Nonlocal minimal surfaces

In broad and vague terms, these surfaces arise as the boundaries of domains $E \subset \mathbb{R}^n$ that are minimizers or critical points (within a class of given admissible configurations) of the energy functional:

\[ J_s(E)= C_{n,s}\int_{E}\int_{E^c}\frac{1}{|x-y|^{n+s}}dxdy,\;\; s \in (0,1) \]

It can be checked easily that this agrees (save for a factor of $2$) with norm of the characteristic function $\chi_E$ in the homogenous Sobolev space $\dot{H}^{\frac{s}{2}}$. The dimensional constant $C_{n,s}$ blows up as $s \to 1^-$, in which case (at least when the boundary of $E$ is smooth enough) one can check that $J_s(E)$ converges to the perimeter of $E$.

Classically, minimal surfaces (or generally surfaces of constant mean curvature ) arise in physical situations where one has two phases interacting (eg. water-air, water-ice ) and the energy of interaction is proportional to the area of the interface, which is due to the interaction between particles/agents in both phases being negligible when they are far apart.

Nonlocal minimal surfaces then describe physical phenomena where the interaction potential does not decay fast enough as particles get farther and farther apart, so that two particles on different phases contribute a non-trivial amount to the total interaction energy even if they are away from the interface. In particular, one may consider much more general energy functionals corresponding to different interaction potentials

\[ J_K(E)= \int_{E}\int_{E^c}K(x,y) dxdy \]

Definition

Following the most accepted convention for minimal surfaces, a (classical) nonlocal minimal surface is (given $s\in (0,1)$) the boundary $\Sigma$ of an open set $E \subset \mathbb{R}^n$ such that $\Sigma$ is at least $C^{1,s+\epsilon}$ and more importantly,

\[ H_s(x): = -C_{n,s}\int_{\mathbb{R}^n} \frac{\chi_E(y)-\chi_{E^c}(y)}{|x-y|^{n+s}}dy=0 \;\;\forall\; x \in \Sigma\]

In this case we say that $\Sigma$ is a nonlocal minimal surface in $\Omega$. The quantity $H_s(x)$ is called the "Nonlocal mean curvature of order $s$ of $\Sigma$ at $x$", or briefly, "Nonlocal mean curvature".

Example: Suppose that $E$ and $\Omega$ are such that for any other set $F$ such that $F \Delta E \subset \subset \Omega$ (i.e. $F$ agrees with $E$ outside $\Omega$) we have

\[J_s(E) \leq J_s(F) \]

Then, if it is the case that $E$ has a smooth enough boundary, one can check that $E$ is a nonlocal minimal surface in $\Omega$.

Note For this definition to make sense, $\Sigma$ must be the boundary of some open set $E$, in this article, we will often refer to the set $E$ itself as "the" minimal surface, and no confusion should arise from this.

Nonlocal mean curvature

The scalar quantity

\[ H_s : \Sigma \to \mathbb{R} \] \[ H_s (x) := -C_{n,s} \int_{\mathbb{R}^n}\frac{\chi_E(y)-\chi_{E^c(y)}}{|x-y|^{n+s}}dy \]

Is called the nonlocal mean curvature of $\Sigma$ (or $E$) at $x$, its a real valued function defined on $\Sigma$. Like the usual mean curvature, it measures in some averaged sense the deviation of $\Sigma$ from its tangent hyperplane at $x$ (note that if $\Sigma$ is a hyperplane, then trivially $H_s \equiv 0$).

Mean curvature vs Nonlocal mean curvature: Whereas the standard mean curvature measures mean deviation from flatness at the infinitesimal scale, the nonlocal mean curvature does this at all scales (infinitesimal and positive scales).

As the kernel is invariant under Euclidean symmetries, we conclude for instance that any sphere $\partial B_r(x_0)$ has constant nonlocal mean curvature. Moreover, via a change of variables in the integral defining $H_s$ ($x \to x_0 \to rx$) one can see that a sphere of radius $r$ has mean curvature equal to $c_{n,s}r^{-s}$ (Note that $s=1$ gives the local mean curvature).