z−∞
k2
1−αXk
k−αknCλ, kzk −1n
∞
k1
1−αYk
kαknCλ, kzk
z∞
k2
hkz−zXk
∞
k1
gnkz−z
Yk
∞
k2
hkzXk
∞
k1
gnkzYkz
1−
∞
k2
Xk−
∞
k1
Yk
∞
k1
hkzXkgnkzYk
, as required.
4.12
Using Corollary 4.3 we have clcoMHn, λ, α MHn, λ, α. Then the statement of Theorem 4.4is really forf ∈MHn, λ, α.
5. An application of neighborhood
In this section, we will prove that the functions in a neighborhood ofMHn, λ, αare starlike harmonic functions.
Following10, we defined theδ-neighborhood of a functionf∈ THby
Nδf
Fz z−∞
k2
Akzk−
∞
k1
Bkzk,
∞
k2
kak−Akbk−Bkb1−B1≤δ
,
5.1
whereδ >0.
Theorem 5.1. Let
δ 2−α2
nλ
1−1α− 2−α2nλ1−1−αb1
2−α2nλ1 . 5.2
Proof. Supposefn ∈ MHn, λ, α. LetFn HGn ∈ Nδ fn,where H z−∞k2Akzk and
Gn −1n∞k1Bkzk. We need to show thatFn ∈ TH. In other words, it suffices to show that
Fnsatisfies the conditionTF ∞k2k|Ak||Bk| |B1| ≤1. We observe that
TF ∞
k2
kAkBkB1
∞
k2
kAk−akakBk−bkbkB1−b1b1
∞
k2
kAk−akBk−bk
∞
k2
kakbkB1−b1b1
∞
k2
kAk−akBk−bkB1−b1
∞
k2
kakbkb1
δb1
∞
k2
kakbk
δb1 1−
α
2−α2nλ1
∞
k2
2−α 1−αak
2α 1−αbk
2nλ1
≤δb1
1−α
2−α2nλ1
∞
k2
k−α
1−αak
kα
1−αbk
knCλ, k
≤δb1 1−α
2−α2nλ1
1−1α 1−αb1
.
5.3
Now this last expression is never greater than one if
δ≤1−b1− 1−
α
2−α2nλ1
1−1α 1−αb1
2−α2
nλ1−1α− 2−α2nλ1−1−αb
1
2−α2nλ1 .
5.4
Acknowledgment
The work presented here was supported by Fundamental Research Grant Scheme UKM-ST-01-FRGS0055-2006.
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