In a two-dimensional space-time we define:
conformal global coordinates;
.
time and distance to an origin (
).
,
):
:
:
and
where
is a constant (Vendrell (1997a)) (The solution depends actually on the
representation of the delta function (eq.3), which is defined here by
, where the function
is continuous except possibly at
.)
The functions
and
are left undetermined for
, contrary to the 4-D case (Synge (1957)).