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Radii problems for some classes of analytic functions associated with Legendre polynomials of odd degree
Journal of Inequalities and Applications volume 2020, Article number: 178 (2020)
Abstract
The aim of the present paper is to study radii problems for two general classes including various known subclasses of analytic functions associated with the normalized form of Legendre polynomials of odd degree. We also obtain some special cases of the main results presented here with some useful examples.
1 Introduction and preliminaries
Let \(\mathbb{U}(r):=\{z\in \mathbb{C}: \vert z \vert < r\}\) be the disk in the complex plane \(\mathbb{C}\) centered at the origin, with radius \(r>0\), and denote by \(\mathbb{U}:=\mathbb{U}(1)\) the unit disk. We denote by \(\mathcal{A}\) the class of analytic functions in the unit disk \(\mathbb{U}\) normalized by \(f(0)=f^{\prime }(0)-1=0\), and let \(\mathcal{S}\) be the subclass of \(\mathcal{A}\) consisting of univalent functions.
We denote by \(\mathcal{S}^{*}(\alpha )\) the subclass of \(\mathcal{A}\) consisting of functions which are starlike of orderα in \(\mathbb{U}\), that is,
Also, let us denote by \(\widetilde{\mathcal{S}}^{*}(\alpha )\) the subclass of \(\mathcal{A}\) consisting of functions which are strongly starlike of orderα in \(\mathbb{U}\), that is,
Thus, in particular, \(\mathcal{S}^{*}:=\mathcal{S}^{*}(0)=\widetilde{\mathcal{S}}^{*}(1)\) represents the class of starlike functions in the open unit disk \(\mathbb{U}\).
The real numbers
and
are called the radius of starlikeness of orderα and the radius of strong starlikeness of orderα of the function f, respectively. In particular, \(r^{\ast }(f):=r_{0}^{\ast }(f)=r_{1}^{\widetilde{\ast }}(f)\) is called the radius of starlikeness of the function f.
Recently, Darus et al. [8] considered the general class \(k-\mathcal{UCST}(\alpha )\) defined as follows.
Definition 1
Let \(f\in \mathcal{A}\). Then \(f\in k-\mathcal{UCST}(\alpha )\) if
where \(k\ge 0\) and \(0\le \alpha \le 1\).
Remark 1
-
(i)
For \(k=0\) we get the class \(0-\mathcal{UCST}(\alpha )=:\mathcal{K}\), which includes the well-known class of convex functions, that is,
$$ \operatorname{Re} \biggl(1+\frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr)>0, \quad z\in \mathbb{U}. $$ -
(ii)
For \(\alpha =1\) we obtain the class \(k-\mathcal{UCST}(1)=:k-\mathcal{UCV}\) (see [11]), which includes the class of k-uniformly convex functions, that is,
$$ \operatorname{Re} \biggl(1+\frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr)>k \biggl\vert \frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr\vert , \quad z\in \mathbb{U}. $$ -
(iii)
For \(k=1\) and \(\alpha =1\) we get the class \(1-\mathcal{UCST}(1)=:\mathcal{UCV}\) (see [13]), which includes the class of uniformly convex functions, that is,
$$ \operatorname{Re} \biggl(1+\frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr)> \biggl\vert \frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr\vert , \quad z\in \mathbb{U}. $$ -
(iv)
For \(\alpha =0\) we have the class \(k-\mathcal{UCST}(0)=:k-\mathcal{MN}\) (see [14]), which represents the functions \(f\in \mathcal{A}\) satisfying
$$ \operatorname{Re} \biggl(1+\frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr)>k \biggl\vert \frac{zf^{\prime }(z)}{f(z)}-1 \biggr\vert , \quad z\in \mathbb{U}. $$ -
(v)
For \(k=1\) and \(\alpha =0\) we get the class \(1-\mathcal{UCST}(0)=:\mathcal{MN}\) (see [15]), which represents the functions \(f\in \mathcal{A}\) satisfying
