Abstract
Let \(\mathcal {H}\) be the class of harmonic functions \(f=h+\overline{g}\) in the unit disk \(\mathbb {D}:=\{z\in \mathbb {C}:|z|<1\}\), where h and g are analytic in \(\mathbb {D}\). In 2020, N. Ghosh and V. Allu introduced the class \(\mathcal {P}_{\mathcal {H}}^0(M)\) of normalized harmonic mappings defined by \(\mathcal {P}_{\mathcal {H}}^0(M)=\{f=h+\overline{g}\in \mathcal {H}: \text {Re}(zh''(z))>-M+|zg''(z)|\;\text {with}\;M>0, g'(0)=0, z\in \mathbb {D}\}\). In this paper, we investigate various geometric properties such as starlikeness, convexity, convex combination and convolution for functions in the class \(\mathcal {P}_{\mathcal {H}}^0(M)\). Furthermore, we determine the sharp Bohr–Rogosinski radius, improved Bohr radius and refined Bohr radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\).
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1 Introduction and Preliminaries
The classical inequality of Bohr says that if f is an analytic function in the unit disk \(\mathbb {D}:=\{z\in \mathbb {C}:|z|<1\}\) with the following Taylor series expansion
such that \(|f(z)|<1\) in \(\mathbb {D}\). Then
Here 1/3 is known as Bohr radius and it can’t be improved, while the inequality (1.2) is known as Bohr inequality. In 1914, H. Bohr [10] obtained the inequality (1.2) for \(r\le 1/6\) but later Weiner, Riesz and Schur [12] independently improved it to 1/3. An observation shows that the quantity \(1-|a_0|\) is equal to \(d\left( f(0), \partial \mathbb {D}\right) \), where d is the Euclidean distance and \(\partial \mathbb {D}\) is the boundary of \(\mathbb {D}\). Therefore, the inequality (1.2) also can be written as
It is important to note that the constant 1/3 is independent of the coefficients of the Taylor series (1.1). This fact can be elucidated by saying that Bohr inequality occurs in the class \(\mathcal {B}\) of analytic self maps of the unit disk \(\mathbb {D}\). Analytic functions \(f\in \mathcal {B}\) of the form (1.1) satisfying the inequality (1.2) for \(|z|=r\le 1/3\), are said to satisfy the classical Bohr phenomenon. The concept of Bohr phenomenon can be generalized to the class \(\mathcal {A}\) consisting of analytic functions of the form (1.1) which map from \(\mathbb {D}\) into a given domain \(\Theta \subseteq \mathbb {C}\) such that \(f(\mathbb {D})\subseteq \Theta \). The class \(\mathcal {A}\) is said to satisfy the Bohr phenomenon if \(\exists \) largest radius \(r_{\Theta }\in (0, 1)\) such that (1.3) holds for \(|z|=r \le r_{\Theta }\). Here \(r_{\Theta }\) is known as Bohr radius for the class \(\mathcal {A}\). The Bohr radius has been obtained for the class \(\mathcal {A}\) when \(\Theta \) is convex domain [4], simply connected domain [1], the exterior of the closed unit disk, the punctured unit disk, and concave wedge domain (see [5]). In 1997, Boas and Khavinson [9] generalized the Bohr inequality in several complex variables by finding multidimensional Bohr radius. In 2021, Liu and Ponnusamy [22] obtained multidimensional analogues of refined Bohr inequality.
There are many improved versions of Bohr’s inequality (1.2) in various forms obtained by several authors. In 2020, Kayumov and Ponnusamy [20] obtained several interesting improved versions of Bohr inequality. For more results on this, we refer the reader to glance through the articles (see [16,17,18,19,20,21, 23, 24]). In 2017, Kayumov and Ponnusamy [18] introduced Bohr–Rogosinski radius motivated by Rogosinski radius for bounded analytic functions in \(\mathbb {D}\). Rogosinski radius is defined as follows: Let \(f(z)=\sum _{n=0}^{\infty }a_nz^n\) be analytic in \(\mathbb {D}\) and its corresponding partial sum of f is defined by \(S_N(z):=\sum _{n=0}^{N-1}a_nz^n\). Then, for every \(N\ge 1\), we have \(|\sum _{n=0}^{N-1}a_nz^n|<1\) in the disk \(|z|<1/2\) and the radius 1/2 is sharp. Motivated by Rogosinski radius, Kayumov and Ponnusamy have considered the Bohr–Rogosinski sum \(R_N^f(z)\) which is defined by
It is worth to point out that \(|S_N(z)|=\left| f(z)-\sum _{n=N}^{\infty }a_nz^n\right| \le R_N^f(z)\). Therefore, it is easy to see that the validity of Bohr-type radius for \(R_N^f(z)\), which is related to the classical Bohr sum (Majorant series) in which f(0) is replaced by f(z), gives Rogosinski radius in the case of bounded analytic functions in \(\mathbb {D}\). We have the following interesting results by Kayumov and Ponnusamy [18].
Theorem A
[18] Let \(f(z)=\sum _{n=0}^{\infty } a_nz^n\) be analytic in \(\mathbb {D}\) and \(|f(z)|\le 1\). Then
for \(|z|=r\le R_N\), where \(R_N\) is the positive root of the equation \(\psi _N(r)=0\), \(\psi _n(r)=2(1+r)r^N-(1-r)^2\). The radius \(R_N\) is the best possible. Moreover,
for \(R_N'\), where \(R_N'\) is the positive root of the equation \((1+r)r^N-(1-r)^2=0\). The radius \(R_N'\) is the best possible.
In 2020, Kayumov and Ponnusamy [20] have proved the following several improved versions of Bohr’s inequality for analytic functions.
