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arXiv:2608.19986v1 [math.AP] 20 Aug 2026

Weakly stable solutions of Serrin’s problem

Michael Eichmair Address: Michael Eichmair
University of Vienna
Faculty of Mathematics
Oskar-Morgenstern-Platz 1
1090 Vienna, Austria
https://orcid.org/0000-0001-7993-9536
michael.eichmair@univie.ac.at
and Thomas Koerber Address: Thomas Koerber
University of Vienna
Faculty of Mathematics
Oskar-Morgenstern-Platz 1
1090 Vienna, Austria
https://orcid.org/0000-0003-1676-0824
thomas.koerber@univie.ac.at
Abstract.

We prove that weakly stable solutions of Serrin’s problem are compact and therefore round balls.

1. Introduction

Let n2n\geq 2 and Ωn\Omega\subset\mathbb{R}^{n} a domain, i.e., open, nonempty, and such that Ω¯\bar{\Omega} is a properly embedded top-dimensional submanifold. We denote the mean curvature of Ω\partial\Omega with respect to the outward pointing normal μ(Ω)\mu(\Omega) by HH. We call Ω\Omega a solution of Serrin’s problem (1) if there is uC(Ω¯)u\in C^{\infty}(\bar{\Omega}) such that

(1) {Δu=nin Ω,u>0in Ω,u=0on Ω, and|Du|=1on Ω.\displaystyle\begin{cases}\quad-\Delta u=n\qquad&\text{in $\Omega$},\\ \quad u>0&\text{in $\Omega$},\\ \quad u=0&\text{on $\partial\Omega$, and}\\ \quad|Du|=1&\text{on $\partial\Omega$}.\end{cases}

Note that μ(Ω)=Du\mu(\Omega)=-Du on Ω\partial\Omega in this setting.

Using the method of moving planes, J. Serrin [19] has shown that if Ω\Omega is compact and a solution of (1), then Ω\Omega is a ball of radius 1. Subsequently, H. Weinberger [25] has found a short alternative proof of this fact. Such a result fails if Ω\Omega is allowed to be noncompact. Indeed, for all integers m,nm,\,n with 1mn11\leq m\leq n-1, the cylinder

(2) {ym:|y|<m/n}×nm\displaystyle\{y\in\mathbb{R}^{m}:|y|<m/n\}\times\mathbb{R}^{n-m}

is a solution of (1). In view of this observation, H. Berestycki, L. Caffarelli, and L. Nirenberg [2, p. 1110] have conjectured that if Ω\Omega is noncompact and a solution of (1), then Ω\Omega is either a ball of radius 11 or congruent to one of the cylinders described in (2). Indeed, they have made a similar conjecture for solutions Ω\Omega of the semilinear over-determined problem

(3) {Δu=f(u)in Ω,u>0in Ω,u=0on Ω, and|Du|=1on Ω,\displaystyle\begin{cases}\quad-\Delta u=f(u)\qquad&\text{in $\Omega$},\\ \quad u>0&\text{in $\Omega$},\\ \quad u=0&\text{on $\partial\Omega$, and}\\ \quad|Du|=1&\text{on $\partial\Omega$},\end{cases}

where fC()f\in C^{\infty}(\mathbb{R}). We note that, by the work of J. Serrin [19], if Ω\Omega is compact and a solution of (3), then Ω\Omega is a ball. Counterexamples to this conjecture have been found in, e.g., [20, 9] for certain choices of ff and, notably, by M. Fall, I. Minlend, and T. Weth [13] for the choice f=nf=n; see also [23] for a related positive result in this direction. In this paper, we show that, in the case where f=nf=n, the conjecture of H. Berestycki, L. Caffarelli, and L. Nirenberg holds under a natural additional assumption on Ω\Omega.

To explain this, recall that, by the pioneering work of H. Alt and L. Caffarelli [1], solutions of (3) are given by Ω={yn:u(y)>0}\Omega=\{y\in\mathbb{R}^{n}:u(y)>0\} where uC(n)u\in C^{\infty}(\mathbb{R}^{n}) is a critical point of the functional

J(u)=12{yn:u(y)>0}|Du|2{yn:u(y)>0}F(u).J(u)=\frac{1}{2}\,\int_{\{y\in\mathbb{R}^{n}:u(y)>0\}}|Du|^{2}-\int_{\{y\in\mathbb{R}^{n}:u(y)>0\}}F(u).

Here, FC()F\in C^{\infty}(\mathbb{R}) is such that F=fF^{\prime}=f; see also, e.g., [23]. In the case where f=nf=n, JJ is not bounded from below. It is therefore natural to study uC(n)u\in C^{\infty}(\mathbb{R}^{n}) that are critical for JJ given the relative volume of {yn:u(y)>0}\{y\in\mathbb{R}^{n}:u(y)>0\}. In this context, we call Ω\Omega weakly stable if

(4) Ω(f(0)H)ϕ2Ω(|Dϕ|2f(u)ϕ2)\displaystyle\int_{\partial\Omega}(f(0)-H)\,\phi^{2}\leq\int_{\Omega}(|D\phi|^{2}-f^{\prime}(u)\,\phi^{2})

for all ϕCc(Ω¯)\phi\in C_{c}^{\infty}(\bar{\Omega}) such that

Ωϕ=0.\int_{\partial\Omega}\phi=0.

We call Ω\Omega stable if (4) holds for all ϕCc(Ω¯)\phi\in C_{c}^{\infty}(\bar{\Omega}). As we explain in Appendix A, Ω\Omega is weakly stable if and only if uu passes the second derivative test for JJ among compact perturbations that preserve the relative volume of {yn:u(y)>0}\{y\in\mathbb{R}^{n}:u(y)>0\}.

Notably, domains Ω\Omega that are solutions of (1) and are weakly stable arise in the context of minimal surface theory. To explain this, let Sn+1S\subset\mathbb{R}^{n+1} be a closed hypersurface with positive mean curvature bounding an open and bounded set Mn+1M\subset\mathbb{R}^{n+1}. Let ΣM¯\Sigma\subset\bar{M} be a relative boundary. In particular, ΣS\partial\Sigma\subset S bounds a closed subset S(Σ)SS(\Sigma)\subset S called the wetting surface of Σ\Sigma. Σ\Sigma is called a minimal capillary surface supported on SS if the mean curvature of Σ\Sigma vanishes and if Σ\Sigma and SS intersect along Σ\partial\Sigma at a constant angle θ(0,π)\theta\in(0,\pi). Minimal capillary surfaces are critical for area given the area of their wetting surface. They are called weakly stable if they pass the second derivative test for area among perturbations that fix the area of their wetting surface. In the case where n=2n=2, the authors [12] have shown weakly stable solutions Ω\Omega of (1) arise as certain blowup limits of weakly stable minimal capillary surfaces supported on SS with θ\theta close to either 00 or π\pi. This has led to a characterization of all weakly stable minimal capillary surfaces supported on SS with angle close to 00 or π\pi; see [12, Theorem 6]. A fundamental ingredient in the proof is the following rigidity result for weakly stable solutions of (1).

