Abstract
The main idea of the study on coefficient problems in various classes of analytic functions (univalent or nonunivalent) is to express the coefficients of functions in a given class by the coefficients of corresponding functions with positive real part. Thus, coefficient functionals can be studied using inequalities known for the class \({\mathcal {P}}\). Lemmas obtained by Libera and Złotkiewicz and by Prokhorov and Szynal play a special role in this approach. Recently, a new way leading to results on coefficient functionals has been pointed out. This approach is based on relating the coefficients of functions in a given class and the coefficients of corresponding Schwarz functions. In many cases, if we follow this approach, it is easy to predict the exact estimate of the functional and make the appropriate computations. In the proofs of these estimates are used not only classical results (the Schwarz–Pick Lemma or Wiener’s inequality), but also inequalities obtained either recently (e.g. by Efraimidis) or long ago yet almost forgotten (Carlson’s inequality). In this paper, a number of coefficient problems will be solved using the new approach described above. The object of our study is the class of starlike functions with respect to symmetric points associated with the exponential function.
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1 Introduction
Let \({\mathbb {D}}\) be the unit disk \(\{z\in {\mathbb {C}}:|z|<1\}\) and \({\mathcal {A}}\) be the family of all functions f analytic in \({\mathbb {D}}\), normalized by the condition \(f(0)=f'(0)-1=0\). It means that f has the expansion
Let also \({\mathcal {B}}_0\) be the class of Schwarz functions, i.e., analytic functions \(\omega :{\mathbb {D}}\rightarrow {\mathbb {D}}\), \(\omega (0)=0\). The function \(\omega \in {\mathcal {B}}_0\) can be written as a power series
For given analytic functions f and g in \({\mathbb {D}}\), we say that f is subordinate to g in \({\mathbb {D}}\) and write \(f\prec g\) if there exists \(\omega \in {\mathcal {B}}_0\) such that
Moreover, if the function g is univalent in \({\mathbb {D}}\), then \(f\prec g\) if and only if \(f(0) = g(0)\) and \(f({\mathbb {D}})\subset g({\mathbb {D}})\).
Let \({\mathcal {S}}_S^*\) denote the class of functions which are starlike with respect to the symmetric points. A function f is in \({\mathcal {S}}_S^*\) if
where
If the function \(\varphi _0(z)\) is replaced by any analytic univalent function \(\varphi\) with positive real part in \({\mathbb {D}}\) and symmetric with respect to the real axis, then we obtain the class \({\mathcal {S}}_S^*(\varphi (z))\).
In this paper, we consider the class \({\mathcal {S}}_S^*(\varphi (z))\) with \(\varphi (z)=e^z\). Hence, we can write
This class was first discussed by Ganesh et al. in [3], where some coefficients functionals were estimated. The majority of results were not sharp. The main tool used to obtain those results was a lemma proved by Libera and Złotkiewicz.
In this paper, we follow a new approach which is based on relating the coefficients of functions in a given class and the coefficients of corresponding Schwarz functions. In many cases, it is easy to predict the exact estimate of the functional and make the appropriate computations. It is the case for the class \({\mathcal {S}}_S^*(e^z)\). By applying the lemmas proved by Libera and Złotkiewicz and by Prokhorov and Szynal as well as some other tools, and by performing the calculus more precisely, we are able to derive better estimates, almost all of them being sharp.
To prove our results, we need the following lemmas for Schwarz functions. The first one is the above-mentioned result obtained by Prokhorov and Szynal.
Lemma 1
([5]) Let \(\omega (z)=c_{1}z+c_{2}z^{2}+\cdots\) be a Schwarz function. Then, for any real numbers \(\mu\) and \(\nu\) such that
the following sharp estimate holds
From the Schwarz–Pick Lemma, it follows that for \(\omega \in {\mathcal {B}}_0\) of the form (1.2),
This inequality can be improved (see, for example, [2]) as follows. For any \(\lambda \in {\mathbb {C}}\),
Carlson in [1] obtained another generalization of the Schwarz–Pick Lemma. Here, we state only these inequalities which are useful for our purpose (for all details, see [7]).
Lemma 2
( [1]) Let \(\omega (z)=c_{1}z+c_{2}z^{2}+\cdots\) be a Schwarz function. Then,
The above lemma immediately results in the following fact.
