Abstract
Let \(M\) be a complete, simply connected Riemannian manifold with negative curvature. We obtain some Moser–Trudinger inequalities with sharp constants on \(M\).
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1 Introduction
Moser [14] found the largest positive constant \(\beta _{0}\) such that if \(\Omega \) is an open domain in \({\mathbb {R}}^{n}\), \(n\ge 2\), with finite \(n\)-measure, then there exists a constant \(C_{0}\) which depends only on \(n\) such that if \(u\) is smooth and has compact support contained in \(\Omega \), then
for any \(\beta \le \beta _{0}\) when \(u\) is normalized so that
In fact, Moser showed \(\beta _{0}=n\omega ^{1/(n-1)}_{n-1}\), where \(\omega _{n-1}\) is the surface measure of the unit sphere in \({\mathbb {R}}^{n}\). This inequality sharpened the result of N. S. Trudinger [18]. In 1988, D. Adams extended such inequality to high-order Sobolev spaces in \({\mathbb {R}}^{n}\) via a quite different method. In the case of unbounded domains, Ruf [16] and Li-Ruf [11] obtained the following inequality:
for any \(u\in C^{\infty }_{0}({\mathbb {R}}^{n})\) when \(u\) is normalized so that
The constant \(\beta _{0}\) in (1.2) is also sharp.
There has also been substantial progress for Moser–Trudinger inequalities on Riemannian manifolds. In the case of compact Riemannian manifolds, the study of Trudinger-Moser inequalities can be traced back to Aubin [3], Cherrier [4, 5], and Fontana [6]. In particular, the following Moser–Trudinger inequality is held in \(n\)-dimensional compact Riemannian manifold (\(M\), \(g\)) (see [6]):
The constant \(\beta _{0}\) in (1.3) is also sharp. In the case of complete noncompact Riemannian manifolds, Yang [19] has showed that if the Ricci curvature has a lower bound and the injectivity radius has a positive lower bound, then Trudinger-Moser inequality holds. However, the constant obtained in [19] is not sharp. Furthermore, if \(M\) is the hyperbolic space \({\mathbb {H}}^{2}\), Mancini and Sandeep [12] (see also [2]) proved the following inequality on \({\mathbb {H}}^{2}\):
where \(\mathbb {B}^{2}\) is the unit ball at origin of \({\mathbb {R}}^{2}\). Furthermore, the constants \(4\pi \) is sharp. Later, inequality (1.4) has been extended by themselves and Tintarev [13] to any dimension.
To our knowledge, much less is known about sharp constants of Moser–Trudinger inequalities on complete noncompact Riemannian manifolds except Euclidean spaces and Hyperbolic spaces. The aim of this paper is to look for the sharp constants of Moser–Trudinger inequalities on a complete, simply connected Riemannian manifold \(M\) with negative curvature. In fact, the optimal constants turn out to be the same for every such \(M\) as they are in Euclidean space. For simplicity, we also denote by \(\Delta \) the Laplace-Beltrami operator on \(M\) and by \(\nabla \) the corresponding gradient. Let \(\Omega \) be a domain in \(M\). The Sobolev space \(W_{0}^{1,n}(\Omega )\) is the completion of \(C^{\infty }_{0}(\Omega )\) under the norm
One of our main results is the following
Theorem 1.1
Let \(M\) be a complete, simply connected Riemannian manifold of dimension \(n\ge 2\) and \(\Omega \) be a domain in \(M\) with \(|\Omega |=\int _{\Omega }\hbox {d}V<\infty \). There exists a positive constant \(C_{1}=C_{1}(n,M)\) such that for all \(u\in W_{0}^{1,n}(\Omega )\) with \(\int _{\Omega }|\nabla u|^{n}\hbox {d}V\le 1\), the following uniform inequality holds
Furthermore, the constant \(\beta _{0}\) in (1.5) is sharp.