Theorem 1.

[12, Proposition 31] Let n=2n=2. Assume that Ω\Omega is a weakly stable solution of (1) and that Ω\partial\Omega has bounded curvature. Then Ω\Omega is a ball of radius 11.

In this paper, we show that Theorem 1 holds in all dimensions, even without the assumption that the curvature of Ω\partial\Omega is bounded. In the case where f=nf=n, this gives an affirmative answer to the conjecture of H. Berestycki, L. Caffarelli, and L. Nirenberg under the, from a variational point of view, most natural additional assumption.

Theorem 2.

Let n2n\geq 2. Assume that Ω\Omega is a weakly stable solution of (1). Then Ω\Omega is a ball of radius 11.

It is remarkable that Theorem 2 holds in all dimensions. Indeed, J. Serrin’s overdetermined problem (1) is closely related to the one-phase Bernoulli problem; see [1] and also [5] for a connection between the one-phase Bernoulli problem and minimal capillary surfaces. The one-phase Bernoulli problem is (3) with f=0f=0, i.e.,

(5) {Δu=0in Ω,u>0in Ω,u=0on Ω, and|Du|=1on Ω.\displaystyle\begin{cases}\quad-\Delta u=0\qquad&\text{in $\Omega$},\\ \quad u>0&\text{in $\Omega$},\\ \quad u=0&\text{on $\partial\Omega$, and}\\ \quad|Du|=1&\text{on $\partial\Omega$}.\end{cases}

In the case where n3n\leq 3, stable solutions Ω\Omega of (5) are known to be half-spaces; see [4] and, e.g., [15]. By contrast, in the case where n7n\geq 7, there are infinitely many geometrically distinct stable solutions of (5); see [8]. This shows that the assumption that f=nf=n in Theorem 2 cannot be dropped altogether. We note that, in a similar context, M. do Carmo [11] has conjectured that constant mean curvature hypersurfaces in n+1\mathbb{R}^{n+1} that pass the second derivative test for area among all hypersurfaces enclosing the same relative volume are round spheres for all n2n\geq 2. By contrast, stable minimal hypersurfaces in n+1\mathbb{R}^{n+1} are known to be hyperplanes in the case where n5n\leq 5 while there are infinitely many geometrically distinct stable minimal hypersurfaces in n+1\mathbb{R}^{n+1} in the case where n7n\geq 7; see, e.g., [10, 18, 14, 7, 6, 16] and [21].

Outline of our arguments

Our approach toward Theorem 2 differs substantially from our proof of Theorem 1 in [12], which is based on the Gauss-Bonnet theorem and therefore specific to the case where n=2n=2. It also differs substantially from the arguments employed in the recent work of H. Chan, X. Fernández-Real, A. Figalli, and J. Serra [4] on (5), which are specific to the case where n=3n=3 and, in view of the counterexamples found in [8], cannot possibly be adapted to the case where n7n\geq 7.

First, we suppose, for a contradiction, that Ω\Omega has infinite volume. Given λ>0\lambda>0, let A(λ)=|Bλ(0)Ω|A(\lambda)=|B_{\lambda}(0)\cap\partial\Omega| and V(λ)=|Bλ(0)Ω|V(\lambda)=|B_{\lambda}(0)\cap\Omega|. Using (1), we show that

(6) A(λ)nV(λ)\displaystyle A(\lambda)\approx n\,V(\lambda)

for suitable numbers λ1\lambda\gg 1; see Proposition 14. In conjunction with a balancing argument, (6) implies that Ω\Omega is stable; see Lemma 20. The proof relies on certain gradient estimates for uu that we establish in Section 2. We then choose a sequence {ηk}k=1\{\eta_{k}\}_{k=1}^{\infty} of suitable cutoff functions ηkCc(n)\eta_{k}\in C^{\infty}_{c}(\mathbb{R}^{n}) with ηk1\eta_{k}\to 1 locally smoothly. Applying the stability of Ω\Omega with ϕ=ηk\phi=\eta_{k} and using (6), we obtain that

Ωηk2(n1H)o(1)A(λk)A(λk).\int_{\partial\Omega}\eta_{k}^{2}\,(n-1-H)\leq o(1)\,A(\lambda_{k})-A(\lambda_{k}).

Applying the stability of Ω\Omega with ϕ=ηkφ\phi=\eta_{k}\,\varphi where φ=u+|Du|2/2\varphi=u+|Du|^{2}/2 and using (6) again, we conclude that

Ωηk2(nH)(2+o(1))A(λk);\int_{\partial\Omega}\eta_{k}^{2}\,(n-H)\leq-(2+o(1))\,A(\lambda_{k});

see (20). A crucial ingredient here is that φ\varphi is subharmonic in Ω\Omega and satisfies μ(Ω)Dφ=n1H\mu(\Omega)\cdot D\varphi=n-1-H on Ω\partial\Omega; see Lemma 15. By contrast, the gradient estimates in Section 2 show that nHn\geq H; see Lemma 12. This leads to a contradiction.

It follows that Ω\Omega has finite volume. In view of the gradient estimates in Section 2, we show how to adapt the argument of H. Weinberger [25] to this setting; see Proposition 18. In particular, every component of Ω\Omega is a ball of radius 1. Using the weak stability of Ω\Omega, we see that Ω\Omega is connected.

On the use of artificial intelligence (A.I.)

None of the arguments employed here have been suggested by or discussed with A.I. tools. The paper does not contain text written by A.I. tools. The authors have used Claude Opus 5 to check the typesetting of this paper.

Acknowledgments

This research was funded in whole or in part by the Austrian Science Fund (FWF) [10.55776/PAT1307525, 10.55776/PAT2423724].

2. Gradient estimates

Throughout, we assume that n2n\geq 2. We use O(1)O(1) to denote constants that only depends on nn.

The arguments in this section are well-known to experts in the field.

Lemma 3.

There holds Ωn\Omega\neq\mathbb{R}^{n}.

Proof.

Suppose, for a contradiction, that Ω=n\Omega=\mathbb{R}^{n}. Then vC(n)v\in C^{\infty}(\mathbb{R}^{n}) given by

v(x)=u(x)+12|x|2v(x)=u(x)+\frac{1}{2}\,|x|^{2}

is positive and harmonic. By the Liouville theorem, vv is a positive constant. Since u>0u>0, this leads to a contradiction. ∎

Given xnx\in\mathbb{R}^{n} and r>0r>0, let

Br(x)={yn:|yx|<r}.B_{r}(x)=\{y\in\mathbb{R}^{n}:|y-x|<r\}.

Given xΩx\in\Omega, let

r(x)=dist(x,Ω).r(x)=\operatorname{dist}(x,\partial\Omega).

