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Abstract

In this paper, we mainly study the order of $q$-starlikeness of the well-known basic hypergeometric function. In addition, we obtain the Bieberbach-type problem for a generalized class of starlike functions. We also discuss the Fekete-szegö and the Hankel determinant problems for the same class of functions.

Results & Lemmas (10)

Each result is auto-extracted from the paper via OCR - the math is shown verbatim and may carry occasional transcription artifacts. Click to expand the full statement.

Theorem 2.1 · radius Theorem 2.1. Let a, b, c be non-negative real numbers with 0 < 1 − aq < 1 − cq and 0 < 1 − b < 1 − c. For 0 < q < 1 and r ∈ (0, 1], the…
Theorem 2.1. Let a, b, c be non-negative real numbers with 0 < 1 − aq < 1 − cq and 0 < 1 − b < 1 − c. For 0 < q < 1 and r ∈ (0, 1], the function z 7→ zΦ[a, b; c; q, rz] has the order of q-starlikeness $$\sigma_q(z\Phi[a,b;c;q,rz]) = 1 + \rho q \frac{(1-a)(1-b)}{(1-c)(1-q)} \frac{\Phi[aq,bq;cq;q,\rho]}{\Phi[a,b;c;q,\rho]}$$ where $$\rho = -r \text{ if } \frac{q(1-a)}{a(1-q)} =: s > 0 \text{ and } \rho = r \text{ if } s < 0.$$ In particular, we have $$1 + \frac{s\rho}{1 - \rho} \le \sigma_q(z\Phi[a, b; c; q, rz]) \le 1 + \frac{\rho s(1 - b)}{2(1 - c)}.$$ From this we can observe the following Remark 2.2. The case s < 0 with r = 1 in Theorem [2.1](#page-2-1) is considered in the limiting sense. In this case, the lower bound 1 + sr 1 − r is equal to −∞. Proof of Theorem 2.1. Set $\Phi(z) = \Phi[a, b; c; q, z]$ and $f(z) = z\Phi(z)$ . Now, by (1.3) we have $$\begin{array}{lcl} (D_q f)(z) & = & \dfrac{\Phi(z) - q \Phi(qz)}{1 - q} \\ \\ & = & \dfrac{\Phi(z) - q \Phi(z) + q \Phi(z) - q \Phi(qz)}{1 - q} \\ \\ & = & \dfrac{\Phi(z)(1 - q) + q(\Phi(z) - \Phi(qz))}{1 - q} \\ \\ & = & \Phi(z) + zq(D_q \Phi)(z). \end{array}$$ Hence. (2.1) $$w = \frac{z(D_q f)(z)}{f(z)} = 1 + zq \frac{(1-a)(1-b)}{(1-c)(1-q)} \frac{\Phi[aq, bq; cq; q, z]}{\Phi[a, b; c; q, z]},$$ where the last equality holds by [7, 1.12(ii), pp. 27]. Recall the difference equation stated in [1], which is equivalent to $$\frac{\Phi[aq,bq;cq;q,z]}{\Phi[a,b;c;q,z]} = \frac{(1-c)}{a(1-b)z} \left[ \frac{\Phi[aq,b;c;q,z]}{\Phi[a,b;c;q,z]} - 1 \right].$$ Substituting this ratio in (2.1), we get $$w = 1 + s \left[ \frac{\Phi[aq, b; c; q, z]}{\Phi[a, b; c; q, z]} - 1 \right] = 1 - s + s \frac{\Phi[aq, b; c; q, z]}{\Phi[a, b; c; q, z]},$$ where s is defined in the statement of our theorem with $q \in (0,1)$ . It follows from [1] that w has an integral representation (2.2) $$w = 1 - s + s \int_0^1 \frac{1}{1 - tz} d\mu(t),$$ with the non-negative real numbers a,b,c satisfying the conditions $0 \le 1 - aq \le 1 - cq$ and 0 < 1 - b < 1 - c. Now, for s > 0, $r \in (0,1]$ and from equation (2.2) it follows that the minimum of Re w for $|z| \le r$ is attained at the point z = -r and that the minimum is $1 - \frac{rs}{(1+r)}$ . Secondly, for s < 0, $r \in (0,1]$ and from equation (2.2), it follows that the minimum of Re w for $|z| \le r$ is attained at the point z = r and that the minimum is $1 + \frac{rs}{(1-r)}$ . This in combination with (2.1), yields the order of q-starlikeness of $z\Phi[a,b;c;q,rz]$ . The upper estimate for Re w follows from (2.1) and an integral representation of the ratio $\Phi[aq,bq;cq;q,z]/\Phi[a,b;c;q,z]$ obtained in [1, Theorem 2.13]. Hence, the conclusion of our theorem follows immediately. Remark 2.3. Making the substitutions $a \to q^a$ , $b \to q^b$ and $c \to q^c$ , and taking the limit as $q \to 1^-$ , we achieve the result of Küstner [15, Theorem 1.1] as special case.
Corollary 2.4 Corollary 2.4. Let, a,b,c be non-negative real numbers such that and. Then where.
Corollary 2.4. Let $q \in (0,1)$ , a,b,c be non-negative real numbers such that $1 > a \ge b \ge c$ and $r \in (0,1]$ . Then $$z\Phi[a,b;c;q,rz] \in \mathcal{S}_q\left(1-\frac{rs}{1+r}\right),$$ where $$s = \frac{q(1-a)}{a(1-q)}$$ .
