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Let us now investigate the propagation of electromagnetic radiation through
a dispersive medium by studying a simple one-dimensional problem.
Suppose that our dispersive medium extends from
, where it interfaces
with a vacuum, to
. Suppose further that a wave is incident
normally
on the medium, so that the field quantities only depend on
and
.
The wave is specified as a given function of
at
. Since we are
not interested in the reflected wave, let this function,
, say,
give the wave amplitude just inside the surface of the dispersive medium.
Suppose that the wave arrives at this surface at
, and
that
 |
(704) |
How does the wave subsequently develop in the region
? In order to
answer this question we must first of all decompose
into harmonic
components of the form
(i.e., Fourier
harmonics). Unfortunately, if we attempt this using only real frequencies,
, we encounter convergence difficulties, since
does not
vanish at
. For the moment, we can circumvent these difficulties
by only considering finite (in time) wave forms. In other words, we now
imagine that
for
and
. Such a wave form can be thought
of as the superposition of two infinite (in time) wave forms, the first
beginning at
and the second at
with the opposite phase, so
that the two cancel for all time
.
According to standard Fourier transform theory
 |
(705) |
Since
is a real function of
which is zero for
and
, we can write
![\begin{displaymath}
f(t) = \frac{1}{2\pi}\int_{-\infty}^{\infty} d\omega
\int_0^Tf(t')\,\cos[\omega(t-t')\,]\,dt'.
\end{displaymath}](img1603.png) |
(706) |
Finally, it follows from symmetry (in
) that
![\begin{displaymath}
f(t) = \frac{1}{\pi}\int_0^{\infty} d\omega
\int_0^Tf(t')\,\cos[\omega(t-t')\,]\,dt'.
\end{displaymath}](img1604.png) |
(707) |
Equation (4.69) yields
![\begin{displaymath}
f(t) = \frac{1}{\pi}\int_0^{\infty} d\omega \int_0^T
\sin\!\left(\frac{2\pi t'}{\tau}\right) \,\cos[\omega(t-t')\,]\,dt',
\end{displaymath}](img1605.png) |
(708) |
or
Let us assume, for the sake of simplicity, that
 |
(709) |
where
is a positive integer. This ensures that
is continuous
at
. Equation (4.74) reduces to
![\begin{displaymath}
f(t) = \frac{2}{\tau} \int_0^\infty \frac{d\omega}{\omega^2 ...
.../\tau)^2}
\left(\, \cos[\omega(t-T)\,] -\cos\omega t\,\right).
\end{displaymath}](img1609.png) |
(710) |
This expression can be written
![\begin{displaymath}
f(t) = \frac{1}{\tau} \int_{-\infty}^{\infty} \frac{d\omega}...
.../\tau)^2}
\left(\, \cos[\omega(t-T)\,] -\cos\omega t\,\right),
\end{displaymath}](img1610.png) |
(711) |
or
 |
(712) |
It is not entirely obvious that Eq. (4.78) is equivalent to Eq. (4.77).
However, we can easily prove that this is the case by taking Eq. (4.78)
and using the standard definition of a real part (i.e., half the
sum of the quantity in question and its complex conjugate) to give
Replacing the dummy integration variable
by
in the
second integral and then making
use of symmetry, it is easily seen that the above expression reduces to
Eq. (4.77).
Equation (4.77) can be written
![\begin{displaymath}
f(t) = \frac{2}{\tau}\int_{-\infty}^{\infty}d\omega\,
\sin[\omega(t-T/2)]\, \frac{\sin(\omega T/2)}{\omega^2 -(2\pi/\tau)^2}.
\end{displaymath}](img1615.png) |
(714) |
Note that the integrand is finite at
, since at this
point the vanishing of the denominator is compensated for by the
simultaneous vanishing of the numerator. It follows that the integrand in
Eq. (4.78) is also not infinite at
, as long as we do
not separate the two exponentials. Thus,
we can replace the integration along the real axis through this point by a small semi-circle
in the upper half of the complex plane. Once this has been done, we can deform
the path still further and can integrate the two exponentials
in Eq. (4.78) separately:
 |
(715) |
The contour
is sketched in Fig. 6. Note that it runs from
to
, which accounts for the change of sign between Eqs. (4.78)
and (4.81).
Figure 6:
Sketch of the integration contours used to evaluate
Eqs. (4.78) and (4.81)
 |
We have already noted that a finite wave form which is zero for
and
can be through of as the superposition of two out of phase infinite
wave forms, one starting at
and the other at
. It is plausible,
therefore, that the first term in the above expression corresponds
to the infinite wave form starting at
, and the second to the
infinite wave form starting at
. If this is the case then
the signal
(4.69), which starts at
and ends at
, can be written
in the form
 |
(716) |
Let us test this proposition. In order to do this we must replace the
original path of integration
by two equivalent paths.
First, consider
. In this case,
has a negative
real part in the upper half plane which increases indefinitely with
increasing distance from the axis. Thus, we can replace the original
path of integration by the path
(see Fig. 7). The integral clearly
vanishes along this path if we let
approach infinity in the upper
half plane. Consequently,
 |
(717) |
for
.
Next, consider
. Now,
has a negative
real part in the lower half plane, so that the exponential vanishes at
infinity in this half plane. If we attempt to deform
to infinity
in the lower half plane, the path of integration ``catches'' on the
singularity of the integrand at
(see Fig. 7).
The path of integration
therefore consists of three parts: the
part at infinity,
, where the integral vanishes due
to the exponential factor
;
, the
two parts leading to infinity which cancel each other and thus contribute
nothing to the integral; the path
around the singularity. This
latter contribution can easily be evaluated using the Cauchy
residue theorem:
 |
(718) |
Thus, it is proven that the expression (4.82) actually describes a wave form
beginning at
whose subsequent motion is specified by Eq. (4.69).
Figure 7:
Sketch of the integration contours used to evaluate Eq. (4.82)
 |
Equation (4.82) can immediately be generalized to give the wave motion
in the region
:
 |
(719) |
This follows from standard wave theory, because we know that an
unterminated wave motion at
of the form
takes the form
after moving a distance
in the dispersive medium, provided that
and
are related by the appropriate dispersion relation. For a medium consisting
of a single resonant species this dispersion relation is written
(see Eq. (4.17))
 |
(720) |
Next: Propagation of the wave
Up: Electromagnetic wave propagation in
Previous: Wave propagation through a
Richard Fitzpatrick
2002-05-18