By Lemma 3, r(x)<r(x)<\infty. Note that Br(x)(x)ΩB_{r(x)}(x)\subset\Omega and ΩBr(x)(x)\partial\Omega\cap\partial B_{r(x)}(x)\neq\emptyset. Moreover,

μ(Ω)(z)=zx|zx|\mu(\Omega)(z)=\frac{z-x}{|z-x|}

for all zΩBr(x)(x)z\in\partial\Omega\cap\partial B_{r(x)}(x).

Lemma 4 (cp. [12, Lemma 25]).

Let xΩx\in\Omega. There holds

r(x)1.r(x)\leq 1.
Proof.

Let vC(n)v\in C^{\infty}(\mathbb{R}^{n}) be given by

v(y)=12r(x)212|yx|2.v(y)=\frac{1}{2}\,r(x)^{2}-\frac{1}{2}\,|y-x|^{2}.

Note that uvu-v is harmonic in Br(x)(x)B_{r(x)}(x) and nonnegative on Br(x)(x)\partial B_{r(x)}(x). By the maximum principle, uvu\geq v in Br(x)(x)B_{r(x)}(x). Also note that u(z)=v(z)u(z)=v(z) for all zΩBr(x)(x)z\in\partial\Omega\cap\partial B_{r(x)}(x). At such zz,

0μ(Ω)Duμ(Ω)Dv=1+r(x).0\geq\mu(\Omega)\cdot Du-\mu(\Omega)\cdot Dv=-1+r(x).

This completes the proof of the lemma. ∎

Lemma 5.

There holds

12Δ|Du|2n\frac{1}{2}\,\Delta|Du|^{2}\geq n

in Ω\Omega.

Proof.

By the Bochner formula,

(7) 12Δ|Du|2=DuDΔu+|D2u|2=|D2u|2.\displaystyle\frac{1}{2}\,\Delta|Du|^{2}=Du\cdot D\Delta u+|D^{2}u|^{2}=|D^{2}u|^{2}.

By the inequality of arithmetic and geometric means,

(8) |D2u|2(Δu)2n=n.\displaystyle|D^{2}u|^{2}\geq\frac{(\Delta u)^{2}}{n}=n.

This completes the proof of the lemma.

Corollary 6.

Assume that Ω\Omega is connected and that

12Δ|Du|2=n.\frac{1}{2}\,\Delta|Du|^{2}=n.

There is xnx\in\mathbb{R}^{n} such that Ω=B1(x)\Omega=B_{1}(x).

Proof.

By assumption, equality holds in (8). It follows that D2u=IdD^{2}u=-\operatorname{Id}. Equivalently, there is xnx\in\mathbb{R}^{n} such that

u(y)+12|yx|2u(y)+\frac{1}{2}\,|y-x|^{2}

is constant in Ω\Omega. Since u=0u=0 and |Du|=1|Du|=1 on Ω\partial\Omega, Ω=B1(x),\Omega=B_{1}(x), as asserted. ∎

Lemma 7 (cp. [24, Lemma 2.3]).

There holds

sup{|Du(x)|:xΩ}<.\sup\{|Du(x)|:x\in\Omega\}<\infty.
Proof.

Fix xΩx\in\Omega. Let v:nv:\mathbb{R}^{n}\to\mathbb{R} be given by

v(y)=12r(x)212|yx|2.v(y)=\frac{1}{2}\,r(x)^{2}-\frac{1}{2}\,|y-x|^{2}.

Note that uvu-v is harmonic in Br(x)(x)B_{r(x)}(x) and that uv0u-v\geq 0 on Br(x)(x)\partial B_{r(x)}(x) with equality for all zΩBr(x)(x)z\in\partial\Omega\cap\partial B_{r(x)}(x). By the strong maximum principle, either u(y)=v(y)u(y)=v(y) for all yBr(x)(x)y\in B_{r(x)}(x) or u(y)>v(y)u(y)>v(y) for all yBr(x)(x)y\in B_{r(x)}(x). Since Dv(x)=0Dv(x)=0, we may assume that u(y)>v(y)u(y)>v(y) for all yBr(x)(x)y\in B_{r(x)}(x). Let

κ=inf{u(y)v(y):yBr(x)/2(x)}.\kappa=\inf\left\{u(y)-v(y):y\in\partial B_{r(x)/2}(x)\right\}.

By the Harnack inequality,

(9) u(x)v(x)=O(1)κ.\displaystyle u(x)-v(x)=O(1)\,\kappa.

Let h:n{x}h:\mathbb{R}^{n}\setminus\{x\}\to\mathbb{R} be the harmonic function given by

h(y)=1log2κ(logr(x)log|yx|)\displaystyle h(y)=\frac{1}{\log 2}\,\kappa\,(\log r(x)-\log|y-x|)

if n=2n=2 and

h(y)=r(x)n22n21κ(|yx|2nr(x)2n)\displaystyle h(y)=\frac{r(x)^{n-2}}{2^{n-2}-1}\,\kappa\,(|y-x|^{2-n}-r(x)^{2-n})

if n3n\geq 3. Note that

h(y)={κif |yx|=r(x)/2 and0if |yx|=r(x).h(y)=\begin{cases}\kappa\qquad&\text{if $|y-x|={r(x)}/2$ and}\\ 0&\text{if $|y-x|=r(x)$.}\end{cases}

By the maximum principle, uvhu-v\geq h in B¯r(x)(x)Br(x)/2(x)\bar{B}_{r(x)}(x)\setminus B_{r(x)/2}(x) with equality for all zΩBr(x)(x)z\in\partial\Omega\cap\partial B_{r(x)}(x). At such zz, there holds

0μ(Ω)D(uv)μ(Ω)Dh=1+r(x)+1log2κr(x)0\geq\mu(\Omega)\cdot D(u-v)-\mu(\Omega)\cdot Dh=-1+r(x)+\frac{1}{\log 2}\,\frac{\kappa}{r(x)}\quad\,\,\,\,\,

if n=2n=2 and

0μ(Ω)D(uv)μ(Ω)Dh=1+r(x)+n22n21κr(x)0\geq\mu(\Omega)\cdot D(u-v)-\mu(\Omega)\cdot Dh=-1+r(x)+\frac{n-2}{2^{n-2}-1}\,\frac{\kappa}{r(x)}

if n3n\geq 3. It follows that κ=O(1)r(x)\kappa=O(1)\,r(x). In conjunction with (9) and the gradient estimate for positive harmonic functions,

|D(uv)(x)|=O(1)u(x)v(x)r(x)=O(1).|D(u-v)(x)|=O(1)\,\frac{u(x)-v(x)}{r(x)}=O(1).

Since Dv(x)=0Dv(x)=0, the assertion follows. ∎

Corollary 8 (cf. [24, Proposition 2.1]).

There holds |Du|<1|Du|<1 in Ω\Omega.

Proof.

