A Level Physics Notes: Electrons and Photons – Photon Pressure
Photons have both wave and particle characteristics and observe
wave particle duality. Though they have no mass, they carry momentum
via the De Broglie equation
Then
for example whenever they are reflected from a mirror or interact
with matter, an exchange of momentum takes place. At all stages total
momentum is conserved as in classical mechanics, even if the actual
definition of momentum changes slightly and is not now equal
to
Suppose
then that a photon is bounced between two mirrors a distance
apart.
The photon travels with speed
the
speed of light, so travels a distance
in
seconds.
Before returning to the mirror it must travel to the second mirror,
undergo reflection and return to the first one. The time taken to
return is then
and
the photon strikes the mirror
times
per second. Each time it strikes the mirror it transfers momentum
equal to
to
the mirror so the force exerted on the mirror is equal to the rate of
change of momentum
The pressure exerted is tiny. One photon with a wavelength of
bouncing
between mirrors 1 m apart exerts a pressure of![]()
The pressure exerted by photons is the principle behind the solar sail. Photons from the Sun bounce off a large flat sail in space, pushing the sail away from the Sun. A very large surface area must be used to generate a force sufficient to accelerate the sail to an appreciable speed.