Plasma Frequency
Source lecture(s): pc368_lec03_frequency
Intuition
Pluck an electron cloud away from the ion background and it will oscillate. The natural frequency of this sloshing is the electron plasma frequency \(\omega_{pe}\). It sets the timescale for virtually every electrostatic process in a plasma, from Langmuir waves to Landau damping.
Formal Definition
For a cold electron–ion plasma with stationary ions:
where \(n_e\) is the electron number density.
Mathematical Formulation
Displace electrons by a small distance \(x\) relative to the fixed ion background. The charge imbalance creates an electric field \(E = n_e e x / \varepsilon_0\) (from Gauss’s law). Newton’s second law for the electron fluid gives:
This is simple harmonic motion with frequency \(\omega = \sqrt{n_e e^2/(m_e \varepsilon_0)}\).
Derivation
- Linearize continuity, momentum, and Poisson equations about a uniform equilibrium with stationary ions.
- For isothermal electrons (\(T_e\) constant), momentum equation gives \(m_e \partial v_e / \partial t = -e E\).
- Combining with \(\partial n_1 / \partial t + n_0 \nabla \cdot v_e = 0\) and \(\nabla \cdot E = e n_1 / \varepsilon_0\), eliminate \(v_e\) and \(n_1\).
- The result is the wave equation \(\nabla^2 E = (\omega_{pe}^2 / c^2) E\), or more precisely, \(\omega^2 = \omega_{pe}^2 + c^2 k^2\) for electromagnetic disturbances.
Worked Example
Problem: What is \(\omega_{pe}\) in the solar corona (\(n_e \sim 10^{15}\,\text{m}^{-3}\))?
\(\omega_{pe} = \sqrt{10^{15} \times (1.6\times 10^{-19})^2 / (9.11\times 10^{-31} \times 8.85\times 10^{-12})} \approx 5.6\times 10^8\,\text{rad/s}\) (\(f_{pe} \approx 89\) MHz).
Common Mistakes
- \(\omega_{pe}\) depends only on density. Confirm before using.
- The ion plasma frequency matters for high-frequency electromagnetic waves.
- Plasma oscillation is not a sound wave. It is an electrostatic Langmuir mode.
Related Concepts
Quiz Questions
- Conceptual: If you suddenly removed all ions from a plasma, what would the electron frequency become?
- Computational: Compute \(\omega_{pe}\) for a dusty plasma with \(n_e = 10^{12}\,\text{m}^{-3}\).
- MCQ: For which of these parameters does \(\omega_{pe}\) increase?
- A) Lowering \(n_e\)
- B) Increasing \(m_e\)
- C) Increasing \(T_e\)
- D) Increasing \(n_e\)
Further Reading
- T. J. M. Boyd & J. J. Sanderson, Plasma Dynamics via Atoms.