Let 0<ε<10<\varepsilon<1. By Lemma 5, ψεC(Ω¯)\psi_{\varepsilon}\in C^{\infty}(\bar{\Omega}) given by

ψε(y)=|Du(y)|2ε|y|2\psi_{\varepsilon}(y)=|Du(y)|^{2}-\varepsilon\,|y|^{2}

is strictly subharmonic. By the maximum principle and Lemma 7, ψε\psi_{\varepsilon} attains its maximum on Ω\partial\Omega. In particular, |Du(y)|2ε|y|2<1|Du(y)|^{2}-\varepsilon\,|y|^{2}<1 for all yΩy\in\Omega. Letting ε0\varepsilon\to 0, we obtain that |Du(y)|1|Du(y)|\leq 1 for all yΩy\in\Omega. By the strong maximum principle, either |Du|=1|Du|=1 in Ω\Omega or |Du|<1|Du|<1 in Ω\Omega. In view of Lemma 5, the former alternative is impossible. This completes the proof of the corollary. ∎

Remark 9.

The estimate

12|Du|2F(u)\frac{1}{2}\,|Du|^{2}\leq F(u)

for solutions of (3) where FC()F\in C^{\infty}(\mathbb{R}) is such that F(0)=1/2F(0)=1/2 and F=fF^{\prime}=f proven in [24, Proposition 6.3] gives

|Du|21+n2u|Du|^{2}\leq 1+\frac{n}{2}\,u

in the case where f=nf=n; see also [17]. Note that, unlike Corollary 8, this estimate is not optimal.

Corollary 10.

There holds 0<u<10<u<1 in Ω\Omega.

Proof.

This follows from Lemma 4 and Corollary 8. ∎

Lemma 11.

There holds

D2u(Du,Du)=HnD^{2}u(Du,Du)=H-n

on Ω\partial\Omega.

Proof.

There holds

Δv=ΔΩv+D2v(μ(Ω),μ(Ω))+Hμ(Ω)Dv\Delta v=\Delta^{\partial\Omega}v+D^{2}v(\mu(\Omega),\mu(\Omega))+H\,\mu(\Omega)\cdot Dv

for every vC(Ω¯)v\in C^{\infty}(\bar{\Omega}). The assertion follows from this, taking v=uv=u. ∎

Lemma 12 (cf. [24, Lemma 6.3] and [3]).

There holds HnH\leq n on Ω\partial\Omega.

Proof.

By Corollary 8,

μ(Ω)D|Du|20\mu(\Omega)\cdot D|Du|^{2}\geq 0

and μ(Ω)D|Du|2=2D2u(Du,Du)\mu(\Omega)\cdot D|Du|^{2}=-2\,D^{2}u(Du,Du) on Ω\partial\Omega. The assertion follows from this and Lemma 11. ∎

3. Asymptotics

Given λ>0\lambda>0, let

A(λ)=|Bλ(0)Ω|andV(λ)=|Bλ(0)Ω|.A(\lambda)=|B_{\lambda}(0)\cap\partial\Omega|\qquad\text{and}\qquad V(\lambda)=|B_{\lambda}(0)\cap\Omega|.

Note that V(λ)|Bλ(0)|=λn|B1(0)|V(\lambda)\leq|B_{\lambda}(0)|=\lambda^{n}\,|B_{1}(0)| for all λ>0\lambda>0 and that VV is nondecreasing and Lipschitz. For almost every λ>0\lambda>0, Bλ(0)\partial B_{\lambda}(0) and Ω\partial\Omega intersect transversely. VV is differentiable at such λ>0\lambda>0 and there holds

V(λ)=|Bλ(0)Ω|.V^{\prime}(\lambda)=|\partial B_{\lambda}(0)\cap\Omega|.

Moreover, by the divergence theorem,

A(λ)=Bλ(0)Ωμ(Ω)Du=nV(λ)+ΩBλ(0)x|x|Du.A(\lambda)=-\int_{B_{\lambda}(0)\cap\partial\Omega}\mu(\Omega)\cdot Du=n\,V(\lambda)+\int_{\Omega\cap\partial B_{\lambda}(0)}\frac{x}{|x|}\cdot Du.

Let E:(0,)E:(0,\infty)\to\mathbb{R} be given by

E(λ)=ΩBλ(0)x|x|Du.E(\lambda)=\int_{\Omega\cap\partial B_{\lambda}(0)}\frac{x}{|x|}\cdot Du.

By Corollary 8,

|E(λ)|V(λ)|E(\lambda)|\leq V^{\prime}(\lambda)

for all λ>0\lambda>0 as above and

(10) A(λ)=nV(λ)+E(λ).\displaystyle A(\lambda)=n\,V(\lambda)+E(\lambda).
Lemma 13.

There is a sequence {mk}k=1\{m_{k}\}_{k=1}^{\infty} of positive integers with mkm_{k}\to\infty such that

V(mk+2)V(mk)V(mk)=o(1).\frac{V(m_{k}+2)-V(m_{k})}{V(m_{k})}=o(1).
Proof.

We may assume that V(1)>0V(1)>0. For every integer M1M\geq 1, there holds

m=1MV(m+2)V(m)V(m+2)\displaystyle\sum_{m=1}^{M}\frac{V(m+2)-V(m)}{V(m+2)} m=1MV(m)V(m+2)1t𝑑t\displaystyle\leq\sum_{m=1}^{M}\int_{V(m)}^{V(m+2)}\frac{1}{t}\,\mathrm{d}t
2V(1)V(M+2)1t𝑑t\displaystyle\leq 2\,\int_{V(1)}^{V(M+2)}\frac{1}{t}\,\mathrm{d}t
=2logV(M+2)V(1)\displaystyle=2\,\log\frac{V(M+2)}{V(1)}
=O(1)logM.\displaystyle=O(1)\,\log M.

It follows that there is a sequence {mk}k=1\{m_{k}\}_{k=1}^{\infty} of positive integers with mkm_{k}\to\infty such that

V(mk+2)V(mk)V(mk+2)=o(1).\frac{V(m_{k}+2)-V(m_{k})}{V(m_{k}+2)}=o(1).

In particular,

V(mk+2)V(mk)=1+o(1).\frac{V(m_{k}+2)}{V(m_{k})}=1+o(1).

The assertion follows from these estimates. ∎

Proposition 14.

There is a sequence {λk}k=1\{\lambda_{k}\}_{k=1}^{\infty} of positive numbers with λk\lambda_{k}\to\infty such that

(11) V(λk+1)V(λk)A(λk)=o(1)\displaystyle\frac{V(\lambda_{k}+1)-V(\lambda_{k})}{A(\lambda_{k})}=o(1)

and

(12) nV(λk)A(λk)=1+o(1).\displaystyle\frac{n\,V(\lambda_{k})}{A(\lambda_{k})}=1+o(1).
Proof.