Theorem B
[20] Let \(f(z)=\sum _{n=0}^{\infty } a_nz^n\) be analytic in \(\mathbb {D}\), \(|f(z)|\le 1\) and \(S_r\) denotes the area of the image of the subdisk \(|z|<r\) under mapping f. Then
and the numbers 1/3, 16/9 cannot be improved. Moreover,
and the numbers 1/2, 9/8 cannot be improved.
In 2020, Ponnusamy et al. [23] established the following refined Bohr inequality by applying a refined version of the coefficient inequalities.
Theorem C
[23] Let \(f(z)=\sum _{n=0}^{\infty } a_nz^n\) be analytic in \(\mathbb {D}\) and \(|f(z)|\le 1\). Then
for \(r\le 1/(2+|a_0|)\) and the numbers \(1/(1+|a_0|)\) and \(1/(2+|a_0|)\) cannot be improved. Moreover,
for \(r\le 1/2\) and the numbers \(1/(1+|a_0|)\) and 1/2 cannot be improved.
Bohr’s phenomenon for the complex-valued harmonic mappings have been studied extensively by many authors (see [1, 2, 6, 7]). Improved Bohr inequality for locally univalent harmonic mappings have been discussed by Evdoridis et al. [13].
A complex-valued function \(f=u+iv\) is harmonic if u and v are real-harmonic in \(\mathbb {D}\). Every harmonic function f has the canonical representation \(f=h+\overline{g}\), where h and g are analytic in \(\mathbb {D}\) known respectively as the analytic and co-analytic parts of f. A locally univalent harmonic function f is said to be sense-preserving if the Jacobian of f, defined by \(J_f(z):=|h'(z)|^2-|g'(z)|^2\), is positive in \(\mathbb {D}\) and sense-reversing if \(J_f(z)\) is negative in \(\mathbb {D}\). Let \(\mathcal {H}\) be the class of all complex- valued harmonic functions \(f=h+\overline{g}\) defined in \(\mathbb {D}\), where h and g are analytic in \(\mathbb {D}\) such that \(h(0)=h'(0)-1=0\) and \(g(0)=0\). If the co-analytic part \(g(z) \equiv 0\) in \(\mathbb {D}\), then the class \(\mathcal {H}\) reduces to the class \(\mathcal {A}\) of analytic functions in \(\mathbb {D}\) with \(f(0)=0\) and \(f'(0)=1\). A function \(f\in \mathcal {H}\) is said to be in \(\mathcal {H}_0\) if \(g'(0)=0\). Thus, every \(f=h+\overline{g}\in \mathcal {H}_0\) has the following form
A domain \(\Omega \) is called starlike with respect to a point \(z_0\in \Omega \) if the line segment joining \(z_0\) to any point in \(\Omega \) lies in \(\Omega \). In particular, if \(z_0=0\), then \(\Omega \) is simply called starlike. A complex-valued harmonic mapping \(f\in \mathcal {H}\) is said to be starlike if \(f(\mathbb {D})\) is starlike. We denote the class of harmonic starlike functions in \(\mathbb {D}\) by \(\mathcal {S}_{\mathcal {H}}^*\). A domain \(\Omega \) is called convex if it is starlike with respect to every point in \(\Omega \). A function \(f\in \mathcal {H}\) is said to be convex if \(f(\mathbb {D})\) is convex. We denote \(\mathcal {K}_{\mathcal {H}}\) by the class of harmonic convex mappings in \(\mathbb {D}\).
Definition A
The polylogarithm \(Li_s(z)\), also known as Jonquière’s function, is a special function of order s and argument z
defined in the complex plane over the unit disk. The special case \(s=1\) involves the ordinary natural logarithm, \(Li_1(z)=-\ln (1-z)\), while the special cases \(s=2\) and \(s=3\) are called the dilogarithm (also known as Spence’s function) and trilogarithm respectively.
In 2020, Ghosh and Allu [14] considered the following class for \(M>0\),
The organization of this paper is: In Sect. 3, we discuss some geometric properties for functions in the class \(\mathcal {P}_{\mathcal {H}}^0(M)\). In Sect. 4, we obtain sharp Bohr–Rogosinski radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\). In Sect. 5, we establish interesting sharp improved Bohr radius \(\mathcal {P}_{\mathcal {H}}^0(M)\). In Sect. 6, we prove sharp refined Bohr radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\). The rest sections are for lemmas and proofs of the main results.
2 Some Lemmas
We have the following lemmas related to coefficient bounds and growth estimates for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\).
Lemma 2.1
[14] The harmonic map \(f=h+\overline{g}\) belongs to \(\mathcal {P}_{\mathcal {H}}^0(M)\) if and only if the function \(F_\epsilon =h +\epsilon g\) belongs to \(\mathcal {P}(M\)) for \(|\epsilon |=1\), where \(\mathcal {P}(M)\) is defined by
Lemma 2.2
[14] Let \(f \in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(M>0\) be given by (1.10). Then for each \(n\ge 2\), we have \(|b_n|\le \frac{2M}{n(n-1)}\). The result is sharp with \(f(z)=z-\frac{M}{n(n-1)}\overline{z^n}\) being extremal.
Remark 2.1
We have found some typographical error in Lemma 2.2 of [14] and the correct statement is given below:
If \(f \in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(M>0\) is given by (1.10). Then for each \(n\ge 2\), we have \(|b_n|\le \frac{M}{n(n-1)}\). The result is sharp with \(f(z)=z-\frac{M}{n(n-1)}\overline{z^n}\) being extremal.
