Work function
The work function is the minimum energy (usually measured in electron volts) needed to remove an electron from the Fermi level in a metal to a point at infinite distance away outside the surface. The work function is generally about half the ionization energy of a free atom of the metal. E.g Cs has ionization energy 3.9eV and work function 1.9eV.
<math> W = -E_{tot}(N+1) + \{E_{tot}(N) + V(\infty) \} = - {\partial E_{tot} \over {\partial N} } + V(\infty) = - \mu + V(\infty) <math>
<math> E_{tot}(N+1) - E_{tot}(N) = {\partial E_{tot} \over {\partial N} } = \mu <math>
<math> \epsilon_F = \, \mu <math>
Here V is vacuum level and F is fermi level
Photoelectric work function
In photoelectric emission, the electron gains the kinetic energy needed to escape from photons, such an electron is called a photoelectron and the emission is called the photoelectric effect.
Photoelectric work function:
φ=hf0,
where h is Planck's constant and f0 is the critical frequency required for photoelectric emission.
Thermionic work function
The work function is also important in the theory of thermionic emission, here the electron gains its energy from heat rather than photons. In this case, as for example that of an electron escaping from the headed negatively-charged filament of a vacuum tube, the work function may be called the thermionic work function.
Applications
In electronics the work function is important for design of the metal junction in Schottky diodes and for design of vacuum tubes.
The work function for most metals can be approximated as 4.5 eV.
See also
- free energy for the Helmholtz free energy equation, which is the thermodynamic work, note that this work is not related to electron emission and is thus not directly related to the work function.
- Electron affinity
