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Energy flow

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 $I$ 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 $F$ 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 $P$ joule/sec uniformly into all directions and summed over all frequencies, then the flux through a sphere around it of radius $r$ is simply

\begin{displaymath}F = P / (4 \pi r^2) \end{displaymath} (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 $h\nu$. Since these quanta travel at the speed of light $c$, those in a shell of thickness $dr$ will pass through the outer surface of the shell in the time $dr/c$. Since the area of the shell is $4 \pi r^2$, if there are $n$ photons per unit volume in the shell, the number passing through the surface per second will be

\begin{displaymath}
\left(n 4 \pi r^2 dr\right)/\left(dr/c\right) = 4 \pi r^2 n c
\end{displaymath} (12)

each with energy $h\nu$. With this quantum view, the flux must be this number times the energy per photon, divided by the surface area, or
$\displaystyle F = h \nu \left(4 \pi r^2 n c\right) / \left(4 \pi r^2 \right)$     (13)
$\displaystyle F = h \nu n c$     (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
$\displaystyle h \nu n c = P / (4 \pi r^2)$     (15)
$\displaystyle n = P / (4 \pi r^2 h \nu c)$     (16)

The photon density also decreases as the $2^{nd}$ power of $r$. Either a detector counting photons or one measuring energy will show an inverse square law with distance from the source.


next up previous contents
Next: The experiment Up: Inverse square law Previous: Inverse square law   Contents
John Kielkopf 2001-01-23