In special relativity, electromagnetism and wave theory, the d'Alembert operator (denoted by a box:
\Box
In Minkowski space, in standard coordinates, it has the form
\begin{align} \Box&=\partial\mu\partial\mu=η\mu\nu\partial\nu\partial\mu=
1 | |
c2 |
\partial2 | |
\partialt2 |
-
\partial2 | |
\partialx2 |
-
\partial2 | |
\partialy2 |
-
\partial2 | |
\partialz2 |
\\ &=
1 | |
c2 |
{\partial2\over\partialt2}-\nabla2=
1 | |
c2 |
{\partial2\over\partialt2}-\Delta~~. \end{align}
Here
\nabla2:=\Delta
η00=1
η11=η22=η33=-1
η\mu\nu=0
\mu ≠ \nu
(Some authors alternatively use the negative metric signature of, with
η00=-1, η11=η22=η33=1
Lorentz transformations leave the Minkowski metric invariant, so the d'Alembertian yields a Lorentz scalar. The above coordinate expressions remain valid for the standard coordinates in every inertial frame.
There are a variety of notations for the d'Alembertian. The most common are the box symbol
\Box
\Box2
\DeltaM
Another way to write the d'Alembertian in flat standard coordinates is
\partial2
Sometimes the box symbol is used to represent the four-dimensional Levi-Civita covariant derivative. The symbol
\nabla
The wave equation for small vibrations is of the form
\Boxcu\left(x,t\right)\equivutt-
2u | |
c | |
xx |
=0~,
The wave equation for the electromagnetic field in vacuum is
\BoxA\mu=0
The Klein–Gordon equation has the form
\left(\Box+
m2c2 | |
\hbar2 |
\right)\psi=0~.
The Green's function,
G\left(\tilde{x}-\tilde{x}'\right)
\BoxG\left(\tilde{x}-\tilde{x}'\right)=\delta\left(\tilde{x}-\tilde{x}'\right)
where
\delta\left(\tilde{x}-\tilde{x}'\right)
\tilde{x}
\tilde{x}'
A special solution is given by the retarded Green's function which corresponds to signal propagation only forward in time[2]
G\left(\vec{r},t\right)=
1 | |
4\pir |
\Theta(t)\delta\left(t-
r | |
c |
\right)
where
\Theta