Lemma 2.3
[14] Let \(f \in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(M>0\) be given by (1.10). Then for any \(n\ge 2\), we have (i) \(|a_n|+|b_n|\le \frac{2M}{n(n-1)}\); (ii) \(\left| |a_n|-|b_n|\right| \le \frac{2M}{n(n-1)}\); (iii) \(|a_n|\le \frac{2M}{n(n-1)}\).
The result is sharp for the function f given by \(f'(z)=1-2M\ln (1-z)\).
Lemma 2.4
[7, 14] Let \(f=h+\overline{g}\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(M>0\) be given by (1.10). Then
Both the inequalities are sharp for the function \(f_M=z+2M\sum _{n=2}^\infty \frac{1}{n(n-1)}z^n\).
To prove our convolution results, we need the following definitions and lemmas.
Definition 2.1
[11, 25] Let \(\psi _1\) and \(\psi _2\) be two analytic functions in \(\mathbb {D}\) given by \(\psi _1(z)=\sum _{n=0}^{\infty }a_nz^n\) and \(\psi _2(z)=\sum _{n=0}^{\infty }b_nz^n\). The convolution (or, Hadamard product) is defined by
Definition 2.2
[15] For harmonic functions \(f_1=h_1+\overline{g_1}\) and \(f_2=h_2+\overline{g_2}\) in \(\mathcal {H}\), the convolution is defined as \(f_1*f_2=h_1*h_2+\overline{g_1*g_2}\).
Definition 2.3
[25] A sequence \(\{a_n\}\) of non-negative numbers is said to be a convex null sequence if \(a_n\rightarrow 0\) as \(n\rightarrow \infty \) and \(a_0-a_1\ge a_1-a_2\ge \cdots \ge a_{n-1}-a_n\ge \cdots \ge 0\).
Lemma 2.5
[25] Let \(\{a_n\}\) be a convex null sequence. Then the function p given by \(p(z)=\frac{a_0}{2}+\sum \limits _{n=1}^{\infty } a_nz^n\) is analytic in \(\mathbb {D}\) and \(\text {Re}(p(z))>0, z\in \mathbb {D}\).
Lemma 2.6
[25] Let the function p be analytic in \(\mathbb {D}\) with \(p(0)=1\) and \(\text {Re}\;p(z)>\frac{1}{2}\) in \(\mathbb {D}\). Then for any analytic function f in \(\mathbb {D}\), the function \(p*f\) takes values in the convex hull of the image of \(\mathbb {D}\) under f.
Lemma 2.7
Let \(\mathcal {P}(M)\) be the subclass of \(\mathcal {A}\) defined in (2.1). If \(F\in \mathcal {P}(M)\) with \(0<M\le \frac{3}{5}\). Then \(\text {Re}\left( \frac{F(z)}{z}\right) >\frac{1}{2}\).
Proof
Let \(F\in \mathcal {P}(M)\) be given by \(F(z)=z+\sum \limits _{n=2}^\infty A_nz^n\). Then, we have
Let \(p(z)=1+\frac{1}{2M}\sum \nolimits _{n=2}^\infty n(n-1)A_nz^{n-1}\). Then \(p(0)=1\) and \(\text {Re}(p(z))>\frac{1}{2}\) in \(\mathbb {D}\). Now, we consider a sequence \(\{c_n\}\) defined by \(c_0=1\) and \(c_{n-1}=\frac{2M}{n(n-1)}\) for \(n\ge 2\). It is clear that \(c_n\rightarrow 0\) as \(n\rightarrow \infty \). Note that \(c_0-c_1=1-M\) and \(c_1-c_2=2\,M/3\). So \(c_0-c_1\ge c_1-c_2\ge \cdots \ge c_{n-1}-c_n\ge \cdots \ge 0\) is possible only when \(0<M\le 3/5\). Thus \(\{c_n\}\) is a convex null sequence. In view of Lemma 2.5, the function
is analytic in \(\mathbb {D}\) with \(\text {Re} (q(z))>0\). Now,
In view of Lemma 2.6 and (2.2), we have \(\text {Re}\left( \frac{F(z)}{z}\right) >\frac{1}{2}\) for \(z\in \mathbb {D}\). This completes the proof. \(\square \)
Lemma 2.8
Let \(F_1,F_2\in \mathcal {P}(M)\) with \(0<M\le \frac{3}{5}\), where \(\mathcal {P}(M)\) is defined in (2.1). Then \(F_1*F_2\in \mathcal {P}(M)\).
Proof
Let \(F_1(z)=z+\sum \nolimits _{n=2}^\infty A_nz^n\) and \(F_2(z)=z+\sum \nolimits _{n=2}^\infty B_nz^n\). Then the convolution of \(F_1\) and \(F_2\) is given by
Now,
Since \(F_1, F_2\in \mathcal {P}(M)\), so \(\text {Re}(zF_1''(z))>-M\) and in view of Lemma 2.7, we have \(\text {Re}\left( \frac{F_2(z)}{z}\right) >\frac{1}{2}\). In view of Lemma 2.6 and (2.3), we have \(\text {Re}(zF''(z))>-M\) in \(\mathbb {D}\). Therefore \(F=F_1*F_2\in \mathcal {P}(M)\). This completes the proof. \(\square \)
Lemma 2.9
[8] Let \(f=h+\overline{g}\) be given by (1.10).
-
(i)
If \(\sum \nolimits _{n=2}^{\infty } n\left( |a_n|+|b_n|\right) \le 1\), then f is starlike in \(\mathbb {D}\);
-
(ii)
If \(\sum \nolimits _{n=2}^{\infty } n^2\left( |a_n|+|b_n|\right) \le 1\), then f is convex in \(\mathbb {D}\).