Next we consider the Moser–Trudinger inequalities on the whole space \(M\). The basic idea of the proof is given by Lam and Lu [8, 9], and the main result is the following
Theorem 1.2
Let \(M\) be a complete, simply connected Riemannian manifold of dimension \(n\ge 2\) and \(\tau \) be any positive number. There exists a constant \(C_{2}=C_{2}(\tau ,n,M)\) such that for all \(u\in W_{0}^{1,n}(M)\) with \(\int _{M}(|\nabla u|^{n}+\tau |u|^{n})\hbox {d}V\le 1\), the following uniform inequality holds
Furthermore, the constant \(\beta _{0}\) in (1.6) is sharp.
2 Notations and preliminaries
We begin by quoting some preliminary facts which will be needed in the sequel and refer to [7, 10, 17] for more precise information about this subject.
Let \(M\) be an \(n\)-dimensional complete Riemannian manifold with Riemannian metric \(\mathrm{d}s^{2}\). If \(\{x^{i}\}_{1\le i\le n}\) is a local coordinate system, then we can write
so that the Laplace-Beltrami operator \(\Delta \) in this local coordinate system is
where \(g=\det (g_{ij})\) and \((g^{ij})=(g_{ij})^{-1}\). Denote by \(\nabla \) the corresponding gradient.
Let \(K\) be the sectional curvature on \(M\). \(M\) is said to be with negative curvature (respectively, with strictly negative curvature) if \(K\le 0\) (respectively, \(K\le c<0\)) along each plane section at each point of \(M\). If \(M\) is with negative curvature, then for each \(p\in M\), \(M\) contains no points conjugate to \(p\). Furthermore, if \(M\) is simply connected, then the exponential mapping \(\mathrm Exp _{p}: T_{p}M\rightarrow M\) is a diffeomorphism, where \(T_{p}M\) is the tangent space to \(M\) at \(p\) (see e.g. [7]).
From now on, we let \(M\) be a complete, simply connected Riemannian manifold with negative curvature. Let \(p\in M\) and denote by \(\rho (x)=\mathrm dist (x,p)\) for all \(x\in M\), where \(\mathrm{dist}(\cdot ,\cdot )\) denotes the geodesic distance. Then \(\rho (x)\) is smooth on \(M\setminus \{p\}\) and it satisfies
By Gauss’s lemma, the radial derivative \(\partial _{\rho }=\frac{\partial }{\partial \rho }\) satisfies
For any \(\delta >0\), denote by \(B_{\delta }(p)=\{x\in M: \rho (x)<\delta \}\) the geodesic ball in \(M\). We introduce the density function \(J_{p}(\theta ,t)\) of the volume form in normal coordinates as follows (see e.g. [7], page 166-167). Choose an orthonormal basis \(\{\theta ,e_{2},\ldots ,e_{n}\}\) on \(T_{p}M\) and let \(c(t)=\mathrm Exp _{p}t\theta \) be a geodesic. \(\{Y_{i}(t)\}_{2\le i\le n}\) are Jacobi fields satisfying the initial conditions
so that the density function can be given by
We note that \(J_{p}(\theta ,t)\) does not depend on \(\{e_{2},\ldots ,e_{n}\}\) and \(J_{p}(\theta ,t)\in C^{\infty }(T_{p}M\backslash \{p\})\) by the definition of \(J_{p}(\theta ,t)\). Furthermore, if we set \(J_{p}(\theta ,0)\equiv 1\), then \(J_{p}(\theta ,t)\in C(T_{p}M)\) and
since \(Y_{i}(t)\) has the asymptotic expansion (see e.g. [7], page 169)
where \(R(\cdot ,\cdot )\) is the curvature tensor on \(M\).
By the definition of \(J_{p}(\theta ,t)\), we have the following formula in polar coordinates on \(M\):
where \(\hbox {d}\sigma \) denotes the canonical measure of the unit sphere of \(T_{p}(M)\).
If \(M\) is with constant sectional curvature, then \(J_{p}(\theta ,t)\) depends only on \(t\). We denote by \(J_{b}(t)\) the corresponding density function if \(K\equiv -b\) for some \(b\ge 0\). It is well known that \(J_{0}(t)= 1\) for \(t>0\) since in this case \(M\) is isomorphic to the Euclidean space.