$$ \operatorname{Re} \biggl(1+\frac{zf^{\prime \prime }(z)}{f^{\prime }(z)} \biggr)> \biggl\vert \frac{zf^{\prime }(z)}{f(z)}-1 \biggr\vert , \quad z\in \mathbb{U}. $$
The real number
is called the \(k-\mathcal{UCST}(\alpha )\)radius of the function f. We note that
We recall that the Legendre polynomials are solutions of the Legendre differential equation
while the Rodrigues formula for the Legendre polynomials is
The Legendre polynomials are symmetric or antisymmetric, that is,
Since we will study different radius properties for the Legendre polynomials of odd degree, let us consider the following normalized form of the Legendre \(P_{2n-1}\) polynomials, that is, \(\mathcal{P}_{2n-1}\) given by
It is well known that the Rodrigues formula implies that the Legendre polynomials of odd degree have only real roots, and the roots of \(P_{2n-1}(z)\) are \(0=z_{0}< z_{1}<\cdots <z_{n-1}\) and \(-z_{1},-z_{2},\ldots,-z_{n-1}\), while the product representation of the polynomial \(\mathcal{P}_{2n-1}\) is
Bulut and Engel [7] have obtained the radius of starlikeness, convexity, and uniform convexity (see [10, 12, 13]) of the normalized form of the Legendre polynomial of odd degree. In the recent years, several authors determined the radius of starlikeness, convexity, and uniform convexity for some special functions, that is a relative new direction in the geometric function theory (see, for example, [1–6]).
In the present paper we obtain the radius of strong starlikeness and other related radius of the normalized form of Legendre polynomials of odd degree, and the technique of the proofs used in our paper is similar to that of several papers [1, 3–6]. Further, our results are well supported by some examples.
In order to prove our main results, we require the following lemmas.
Lemma 1
([7, Lemma 1.1])
If\(\vert z \vert \leq r<\gamma \), where\(\gamma >0\), then we have
Lemma 2
([9, Lemma 3.1])
If
then the disk\(\vert w-a \vert \le R_{a}\)is contained in the sector\(\vert \arg w \vert \le \pi \gamma /2\), where\(0<\gamma \le 1\).
Lemma 3
([9, Lemma 3.2])
For\(\vert z \vert \leq r<1\)and\(\vert z_{k} \vert =R>r\), we have
2 Main results
Using the first of the above lemmas, we obtain the \(k-\mathcal{UCST}(\alpha )\) radius of \(\mathcal{P}_{2n-1}\) as follows.
Theorem 1
The radius of\(k-\mathcal{UCST}(\alpha )\)of\(\mathcal{P}_{2n-1}\)is\(r_{\alpha }^{k-\mathcal{UCST}}(\mathcal{P}_{2n-1})=r_{1}\), where\(r_{1}\)denotes the smallest positive root of the equation
Proof
Differentiating logarithmically the product representation (1) of the \(\mathcal{P}_{2n-1}\) polynomial, we have
where \(z_{k}\), with \(k\in \{1,2,\ldots,n-1\}\), is the kth positive zero of the normalized Legendre polynomial of odd degree. The logarithmical differentiation of the above equality leads to
that is,
If \(\vert z \vert \le r< z_{1}\), then it follows that \(\vert z \vert \le r< z_{k}\) for all \(k\in \{1,2,\ldots,n-1\}\). Hence, replacing z by \(z^{2}\) and γ by \(z^{2}_{k}\) for all \(k\in \{1,2,\ldots,n-1\}\) in inequalities (2) and (4) of Lemma 1, we get
and
respectively. Now, for \(\vert z \vert \le r< z_{1}\) from (6) and two above inequalities, we deduce the following inequalities:
On the other hand, replacing z by \(z^{2}\) and γ by \(z_{k}\) for all \(k\in \{1,2,\ldots,n-1\}\) in inequality (3) of Lemma 1 and using relations (5) and (6), we obtain
for \(\vert z \vert \le r< z_{1}\).
