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6.2. Some Liouville type theorems and removable singularity theorems [0550]

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6.2. Some Liouville type theorems and removable singularity theorems

In this subsection, we introduce some removable singularity and Liouville type theorems, which will be needed in the proof of Proposition 7.15. For the convenience of discussions, we give precise statement here.

Lemma 6.5 (Removable singularity).

Let (Mn,g)(M^{n},g) be a Riemannian manifold such that BR​(p)B_{R}(p) has a compact closure in B2​R​(p)B_{2R}(p). Let KβŠ‚MnK\subset M^{n} be a smooth submanifold with dim(K)=k0≀nβˆ’3\dim(K)=k_{0}\leq n-3. If uu is harmonic in BR​(p)βˆ–KB_{R}(p)\setminus K and there is some ϡ∈(0,1)\epsilon\in(0,1) such that

(6.41) |u⁑(x)|≀Cdg​(x,K)(nβˆ’2βˆ’k0)βˆ’Ο΅,|u(x)|\leq\frac{C}{d_{g}(x,K)^{(n-2-k_{0})-\epsilon}},

then uu is harmonic in BR​(p)B_{R}(p).

Proof.

The point is to apply integration by parts to show that uu is a weak solution to Δ​u=0\Delta u=0 on BR​(p)B_{R}(p). The computations are routine and standard in the literature, so we just skip it. ∎

Lemma 6.6 (Liouville theorem on ℝm+n\mathbb{R}^{m+n}).

Given m,nβˆˆβ„€+m,n\in\mathbb{Z}_{+} with m+nβ‰₯3m+n\geq 3, Let ΞΌp∈(βˆ’1,1)βˆ–{0}\mu_{p}\in(-1,1)\setminus\{0\} and let u∈Cβˆžβ€‹(ℝm+n)u\in C^{\infty}(\mathbb{R}^{m+n}) be a harmonic function on the Euclidean space (ℝm+n,gℝmβŠ•gℝn)(\mathbb{R}^{m+n},g_{\mathbb{R}^{m}}\oplus g_{\mathbb{R}^{n}}). If uu satsifies

(6.42) |u⁑(x,y)|≀C|x|ΞΌp,βˆ€(x,y)∈(ℝmβˆ–{0})×ℝn,\displaystyle|u(x,y)|\leq\frac{C}{|x|^{\mu_{p}}},\ \forall(x,y)\in(\mathbb{R}^{m}\setminus\{0\})\times\mathbb{R}^{n},

then u≑0u\equiv 0 on ℝm+n\mathbb{R}^{m+n}.

Proof.

The proof is rather standard and straightforward, which can be achieved by using separation of variables.

For the simplicity of notations, we denote

(6.43) d≑m+nβ‰₯3.d\equiv m+n\geq 3.

Let (r,Θ)βˆˆβ„d(r,\Theta)\in\mathbb{R}^{d} be the polar coordinate system in ℝd\mathbb{R}^{d}, so the Laplacian of uu can be written as

(6.44) Δℝd​u=βˆ‚2uβˆ‚r2+dβˆ’1rβ‹…βˆ‚uβˆ‚r+1r2β‹…Ξ”π•Šdβˆ’1​u.\Delta_{\mathbb{R}^{d}}u=\frac{\partial^{2}u}{\partial r^{2}}+\frac{d-1}{r}\cdot\frac{\partial u}{\partial r}+\frac{1}{r^{2}}\cdot\Delta_{\mathbb{S}^{d-1}}u.

We make separation of variables on the punctured Euclidean space ℝdβˆ–{0d}\mathbb{R}^{d}\setminus\{0^{d}\}. Let

(6.45) Ξ»j≑j⁑(j+dβˆ’2),jβˆˆβ„•,\lambda_{j}\equiv j(j+d-2),\ j\in\mathbb{N},

be the spectrum of the unit round sphere π•Šdβˆ’1\mathbb{S}^{d-1}. Correspondingly, let Ο†j∈Cβˆžβ€‹(π•Šdβˆ’1)\varphi_{j}\in C^{\infty}(\mathbb{S}^{d-1}) satisfy

(6.46) βˆ’Ξ”π•Šdβˆ’1​φj​(Θ)=Ξ»j​φj​(Θ).-\Delta_{\mathbb{S}^{d-1}}\varphi_{j}(\Theta)=\lambda_{j}\varphi_{j}(\Theta).

Then the function u⁑(r,Θ)u(r,\Theta) has the expansion along the fiber π•Šdβˆ’1\mathbb{S}^{d-1},

(6.47) u⁑(r,Θ)=βˆ‘j=0∞uj​(r)β‹…Ο†j​(Θ).u(r,\Theta)=\sum\limits_{j=0}^{\infty}u_{j}(r)\cdot\varphi_{j}(\Theta).