Let {mk}k=1\{m_{k}\}_{k=1}^{\infty} be as in Lemma 13. Since VV is Lipschitz, there is λk(mk,mk+1)\lambda_{k}\in(m_{k},m_{k}+1) such that Bλk(0)\partial B_{\lambda_{k}}(0) and Ω\partial\Omega intersect transversely and

V(λk)V(mk+1)V(mk).V^{\prime}(\lambda_{k})\leq V(m_{k}+1)-V(m_{k}).

Using also that VV is nondecreasing,

V(λk)V(mk+2)V(mk)=o(1)V(mk)o(1)V(λk).V^{\prime}(\lambda_{k})\leq V(m_{k}+2)-V(m_{k})=o(1)\,V(m_{k})\leq o(1)\,V(\lambda_{k}).

In conjunction with (10),

A(λk)=(1+o(1))nV(λk).A(\lambda_{k})=(1+o(1))\,n\,V(\lambda_{k}).

Note that

V(λk+1)V(λk)V(mk+2)V(mk)=o(1)V(mk).V(\lambda_{k}+1)-V(\lambda_{k})\leq V(m_{k}+2)-V(m_{k})=o(1)\,V(m_{k}).

Using that

nV(mk)nV(λk)=(1+o(1))A(λk),n\,V(m_{k})\leq n\,V(\lambda_{k})=(1+o(1))\,A(\lambda_{k}),

the assertion follows. ∎

4. Finite volume

Let φC(Ω¯)\varphi\in C^{\infty}(\bar{\Omega}) be given by

(13) φ(x)=u(x)+12|Du(x)|2.\displaystyle\varphi(x)=u(x)+\frac{1}{2}\,|Du(x)|^{2}.
Lemma 15.

There holds

Δφ0-\Delta\varphi\leq 0

in Ω\Omega and

φ=12andμ(Ω)Dφ=n1H\varphi=\frac{1}{2}\qquad\text{and}\qquad\mu(\Omega)\cdot D\varphi=n-1-H

on Ω\partial\Omega.

Proof.

This follows from Lemma 5 and Lemma 11. ∎

Corollary 16.

Assume that Ω\Omega is connected and that φ=1/2\varphi=1/2 in Ω\Omega. There is xnx\in\mathbb{R}^{n} such that Ω=B1(x)\Omega=B_{1}(x).

Proof.

In view of Lemma 5, the proof of Lemma 15 shows that

12Δ|Du|2=n.\frac{1}{2}\,\Delta|Du|^{2}=n.

The assertion now follows from Corollary 6. ∎

Lemma 17.

There holds φ<3/2\varphi<3/2 in Ω\Omega.

Proof.

The assertion follows from Corollary 8 and Corollary 10. ∎

The proof of the following proposition adapts that of [25, Theorem 1] to the case where Ω\Omega is not a-priori bounded.

Proposition 18.

Assume that Ω\Omega is connected and has finite volume. There is xnx\in\mathbb{R}^{n} such that Ω=B1(x)\Omega=B_{1}(x).

Proof.

Since Ω\Omega has finite volume, there is a sequence {λk}k=1\{\lambda_{k}\}_{k=1}^{\infty} of positive numbers such that λk\lambda_{k}\to\infty and

(14) |(Bλk+1(0)Bλk(0))Ω|=o(1)1λk.\displaystyle|(B_{\lambda_{k}+1}(0)\setminus B_{\lambda_{k}}(0))\cap\Omega|=o(1)\,\frac{1}{\lambda_{k}}.

Let ηkCc(n),\eta_{k}\in C_{c}^{\infty}(\mathbb{R}^{n}), k1,k\geq 1, be such that

  • \circ

    ηk(x)=1\eta_{k}(x)=1 for all xBλk(0)x\in B_{\lambda_{k}}(0),

  • \circ

    ηk(x)=0\eta_{k}(x)=0 for all xnBλk+1(0)x\in\mathbb{R}^{n}\setminus B_{\lambda_{k}+1}(0),

  • \circ

    |Dηk|=O(1)|D\eta_{k}|=O(1), and

  • \circ

    |D2ηk|=O(1)|D^{2}\eta_{k}|=O(1).

Note that

Δ(xDu)=2n.-\Delta(x\cdot Du)=2\,n.

By the divergence theorem,

2nΩηkunΩηkxDu\displaystyle 2\,n\,\int_{\Omega}\eta_{k}\,u-n\,\int_{\Omega}\eta_{k}\,x\cdot Du
=ΩηkuΔ(xDu)+Ωηk(xDu)Δu\displaystyle\qquad=-\int_{\Omega}\eta_{k}\,u\,\Delta(x\cdot Du)+\int_{\Omega}\eta_{k}\,(x\cdot Du)\,\Delta u
=Ωηk(xDu)μ(Ω)Du+ΩuD(xDu)DηkΩ(xDu)DuDηk\displaystyle\qquad=\int_{\partial\Omega}\eta_{k}\,(x\cdot Du)\,\mu(\Omega)\cdot Du+\int_{\Omega}u\,D(x\cdot Du)\cdot D\eta_{k}-\int_{\Omega}(x\cdot Du)\,Du\cdot D\eta_{k}
=Ωηk(xDu)Ωu(xDu)Δηk2Ω(xDu)DuDηk.\displaystyle\qquad=-\int_{\partial\Omega}\eta_{k}\,(x\cdot Du)-\int_{\Omega}u\,(x\cdot Du)\,\Delta\eta_{k}-2\,\int_{\Omega}(x\cdot Du)\,Du\cdot D\eta_{k}.

Moreover, using that divx=n\operatorname{div}x=n,

Ωηk(xDu)=Ωηkμ(Ω)x=nΩηk+ΩxDηk.-\int_{\partial\Omega}\eta_{k}\,(x\cdot Du)=\int_{\partial\Omega}\eta_{k}\,\mu(\Omega)\cdot x=n\,\int_{\Omega}\eta_{k}+\int_{\Omega}x\cdot D\eta_{k}.

By (14),

ΩxDηk=o(1).\int_{\Omega}x\cdot D\eta_{k}=o(1).

By Corollary 8, Corollary 10, and (14),

Ωu(xDu)Δηk=o(1).\int_{\Omega}u\,(x\cdot Du)\,\Delta\eta_{k}=o(1).

By Corollary 8 and (14),

Ω(xDu)DuDηk=o(1).\int_{\Omega}(x\cdot Du)\,Du\cdot D\eta_{k}=o(1).

By the divergence theorem,

ΩηkxDu=nΩηkuΩuxDηk.\int_{\Omega}\eta_{k}\,x\cdot Du=-n\,\int_{\Omega}\eta_{k}\,u-\int_{\Omega}u\,x\cdot D\eta_{k}.

By Corollary 10 and (14),

ΩuxDηk=o(1).\int_{\Omega}u\,x\cdot D\eta_{k}=o(1).

By the dominated convergence theorem, using Corollary 10, we conclude that

(15) (n+2)Ωu=|Ω|.\displaystyle(n+2)\,\int_{\Omega}u=|\Omega|.