Corollary 2.5 Corollary 2.5. Let a, b, c be non-negative real numbers such that. Then where. In particular, when s=2, the shifted basic hypergeometric…
Corollary 2.5. Let a, b, c be non-negative real numbers such that $1 > a \ge b \ge c$ . Then $$z\Phi[a,b;c;q,z] \in \mathcal{S}_q(1-s/2),$$ where $$s = \frac{q(1-a)}{a(1-q)}$$ . In particular, when s=2, the shifted basic hypergeometric function $z\Phi[a,b;c;q,z] \in \mathcal{S}_q$ . When we put $a=q^a,b=q^b$ and $c=q^c$ and allow $q\to 1^-$ , then Corollary 2.5 leads to an well-known result on the order of starlikeness of the Gaussian hypergeometric functions namely,
Corollary 2.6 Corollary 2.6. [25, Theorem B] Let a, b, c be non-negative real numbers such that. Then This result on Gaussian hypergeometric function of…
Corollary 2.6. [25, Theorem B] Let a, b, c be non-negative real numbers such that $a \le b \le c$ . Then $$zF(a, b; c; z) \in \mathcal{S}^*(1 - a/2).$$ This result on Gaussian hypergeometric function of Corollary 2.6 is not only interesting by itself, but also useful and employed for further research in geometric function theory. Many researchers used this result, particularly Ponnusamy and Sahoo in [23] used it innovatively to study pre-Schwarzian norm estimates for integral operators (defined by convolution) of functions belonging to special subclasses of the class of univalent functions with hypergeometric functions. Similarly, we expect that these results on basic hypergeometric functions will be fruitful and pave the way for further research in function theory as well as in physics.
Lemma 3.1 Lemma 3.1. [16, pp. 254-256] Let the function and be given by the power series (3.1). Then for some x and z satisfying,, and.
Lemma 3.1. [16, pp. 254-256] Let the function $p \in \mathcal{P}$ and be given by the power series (3.1). Then $$2p_2 = p_1^2 + x(4 - p_1^2),$$ $$4p_3 = p_1^3 + 2(4 - p_1^2)p_1x - p_1(4 - p_1^2)x^2 + 2(4 - p_1^2)(1 - |x|^2)z,$$ for some x and z satisfying $|x| \le 1$ , $|z| \le 1$ , and $p_1 \in [0,2]$ .
Lemma 3.2 Lemma 3.2. [19, Lemma 1] Let the function and be given by the power series (3.1). Then for any real number, and the result is sharp.
Lemma 3.2. [19, Lemma 1] Let the function $p \in \mathcal{P}$ and be given by the power series (3.1). Then for any real number $\lambda$ , $$|p_2 - \lambda p_1^2| \le 2 \max\{1, |2\lambda - 1|\}$$ and the result is sharp.
Lemma 3.3 Lemma 3.3. (Carathédory lemma). If a function, then The result is sharp for 3.1. The Bieberbach-type problem. The Bieberbach-type problem…
Lemma 3.3. (Carathédory lemma). If a function $p(z) = 1 + \sum_{n=1}^{\infty} p_n z^n \in \mathcal{P}$ , then $|p_n| \leq 2, n = 1, 2, \ldots$ The result is sharp for $$p(z) = \frac{1+z}{1-z} = 1 + \sum_{n=1}^{\infty} 2z^n.$$ 3.1. The Bieberbach-type problem. The Bieberbach-type problem for the class $S_q$ is investigated and we prove the following result.
Theorem 3.4 · coeff Theorem 3.4. If, then for all, Equality holds for the function F satisfying.
Theorem 3.4. If $f(z) = z + \sum_{n=2}^{\infty} a_n z^n \in \mathcal{S}_q$ , then for all $n \geq 2$ , $$|a_n| \le \prod_{j=2}^n \left( \frac{\frac{1-q^{j-1}}{1-q}+1}{\frac{1-q^j}{1-q}-1} \right).$$ Equality holds for the function F satisfying $z(D_qF)(z)/F(z) = (1+z)/(1-z)$ .
Theorem 3.5 · coeff Theorem 3.5. Let be of the form (1.1) and be any complex number. Then Equality occurs for the functions F and G satisfying and (3.8)
Theorem 3.5. Let $f \in \mathcal{S}_q$ be of the form (1.1) and $\mu$ be any complex number. Then $$|a_3 - \mu a_2^2| \le \max \left\{ \left| \frac{2(2+q) - 4\mu(1+q)}{q^2(1+q)} \right|, \frac{2}{q(1+q)} \right\}.$$ Equality occurs for the functions F and G satisfying $$\frac{z(D_q F)(z)}{F(z)} = \frac{1+z}{1-z}$$ and (3.8) $$\frac{z(D_qG)(z)}{G(z)} = \frac{1+z^2}{1-z^2}.$$
Theorem 3.7 · coeff Theorem 3.7. Let be of the form (1.1). Then Equality occurs for the function G(z) defined in (3.8).
Theorem 3.7. Let $f \in S_q$ be of the form (1.1). Then $$|H_2(2)| = |a_2a_4 - a_3^2| \le \frac{4}{q^2(1+q)^2}.$$ Equality occurs for the function G(z) defined in (3.8).

