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A reverse Mulholland-type inequality in the whole plane
Journal of Inequalities and Applications volume 2018, Article number: 79 (2018)
Abstract
We present a new reverse Mulholland-type inequality in the whole plane with a best possible constant factor by introducing multiparameters, applying weight coefficients, and using the Hermite–Hadamard inequality. Moreover, we consider equivalent forms and some particular cases.
1 Introduction
Assuming that \(p > 1,\frac{1}{p} + \frac{1}{q} = 1,a_{m},b_{n} \ge 0,0 < \sum_{m = 1}^{\infty} a_{m}^{p} < \infty\), and \(0 < \sum_{n = 1}^{\infty} b_{n}^{q} < \infty\), the Hardy–Hilbert inequality is provided as follows (see [1]):
where \(\frac{\pi}{\sin (\pi /p)}\) is the best possible constant factor. By Theorem 343 in [1] (replacing \(\frac{a_{m}}{m}\) and \(\frac{b_{n}}{n}\) by \(a _{m}\) and \(b _{n}\), respectively), it yields the following Mulholland inequality with the same best value:
Inequalities (1) and (2) play an important role in analysis and its applications (see [1, 2]).
In 2007, Yang [3] published a Hilbert-type integral inequality in the whole plane. Various extensions of (1)–(2) and Yang’s work have been presented since then [4–12]. Recently, Yang and Chen [13] presented the following extension of (1) in the whole plane:
where the constant factor \(2B(\lambda_{1},\lambda_{2})\ (0 < \lambda_{1},\lambda_{2} \le 1,\lambda_{1} + \lambda_{2} = \lambda,\xi,\eta \in [0,\frac{1}{2}])\) is the best possible. In addition, Xin et al. [14] also carried out a similar result, and Zhong et al. [15] gave the reverse Mulholland’s inequality in the whole plane.
In this paper, we present a new reverse Mulholland-type inequality in the whole plane with a best possible constant factor, which is similar to the results of [13], via introducing multiparameters, applying weight coefficients, and using the Hermite–Hadamard inequality. Moreover, we consider equivalent forms and some particular cases.
2 An example and two lemmas
We further assume that \(\lambda_{1},\lambda_{2} > 0,\lambda_{1} + \lambda_{2} = \lambda \le 1,\xi,\eta \in [0,\frac{1}{2}], \alpha,\beta \in [\arccos \frac{1}{3},\frac{\pi}{2}]\), and
Remark 1
Since \(\alpha,\beta \in [\arccos \frac{1}{3},\frac{\pi}{ 2}],\xi,\eta \in [0,\frac{1}{2}]\), it follows that
Example 1
We set \(g(u): = \frac{\ln u}{u - 1}\ (u > 0),g(1): = \lim_{u \to 1}g(u) = 1\). Then we have \(g(u) > 0,g'(u) < 0,g''(u) > 0\ (u > 0)\). By Tailor’s formula we find
and then \(g^{(k)}(1) = \frac{( - 1)^{k}k!}{k + 1}\ (k = 0,1,2, \ldots )\). Hence, \(g^{(0)}(1) = g(1) = 1,g'(1) = - \frac{1}{2},g''(1) = \frac{2}{3}\). It is evident that \(g(u) > 0\). We obtain \(g'(u) = \frac{h(u)}{u(u - 1)^{2}},h(u): = u - 1 - u\ln u\). Since
it follows that \(h_{\max} = h(1) = 0\) and \(h(u) < 0\ (u \ne 1)\). Then we have \(g'(u) < 0\ (u \ne 1)\). Since \(g'(1) = - \frac{1}{2} < 0\), it follows that \(g'(u) < 0\ (u > 0)\). We find
\(J'(u) = - 4(u - 1) + 4u\ln u\), and
It follows that \(J'_{\min} = J'(1) = 0\), \(J'(u) > 0\ (u \ne 1)\), and \(J(u)\) is strictly increasing. Since \(J(1) = 0\), we have
and \(g''(u) > 0\ (u \ne 1)\). Since \(g''(1) = \frac{2}{3} > 0\), we find \(g''(u) > 0\ (u > 0)\).