Therefore, from (7) and (8), for any \(k\ge 0\) we have
for \(\vert z \vert \le r< z_{1}\).
Let \(\omega:I\rightarrow\mathbb{R}\), where I is the open interval \((0,z_{1})\) which is subset of \(\mathbb{R}\) be the function defined by
Since \(\lim_{r\searrow 0}\omega (r)=1\), \(\lim_{r\nearrow z_{1}}\omega (r)=-\infty \), and the function ω is continuous, it follows that the equation \(\omega (r)=0\) has at least a root in \((0,z_{1})\). Thus, if \(r_{1}\) is the smallest positive root of the equation \(\omega (r)=0\), then we have
for \(\vert z \vert < r_{1}\), and
It follows that \(r_{\alpha }^{k-\mathcal{UCST}}(\mathcal{P}_{2n-1})=r_{1}\) is the radius of \(k-\mathcal{UCST}(\alpha )\) of the normalized Legendre polynomial \(\mathcal{P}_{2n-1}\), and hence this completes our proof. □
Choosing \(k=0\) in Theorem 1, we obtain the next result which was given by Bulut and Engel for \(\beta =0\) in [7, Theorem 2.2].
Corollary 1
The radius of convexity of\(\mathcal{P}_{2n-1}\)is\(r^{c}(\mathcal{P}_{2n-1})=r_{2}\), where\(r_{2}\)denotes the smallest positive root of the equation
Example 1
For \(n=2\) we have
Like we see from Fig. 1(a) the domain \(\mathcal{P}_{3}(\mathbb{U})\) is not convex; moreover, the function \(\mathcal{P}_{3}\) is not univalent in \(\mathbb{U}\). From Corollary 1 it follows that the radius of convexity of \(\mathcal{P}_{3}\) is \(r^{c}(\mathcal{P}_{3})={1}/{\sqrt{15}}\simeq 0.2581988897\ldots\) , where \({1}/{\sqrt{15}}\) denotes the smallest positive root of the equation
According to the above result, the domain \(\mathcal{P}_{3} (\mathbb{U} (r^{c}(\mathcal{P}_{3}) ) )\) shown in Fig. 1(b) is convex.
Letting \(\alpha =1\) in Theorem 1, we obtain the next special case.
Corollary 2
The radius ofk-uniformly convexity of\(\mathcal{P}_{2n-1}\)is\(r^{ucv}(\mathcal{P}_{2n-1})=r_{3}\), where\(r_{3}\)denotes the smallest positive root of the equation
Setting \(k=1\) in Corollary 2, we obtain the following result which was given by Bulut and Engel in [7, Theorem 2.3].
Example 2
The radius of uniform convexity of \(\mathcal{P}_{2n-1}\) is \(r^{uc}(\mathcal{P}_{2n-1})=r_{4}\), where \(r_{4}\) denotes the smallest positive root of the equation
Example 3
For \(n=3\) we have
Like we see from Fig. 2(a) the function \(\mathcal{P}_{5}\) is not univalent in \(\mathbb{U}\). From Example 2 it follows that the radius of uniform convexity of \(\mathcal{P}_{5}\) is \(r^{uc}(\mathcal{P}_{5})={\sqrt{735-42 \sqrt{259}}}/{63}\simeq 0.1219993521 \ldots\) , where \({\sqrt{735-42 \sqrt{259}}}/{63}\) denotes the smallest positive root of the equation
According to the above result, the domain \(\mathcal{P}_{5} (\mathbb{U} (r^{uc}(\mathcal{P}_{5}) ) )\) is uniformly convex, and it is plotted in Fig. 2(b).
Letting \(\alpha =0\) in Theorem 1, we deduce the next result.
Corollary 3
The radius of\(k-\mathcal{MN}\)of\(\mathcal{P}_{2n-1}\)is\(r^{k-\mathcal{MN}}(\mathcal{P}_{2n-1})=r_{5}\), where\(r_{5}\)denotes the smallest positive root of the equation
Letting \(k=1\) in Corollary 3, we obtain the following special case.
