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RADIATED POWER
The electric and magnetic field components are obtained from the wave
function
by taking the partial derivatives
listed in the tables in Section II.C. With their help we shall now
find the Poynting vector component along the
-direction, namely
Its space integral,
 |
(57) |
is the total radiated momentum (=radiant energy flow) into the
-direction. It is positive (resp. negative) whenever the source
is confined to Rindler sector
(resp.
). Furthermore, the
-momentum is independent of the synchronous time
because
is a cyclic coordinate. This
-momentum measures the
energy radiated by the two accelerated sources, and it takes the place
of what in a static inertial reference frame is the emitted energy.
Both the T.E. and the T.M. field have the same Poynting vector
component along the
-direction. More precisely, reference to
the table of T.E. and the T.M. field components (Section II) shows that
in Rindler sector
this Poynting object is
![\begin{displaymath}
T^\xi_{~\tau}=\frac{\xi}{4\pi}
\left[
\frac{\partial}{\part...
...ac{1}{r}\frac{\partial\psi}{\partial \theta}\right)
\right]
~,
\end{displaymath}](img316.png) |
(58) |
the same for both types of fields. Furthermore, the wave function
is governed by a wave equation, which is also common to both
fields. Consequently, the mathematical analysis which relates
observations to the radiation sources is the same for both types of
radiation fields. However, it is the difference in two types of
sources which is important from the viewpoint of physics.
The only difference lies in the source and hence in the amplitude and
phase of
in
. Comparing the ensuing Eq.(60) with Eq.(63), one sees
that T.E. and T.M. polarized radiation are caused by the densities of
magnetic and electric dipole moment respectively.
Subsections
Next: Axially Symmetric Source and
Up: RADIATION FROM VIOLENTLY ACCELERATED
Previous: The Rindler Interferometer
Ulrich Gerlach
2001-10-09