Lemma 3
Let \(\omega (z)=c_{1}z+c_{2}z^{2}+\cdots\) be a Schwarz function. Then
We also need the results obtained by Efraimidis.
Lemma 4
([2]) Let \(\omega (z)=c_{1}z+c_{2}z^{2}+\cdots\) be a Schwarz function and \(\lambda \in {\mathbb {C}}\). Then
and
The method used by Efraimidis in the proof of his lemma has much greater potential. Based on this method, we can obtain some inequalities involving the fifth coefficient of \(\omega \in {\mathcal {B}}_0\) (see also [6]).
Lemma 5
If \(\omega \in {\mathcal {B}}_0\) is of the form (1.2) and \(\mu \in {\mathbb {C}}\), \(|\mu |\le 1\), then
2 Coefficient bounds
We start with the coefficients of \(f\in {\mathcal {S}}_S^*(e^z)\). Applying in
the expansions of f and \(\omega\) given by (1.1) and (1.2), we obtain
From [3], it is known that if \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then \(|a_2|\le \tfrac{1}{2}\) and \(|a_3|\le \tfrac{1}{2}\).
Theorem 1
If \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then
The bounds are sharp.
Proof
Lemma 1 with \(\mu =\tfrac{3}{2}\) and \(\nu =\tfrac{5}{12}\) applied to
results in the first inequality.
To prove the second inequality, we can write
From (1.4) with \(\lambda =1\), the first component is bounded by 1/2. By Lemma 2, the second component, can be estimated as follows
Combining the estimates of both components of (2.3), we get \(|a_5|\le \tfrac{1}{4}\).
If \(c_3=1\) and \(c_k=0\) for \(k\ne 3\), then \(a_4=\tfrac{1}{4}\). Similarly, if \(c_4=1\) and \(c_k=0\) for \(k\ne 4\), then \(a_5=\tfrac{1}{4}\). This means that the equalities in the assertion of this theorem hold for the functions given by (2.1) with \(\omega (z)=z^3\) and \(\omega (z)=z^4\), respectively. \(\square\)
The logarithmic coefficients of a given univalent function f, denoted by \(\gamma _n=\gamma _n(f)\), are defined as
If f is given by (1.1), then its logarithmic coefficients are given as follows
The sharp bounds of \(\gamma _k\), \(k=1,2,3,4,5\) are established in the next theorem.
Theorem 2
If \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then
The bounds are sharp.
Proof
Applying (2.2) in (2.5), we have
The bounds of \(\gamma _1\) and \(\gamma _2\) are clear. The result for \(\gamma _3\) immediately follows from Lemma 1 with \(\mu =\tfrac{1}{2}\) and \(\nu =\tfrac{1}{12}\).
Observe that
Indeed, from (1.4) with \(\lambda =0\),
which is clearly less than or equal to 1/2.
For \(\gamma _5\), we have
The bound of the first component follows from (1.6) with \(\mu =0\). The triangle inequality and Lemma 2 result in
The above expression takes its greatest value with respect to \(|c_3|\) when \(|c_3|=\tfrac{1}{4}(|c_2|+|c_1|^2)(1+|c_1|)\), so
Since \(|c_1|^3|c_2|\le |c_1|^2|c_2|\), we can write
where \(c=|c_1|\), \(d=|c_2|\) and
The shape of the region of variability of (c, d) is a simple consequence of the Schwarz–Pick Lemma. It coincides with
It is not difficult to show that (0, 0) is the only critical point of h in \(\varOmega\). Consequently, it is enough to derive the greatest value of h on the boundary of \(\varOmega\). But,
Since \(\tfrac{5}{4} (c^2-c^4)\le \tfrac{5}{16}\) and \(\tfrac{5}{16}(c-2c^3+c^5)\le \tfrac{\sqrt{5}}{25}\) we conclude that
Combining all these inequalities, we get
which results in the desired bound.
Observe that we obtain equalities in each bound of \(\gamma _k\), \(k=1,2,3,4,5\) when \(\omega (z)=z^k\). This means that the obtained estimates are sharp. \(\square\)
3 Estimates of Zalcman functionals and Hankel determinants
It is known ([3]) that if \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then \(|a_3-a_2^2|\le \tfrac{1}{2}\). This functional, known as the Fekete–Szegö functional, is a particular case of the Zalcman functional \(a_{n+m-1}-a_na_m\). Let us consider other cases of the Zalcman functional.