Suppose, for a contradiction, that Ω\Omega is unbounded. Let {x}=1\{x_{\ell}\}_{\ell=1}^{\infty} be a sequence of points in Ω\Omega such that |x||x_{\ell}|\to\infty. Since Ω\Omega has finite volume, there holds r(x)=o(1)r(x_{\ell})=o(1). By Corollary 8, u(x)=o(1)u(x_{\ell})=o(1). Using Corollary 8 again, we conclude that φ(x)1/2+o(1)\varphi(x_{\ell})\leq 1/2+o(1). By Lemma 15 and the maximum principle,

(16) φ12\displaystyle\varphi\leq\frac{1}{2}

in Ω\Omega. By the divergence theorem,

Ωηk|Du|2=nΩηkuΩuDuDηk.\int_{\Omega}\eta_{k}\,|Du|^{2}=n\,\int_{\Omega}\eta_{k}\,u-\int_{\Omega}u\,Du\cdot D\eta_{k}.

By the dominated convergence theorem, using Corollary 8, Corollary 10, and (14),

Ω|Du|2=nΩu.\int_{\Omega}|Du|^{2}=n\,\int_{\Omega}\,u.

Thus,

2Ωφ=2Ωu+Ω|Du|2=(n+2)Ωu.2\,\int_{\Omega}\varphi=2\,\int_{\Omega}u+\int_{\Omega}|Du|^{2}=(n+2)\,\int_{\Omega}u.

In view of (15) and (16), we conclude that φ=1/2\varphi=1/2. By Corollary 16, there is xnx\in\mathbb{R}^{n} such that Ω=B1(x)\Omega=B_{1}(x), contradicting that Ω\Omega is unbounded.

It follows that Ω\Omega is bounded. As in the previous paragraph, we see that there is xnx\in\mathbb{R}^{n} such that Ω=B1(x)\Omega=B_{1}(x). This completes the proof of the proposition. ∎

5. Stability and weak stability

The following lemma has essentially been observed in [22, Theorem 3.5].

Lemma 19.

Let ηCc(Ω¯)\eta\in C_{c}^{\infty}(\bar{\Omega}). There holds

(17) Ω|D(|Du|η)|2+Ω(Hn)η2Ω|Dη|2.\displaystyle\int_{\Omega}|D(|Du|\,\eta)|^{2}+\int_{\partial\Omega}(H-n)\,\,\eta^{2}\leq\int_{\Omega}|D\eta|^{2}.
Proof.

By the divergence theorem, using (7) and Lemma 11,

12ΩD|Du|2Dη2=Ω|D2u|2η2+Ω(nH)η2.\frac{1}{2}\,\int_{\Omega}D|Du|^{2}\cdot D\eta^{2}=-\int_{\Omega}|D^{2}u|^{2}\,\eta^{2}+\int_{\partial\Omega}(n-H)\,\eta^{2}.

Thus,

Ω|D(|Du|η)|2+Ω(Hn)η2\displaystyle\int_{\Omega}|D(|Du|\,\eta)|^{2}+\int_{\partial\Omega}(H-n)\,\eta^{2}
=Ω|D2u|2η2+Ω|D|Du||2η2+Ω|Du|2|Dη|2.\displaystyle\qquad=-\int_{\Omega}|D^{2}u|^{2}\,\eta^{2}+\int_{\Omega}|D|Du||^{2}\,\eta^{2}+\int_{\Omega}|Du|^{2}\,|D\eta|^{2}.

Note that |D2u||D|Du|||D^{2}u|\geq|D|Du|| almost everywhere. Using also Corollary 8, we obtain (17). ∎

In the case where n=2n=2 and Ω\partial\Omega has bounded curvature, the following lemma has been obtained in [12, Lemma 26].

Lemma 20.

Assume that Ω\Omega has infinite volume and is weakly stable. Then Ω\Omega is stable.

Proof.

Let ϕCc(Ω¯)\phi\in C_{c}^{\infty}(\bar{\Omega}) be such that

Ωϕ=1.\int_{\partial\Omega}\phi=1.

Let λ>2\lambda>2 be such that spt(ϕ)Bλ2(0)\operatorname{spt}(\phi)\subset B_{\lambda-2}(0). Let {λk}k=1\{\lambda_{k}\}_{k=1}^{\infty} be as in Proposition 14. We may assume that λk>λ\lambda_{k}>\lambda for all kk. We choose ηkCc(n),\eta_{k}\in C_{c}^{\infty}(\mathbb{R}^{n}), k1k\geq 1, such that

  • \circ

    ηk(x)=1\eta_{k}(x)=1 for all xBλk(0)Bλ(0)x\in B_{\lambda_{k}}(0)\setminus B_{\lambda}(0),

  • \circ

    ηk(x)=0\eta_{k}(x)=0 for all xBλ1(0)x\in B_{\lambda-1}(0) and xnBλk+1(0)x\in\mathbb{R}^{n}\setminus B_{\lambda_{k}+1}(0),

  • \circ

    0ηk10\leq\eta_{k}\leq 1, and

  • \circ

    |Dηk|=O(1)|D\eta_{k}|=O(1).

By (12), using that V(λk)V(\lambda_{k})\to\infty, there holds A(λk)A(\lambda_{k})\to\infty and

Ωηk.\int_{\partial\Omega}\eta_{k}\to\infty.

In conjunction with (11),

(18) Ω|Dηk|2=o(1)Ωηk.\displaystyle\int_{\Omega}|D\eta_{k}|^{2}=o(1)\,\int_{\partial\Omega}\eta_{k}.

Note that sptηksptϕ=\operatorname{spt}\eta_{k}\cap\operatorname{spt}\phi=\emptyset. Let εk>0\varepsilon_{k}>0, k1k\geq 1, be such that

Ωϕ~k=0\int_{\partial\Omega}\tilde{\phi}_{k}=0

where ϕ~k=ϕεk|Du|ηk\tilde{\phi}_{k}=\phi-\varepsilon_{k}\,|Du|\,\eta_{k}. Note that

εkΩηk=O(1).\varepsilon_{k}\,\int_{\partial\Omega}\eta_{k}=O(1).

In particular, εk=o(1)\varepsilon_{k}=o(1). By (18),

εk2Ω|Dηk|2=o(1).\varepsilon^{2}_{k}\,\int_{\Omega}|D\eta_{k}|^{2}=o(1).

By the weak stability of Ω\Omega,

Ω(nH)ϕ~k2Ω|Dϕ~k|2.\int_{\partial\Omega}(n-H)\,\tilde{\phi}_{k}^{2}\leq\int_{\Omega}|D\tilde{\phi}_{k}|^{2}.