Example 4
The radius of \(\mathcal{MN}\) of \(\mathcal{P}_{2n-1}\) is \(r^{\mathcal{MN}}(\mathcal{P}_{2n-1})=r_{6}\), where \(r_{6}\) denotes the smallest positive root of the equation
In the following theorem we obtain the radius of strong starlikeness of order α of \(\mathcal{P}_{2n-1}\).
Theorem 2
The radius of strong starlikeness of orderαof\(\mathcal{P}_{2n-1}\)is\(\widetilde{r_{\alpha }^{\ast }}(\mathcal{P}_{2n-1})=r^{*}_{1}\), where\(r^{*}_{1}\)is the smallest positive root of the equation
Proof
If \(\vert z \vert \le r< z_{1}\), then it follows that \(\vert z \vert \le r< z_{k}\) for all \(k\in \{1,2,\ldots,n-1\}\), where \(z_{k}\), with \(k\in \{1,2,\ldots,n-1\}\), is the kth positive zero of the normalized Legendre polynomial of odd degree. Hence, replacing z by \(z^{2}\) and R by \(z^{2}_{k}\) for all \(k\in \{1,2,\ldots,n-1\}\) in the inequality of Lemma 3, we get
Using the above inequalities, from relation (5) we get
for \(\vert z \vert \le r< z_{1}\).
Denoting
we see that \(\operatorname{Im}a=0\), and from Lemma 2 and the above inequality it follows that the disc \(\vert w-a \vert \le R_{a}\) is contained in the sector \(\vert \arg w \vert \le \pi \alpha /2\), that is,
if we assume that the inequality
holds.
Let \(\psi:I\rightarrow\mathbb{R}\), where I is the open interval \((0,z_{1})\) which is subset of \(\mathbb{R}\) be defined by
The above inequality implies that \(\psi (r)\le 0\) for \(r\in (0,z_{1})\). Also, we have \(\lim_{r\searrow 0}\psi (r)=-\sin \frac{\pi \alpha }{2}<0\) and \(\lim_{r\nearrow z_{1}}\psi (r)=+\infty \). On the other the hand, we have \(\psi ^{\prime }(r)\ge 0\) for \(z\in (0,z_{1})\). It follows that the equation \(\psi (r)=0\) has a unique root \(r^{*}_{1}\) in \((0,z_{1})\). Therefore, the radius of strong starlikeness of order α of \(\mathcal{P}_{2n-1}\) is \(\widetilde{r_{\alpha }^{\ast }}(\mathcal{P}_{2n-1})=r^{*}_{1}\). □
Example 5
For \(n=2\) we have
where the roots of \(P_{3}\) are \(z_{0}=0\) and \(z_{1}=\pm {\sqrt{15}}/{5}\). From Theorem 2 it follows that the radii of strong starlikeness of order \(1/3\), \(1/2\), and \(2/3\) of \(\mathcal{P}_{3}\) are \(\widetilde{r_{1/3}^{\ast }}(\mathcal{P}_{3})={\sqrt{-10+5\sqrt{7}}}/{5} \simeq 0.3593748213\ldots\) , \(\widetilde{r_{1/2}^{\ast }}(\mathcal{P}_{3})={\sqrt{-5\sqrt{2}+5\sqrt{5}}}/{5} \simeq 0.4054267912\ldots\) , and \(\widetilde{r_{2/3}^{\ast }}(\mathcal{P}_{3})= \frac{\sqrt{15\sqrt{39}-30\sqrt{3}}}{15}\simeq 0.4305729813\ldots\) , where \(\frac{\sqrt{-10+5\sqrt{7}}}{5}\), \({\sqrt{-5\sqrt{2}+5\sqrt{5}}}/{5}\), and \({\sqrt{15\sqrt{39}-30\sqrt{3}}}/{15}\) denote the smallest positive roots of the equations
and
respectively. According to the above result, the domains \(\mathcal{P}_{3} (\mathbb{U} (\widetilde{r_{1/3}^{\ast }}( \mathcal{P}_{3}) ) )\), \(\mathcal{P}_{3} (\mathbb{U} (\widetilde{r_{1/2}^{\ast }}( \mathcal{P}_{3}) ) )\), and \(\mathcal{P}_{3} (\mathbb{U} (\widetilde{r_{2/3}^{\ast }}( \mathcal{P}_{3}) ) )\) are strongly starlike of order \(1/3\), \(1/2\), and \(2/3\), respectively.