Finally, we recall a useful fact of \(J_{p}(\theta ,t)\) which play an important role in the study of Moser–Trudinger inequalities. If the sectional curvature \(K\) on \(M\) satisfies \(K\le -b\), then (see [7], page 172, line -2, the proof of Bishop-Gunther comparison theorem)
Therefore, since \(M\) is with negative curvature, we have
which means \(J_{p}(\theta ,t)\), as a function of \(t\) on \([0,+\infty )\), is monotonically increasing.
3 Proof of Theorem 1.1
We firstly show the following pointwise estimates for \(f\in C^{\infty }_{0}(M)\).
Lemma 3.1
There holds, for any \(f\in C^{\infty }_{0}(M)\) and \(p\in M\),
where \(\omega _{n-1}\) is the surface measure of the unit sphere \(\mathbb {S}^{n-1}\) in \({\mathbb {R}}^{n}\).
Proof
Since \(f\) has compact support, taking the radial derivative in an arbitrary direction, we have
Integrating both sides over the unit sphere yields
Using polar coordinate and (2.1), we have
This concludes the proof of lemma 3.1.
We now recall the rearrangement of functions on \(M\). Suppose \(F\) is a nonnegative function on \(M\). The non-increasing rearrangement of is defined by
where \(\lambda _{F}(s)=|\{x\in M: F(x)>s\}|\). Here we use the notation \(|\Sigma |\) for the measure of a measurable set \(\Sigma \subset M\).
Lemma 3.2
Let \(g=\frac{1}{\rho ^{n-1}J_{p}(\theta ,\rho )}\) be in the Lemma 3.1. Then
Proof
Define, for any \(s>0\),
We note that \(\rho ^{n-1}J_{p}(\theta ,\rho )\), as a function of \(\rho \) on \([0,+\infty )\), is strictly decreasing since \(J_{p}(\theta ,\rho )\), as a function of \(\rho \) on \([0,+\infty )\), is monotonically increasing. Therefore, for every \(\theta \in \mathbb {S}^{n-1}\) and \(s>0\), the equation \(\rho ^{n-1}J_{p}(\theta ,\rho )=s^{-1}\) has only one solution in \((0,+\infty )\) and we denote it by \(\rho _{\theta }(s)\). Then \(\rho _{\theta }(s)\) satisfies
and
Therefore, since \(g^{*}(t)=\inf \{s>0: \lambda _{g}(s)\le t\}\),
where \(\rho _{\theta }(g^{*}(t))\) satisfies
For simplicity, we set \(\rho _{\theta }(t)=\rho _{\theta }(g^{*}(t))\) in the rest of proof. Then,
and \(\rho _{\theta }(t)\) satisfies
Thus, since \(J_{p}(\theta ,\rho )\), as a function of \(\rho \) on \([0,+\infty )\), is monotonically increasing and \(J_{p}(\theta ,\rho )\ge J_{p}(\theta ,0)=1\), we have
The desired result follows.
Define \(F^{**}(t)=\frac{1}{t}\int ^{t}_{0}F^{*}(t)\hbox {d}t\), where \(F^{*}\) is defined in (3.2). Before the proof of Theorem 1.1, we need the following lemma from Adams’ paper [1].
Lemma 3.3
Let \(a(s,t)\) be a nonnegative measurable function on \((-\infty ,+\infty )\times [0,+\infty )\) such that (a.e.)
where \(n'=\frac{n}{n-1}\). Then there is a constant \(c_{0}=c_{0}(n,b)\) such that if for \(\phi \ge 0\) with \(\int ^{\infty }_{-\infty }\phi (s)^{n}\hbox {d}s\le 1\), then
where
Proof of Theorem 1.1
The proof use ideas from [1] and the main tool is O’Neil’s lemma ([15], Lemma 1.5). Let \(u\in C^{\infty }_{0}(\Omega )\) be such that \(\int _{\Omega }|\nabla u|^{n}\mathrm{d}V\le 1\). Without loss of generality, we may assume \(u\ge 0\). By Lemma 3.1 and O’Neil’s lemma, for \(t>0\),
where \(g=\frac{1}{\rho ^{n-1}J_{p}(\theta ,\rho )}\). By Lemma 3.2,
Combining (3.6) and (3.7) yields
Following [1], we set
Then
The auxiliary function \(a(s,t)\) is defined to be
where \(n'=n/(n-1)\). It is easy to check
By Lemma 3.3,
where
On the other hand, by (3.8),
Using the change of variables \(t\rightarrow |\Omega |e^{-t}\), one can check that
This concludes the proof of the first statement of the theorem.