In conjunction with (17), we see that

Ω(nH)ϕ2Ω|Dϕ|2+εk2Ω|Dηk|2=Ω|Dϕ|2+o(1).\int_{\partial\Omega}(n-H)\,\phi^{2}\leq\int_{\Omega}|D\phi|^{2}+\varepsilon^{2}_{k}\,\int_{\Omega}|D\eta_{k}|^{2}=\int_{\Omega}|D\phi|^{2}+o(1).

This completes the proof of the lemma. ∎

6. Proof of Theorem 2

Lemma 21.

Suppose that Ω\Omega is stable. Let ηCc(Ω¯)\eta\in C_{c}^{\infty}(\bar{\Omega}). There holds

(19) Ωη2(nH)9Ω|Dη|2+2Ωη2(n1H).\displaystyle\int_{\partial\Omega}\eta^{2}\,(n-H)\leq 9\,\int_{\Omega}|D\eta|^{2}+2\,\int_{\partial\Omega}\eta^{2}\,(n-1-H).
Proof.

Recall the definition (13) of φC(Ω¯)\varphi\in C^{\infty}(\bar{\Omega}). Since Ω\Omega is stable and φ=1/2\varphi=1/2 on Ω\partial\Omega,

14Ω(nH)η2Ω|D(ηφ)|2.\frac{1}{4}\,\int_{\partial\Omega}(n-H)\,\eta^{2}\leq\int_{\Omega}|D(\eta\,\varphi)|^{2}.

Note that

|D(ηφ)|2=φ2|Dη|2+2ηφDηDφ+η2|Dφ|2.|D(\eta\,\varphi)|^{2}=\varphi^{2}\,|D\eta|^{2}+2\,\eta\,\varphi\,D\eta\cdot D\varphi+\eta^{2}\,|D\varphi|^{2}.

Integrating by parts and using Lemma 15, we have

2ΩηφDηDφ+Ωη2|Dφ|2\displaystyle 2\,\int_{\Omega}\eta\,\varphi\,D\eta\cdot D\varphi+\int_{\Omega}\eta^{2}\,|D\varphi|^{2} =Ωη2φΔφ+Ωη2φμ(Ω)Dφ\displaystyle=-\int_{\Omega}\eta^{2}\,\varphi\Delta\varphi+\int_{\partial\Omega}\eta^{2}\,\varphi\,\mu(\Omega)\cdot D\varphi
12Ωη2μ(Ω)Dφ\displaystyle\leq\frac{1}{2}\,\int_{\partial\Omega}\eta^{2}\,\mu(\Omega)\cdot D\varphi
=12Ωη2(n1H).\displaystyle=\frac{1}{2}\,\int_{\partial\Omega}\eta^{2}\,(n-1-H).

Thus,

Ωη2(nH)4Ωφ2|Dη|2+2Ωη2(n1H).\int_{\partial\Omega}\eta^{2}\,(n-H)\leq 4\,\int_{\Omega}\varphi^{2}\,|D\eta|^{2}+2\,\int_{\partial\Omega}\eta^{2}\,(n-1-H).

The assertion follows from Lemma 17. ∎

Proof of Theorem 2.

Suppose, for a contradiction, that Ω\Omega has infinite volume. By Lemma 20, Ω\Omega is stable. Let {λk}k=1\{\lambda_{k}\}_{k=1}^{\infty} be as in Proposition 14. We choose ηkCc(n),\eta_{k}\in C_{c}^{\infty}(\mathbb{R}^{n}), k1k\geq 1, such that

  • \circ

    ηk(x)=1\eta_{k}(x)=1 for all xBλk(0)x\in B_{\lambda_{k}}(0),

  • \circ

    ηk(x)=0\eta_{k}(x)=0 for all xnBλk+1(0)x\in\mathbb{R}^{n}\setminus B_{\lambda_{k}+1}(0), and

  • \circ

    |Dηk|2|D\eta_{k}|\leq 2.

By the stability of Ω\Omega and (11),

Ωηk2(nH)Ω|Dηk|2=o(1)A(λk).\int_{\partial\Omega}\eta_{k}^{2}\,(n-H)\leq\int_{\Omega}|D\eta_{k}|^{2}=o(1)\,A(\lambda_{k}).

It follows that

Ωηk2(n1H)o(1)A(λk)Ωηk2(1+o(1))A(λk).\int_{\partial\Omega}\eta_{k}^{2}\,(n-1-H)\leq o(1)\,A(\lambda_{k})-\int_{\partial\Omega}\eta_{k}^{2}\leq-(1+o(1))\,A(\lambda_{k}).

In conjunction with (19), using (11) again,

(20) Ωηk2(nH)(2+o(1))A(λk)+36(V(λk+1)V(λk))=(2+o(1))A(λk).\displaystyle\int_{\partial\Omega}\eta_{k}^{2}\,(n-H)\leq-(2+o(1))\,A(\lambda_{k})+36\,(V(\lambda_{k}+1)-V(\lambda_{k}))=-(2+o(1))\,A(\lambda_{k}).

By Lemma 12, the left side is nonnegative. Since A(λk)A(\lambda_{k})\to\infty by (12), this leads to a contradiction.

It follows that Ω\Omega has finite volume. Applying Proposition 18 to each component of Ω\Omega, we see that Ω\Omega is the union of finitely many balls of radius 1. If Ω\Omega has at least two components, say Ω1\Omega_{1} and Ω2\Omega_{2}, then the function f=χΩ1χΩ2f=\chi_{\Omega_{1}}-\chi_{\Omega_{2}} satisfies

Ωf=0,Ω|Df|2=0,andΩ(nH)f2=2n|B1(0)|.\int_{\partial\Omega}f=0,\qquad\int_{\Omega}|Df|^{2}=0,\qquad\text{and}\qquad\int_{\partial\Omega}(n-H)f^{2}=2\,n\,|B_{1}(0)|.

This contradicts the weak stability of Ω\Omega. Thus, Ω\Omega is connected. This completes the proof of the theorem. ∎

Appendix A First and second variation

Let FC()F\in C^{\infty}(\mathbb{R}) and UnU\subset\mathbb{R}^{n} be nonempty, open, and bounded. Given uC(n)u\in C^{\infty}(\mathbb{R}^{n}), let

JU(u)=12U{yn:u(y)>0}|Du|2U{yn:u(y)>0}F(u).J_{U}(u)=\frac{1}{2}\,\int_{U\cap\{y\in\mathbb{R}^{n}:u(y)>0\}}|Du|^{2}-\int_{U\cap\{y\in\mathbb{R}^{n}:u(y)>0\}}F(u).

Let Ω={yn:u(y)>0}\Omega=\{y\in\mathbb{R}^{n}:u(y)>0\}. We assume that Ω\Omega is nonempty and that Du(y)0Du(y)\neq 0 for all yΩy\in\partial\Omega. By the regular value theorem, Ω\Omega is a domain with outward normal

μ(Ω)=Du|Du|.\mu(\Omega)=-\frac{Du}{|Du|}.