Definitions (1)

Def 1.1 Definition 1.1. A function is said to be in the class of q-starlike functions of order, denoted by,, if Re Clearly, and as,. Set so that…
Definition 1.1. A function $f \in \mathcal{A}$ is said to be in the class of q-starlike functions of order $\alpha$ , denoted by $\mathcal{S}_q(\alpha)$ , $0 \le \alpha < 1$ , if Re $$\left(\frac{z(D_q f)(z)}{f(z)}\right) > \alpha, \quad z \in \mathbb{D}.$$ Clearly, $S_q(\alpha) \supset S_q^(\alpha)$ and as $q \to 1^-$ , $S_q(\alpha) = S^(\alpha)$ . Set $S_q := S_q(0)$ so that as $q \to 1^-$ , $S_q(0) = S^*$ . In Section 2, we establish a result on the order of q-starlikeness of shifted basic hypergeometric functions $$z\Phi[a,b;c;q,z] = z \sum_{n=0}^{\infty} \frac{(a;q)_n(b;q)_n}{(c;q)_n(q;q)_n} z^n, \quad z \in \mathbb{D},$$ where $(a;q)_n = (1-a)(1-aq)(1-aq^2)\cdots(1-aq^{n-1})$ , $(a;q)_0 = 1$ with $0 \le q < 1$ , a,b,c are real parameters and $(c;q)_n \ne 0$ . For the basic properties of Heine's hypergeometric functions the basic references are [3,27]. Interestingly, the replacements of a,b and c by $q^a,q^b$ and $q^c$ respectively, then as $q \to 1^-$ , the function $\Phi[q^a,q^b;q^c;q,z]$ tends to the well-known Gaussian hypergeometric functions $$zF(a,b;c;z) = z \sum_{n=0}^{\infty} \frac{(a)_n(b)_n}{(c)_n(1)_n} z^n, \quad z \in \mathbb{D},$$ where a, b, c are real parameters, (a)<sup>0</sup> = 1, (a)<sup>n</sup> = a(a+ 1)· · ·(a+n−1) is the Pochhammer symbol and c is neither 0 nor a negative integer (except in special cases where a = −m or b = −m and c = −p with p > m).
Function classes studied:

Coefficient bounds & claims (4)

Machine-extracted from the paper text - useful for cross-referencing, not a verified fact.
coefficient_bound
S_q: |a3 - mu*a2^2| <= (2/q(1+q)) * max(|(2(2+q) - 4mu(1+q))/(q(1+q))|, 1) (sharp) [Theorem 3.5]
coefficient_bound
H_2(2) = |a2*a4 - a3^2| ≤ 4/(q**2*(1+q)**2) for class S_q (sharp) [Theorem 3.7]
function_family
Class S_q(alpha): f in A with Re(z(D_q f)(z)/f(z)) > alpha for z in D, where D_q is the q-difference operator, 0 <= alpha < 1
function_family
Class S_q: S_q(0): f in A with Re(z(D_q f)(z)/f(z)) > 0, the q-starlike functions

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