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The power radiated by a source of light is described by the flow of light away
from it, into a particular direction, and through a defined surface. The
intensity
is the energy emitted per unit time, per unit area of the
source, per unit frequency interval, per unit solid angle into a chosen
direction. The flux
is the energy flowing per unit time onto a detector,
through a unit area of its surface, per unit frequency interval. So if a point
source emits energy at a rate
joule/sec uniformly into all directions
and summed over all frequencies, then the flux through a sphere around it of
radius
is simply
 |
(11) |
This
is the inverse square law describing the decline of flux with increasing
distance from the source.
The energy of light is carried by quanta, each with energy
. Since
these quanta travel at the speed of light
, those in a shell of thickness
will pass through the outer surface of the shell in the time
.
Since the area of the shell is
, if there are
photons per unit
volume in the shell, the number passing through the surface per second will be
 |
(12) |
each with energy
. With this quantum view, the flux must be
this number times the energy per photon, divided by the surface area, or
 |
|
|
(13) |
 |
|
|
(14) |
The equations for flux must measure the same thing. It
follows that the density of photons depends on distance from the source too
according to
 |
|
|
(15) |
 |
|
|
(16) |
The photon density also decreases as the
power of
.
Either a detector counting photons or one measuring energy will show an
inverse square law with distance from the source.
Next: The experiment
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John Kielkopf
2001-01-23