To prove the second statement, we let \(\Omega =B_{1}=\{x\in M:\rho (x)<1\}\). Set, for each \(\varepsilon \in (0,1)\),
where \(B_{\varepsilon }=\{x\in M:\rho (x)<\varepsilon \}\). We compute
and
By the asymptotic expansion of \(J_{p}(\theta ,\rho )\) (see (2.2)), it is easy to check
Now assume that
for some \(\beta >0\). Using the fact \(f_{\varepsilon }\equiv 1\) on \(B_{\varepsilon }\), we have
i.e.,
Passing the limit \(\varepsilon \rightarrow 0+\) and using (3.11) yields
This concludes the proof of Theorem.
4 Proof of Theorem 1.2
The proof of Theorem 1.2 follows closely Lam and Lu’s proof (see [8], section 2 or [9], section 5). Let \(u\in C^{\infty }_{0}(M)\) be such that \(\int _{M}(|\nabla u|^{n}+\tau |u|^{n})\mathrm{d}V\le 1\). Without loss of generality, we may assume \(u\ge 0\).
Set \(A(u)=2^{-\frac{1}{n(n-1)}}\tau ^{\frac{1}{n}}\Vert u\Vert _{n}\) and \(\Omega (u)=\{x\in M: u(x)> A(u)\}\), where \(\Vert u\Vert _{n}=\root n \of {\int _{M}|u|^{n}\mathrm{d}V}.\) Then
We write
By (4.1), \(M\setminus \Omega (u)=\{x\in M: 0\le u(x)\le A(u)\}\subset \{x\in M: 0\le u(x)\le 1\}\). Therefore,
Now we will show \(I_{1}\) is also bounded by a constant \(C_{3}(\tau ,n,M)\). Set
Then \(v\in W^{1,n}_{0}(\Omega )\) and
where we used the following elementary inequality
By Young’s inequality,
Combing (4.4) and (4.5) yields
where
Set
Since \(v\in W^{1,n}_{0}(\Omega )\), so does \(w\). Moreover, by (4.6),
We compute
Therefore,
To get the second inequality in (4.10), we use the following elementary inequality
By Theorem 1.1, there exists a constant \(C_{5}=C_{5}(n,M)\) such that
We have, by (4.8), (4.11) and (4.2),
This concludes the proof of the first statement of the theorem.
To prove the second statement, we employ the following Moser function sequence:
where \(\delta >0\) and \(\varepsilon \in (0,1)\). We compute
By the asymptotic expansion of \(J_{p}(\theta ,\rho )\) (see (2.2)), we have
Thus
Let \(\widetilde{g}_{\varepsilon }=g_{\varepsilon }/\Vert g_{\varepsilon }\Vert _{W_{0}^{1,n}(M)}\). It follows that, for \(\beta >\beta _{0}=n\omega ^{1/(n-1)}_{n-1}\),
as \(\varepsilon \rightarrow 0+\). This shows
if \(\beta >\beta _{0}\). The proof of Theorem 1.2 is thereby completed.
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Acknowledgments
The third author would like to express his sincere thanks to Professor Deng Guantie and School of Mathematical Science of Beijing Normal University for giving him a chance to be a visiting scholar. All the authors thank the referee for his/her careful reading and very useful comments which improved the final version of this paper.
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The first author is supported by the National Natural Science Foundation of China (No. 11201346). The second author is supported by Program for Innovative Research Team in UIBE. The third author is supported by the National Natural Science Foundation of China (No. 11101096 and No. 11301140).
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Yang, Q., Su, D. & Kong, Y. Sharp Moser–Trudinger inequalities on Riemannian manifolds with negative curvature. Annali di Matematica 195, 459–471 (2016). https://doi.org/10.1007/s10231-015-0472-4
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DOI: https://doi.org/10.1007/s10231-015-0472-4