3 Convex Combinations and Convolutions
In this section, we will show that \(\mathcal {P}_{\mathcal {H}}^0(M)\) is closed under convex combinations and convolutions.
Theorem 3.1
The class \(\mathcal {P}_{\mathcal {H}}^0(M)\) is closed under convex combinations.
Proof
Let \(f_i=h_i+\overline{g_i}\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(1\le i\le n\) and \(\sum \nolimits _{i=1}^n t_i=1\), where \(0\le t_i\le 1\) for each i. Then, we have
The convex combination of the \(f_i\)’s can be written as
where \(h(z)=\sum \nolimits _{i=1}^n t_i h_i(z)\) and \(g(z)=\sum \nolimits _{i=1}^n t_ig_i(z)\). Then both h and g are analytic in \(\mathbb {D}\) with \(h(0)=g(0)=h'(0)-1=g'(0)=0\). Now,
This shows that \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\). This completes the proof.\(\square \)
Theorem 3.2
Let \(F_1,F_2\in \mathcal {P}_{\mathcal {H}}^0(M)\) with \(0<M\le \frac{3}{5}\). Then \(F_1*F_2\in \mathcal {P}_{\mathcal {H}}^0(M)\).
Proof
Let \(F_1=h_1+\overline{g_1}\) and \(F_2=h_2+\overline{g_2}\) be two functions in \(\mathcal {P}_{\mathcal {H}}^0(M)\). Then the convolution of \(F_1\) and \(F_2\) is given by \(F_1*F_2=h_1*h_2+\overline{g_1*g_2}\). To show that \(F_1*F_2\in \mathcal {P}_{\mathcal {H}}^0(M)\), it is sufficient to show that \(F=h_1*h_2+\epsilon \left( g_1*g_2\right) \in \mathcal {P}(M)\) for each \(\epsilon \) with \(|\epsilon |=1\). By Lemma 2.1, we have \(h_1+\epsilon g_1, h_2+\epsilon g_2\in \mathcal {P}(M)\) for each \(\epsilon \) with \(|\epsilon |=1\). Thus, we deduce that
In view of Lemma 2.8, we have \((h_1-g_1)*(h_2-\epsilon g_2), (h_1+g_1)*(h_2+\epsilon g_2)\in \mathcal {P}(M)\). Then in view of Theorem 3.1, we get \(F\in \mathcal {P}(M)\). Hence \(\mathcal {P}_{\mathcal {H}}^0(M)\) is closed under convolution. This completes the proof. \(\square \)
In 2002, Goodloe [15] considered the Hadamard product of a harmonic function with an analytic function as follows.
where \(f=h+\overline{g}\) is harmonic and \(\phi \) is an analytic function in \(\mathbb {D}\).
Theorem 3.3
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) and \(\phi \in \mathcal {A}\) be such that \(\text {Re}\left( \frac{\phi (z)}{z}\right) >\frac{1}{2}\) for \(z\in \mathbb {D}\). Then \(f\tilde{*}\phi \in \mathcal {P}_{\mathcal {H}}^0(M)\).
Proof
Let \(f=h+\overline{g}\in \mathcal {P}_{\mathcal {H}}^0(M)\). In view of Lemma 2.1, we have \(f_1=h+\epsilon g\in \mathcal {P}(M)\) for each \(\epsilon \) with \(|\epsilon |=1\). To prove that \(f\tilde{*}\phi =h*\phi +\overline{g*\phi }\in \mathcal {P}_{\mathcal {H}}^0(M)\), it is sufficient to show that \(F(z)=h*\phi +\epsilon (g*\phi )\in \mathcal {P}(M)\) for each \(\epsilon (|\epsilon |=1)\). Since \(f_1\in \mathcal {P}(M)\) and \(\phi \in \mathcal {A}\), so we assume that \(f_1(z)=z+\sum _{n=2}^\infty A_nz^n\) and \(\phi (z)=z+\sum _{n=2}^\infty B_nz^n\). Then, we deduce that
Since \(\text {Re}\left( \frac{\phi (z)}{z}\right) >\frac{1}{2}\) and \(f_1\in \mathcal {P}(M)\), \(\text {Re}(zf_1''(z))>-M\), so in view of Lemma 2.6 and (3.1), we have \(\text {Re}(zF''(z))>-M\) in \(\mathbb {D}\). Hence \(F\in \mathcal {P}(M)\). This completes the proof. \(\square \)
Corollary 3.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) and \(\phi \in \mathcal {K}\), where \(\mathcal {K}\) denotes the family of all convex functions in \(\mathbb {D}\). Then \(f\tilde{*}\phi \in \mathcal {P}_{\mathcal {H}}^0(M)\).
Proof
Since \(\phi \in \mathcal {K}\), so \(\text {Re}\left( \frac{\phi (z)}{z}\right) >\frac{1}{2}\) for \(z\in \mathbb {D}\). The result immediately follows from Theorem 3.3.\(\square \)
Theorem 3.4
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) and \(\phi \in \mathcal {A}\) be such that \(\text {Re}\left( \frac{\phi (z)}{z}\right) >\frac{1}{2}\) for \(z\in \mathbb {D}\). Then \(f*\left( \phi +\beta \overline{\phi }\right) \in \mathcal {P}_{\mathcal {H}}^0(M)\), where \(|\beta |=1\).