For \(0 < \lambda \le 1,0 < \lambda_{2} < 1\), setting \(G(u): = g(u^{\lambda} )u^{\lambda_{2} - 1}\ (u > 0)\), we have \(G(u) > 0\),
We set \(F(x,y): = \frac{\ln (x/y)}{x^{\lambda} - y^{\lambda}}\ (\frac{y}{x})^{\lambda_{2} - 1}(x,y > 0)\). Since \(F(x,y) = \frac{1}{x^{\lambda}} G(\frac{y}{x})\), we have
Hence, for \(x,y > 1\), we have
Lemma 1
If \(f(u) > 0,f'(u) < 0,f''(u) > 0\ (u > \frac{3}{2})\) and \(\int_{\frac{3}{2}}^{\infty} f(u) \,du < \infty\), then we have the following Hermite–Hadamard inequality (see [16]):
and then
For \(\vert x \vert , \vert y \vert \ge \frac{3}{2}\), define
\(A_{\eta,\beta} (y) = \vert y - \eta \vert + (y - \eta )\cos \beta\), and
We define two weight coefficients as follows:
where \(\sum_{ \vert j \vert = 2}^{\infty} \cdots = \sum_{j = - 2}^{ - \infty} \cdots+ \sum_{j = 2}^{\infty} \cdots\) (\(j = m,n\)).
Lemma 2
We have the inequalities
where
Proof
For \(\vert m \vert \in \mathbf{N}\backslash \{ 1\}\), let
Then the equality
yields
Since \(0 < \lambda \le 1,0 < \lambda_{2} < 1\), by Example 1 we find that, for \(y > \frac{3}{2}\),
from which it follows that
are strictly decreasing and convex in (\(\frac{3}{2},\infty \)). Then (5) and (11) yield that
Setting \(u = \frac{\ln [(y + \eta )(1 - \cos \beta )]}{\ln A_{\xi,\alpha} (m)}\ (u = \frac{\ln [(y - \eta )(1 + \cos \beta )]}{\ln A_{\xi,\alpha} (m)})\) in the first (second) integral, from Remark 1 we obtain
by simplifications. Similarly, (5) and (11) also yield that
where \(\theta (\lambda_{2},m)( < 1)\) is defined in (10). Since
there exists a positive constant C such that \(\frac{\ln u}{u^{\lambda} - 1}u^{\lambda_{2}/2} \le C\ (0 < u \le 1)\). Then for \(A_{\xi,\alpha} (m) \ge (2 + \eta )(1 + \cos \beta )\), we have
Hence, (9) and (10) are valid. □
Similarly, we have the following:
Lemma 3
For \(0 < \lambda \le 1,0 < \lambda_{1} < 1\), we have the inequalities
where
Lemma 4
If \((\varsigma,\gamma ) = (\xi,\alpha )\) (or \((\eta,\beta )\)), \(\rho > 0\), then we have
Proof
By (5) we obtain
and
Therefore, (15) is valid. □
3 Main results and a few particular cases
Theorem 1
Suppose that \(0 < p < 1,\frac{1}{p} + \frac{1}{q} = 1\),
If \(a_{m},b_{n} \ge 0\ ( \vert m \vert , \vert n \vert \in \mathbf{N}\backslash \{ 1\} )\), satisfy
then for
we obtain the following equivalent reverse Mulholland-type inequalities:
Particularly, (i) for \(\alpha = \beta = \frac{\pi}{2},\xi,\eta \in [0,\frac{1}{2}]\), setting
we have the following equivalent reverse Mulholland-type inequalities:
(ii) For \(\xi = \eta = 0,\alpha,\beta \in [\arccos \frac{1}{3},\frac{\pi}{ 2}]\), setting
we have the following equivalent reverse Mulholland-type inequalities:
Proof
Applying the reverse Hölder inequality with weight (see [17]) and (8), we find
Then since \(0 < p < 1\), by (13) this yields
Combining (9) and (16), we obtain (18).