The estimate of \(a_{4}-a_2a_3\) is a simple consequence of Lemma 1. Namely,
so taking \(\mu =\tfrac{1}{2}\) and \(\nu =-\tfrac{1}{12}\) in Lemma 1 yields
To estimate \(a_{5}-a_3^2\), we write this expression as follows
Applying (1.5) with \(\lambda =-\tfrac{1}{2}\), the first component is bounded by 1/2. To estimate the other, we use the triangle inequality and Lemma 2. Hence
so
Considering \(\omega (z)=z^3\) and \(\omega (z)=z^4\), we can observe that the estimates of the two cases of the Zalcman functional are sharp. We have proved what follows.
Theorem 3
If \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then the following sharp bounds hold
Let us turn to Hankel determinants for the class \({\mathcal {S}}_S^*(e^z)\). The first result is easy to obtain.
Theorem 4
If \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then
Proof
If \(f\in {\mathcal {S}}_S^*(e^z)\), then
Since
and
is a decreasing function, we conclude that
This and Lemma 3 result in the declared bound of \(H_{2,2}\).
Furthermore, \(|H_{2,2}| = \tfrac{1}{4}\) if \(c_2=1\) and \(c_k=0\) for \(k\ne 2\), i.e. if \(\omega (z)=z^2\). \(\square\)
Theorem 5
If \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), the following sharp bound holds
Proof
Assume that \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1). Then
By the triangle inequality and Lemma 2,
Let \(h(|c_1|,|c_2|)\) denote the right hand side of the above inequality and let \(c=|c_1|\), \(d=|c_2|\). Since
replacing \(d^2\) by d and omitting \(c^4\) in the last component, we get
with
A straightforward algebraic computation shows that the critical points of g satisfy
so in \(\varOmega\) given by (2.7), there is only one critical point \((c_0,d_0)\) where \(c_0=0.345\ldots\) and \(d_0=0.722\ldots\). For this point,
On the boundary of \(\varOmega\), we have
It is a simple task to show that \(12-24c+3c^2+19c^3>0\) in [0, 1], so
This means that
Consequently,
The function \(h(c,1-c^2)\) is decreasing for \(c\in [0,1]\), so
Similarly as in Theorem 4, the equality \(|H_{2,3}| = \tfrac{1}{8}\) holds if \(c_2=1\) and \(c_k=0\) for \(k\ne 2\), i.e. if \(\omega (z)=z^2\). \(\square\)
Theorem 6
If \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then
Proof
If \(f\in {\mathcal {S}}_S^*(e^z)\), then
At the beginning, it should be noted that
by Lemma 1 with \(\mu =-1\) and \(\nu =-\tfrac{1}{6}\). Under Lemma 2,
Applying it and \(|c_4|\le 1-|c_1|^2 -|c_2|^2\), we get
where
But h is a decreasing function of the variable c; consequently,
The function h(0, d) achieves its greatest value in [0, 1] if \(d=1/2\), so \(h(0,d)\le \tfrac{13}{8}\), which completes the proof. \(\square\)
This result is not sharp. Based on Formula (3.1), it is expected that the sharp bound of \(|H_{3,1}|\) is equal to \(\tfrac{1}{16}\).
The method used in the proof of Theorem 2 for the bound \(|\gamma _5|\le \tfrac{1}{12}\) may be adopted to prove that if \(f\in {\mathcal {S}}_S^*(e^z)\) is of the form (1.1), then \(|a_6-a_2a_5|\le \tfrac{1}{6}\). This result is also sharp. Unfortunately, the sharp bound of \(a_6\) has not been obtained. From (2.2), we can only obtain that
with an obvious conjecture that the exact value of the bound is equal to 1/6.
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Zaprawa, P. On coefficient problems for functions starlike with respect to symmetric points. Bol. Soc. Mat. Mex. 28, 17 (2022). https://doi.org/10.1007/s40590-022-00409-8
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DOI: https://doi.org/10.1007/s40590-022-00409-8
Keywords
- Coefficient problems
- Logarithmic coefficients
- Zalcman functionals
- Hankel determinants
- Starlike functions