Given ε>0\varepsilon>0, let

(21) {ut:t(ε,ε)}\displaystyle\{u_{t}:t\in(-\varepsilon,\varepsilon)\}

be a smooth family of functions utC(n)u_{t}\in C^{\infty}(\mathbb{R}^{n}) such that u0=uu_{0}=u. Let Ωt={yn:ut(y)>0}\Omega_{t}=\{y\in\mathbb{R}^{n}:u_{t}(y)>0\}. We assume that there is KUK\Subset U such that

{yn:u(y)ut(y)}K\{y\in\mathbb{R}^{n}:u(y)\neq u_{t}(y)\}\subset K

for all t(ε,ε)t\in(-\varepsilon,\varepsilon). Shrinking ε>0\varepsilon>0, if necessary, we may assume that Dut(y)0Du_{t}(y)\neq 0 for all t(ε,ε)t\in(-\varepsilon,\varepsilon) and yΩty\in\partial\Omega_{t}. By the regular value theorem, Ωt\Omega_{t} is a domain. Let ϕCc(n)\phi\in C^{\infty}_{c}(\mathbb{R}^{n}) be given by

ϕ=ddt|t=0ut.\phi=\frac{d}{dt}\bigg|_{t=0}u_{t}.

Let γt\gamma_{t} be the normal speed of the variation {Ωt:t(ε,ε)}\{\partial\Omega_{t}:t\in(-\varepsilon,\varepsilon)\} of hypersurfaces with respect to the normal pointing out of Ωt\Omega_{t}. Note that

(22) γ0=ϕ|Du|.\displaystyle\gamma_{0}=\frac{\phi}{|Du|}.

We assume that

ddt|t=0|UΩt|=d2dt2|t=0|UΩt|=0.\frac{d}{dt}\bigg|_{t=0}|U\cap\Omega_{t}|=\frac{d^{2}}{dt^{2}}\bigg|_{t=0}|U\cap\Omega_{t}|=0.

It follows that

(23) Ωϕ|Du|=0andddt|t=0Ωtγt=0.\displaystyle\int_{\partial\Omega}\frac{\phi}{|Du|}=0\qquad\text{and}\qquad\frac{d}{dt}\bigg|_{t=0}\int_{\partial\Omega_{t}}\gamma_{t}=0.
Lemma 22.

There holds

(24) ddt|t=0JU(ut)=Ω(Δu+F(u))ϕ12Ω|Du|ϕ.\displaystyle\frac{d}{dt}\bigg|_{t=0}J_{U}(u_{t})=-\int_{\Omega}(\Delta u+F^{\prime}(u))\,\phi-\frac{1}{2}\,\int_{\partial\Omega}|Du|\,\phi.
Proof.

Using (22) and (23), we have

ddt|t=0JU(ut)=Ω(DuDϕF(u)ϕ)+12Ω|Du|ϕ.\frac{d}{dt}\bigg|_{t=0}J_{U}(u_{t})=\int_{\Omega}(Du\cdot D\phi-F^{\prime}(u)\,\phi)+\frac{1}{2}\,\int_{\partial\Omega}|Du|\,\phi.

The assertion now follows from the divergence theorem. ∎

Assume that, for every choice of UU, uu is critical for JUJ_{U} among all variations (21). In particular, the right side of (24) vanishes for all ϕCc(n)\phi\in C^{\infty}_{c}(\mathbb{R}^{n}) with

Ωϕ|Du|=0.\int_{\partial\Omega}\frac{\phi}{|Du|}=0.

It follows that there is ρ>0\rho>0 such that

(25) {Δu=F(u)in Ω and|Du|=ρon Ω.\displaystyle\begin{cases}\quad-\Delta u=F^{\prime}(u)\qquad&\text{in $\Omega$ and}\\ \quad|Du|=\rho&\text{on $\partial\Omega$}.\end{cases}
Lemma 23.

Assume that uC(n)u\in C^{\infty}(\mathbb{R}^{n}) satisfies (25). There holds

d2dt2|t=0JU(ut)=Ω(|Dϕ|2F′′(u)ϕ2)+Ω(HF(0)ρ)ϕ2.\frac{d^{2}}{dt^{2}}\bigg|_{t=0}J_{U}(u_{t})=\int_{\Omega}(|D\phi|^{2}-F^{\prime\prime}(u)\,\phi^{2})+\int_{\partial\Omega}\left(H-\frac{F^{\prime}(0)}{\rho}\right)\,\phi^{2}.
Proof.

Given t(ε,ε)t\in(-\varepsilon,\varepsilon), let Φt:ΩΩt\Phi_{t}:\partial\Omega\to\partial\Omega_{t} be the normal parametrization of Ωt\partial\Omega_{t}. By (22),

ddt|t=0Φt=ϕ|Du|Du|Du|=ϕρ2Du.\frac{d}{dt}\bigg|_{t=0}\Phi_{t}=-\frac{\phi}{|Du|}\,\frac{Du}{|Du|}=-\frac{\phi}{\rho^{2}}\,Du.

Note that

ddt|t=0|(Dut)(Φt)|2=2ρ2D2u(Du,Du)ϕ+2DuDϕ.\frac{d}{dt}\bigg|_{t=0}|(Du_{t})(\Phi_{t})|^{2}=-\frac{2}{\rho^{2}}\,D^{2}u(Du,Du)\,\phi+2\,Du\cdot D\phi.

In conjunction with Lemma 22, we obtain

d2dt2|t=0JU(ut)\displaystyle\frac{d^{2}}{dt^{2}}\bigg|_{t=0}J_{U}\left(u_{t}\right) =Ω(Δϕ+F′′(u)ϕ)ϕ1ρΩϕDuDϕ+1ρ3Ωϕ2D2u(Du,Du).\displaystyle=-\int_{\Omega}(\Delta\phi+F^{\prime\prime}(u)\,\phi)\,\phi-\frac{1}{\rho}\,\int_{\partial\Omega}\phi\,Du\cdot D\phi+\frac{1}{\rho^{3}}\,\int_{\partial\Omega}\phi^{2}\,D^{2}u(Du,Du).

By the divergence theorem,

ΩϕΔϕ=Ω|Dϕ|21ρΩDϕDuϕ.\displaystyle\int_{\Omega}\phi\,\Delta\phi=-\int_{\Omega}|D\phi|^{2}-\frac{1}{\rho}\,\,\int_{\partial\Omega}D\phi\cdot Du\,\phi.

Moreover, on Ω\partial\Omega, using (25),

F(0)=Δu=ΔΩu+D2u(μ(Ω),μ(Ω))+Hμ(Ω)Du=1ρ2D2u(Du,Du)Hρ.-F^{\prime}(0)=\Delta u=\Delta^{\partial\Omega}u+D^{2}u(\mu(\Omega),\mu(\Omega))+H\,\mu(\Omega)\cdot Du=\frac{1}{\rho^{2}}\,D^{2}u(Du,Du)-H\,\rho.

The assertion follows from these identities. ∎

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