Proof
Let \(f=h+\overline{g}\in \mathcal {P}_{\mathcal {H}}^0(M)\). Then \(h(z)=z+\sum _{n=2}^\infty a_nz^n\), \(g(z)=\sum _{n=2}^\infty b_nz^n\). Now,
To prove that \(f*\left( \phi +\beta \overline{\phi }\right) \in \mathcal {P}_{\mathcal {H}}^0(M)\), it is sufficient to show that \(f_{\epsilon }=h*\phi +\epsilon \overline{\beta }(g*\phi )\in \mathcal {P}(M)\) for each \(\epsilon (|\epsilon |=1)\). Let \(\phi (z)=z+\sum \nolimits _{n=2}^\infty C_nz^n\). For each \(|\epsilon |=1\), we have
Since \(f=h+\overline{g}\in \mathcal {P}_{\mathcal {H}}^0(M)\), so in view of Lemma 2.1, we have \(h+\epsilon \overline{\beta } g\in \mathcal {P}(M)\) for \(\epsilon \), \(\beta \) with \(|\epsilon \overline{\beta }|=1\), i.e., \(|\beta |=1\). Thus, we have
Since \(\text {Re}\left( \frac{\phi (z)}{z}\right) >\frac{1}{2}\) for \(z\in \mathbb {D}\), so in view of Lemma 2.6 and (3.2), we have
Hence \(f_{\epsilon }\in \mathcal {P}(M)\). This completes the proof. \(\square \)
Corollary 3.2
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) and \(\phi \in \mathcal {K}\), where \(\mathcal {K}\) denotes the family of all convex functions in \(\mathbb {D}\). Then \(f*\left( \phi +\beta \overline{\phi }\right) \in \mathcal {P}_{\mathcal {H}}^0(M)\), where \(|\beta |=1\).
Proof
Since \(\phi \in \mathcal {K}\), so \(\text {Re}\left( \frac{\phi (z)}{z}\right) >\frac{1}{2}\) for \(z\in \mathbb {D}\). The result immediately follows from Theorem 3.4.\(\square \)
By Lemmas 2.3 and 2.9, it is possible to show that each \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) is convex (resp. starlike) in some disk D, i.e., f(D) is a convex domain (resp. f(D) is a domain starlike with respect to the origin).
Theorem 3.5
Let \(f=h+\overline{g}\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Then f is starlike in \(|z|<1-e^{-\frac{1}{2M}}=r^*\) and convex in \(|z|<r_c\), where \(r_c\in (0,1)\) is the smallest root of the equation \(\frac{r}{1-r}-\ln (1-r)-\frac{1}{2M}=0\).
Proof
Let \(0<r<1\) and \(f_r(z)=\frac{1}{r}f(rz)=z+\sum _{n=2}^{\infty } a_nr^{n-1}z^n+\overline{\sum _{n=2}^{\infty } b_nr^{n-1}z^n}\) for \(z\in \mathbb {D}\). For convenience, we let \(S_1=\sum _{n=2}^{\infty } n\left( |a_n|+|b_n|\right) r^{n-1}\) and \(S_2=\sum _{n=2}^{\infty } n^2\left( |a_n|+|b_n|\right) r^{n-1}\). According to Lemma 2.9, it suffices to show that \(S_1\le 1\) for \(|z|=r<r^*\) and \(S_2\le 1\) for \(|z|=r<r_c\). In view of Lemma 2.3, we have
Thus, \(S_1\le 1\) if \(r< 1-e^{-\frac{1}{2M}}=r^*\). Again
Thus, \(S_2\le 1\) if \(r<r_c\), where \(r_c\in (0,1)\) is the smallest root of the equation \(\frac{r}{1-r}-\ln (1-r)-\frac{1}{2M}=0\). This completes the proof. \(\square \)
4 Bohr–Rogosinski Radius for the Class \(\mathcal {P}_{\mathcal {H}}^0(M)\)
In 2023, Ahamed et al. [3] obtained the following results regarding Bohr–Rogosinski radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\).
Theorem D
[3] Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Then
for \(|z|=r\le r_N(M)\) with \(N\ge 2\), where \(r_N(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_N(M)\) is the best possible.
Theorem E
[3] Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Then
for \(|z|=r\le r_N(M)\) with \(N\ge 2\), where \(r_N(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_N(M)\) is the best possible.
Theorem F
[3] Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Then
for \(|z|=r\le r_{m,N}(M)\) with \(N\ge 2\), where \(r_{m,N}(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_{m,N}(M)\) is the best possible.
Note that, \(0<M<\frac{1}{2(\ln 4-1)}\) in Theorems D-F. Now we focus on the following question.
Question 4.1
Can we further reduce the Bohr–Rogosinski radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\) in Theorems D and E?
Corresponding to the question above, we first prove the following Bohr–Rogosinski radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\).
Theorem 4.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then
for \(|z|=r\le r_{N_1,N_2}(M)\) with \(N_1\ge N_2\ge 2\), where \(r_{N_1,N_2}(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_{N_1,N_2}(M)\) is the best possible (Figs. 1 and 2).
Remark 4.1
Clearly Theorem 4.1 holds for the small Bohr–Rogosinski radius than the radius in Theorem D. It can be checked from the Table 1, e.g., when \(N=3\), then \(r_3(0.4)=0.527\) [3] and \(r_{3,2}(0.4)=0.497629\).
Theorem 4.2
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then
for \(|z|=r\le r_{l,m,N_1,N_2}(M)\) with \(N_1\ge N_2\ge 2\) and \(l,m\in \mathbb {N}\), where \(r_{l,m,N_1,N_2}(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_{l,m,N_1,N_2}(M)\) is the best possible (Figs. 3 and 4).
Remark 4.2
Clearly Theorem 4.2 holds for the small Bohr–Rogosinski radius than the radius in Theorem E. It can be checked from the Table 2, e.g., when \(N=3\), then \(r_3(1.29)=0.053\) [3], and \(r_{2,1,3,2}(1.29)=0.0434376\).
