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Home/Electricity & Magnetism/Langmuir Plasma Oscillations

Langmuir Plasma Oscillations

Langmuir oscillations are the simplest collective mode of an electron plasma: electrons oscillate against a stationary ion background on a timescale set by the plasma frequency ω_p = √(n_e e²/ε₀ m_e). In the electrostatic limit, a uniform displacement of electrons creates a restoring electric field that drives harmonic motion at ω_p. Propagating Langmuir waves add spatial structure with wavevector k and, when thermal motion is included, the Bohm–Gross dispersion ω² = ω_p² + 3 k² v_th² with v_th = √(k_B T_e/m_e). At long wavelength the frequency approaches ω_p; at shorter wavelengths thermal corrections raise ω above ω_p. This simulator animates a sinusoidal density perturbation δn/n ∝ sin(kx − ωt) with fixed ions, plots the ω(k) dispersion against the cold-plasma asymptote ω_p, and shows how ω_p scales as √n_e. It complements the Debye shielding page: λ_D sets spatial shielding while ω_p sets the fastest collective timescale. Landau damping and electromagnetic effects are omitted.

Who it's for: Undergraduate plasma physics or electromagnetism students after Debye shielding and before magnetized waves or kinetic theory.

Key terms

  • Langmuir oscillation
  • Plasma frequency
  • Bohm–Gross dispersion
  • Electron plasma wave
  • Phase velocity
  • Quasineutrality

Langmuir oscillations

18
10000K
500m⁻¹
0.15
1×

Collective electron oscillations at ω_p = √(n_e e²/ε₀m_e). Ions are heavy and stay fixed on this timescale. Langmuir waves disperse as ω² = ω_p² + 3k²v_th² (Bohm–Gross).

Measured values

ω_p5.641e+10rad/s
f_p8.98 GHz
ω(k)5.642e+10rad/s
λ_D (compare)0.01 mm
Phase velocity v_ph1.13e+8m/s

How it works

Langmuir plasma oscillations: ω_p = √(n_e e²/ε₀m_e), animated electron density wave, and Bohm–Gross dispersion ω(k) phase diagram.

Frequently asked questions

Why do ions appear fixed?
Ions are much heavier than electrons (m_i ≫ m_e), so on the electron oscillation period they barely move. The Langmuir mode is an electron sloshing mode against a neutralizing ion background.
What is ω_p physically?
It is the natural frequency at which electrons collectively try to restore charge neutrality after a displacement. Higher density means stronger restoring fields → higher ω_p.
Why does ω increase with k at finite temperature?
Thermal pressure adds a restoring contribution at finite k, giving the Bohm–Gross correction 3k²v_th² under the square root in the dispersion relation.
How is this related to Debye shielding?
Both use the same n_e and T_e. λ_D describes static spatial shielding of a charge; ω_p describes the fastest collective oscillation timescale of the electron fluid.