Photoelectric Effect-Tutorial

The photoelectric effect is the observation that many metals emit electrons when light shines upon them. Electrons emitted in this manner may be called photo electrons.

Overview of the Photoelectric Effect

The photoelectric effect is studied in part because it can be an introduction to wave-particle duality and quantum mechanics.

As shown in video below,when a surface is exposed to sufficiently energetic electromagnetic energy, light will be absorbed and electrons will be emitted. The threshold frequency is different for different materials.

It is visible light for alkali metals, near-ultraviolet light for other metals, and extreme-ultraviolet radiation for non metals. The photoelectric effect occurs with photons having energies from a few electron volts to over 1 MeV. At the high photon energies comparable to the electron rest energy of 511 keV, Compton scattering may occur pair production may take place at energies over 1.022 MeV.

Einstein proposed that light consisted of quanta, which we call photons. He suggested that the energy in each quantum of light was equal to the frequency multiplied by a constant (Planck's constant) and that a photon with a frequency over a certain threshold would have sufficient energy to eject a single electron, producing the photoelectric effect. It turns out that light does not need to be quantized in order to explain the photoelectric effect, but some textbooks persist in saying that the photoelectric effect demonstrates the particle nature of light.

Einstein's Equations for the Photoelectric Effect

Einstein's interpretation of the photoelectric effect results in equations which are valid for visible and ultraviolet light:

energy of photon = energy needed to remove an electron + kinetic energy of the emitted electron

hÎ½ = W + E

where

h is Planck's constant
Î½ is the frequency of the incident photon
W is the work function, which is the minimum energy required to remove an electron from the surface of a given metal: hÎ½0
E is the maximum kinetic energy of ejected electrons: 1/2 mv2
Î½0 is the threshold frequency for the photoelectric effect
m is the rest mass of the ejected electron
v is the speed of the ejected electron

No electron will be emitted if the incident photon's energy is less than the work function.

Applying Einstein's special theory of relativity, the relation between energy (E) and momentum (p) of a particle is

E = [(pc)2 + (mc2)2](1/2)

where m is the rest mass of the particle and c is the velocity of light in a vacuum.

The rate at which photo-electrons are ejected is directly proportional to the intensity of the incident light, for a given frequency of incident radiation and metal.
The time between the incidence and emission of a photo-electron is very small, less than 10–9 second.
For a given metal, there is a minimum frequency of incident radiation below which the photo electric effect will not occur so no photo-electrons can be emitted (threshold frequency).
Above the threshold frequency, the maximum kinetic energy of the emitted photo electrons depends on the frequency of the incident radiation but is independent of its intensity.
If the incident light is linearly polarized then the directional distribution of emitted electrons will peak in the direction of polarization (the direction of the electric field).