In plasma physics, the Debye length, named after the Dutch physical chemist Peter Debye, is the scale over which mobile charge carriers (e.g. electrons) screen out electric fields in plasmas and other conductors. In other words, the Debye length is the distance over which significant charge separation can occur. A Debye sphere is a volume whose radius is the Debye length, in which there is a sphere of influence, and outside of which charges are screened.
In space plasmas where the electron density is relatively low, the Debye length may reach macroscopic values, such as in the Magnetosphere, Solar wind, Interstellar medium and Intergalactic medium (see table):
Plasma | Density ne(m3) |
Electron temperature T(K) |
Magnetic field B(T) |
Debye length λD(m) |
Gas discharge | 1016 | 104 | — | 10−4 |
Tokamak | 1020 | 108 | 10 | 10−4 |
Ionosphere | 1012 | 103 | 10−5 | 10−3 |
Magnetosphere | 107 | 107 | 10−8 | 102 |
Solar core | 1032 | 107 | — | 10−11 |
Solar wind | 106 | 105 | 10−9 | 10 |
Interstellar medium | 105 | 104 | 10−10 | 10 |
Intergalactic medium | 1 | 106 | — | 105 |
http://www.pma.caltech.edu/Courses/ph136/yr2002/
Debye length in a plasma
In a plasma, the Debye length is
- \( \lambda_D = \sqrt{\frac{\varepsilon_0 k/q_e^2}{n_e/T_e+\sum_{ij} j^2n_{ij}/T_i}}\)
where
- λD is the Debye length,
- ε0 is the permittivity of free space,
- k is Boltzmann’s constant,
- qe is the charge on an electron,
- Te and Ti are the temperatures of the electrons and ions, respectively,
- ne is the density of electrons,
- nij‘is the density of atomic species i, with positive ionic charge jqe
The ion term is often dropped, giving
- \( \lambda_D = \sqrt{\frac{\varepsilon_0 k T_e}{n_e q_e^2}}\)
although this is only valid when the ions are much colder than the electrons.
Debye length in an electrolyte
In an electrolyte, the Debye length is
- \( \lambda_D = \sqrt{\frac{\varepsilon_0 \varepsilon_r k T}{2 N_A e^2 I}}\)
where
- I is the ionic strength of the electrolyte,
- ε0 is the permittivity of free space,
- εr is the dielectric constant,
- k is the Boltzmann’s constant,
- T is the Temperature,
- NA is Avogadro’s Number.
- e is the elementary charge,
or when the solute is mono-monovalent and symmetrical,
- \( \lambda_D = \sqrt{\frac{\varepsilon_0 \varepsilon_r R T}{2 F^2 C_0}}\)
where
- R is the gas constant,
- F is the Faraday constant,
- C0 is the molar concentration of the electrolyte.