Using the reverse Hölders inequality again, we obtain
On the other-hand, assuming that (17) is valid, letting
we find
By (26) it follows that \(J_{1} > 0\). If \(J_{1} = \infty\), then (19) is trivially valid; if \(J_{1} < \infty\), then by (17) we have
Thus (18) is valid, which is equivalent to (17).
We further prove that (19) is equivalent to (17). Using the reverse Hölders inequality, we have
and then (19) is valid by (17).
On the other-hand, assuming that (17) is valid, we set
and find
If \(J_{2} = 0\), then (19) is impossible, so that \(J_{2} > 0\). If \(J_{2} = \infty\), then (19) is trivially valid; if \(J_{2} < \infty\), then by (17) we have
Thus (19) is valid, which is equivalent to (17).
Hence, inequalities (17), (18), and (19) are equivalent. □
Theorem 2
Under the assumptions in Theorem 1,
is the best possible constant factor in (17), (18), and (19).
Proof
For \(0 < \varepsilon < \min \{ p\lambda_{1},p(1 - \lambda_{2})\}\), we set \(\tilde{\lambda}_{1} = \lambda_{1} - \frac{\varepsilon}{p}( \in (0,1)),\tilde{\lambda}_{2} = \lambda_{2} + \frac{\varepsilon}{p} ( \in (0,1))\), and
If there exists a positive number \(k \ge k(\lambda_{1})\) such that (17) is still valid when replacing \(k(\lambda_{1})\) by k, then, in particular, we have
We obtain from the previous results that
and then
namely, \(k(\lambda_{1}) = \frac{2\pi^{2}}{\lambda^{2}\sin^{2}(\frac{\pi \lambda_{1}}{\lambda} )}\csc^{\frac{2}{p}}\beta \csc^{\frac{2}{q}}\alpha \ge k\). Hence, \(k = k(\lambda_{1})\) is the best possible constant factor of (17).
The constant factor \(k(\lambda_{1})\) in (18) and (19) is still the best possible. Otherwise, we would reach a contradiction by (27) and (28) that the constant factor in (17) is not the best possible. □
Remark 2
(i) For \(\xi = \eta = 0\) in (20), setting
we have the following new inequality:
It follows that (20) is an extension of (29). In particular, for \(\lambda = 1,\lambda_{1} = \lambda_{2} = \frac{1}{2}\), setting
we have the following simple reverse Mulholland-type inequality in the whole plane:
(ii) If \(a_{ - m} = a_{m},b_{ - n} = b_{n}\ (m,n \in \mathbf{N}\backslash \{ 1\} )\), for \(m \in \mathbf{N}\backslash \{ 1\}\), setting
(20) reduces to
In particular, for \(\xi = \eta = 0,\lambda = 1,\lambda_{1} = \lambda_{2} = \frac{1}{2}\), setting
we have the following simple reverse Mulholland-type inequality:
4 Conclusions
In this paper, we obtain a new reverse Mulholland’s inequality in the whole plane with a best possible constant factor in Theorems 1–2. Equivalent forms and a few particular cases are considered. The method of real analysis is very important and is the key to prove the reverse equivalent inequalities with the best possible constant factor. The lemmas and theorems can provide an extensive account of this type inequalities.
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Acknowledgements
This work is supported by the National Natural Science Foundation (Nos. 61370186, 61640222, and 11401113) and Science and Technology Planning Project Item of Guangzhou City (No. 201707010229).
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BY carried out the mathematical studies, participated in the sequence alignment, and drafted the manuscript. JL participated in the design of the study and performed the numerical analysis. Both authors read and approved the final manuscript.
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Liao, J., Yang, B. A reverse Mulholland-type inequality in the whole plane. J Inequal Appl 2018, 79 (2018). https://doi.org/10.1186/s13660-018-1669-z
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DOI: https://doi.org/10.1186/s13660-018-1669-z