Mechanism
Consider an electrically neutral plasma in equilibrium, consisting of a gas of positively charged ions and negatively charged electrons. If one displaces an electron or a group of electrons slightly with respect to the ions, the Coulomb force pulls the electrons back, acting as a restoring force.
Cold electrons
If the thermal motion of the electrons is ignored, the charge density oscillates at the plasma frequency:
![{\displaystyle \omega _{\mathrm {pe} }={\sqrt {\frac {n_{\mathrm {e} }e^{2}}{m^{*}\varepsilon _{0}}}},\quad {\text{[rad/s]}}\quad {\text{(SI units)}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4910398c95e4e4df567f20a6941f459ec25ed6a6)
![{\displaystyle \omega _{\mathrm {pe} }={\sqrt {\frac {4\pi n_{\mathrm {e} }e^{2}}{m^{*}}}},\quad {\text{[rad/s]}}\quad {\text{(cgs units)}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/6fe0f39b470b6e6e69b69f15e9ed4ae01f7761f3)
where
is the electron number density,
is the elementary charge,
is the electron effective mass, and
is the vacuum permittivity. This assumes infinite ion mass, a good approximation since electrons are much lighter.
A derivation using Maxwell’s equations[2] gives the same result via the dielectric condition
. This is the condition for plasma transparency and wave propagation.
In electron–positron plasmas, relevant in astrophysics, the expression must be modified. As the plasma frequency is independent of wavelength, Langmuir waves have infinite phase velocity and zero group velocity.
For
, the frequency depends only on electron density and physical constants. The linear plasma frequency is:
![{\displaystyle f_{\text{pe}}={\frac {\omega _{\text{pe}}}{2\pi }}\quad {\text{[Hz]}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ce623377541799962e2101c448ca691a2913c45e)
Metals are reflective to light below their plasma frequency, which is in the UV range (~10²³ electrons/cm³). Hence they appear shiny in visible light.
Warm electrons
Including the effects of electron thermal velocity
, the dispersion relation becomes:

This is known as the Bohm–Gross dispersion relation. For long wavelengths, pressure effects are minimal; for short wavelengths, dispersion dominates. At these small scales, wave phase velocity
becomes comparable to
, leading to Landau damping.
In bounded plasmas, plasma oscillations can still propagate due to fringing fields, even for cold electrons.
In metals or semiconductors, the ions' periodic potential is accounted for using the effective mass
.