Theorem 4.3
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then
for \(|z|=r\le r_{l,m,N}(M)\) with \(N\ge 2\) and \(l,m\in \mathbb {N}\), where \(r_{l,m,N}(M)\in (0,1)\) is the smallest root of the equation
where \(Li_2(r)\) is the dilogarithm function. The constant \(r_{l,m,N}(M)\) is the best possible (Figs. 5 and 6; Table 3).
Theorem 4.4
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then
for \(r\le r_{p,k_1,q,k_2,N_1,N_2}(M)\) with \(N_1\ge N_2\ge 2\), \(p,q\in \mathbb {N}\) and \(k_1,k_2\in \mathbb {R}\), where \(r_{p,k_1,q,k_2,N_1,N_2}(M)\in (0,1)\) is the smallest root of the equation
The radius \(r_{p,k_1,q,k_2,N_1,N_2}(M)\) is the best possible (Figs. 7; Table 4).
5 Proof of the Theorems 4.1–4.4
Proof of Theorem 4.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be as (1.10). Using Lemma 2.4, we get
Since \(f(0)=0\), so the Euclidean distance between f(0) and the boundary of \(f(\mathbb {D})\) is \(d\left( f(0),\partial f(\mathbb {D})\right) :=\liminf \limits _{|z|\rightarrow 1}|f(z)-f(0)|=\liminf \limits _{|z|\rightarrow 1}|f(z)|\). Thus from (5.1), we get
In view of Lemmas 2.2, 2.3 and 2.4, we now deduce for \(N_1\ge N_2\ge 2\) that
Now, we deduce that
for \(0<r\le r_{N_1,N_2}(M)<1\), where \(r_{N_1,N_2}(M)\) is the smallest root of the equation
To ensure about the existence of a root \(r_{N_1,N_2}(M)\), we construct the function \(\mathcal {G}_1:[0,1)\rightarrow \mathbb {R}\) such that
It is clear that (i) \(\mathcal {G}_1\) is continuous on [0, 1), (ii) \(\mathcal {G}_1(0)=-1+2M(2\ln 2-1)<0\) and (iii) \(\lim \limits _{r\rightarrow 1}\mathcal {G}_1(r)>0\), since \(\lim \limits _{r\rightarrow 1}(1-r)\ln (1-r)=0\). Thus the claim follows from Intermediate value theorem. Thus, we have
Combining (5.2), (5.3) and (5.4) for \(|z|=r\le r_{N_1,N_2}(M)\), we deduce that
Now we show that the radius \(r_{N_1,N_2}(M)\) is the best possible. We set
Note that \(f_{M}(0)=0\), \(f_{M}\in \mathcal {P}_{\mathcal {H}}^0(M)\). For \(z=r\), we have
and for \(z=-r\), we have
For \(|z|=r_{N_1,N_2}(M)\), it follows from (5.5) and (5.9) that
Thus the result follows. \(\square \)
Proof of Theorem 4.2
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Note that \(N_1\ge N_2\ge 2\) and \(l,m\in \mathbb {N}\). In view of Lemmas 2.2, 2.3 and 2.4, we get
Similarly as the proof of Theorem 4.1, we get (5.2) and
for \(0<r\le r_{l,m,N_1,N_2}(M)\), where \(r_{l,m,N_1,N_2}(M)\) is the smallest root of \(\mathcal {G}_2(r)=0\) in (0, 1), where \(\mathcal {G}_2:[0,1)\rightarrow \mathbb {R}\) is defined by
Similarly as the proof of Theorem 4.1, we have
\(\mathcal {G}_2(r_{l,m,N_1,N_2}(M))=0\), i.e.,
Combining (5.2), (5.10) and (5.11), we obtain for \(|z|=r\le r_{l,m,N_1,N_2}(M)\)
In order to show that \(r_{l,m,N_1,N_2}(M)\) is the best possible, we consider the function \(f=f_{M}\) defined by (5.6) and we again get (5.9). For \(|z|=r_{l,m,N_1,N_2}(M)\), it follows from (5.9) and (5.12) that
Therefore, the radius \(r_{l,m,N_1,N_2}(M)\) is the best possible. Thus the result follows. \(\square \)
Proof of Theorem 4.3
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Note that \(N\ge 2\) and \(l,m\in \mathbb {N}\). In view of Lemmas 2.2, 2.3 and 2.4, we obtain
Similarly as the proof of Theorem 4.1, we get (5.2) and
for \(0< r\le r_{l,m,N}(M)\), where \(r_{l,m,N}(M)\) is the smallest root of \(\mathcal {G}_3(r)=0\) in (0, 1) and \(\mathcal {G}_3:[0,1)\rightarrow \mathbb {R}\) is defined by
Similarly as the proof of Theorem 4.1, we have \(\mathcal {G}_3\left( r_{l,m,N}(M)\right) =0\), i.e.,
Combining (5.2), (5.13) and (5.14), we obtain for \(|z|=r\le r_{l,m,N}(M)\)
In order to show that \(r_{l,m,N}(M)\) is the best possible, we consider the function \(f=f_ M\) defined by (5.6) and we again get (5.9). For \(|z|=r_{l,m,N}(M)\), it follows from (5.9) and (5.15) that
Therefore, the radius \(r_{l,m,N}(M)\) is the best possible. Thus the results follows. \(\square \)
Proof of Theorem 4.4
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). We know that, if \(\phi \) is analytic in \(\mathbb {D}\) with \(\phi (0)=0\) and \(|\phi (z)|<1\), \(\forall z\in \mathbb {D}\), then by Schwarz Lemma, we have \(|\phi (z)|\le |z|\). Note that \(N_1\ge N_2\ge 2\), \(p,q\in \mathbb {N}\) and \(k_1,k_2\in \mathbb {R}\). In view of Lemmas 2.2, 2.3 and 2.4, we obtain
Now, we deduce that
for \(0<r\le r_{p,k_1,q,k_2,N_1,N_2}(M)\), where \(r_{p,k_1,q,k_2,N_1,N_2}(M)\) is the smallest root of \(\mathcal {G}_4(r)=0\) in (0, 1) and \(\mathcal {G}_4:[0,1)\rightarrow \mathbb {R}\) is defined by
Similarly as the proof of Theorem 4.1, we have \(\mathcal {G}_4\left( r_{p,k_1,q,k_2,N_1,N_2}(M)\right) =0\), i.e.,
Combining (5.2), (5.16) and (5.17), we obtain for \(|z|=r\le r_{p,k_1,q,k_2,N_1,N_2}(M)\)
In order to show that \(r_{p,k_1,q,k_2,N_1,N_2}(M)\) is the best possible, we consider the function \(f=f_M\) defined by (5.6) and we again get (5.9). For \(|z|=r_{p,k_1,q,k_2,N_1,N_2}(M)\), it follows from (5.9) and (5.18) that
Therefore, the radius \(r_{p,k_1,q,k_2,N_1,N_2}(M)\) is the best possible. Thus the result follows. \(\square \)
6 Improved Bohr Radius for the Class \(\mathcal {P}_{\mathcal {H}}^0(M)\)
In 2023, Ahamed et al. [3] generalized the harmonic versions of Theorem B for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\) and obtained the following result.
