In mathematics, the capacity of a set in Euclidean space is a measure of the "size" of that set. Unlike, say, Lebesgue measure, which measures a set's volume or physical extent, capacity is a mathematical analogue of a set's ability to hold electrical charge. More precisely, it is the capacitance of the set: the total charge a set can hold while maintaining a given potential energy. The potential energy is computed with respect to an idealized ground at infinity for the harmonic or Newtonian capacity, and with respect to a surface for the condenser capacity.
The notion of capacity of a set and of "capacitable" set was introduced by Gustave Choquet in 1950: for a detailed account, see reference .
Let Σ be a closed, smooth, (n - 1)-dimensional hypersurface in n-dimensional Euclidean space
Rn
C(\Sigma,S)=-
1{(n | |
- |
2)\sigman
where:
\partialu | |
\partial\nu |
(x)=\nablau(x) ⋅ \nu(x)
is the normal derivative of u across ; and
Rn
C(Σ, S) can be equivalently defined by the volume integral
C(\Sigma,S)=
1{(n | |
- |
2)\sigman
The condenser capacity also has a variational characterization: C(Σ, S) is the infimum of the Dirichlet's energy functional
I[v]=
1{(n | |
- |
2)\sigman
over all continuously differentiable functions v on D with v(x) = 1 on Σ and v(x) = 0 on S.
Heuristically, the harmonic capacity of K, the region bounded by Σ, can be found by taking the condenser capacity of Σ with respect to infinity. More precisely, let u be the harmonic function in the complement of K satisfying u = 1 on Σ and u(x) → 0 as x → ∞. Thus u is the Newtonian potential of the simple layer Σ. Then the harmonic capacity or Newtonian capacity of K, denoted C(K) or cap(K), is then defined by
C(K)=
\int | |
Rn\setminusK |
|\nablau|2dx.
If S is a rectifiable hypersurface completely enclosing K, then the harmonic capacity can be equivalently rewritten as the integral over S of the outward normal derivative of u:
C(K)=\intS
\partialu | |
\partial\nu |
d\sigma.
The harmonic capacity can also be understood as a limit of the condenser capacity. To wit, let Sr denote the sphere of radius r about the origin in
Rn
C(K)=\limrC(\Sigma,Sr).
The harmonic capacity is a mathematically abstract version of the electrostatic capacity of the conductor K and is always non-negative and finite: 0 ≤ C(K) < +∞.
The Wiener capacity or Robin constant W(K) of K is given by
C(K)=e-W(K)
In two dimensions, the capacity is defined as above, but dropping the factor of
(n-2)
C(\Sigma,S)=-
1{2\pi} | |
\int |
S'
\partialu | |
\partial\nu |
d\sigma' =
1{2\pi} | |
\int |
D|\nablau|2dx
n\to2
The harmonic function u is called the capacity potential, the Newtonian potential when
n\ge3
n=2
u(x)=\intSG(x-y)d\mu(y)
G(x-y)= | 1{|x-y| |
n-2 |
n\ge3
G(x-y)=log | 1{|x-y|} |
n=2
\mu
C(K)=\intSd\mu(y)=\mu(S)
The variational definition of capacity over the Dirichlet energy can be re-expressed as
C(K)=\left[infλE(λ)\right]-1
λ
λ(K)=1
E(λ)
E(λ)=\int\intK x G(x-y)dλ(x)dλ(y)
The characterization of the capacity of a set as the minimum of an energy functional achieving particular boundary values, given above, can be extended to other energy functionals in the calculus of variations.
Solutions to a uniformly elliptic partial differential equation with divergence form
\nabla ⋅ (A\nablau)=0
I[u]=\intD(\nablau)TA(\nablau)dx
The capacity of a set E with respect to a domain D containing E is defined as the infimum of the energy over all continuously differentiable functions v on D with v(x) = 1 on E; and v(x) = 0 on the boundary of D.
The minimum energy is achieved by a function known as the capacitary potential of E with respect to D, and it solves the obstacle problem on D with the obstacle function provided by the indicator function of E. The capacitary potential is alternately characterized as the unique solution of the equation with the appropriate boundary conditions.