Immediately, for each jβˆˆβ„•j\in\mathbb{N}, the coefficient function uj​(r)u_{j}(r) solves the Euler-Cauchy equation,

(6.48) uj′′​(r)+dβˆ’1rβ‹…uj′​(r)βˆ’1r2β‹…Ξ»jβ‹…uj​(r)=0,u_{j}^{\prime\prime}(r)+\frac{d-1}{r}\cdot u_{j}^{\prime}(r)-\frac{1}{r^{2}}\cdot\lambda_{j}\cdot u_{j}(r)=0,

which has a general solution

(6.49) uj​(r)=Cjβ‹…rpj+Cjβˆ—β‹…rqj,u_{j}(r)=C_{j}\cdot r^{p_{j}}+C_{j}^{*}\cdot r^{q_{j}},

where pj=2βˆ’d+(dβˆ’2)2+4​λj2β‰₯0p_{j}=\frac{2-d+\sqrt{(d-2)^{2}+4\lambda_{j}}}{2}\geq 0 and qj=2βˆ’dβˆ’(dβˆ’2)2+4​λj2<0q_{j}=\frac{2-d-\sqrt{(d-2)^{2}+4\lambda_{j}}}{2}<0 solve the quadratic equation

(6.50) w2+(dβˆ’2)​wβˆ’Ξ»j=0.w^{2}+(d-2)w-\lambda_{j}=0.

So it is obvious

p0\displaystyle p_{0} =0,q0=2βˆ’dβ‰€βˆ’1,\displaystyle=0,\quad q_{0}=2-d\leq-1,
pj\displaystyle p_{j} β‰₯p1=1,\displaystyle\geq p_{1}=1,
(6.51) qj\displaystyle q_{j} ≀q1=1βˆ’dβ‰€βˆ’2,jβˆˆβ„€+.\displaystyle\leq q_{1}=1-d\leq-2,\quad j\in\mathbb{Z}_{+}.

In the following, we will show that, given the growth condition (6.42) for ΞΌp∈(βˆ’1,1)βˆ–{0}\mu_{p}\in(-1,1)\setminus\{0\}, then for each jβˆˆβ„•j\in\mathbb{N} and for each r>0r>0, the coefficient uj​(r)u_{j}(r) satisfies

(6.52) |uj​(r)|≀QjrΞΌp,|u_{j}(r)|\leq\frac{Q_{j}}{r^{\mu_{p}}},

where Qjβˆˆβ„Q_{j}\in\mathbb{R}. In fact, so it follows from the expansion (6.47) that for each jβˆˆβ„•j\in\mathbb{N},

(6.53) uj​(r)=βˆ«π•Šdβˆ’1u⁑(r,Θ)β‹…Ο†j​dvolπ•Šdβˆ’1,u_{j}(r)=\int_{\mathbb{S}^{d-1}}u(r,\Theta)\cdot\varphi_{j}\dvol_{\mathbb{S}^{d-1}},

which implies

(6.54) |uj​(r)|≀|Ο†j|Lβˆžβ€‹(π•Šdβˆ’1)β‹…βˆ«π•Šdβˆ’11|x|ΞΌp​dvolπ•Šdβˆ’1.|u_{j}(r)|\leq|\varphi_{j}|_{L^{\infty}(\mathbb{S}^{d-1})}\cdot\int_{\mathbb{S}^{d-1}}\frac{1}{|x|^{\mu_{p}}}\dvol_{\mathbb{S}^{d-1}}.

Next, we will write the above integral in the polar coordinates Ξ˜β‰‘(ΞΈ1,…,ΞΈdβˆ’1)\Theta\equiv(\theta_{1},\ldots,\theta_{d-1}) with ΞΈ1,…,ΞΈdβˆ’2∈[0,Ο€]\theta_{1},\ldots,\theta_{d-2}\in[0,\pi] and ΞΈdβˆ’1∈[0,2​π]\theta_{d-1}\in[0,2\pi]. Denote by dβ€‹Ξ˜β‰‘d​θ1∧d​θ2βˆ§β€¦βˆ§d​θdβˆ’1d\Theta\equiv d\theta_{1}\wedge d\theta_{2}\wedge\ldots\wedge d\theta_{d-1}, then it is by elementary calculations that, |x|=rmβ‹…βˆk=1dβˆ’m|sin⁑θk||x|=r^{m}\cdot\prod\limits_{k=1}^{d-m}|\sin\theta_{k}| and dvolπ•Šdβˆ’1=∏k=1dβˆ’2(sindβˆ’kβˆ’1⁑θk)β‹…dβ€‹Ξ˜\dvol_{\mathbb{S}^{d-1}}=\prod\limits_{k=1}^{d-2}(\sin^{d-k-1}\theta_{k})\cdot d\Theta. Therefore,