Example 6
For \(n=3\) we have
where the roots of \(P_{5}\) are \(z_{0}=0\), \(z_{1}=\pm {\sqrt{245-14\sqrt{70}}}/{21}\), and \(z_{2}=\pm {\sqrt{245+14\sqrt{70}}}/{21}\). From Theorem 2 it follows that the radii of strong starlikeness of order \(1/3\), \(1/2\), and \(2/3\) of \(\mathcal{P}_{5}\) are \(\widetilde{r_{1/3}^{\ast }}(\mathcal{P}_{5})\simeq 0.2212264225 \ldots\) , \(\widetilde{r_{1/2}^{\ast }}(\mathcal{P}_{5})\simeq 0.2537535993 \ldots\) , and \(\widetilde{r_{2/3}^{\ast }}(\mathcal{P}_{5})\simeq 0.2724589258 \ldots\) , where \(\widetilde{r_{1/3}^{\ast }}(\mathcal{P}_{5})\), \(\widetilde{r_{1/2}^{\ast }}(\mathcal{P}_{5})\), and \(\widetilde{r_{2/3}^{\ast }}(\mathcal{P}_{5})\) denote the smallest positive roots of the equations
and
respectively. According to the above result, the domains \(\mathcal{P}_{5} (\mathbb{U} (\widetilde{r_{1/3}^{\ast }}( \mathcal{P}_{5}) ) )\), \(\mathcal{P}_{5} (\mathbb{U} (\widetilde{r_{1/2}^{\ast }}( \mathcal{P}_{5}) ) )\), and \(\mathcal{P}_{5} (\mathbb{U} (\widetilde{r_{2/3}^{\ast }}( \mathcal{P}_{5}) ) )\) are strongly starlike of order \(1/3\), \(1/2\), and \(2/3\), respectively.
Letting \(\alpha =1\) in the above theorem, we get the following corollary.
Corollary 4
The radius of starlikeness of\(\mathcal{P}_{2n-1}\)is\(r^{\ast }(\mathcal{P}_{2n-1})=r^{*}_{2}\), where\(r^{*}_{2}\)denotes the smallest positive root of the equation
Example 7
For \(n=2\) we have
where the roots of \(P_{3}\) are \(z_{0}=0\) and \(z_{1}=\pm {\sqrt{15}}/{5}\). From Corollary 4 it follows that the radius of starlikeness of \(\mathcal{P}_{3}\) is \(r^{\ast }(\mathcal{P}_{3})={1}/{\sqrt{5}}\simeq 0.4472135954\ldots\) , where \({1}/{\sqrt{5}}\) denotes the smallest positive root of the equation
According to the above result, as Fig. 3, the domain \(\mathcal{P}_{3} (\mathbb{U} ({1}/{\sqrt{5}} ) )\) is starlike.
Remark 2
All the figures inserted in this article have been obtained using MAPLE™ software.
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The second author was supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science, and Technology (No. 2019R1I1A3A01050861).
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Ebadian, A., Cho, N.E., Analouei Adegani, E. et al. Radii problems for some classes of analytic functions associated with Legendre polynomials of odd degree. J Inequal Appl 2020, 178 (2020). https://doi.org/10.1186/s13660-020-02443-4
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DOI: https://doi.org/10.1186/s13660-020-02443-4