Theorem G
[3] Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Then
for \(r\le r_N(M)\), where \(P\left( \omega \right) =\omega ^N+\omega ^{N-1}+\cdots +\omega \) and \(r_N(M)\in (0,1)\) is the smallest root of the equation
where G(r) is defined by \(G(r):=r^2\left( Li_2(r^2)-1\right) +(1-r^2)\ln (1-r^2)\). The constant \(r_N(M)\) is the best possible.
In order to generalize Theorem G, we consider a N-th degree polynomial of the form
where \(c_i\in \mathbb {R}\) \((1\le i\le N)\) with \(c_N\not =0\). Concerning improved Bohr radius for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\), we have obtain the following results.
Theorem 6.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then
for \(r\le r_{N_1,N_2}(M)\) with \(N_1\ge N_2\ge 2\), where \(P\left( \omega \right) \) is defined in (6.3) and \(r_{N_1,N_2}(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_{N_1,N_2}(M)\) is the best possible (Fig. 8 and 9; Tables 5 and 6).
As a consequence of Theorem 6.1, we obtain the following corollary.
Corollary 6.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then,
for \(r\le r_{N_1,N_2}(M)\), where \(r_{N_1,N_2}(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_{N_1,N_2}(M)\) is the best possible.
7 Proof of the Theorem 6.1
Proof of Theorem 6.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). For the analytic functions h and g, the area \(S_r\) of the disk \(|z|<r\) under the harmonic map f is given by
Combining (7.1), (7.2), (7.3) and Lemma 2.3, we obtain
Note that, \(N_1\ge N_2\ge 2\). In view of Lemmas 2.2, 2.3 and 2.4, we obtain
for \(0<r\le r_{N_1,N_2}(M)\), where \(r_{N_1,N_2}(M)\) is the smallest root of \(\mathcal {G}_5(r)=0\) in (0, 1) and \(\mathcal {G}_5:[0,1)\rightarrow \mathbb {R}\) be defined by
Similarly as the proof of Theorem 4.1, we have \(\mathcal {G}_5\left( r_{N_1,N_2}(M)\right) =0\), i.e.,
Combining (5.2), (7.5) and (7.6), we obtain for \(|z|=r\le r_{N_1,N_2}(M)\)
In order to show that \(r_{N_1,N_2}(M)\) is the best possible, we consider the function \(f=f_M\) defined by (5.6) and we again get (5.9). For \(|z|=r_{N_1,N_2}(M)\), it follows from (5.9) and (7.6) that
Hence the radius \(r_{N_1,N_2}(M)\) is the best possible. This completes the proof. \(\square \)
8 Refined Bohr Radius for the Class \(\mathcal {P}_{\mathcal {H}}^0(M)\)
In this section, we establish some sharp results on the harmonic analogue of Theorem C for the class \(\mathcal {P}_{\mathcal {H}}^0(M)\) as follows.
Theorem 8.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) for \(0<M<\frac{1}{2(\ln 4-1)}\) be given by (1.10). Then
for \(r\le r_{p,q,N}(M)\) with \(p,q(\not =1)\in \mathbb {N}\) and \(N\ge 2\), where \(r_{p,q,N}(M)\in (0,1)\) is the smallest root of the equation
The constant \(r_{p,q,N}(M)\) is the best possible (Figs. 10 and 11; Table 7).