(6.55) βˆ«π•Šdβˆ’11|x|ΞΌp​dvolπ•Šdβˆ’1=1rΞΌpβ€‹βˆ«π’ŸΞ˜βˆk=1dβˆ’2(sindβˆ’kβˆ’1⁑θk)∏k=1dβˆ’m|sin⁑θk|ΞΌpβ‹…π‘‘Ξ˜,\int_{\mathbb{S}^{d-1}}\frac{1}{|x|^{\mu_{p}}}\dvol_{\mathbb{S}^{d-1}}=\frac{1}{r^{\mu_{p}}}\int_{\mathcal{D}_{\Theta}}\frac{\prod\limits_{k=1}^{d-2}(\sin^{d-k-1}\theta_{k})}{\prod\limits_{k=1}^{d-m}|\sin\theta_{k}|^{\mu_{p}}}\cdot d\Theta,

where π’ŸΞ˜β‰‘{0≀θ1,…,ΞΈdβˆ’2≀π, 0≀θdβˆ’1≀2Ο€}\mathcal{D}_{\Theta}\equiv\{0\leq\theta_{1},\ldots,\theta_{d-2}\leq\pi,\ 0\leq\theta_{d-1}\leq 2\pi\}. By assumption, ΞΌp∈(βˆ’1,1)βˆ–{0}\mu_{p}\in(-1,1)\setminus\{0\}, then ∏k=1dβˆ’2(sindβˆ’kβˆ’1⁑θk)∏k=1dβˆ’m|sin⁑θk|ΞΌp\frac{\prod\limits_{k=1}^{d-2}(\sin^{d-k-1}\theta_{k})}{\prod\limits_{k=1}^{d-m}|\sin\theta_{k}|^{\mu_{p}}} is integrable in π’ŸΞ˜\mathcal{D}_{\Theta} and we denote

(6.56) ℐ0β‰‘βˆ«π’ŸΞ˜βˆk=1dβˆ’2(sindβˆ’kβˆ’1⁑θk)∏k=1dβˆ’m|sin⁑θk|ΞΌpβ‹…π‘‘Ξ˜.\mathcal{I}_{0}\equiv\int_{\mathcal{D}_{\Theta}}\frac{\prod\limits_{k=1}^{d-2}(\sin^{d-k-1}\theta_{k})}{\prod\limits_{k=1}^{d-m}|\sin\theta_{k}|^{\mu_{p}}}\cdot d\Theta.

Therefore, for each jβˆˆβ„•j\in\mathbb{N}, it holds that

(6.57) |uj​(r)|≀ℐ0β‹…|Ο†j|Lβˆžβ€‹(π•Šdβˆ’1)rΞΌp≑QjrΞΌp|u_{j}(r)|\leq\frac{\mathcal{I}_{0}\cdot|\varphi_{j}|_{L^{\infty}(\mathbb{S}^{d-1})}}{r^{\mu_{p}}}\equiv\frac{Q_{j}}{r^{\mu_{p}}}

for all r>0r>0.

Now we go back to the representation of uj​(r)u_{j}(r) in (6.49) and we analyze the growth behavior of function as rβ‰ͺ1r\ll 1 and r≫1r\gg 1. Applying the assumption ΞΌp∈(βˆ’1,1)βˆ–{0}\mu_{p}\in(-1,1)\setminus\{0\} and the gap obtained in (6.51), we have that, for each jβˆˆβ„•j\in\mathbb{N}, Cj=Cjβˆ—=0C_{j}=C_{j}^{*}=0. Therefore,

(6.58) u≑0​on​ℝm+n.u\equiv 0\ \text{on}\ \mathbb{R}^{m+n}.

∎

Lemma 6.7 (Liouville theorem on a cylinder).

Let (Q,gQ)≑(D×ℝ,gQ)(Q,g_{Q})\equiv(D\times\mathbb{R},g_{Q}) be a cylinder with a product Riemannian metric gQ=gDβŠ•d​z2g_{Q}=g_{D}\oplus dz^{2}, where (D,gD)(D,g_{D}) is a closed Riemannian manifold. Denote by Ξ»D>0\lambda_{D}>0 the lowest eigenvalue of the Laplace-Beltrami operator of (D,gD)(D,g_{D}) acting on functions. If uu is a harmonic function on QQ satisfying the growth control

(6.59) |u|=O⁑(eΞ»cβ‹…z)|u|=O(e^{\lambda_{c}\cdot z})

for some Ξ»c∈(0,Ξ»D)\lambda_{c}\in(0,\sqrt{\lambda_{D}}), then u≑0u\equiv 0.

The proof follows from standard separation of variables, very similar to the proof of Proposition 3.31. We omit the details.

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