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<record version="4" id="5980">
 <title>current</title>
 <name>Current</name>
 <created>2004-07-02 11:31:50</created>
 <modified>2004-07-12 10:32:05</modified>
 <type>Definition</type>
 <creator id="1187" name="paolini"/>
 <author id="1187" name="paolini"/>
 <classification>
	<category scheme="msc" code="58A25"/>
 </classification>
 <defines>
	<concept>mass</concept>
	<concept>support</concept>
 </defines>
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 <content>Let $\Lambda_c^m(\R^n)$ denote the space of $C^\infty$ differentiable $m$-forms with compact support in $\R^n$. A continuous linear operator $T\colon \Lambda_c^m(\R^n)\to \R$ is called an $m$-\emph{current}. Let $\mathcal D_m$ denote the space of $m$-currents in $\R^n$. 
We define a boundary operator $\partial\colon \mathcal D_{m+1}\to \mathcal D_m$ by
\[
  \partial T(\omega) := T(d\omega).
\]

We will see that currents represent a generalization of $m$-surfaces.
In fact if $M$ is a compact $m$-dimensional oriented manifold with boundary, we can associate to $M$ the current $[[M]]$ defined by
\[
  [[M]](\omega)=\int_M \omega.
\]
So the definition of boundary $\partial T$ of a current, is justified by
Stokes Theorem:
\[
  \int_{\partial M} \omega = \int_M d\omega.
\]

The space $\mathcal D_m$ of $m$-dimensional currents is a real vector space with operations defined by
\[
  (T+S)(\omega):= T(\omega)+S(\omega),\qquad
   (\lambda T)(\omega):=\lambda T(\omega).
\]
The sum of two currents represents the \emph{union} of the surfaces they represents. Multiplication by a scalar represents a change in the \emph{multiplicity} of the surface. In particular multiplication by $-1$ represents the change of orientation of the surface.

We define the \emph{support} of a current $T$, denoted by $\mathrm{spt}(T)$, the smallest closed set $C$ such that
\[
  T(\omega)=0\ \text{whenever $\omega=0$ on $C$}.
\]
We denote with $\mathcal E_m$ the vector subspace of $\mathcal D_m$ of currents with compact support.

\section*{Topology}
The space of currents is naturally endowed with the \emph{weak-star} topology, which will be further simply called \emph{weak convergence}. We say that a sequence $T_k$ of currents, weakly converges to a current $T$ if
\[
   T_k(\omega) \to T(\omega),\qquad \forall \omega.
\]

A stronger norm on the space of currents is the \emph{mass norm}. First of all we define the mass norm of a $m$-form $\omega$ as
\[
  ||\omega||:= \sup\{|\langle \omega,\xi\rangle|\colon \text{$\xi$ is a unit, simple, $m$-vector}\}.
\]
So if $\omega$ is a simple $m$-form, then its mass norm is the usual norm of its coefficient. We hence define the \emph{mass} of a current $T$ as
\[
  \mathbf M (T) := \sup\{ T(\omega)\colon \sup_x ||\omega(x)||\le 1\}.
\]
The mass of a currents represents the \emph{area} of the generalized surface.

An intermediate norm, is the \emph{flat norm} defined by
\[
  \mathbf F (T) := \inf \{\mathbf M(A) + \mathbf M(B) \colon
    T= A + \partial B,\ A\in\mathcal E_m,\ B\in\mathcal E_{m+1}\}.
\]

Notice that two currents are close in the mass norm if they coincide apart from 
a small part. On the other hand the are close in the flat norm if they coincide up to a small deformation.


\section*{Examples}
Recall that $\Lambda_c^0(\R^n)\equiv C^\infty_c(\R^n)$ so that the following defines a $0$-current:
\[
  T(f) = f(0). 
\]
In particuar every signed measure $\mu$ with finite mass is a $0$-current:
\[
  T(f) = \int f(x)\, d\mu(x).
\]

Let $(x,y,z)$ be the coordinates in $\R^3$. Then the following defines a $2$-current:
\[
T(a\,dx\wedge dy + b\,dy\wedge dz + c\,dx\wedge dz) = 
 \int_0^1 \int_0^1 b(x,y,0)\, dx \, dy.
\]</content>
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