9 Proof of the Theorem 8.1
Proof of Theorem 8.1
Let \(f\in \mathcal {P}_{\mathcal {H}}^0(M)\) be given by (1.10). Note that \(p,q(\not =1)\in \mathbb {N}\) and \(N\ge 2\). In view of Lemmas 2.3 and 2.4, we obtain
Now,
for \(0<r\le r_{p,q,N}(M)\), where \( r_{p,q,N}(M)\) is the smallest root of \(\mathcal {G}_7(r)=0\) in (0, 1) and \(\mathcal {G}_7:[0,1)\rightarrow \mathbb {R}\) be defined by
Similarly as the proof of Theorem 4.1, we have \(\mathcal {G}_7\left( r_{p,q,N}(M)\right) =0\), i.e.,
Combining (5.2), (9.1) and (9.2), we obtain for \(|z|=r\le r_{p,q,N}(M)\)
In order to show that \(r_{p,q,N}(M)\) is the best possible, we consider the function \(f=f_M\) defined by (5.6) and we again get (5.9). For \(|z|=r_{p,q,N}(M)\), it follows from (5.9) and (9.2) that
Hence the radius \(r_{p,q,N}(M)\) is the best possible. Thus the result follows. \(\square \)
Data Availibility
Not applicable
References
Abu-Muhanna, Y.: Bohr’s phenomenon in subordination and bounded harmonic classes. Complex Var. Elliptic Equ. 55, 1071–1078 (2010)
Abu-Muhanna, Y., Ali, R.M., Ng, Z.C., Hasni, S.F.M.: Bohr radius for subordinating families of analytic functions and bounded harmonic mappings. J. Math. Anal. Appl. 420, 124–136 (2014)
Ahamed, M.B., Allu, V., Halder, H.: Improved Bohr inequalities for certain class of harmonic univalent functions. Complex Var. Elliptic Equ. 68(2), 267–290 (2023). https://doi.org/10.1080/17476933.2021.1988583
Aizenberg, L.: Generalization of results about the Bohr radius for power series. Stud. Math. 180, 161–168 (2007)
Ali, R.M., Barnard, R.W., Solynin, AYu.: A note on Bohr’s phenomenon for power series. J. Math. Anal. Appl. 449, 154–167 (2017)
Allu, V., Halder, H.: Bohr inequality for certain harmonic mappings. Indag. Math. 33(3), 581–597 (2022)
Allu, V., Halder, H.: Bhor phenomenon for certain subclasses of harmonic mappings. Bulletin des Sciences Mathématiques 173, 103053 (2021). https://doi.org/10.1016/j.bulsci.2021.103053
Avci, Y., Zlotkiewicz, E.: On harmonic univalent mappings. Ann. Uni. Mariae Curie-Sklodowska Sect. A 44, 1–7 (1990)
Boas, H.P., Khavinson, D.: Bohr’s power series theorem in several variables. Proc. Am. Math. Soc. 125(10), 2975–2979 (1997)
Bohr, H.: A theorem concerning power series. Proc. Lond. Math. Soc. s2–13, 1–5 (1914)
Duren, P.L.: Univalent functions, Grundlehren Der Mathematischen Wissenschaften, vol. 259. Springer, New York (1983)
Dixon, P.G.: Banach algebras satisfying the non-unital von Neumann inequality. Bull. Lond. Math. Soc. 27(4), 359–362 (1995)
Evdoridis, S., Ponnusamy, S., Rasila, A.: Improved Bohr’s inequality for locally univalent harmonic mappings. Indag. Math. N.S. 30(1), 201–213 (2019)
Ghosh, N., Allu, V.: On some subclasses of harmonic mappings. Bull. Aust. Math. Soc. 101, 130–140 (2020)
Goodloe, R.M.: Hadamard products of convex harmonic mappings. Complex Var. Theory Appl. 47, 81–92 (2002)
Huang, Y., Liu, M.-S., Ponnusamy, S.: Refined Bohr-type inequalities with area measure for bounded analytic functions. Anal. Math. Phys. 10, 50 (2020). https://doi.org/10.1007/s13324-020-000393-0
Ismagilov, A., Kayumov, I.R., Ponnusamy, S.: Sharp Bohr type inequality. J. Math. Anal. Appl. 489, 124–147 (2020)
Kayumov, I.R., Ponnusamy, S.: Bohr–Rogosinski radius for analytic functions, preprint, see arXiv:1708.05585
Kayumov, I.R., Ponnusamy, S.: On a powered Bohr inequality. Ann. Acad. Sci. Fenn. Math. 44, 301–310 (2019)
Kayumov, I.R., Ponnusamy, S.: Improved version of Bohr’s inequalities. C. R. Math. Acad. Sci. (Paris) 358(5), 615–620 (2020)
Liu, G., Liu, Z., Ponnusamy, S.: Refined Bohr inequality for bounded analytic functions. Bulletin des Sciences Mathématiques 173, 103054 (2021)
Liu, M.S., Ponnusamy, S.: Multidimensional analogues of refined Bohr’s inequality. Proc. Am. Math. Soc. 149(5), 2133–2146 (2021)
Ponnusamy, S., Viajayakumar, R., Wirths, K.J.: New inequalities for the coefficients of unimodular bounded functions. Results Math. 75, 107 (2020). https://doi.org/10.1007/s00025-020-01240-1
Ponnusamy, S., Wirths, K.J.: Bohr type inequalities for functions with a multiple zero at the origin. Compt. Methods Funct. Theory 20, 550–570 (2020)
Singh, R., Singh, S.: Convolution properties of a class of starlike functions. Proc. Am. Math. Soc. 106, 145–152 (1989)
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The authors like to thank the anonymous reviewers and and the editing team for their valuable suggestions towards the improvement of the paper.
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The second Author is supported by University Grants Commission (IN) fellowship (NO. F. 44-1/2018 (SA-III)) and the third author is supported by Swami Vivekananda Merit-cum-Means scholarship (WB, India).
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Mandal, R., Biswas, R. & Guin, S.K. Geometric Studies and the Bohr Radius for Certain Normalized Harmonic Mappings. Bull. Malays. Math. Sci. Soc. 47, 131 (2024). https://doi.org/10.1007/s40840-024-01732-1
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DOI: https://doi.org/10.1007/s40840-024-01732-1
Keywords
- Analytic
- Univalent
- Harmonic functions
- Starlike
- Convex
- Close-to-convex functions
- Coefficient estimate
- Growth theorem
- Bohr radius