Copyright © 1999-2000 David E. Rutherford
All Rights Reserved
The scalar electric potential
, or
for short,
at an arbitrary field event
, or
for short,
due to a stationary point charge
at an
event
, or
for short, in the unprimed frame is
where
and
is
the spacetime interval between events
and
in the
unprimed frame from (3.2). Notice that the spatial part of
, can
be zero, while the time part remains non-zero. In this case, the potential
(10.1) does not become infinite at r = 0.
If we transform the components of the primed spacetime interval,
, using
(6.2) with
, since
the primed observer's measurement of the interval between the events is made
instantaneously in his frame, the spacetime interval
becomes
where
or
and
are the components of the spacetime interval between events
and
.
To find the scalar potential
due
to a distribution of stationary charges, we need to sum the contributions
from each of the individual elements of charge. For the contribution of an
element of charge
at an
event
, we make use of the fact that
, where
is the
charge density at the event
, and
is
the element of volume containing
. The
general equation for the scalar potential
at an
arbitrary field event
due
to a distribution of stationary charges is
The components of the potential field four-vector
, not
to be confused with the transformation matrix
, at
the field
event
due to a distribution of moving charges at the field event P(2) are
where the
are the components of the four-velocity of the element of charge
.
Noting that the components of the current density four-vector
at the
event
are
we can write the general relation for the components of the potential field
four-vector
at an
arbitrary field event
due
to a distribution of moving charges. By inserting (10.9) into (10.8), we
get
Copyright © 1999-2000 David E. Rutherford
All Rights Reserved
E-mail: drutherford@softcom.net