plasma parameter

{{Distinguish|Plasma parameters}}

The plasma parameter is a dimensionless number, denoted by capital Lambda, {{math|Λ}}. The plasma parameter is usually interpreted to be the argument of the Coulomb logarithm, which is the ratio of the maximum impact parameter to the classical distance of closest approach in Coulomb scattering. In this case, the plasma parameter is given by:{{ cite book | last = Chen | first = Francis F. | title = Introduction to Plasma Physics and Controlled Fusion | publisher = Springer | location = New York | year = 2006 }}

\Lambda = 4\pi n_\text{e}\lambda_\text{D}^3

where

This expression is typically valid for a plasma in which ion thermal velocities are much less than electron thermal velocities. A detailed discussion of the Coulomb logarithm is available in the NRL Plasma Formulary, pages 34–35.

Note that the word parameter is usually used in plasma physics to refer to bulk plasma properties in general: see plasma parameters.

An alternative definition of this parameter is given by the average number of electrons in a plasma contained within a Debye sphere (a sphere of radius the Debye length). This definition of the plasma parameter is more frequently (and appropriately) called the Debye number, and is denoted N_\text{D}. In this context, the plasma parameter is defined as

N_\text{D} = \frac{4\pi}{3} n_\text{e}\lambda_\text{D}^3 = \frac{1}{3}\Lambda

Since these two definitions differ only by a factor of three, they are frequently used interchangeably.

Often the factor of \frac{4\pi}{3} is dropped. When the Debye length is given by \lambda_\text{D} = \sqrt{\frac{\varepsilon_0 k_\text{B}T_\text{e}}{n_\text{e}q_\text{e}^2}}, the plasma parameter is given by{{cite book | last = Miyamoto | first = K. | title = Fundamentals of Plasma Physics and Controlled Fusion | location = Iwanami, Tokyo | year = 1997}}

N_\text{D} = \frac{{\left(\varepsilon_0 k_\text{B} T_\text{e}\right)}^{3/2}}{q_\text{e}^3 {n_\text{e}}^{1/2}}

= \left(\frac{k_\text{B} T_e}{n_e^{1/3}}\right)^{3/2} \left(\frac{q_e^2}{\varepsilon_0}\right)^{-3/2}

where

Confusingly, some authors define the plasma parameter as:

\varepsilon_p = \Lambda^{-1} .

Coupling parameter

A closely related parameter is the plasma coupling \Gamma, defined as a ratio of the Coulomb energy to the thermal one:

\Gamma = \frac{E_\text{C}}{k_\text{B}T_\text{e}}.

The Coulomb energy (per particle) is

E_\text{C} = \frac{q_\text{e}^2}{4\pi\varepsilon_0\langle r \rangle},

where for the typical inter-particle distance \langle r \rangle usually is taken the Wigner–Seitz radius. Therefore,

\Gamma = \frac{q_\text{e}^2}{4\pi\varepsilon_0 k_\text{B}T_\text{e}}\sqrt[3]{\frac{4\pi n_\text{e}}{3}}.

Clearly, up to a numeric factor of the order of unity,

\Gamma \sim \Lambda^{-2/3}.

In general, for multicomponent plasmas one defines the coupling parameter for each species s separately:

\Gamma_s = \frac{q_s^2}{4\pi \varepsilon_0 k_\text{B}T_s} \sqrt[3]{\frac{4\pi n_s}{3}}.

Here, s stands for either electrons or (a type of) ions.

The ideal plasma approximation

One of the criteria which determine whether a collection of charged particles can rigorously be termed an ideal plasma is that {{math|Λ ≫ 1}}. When this is the case, collective electrostatic interactions dominate over binary collisions, and the plasma particles can be treated as if they only interact with a smooth background field, rather than through pairwise interactions (collisions).J.D. Callen, University of Wisconsin-Madison, Draft Material for Fundamentals of Plasma Physics book: Collective Plasma Phenomena [http://homepages.cae.wisc.edu/~callen/chap1.pdf PDF] The equation of state of each species in an ideal plasma is that of an ideal gas.

Plasma properties and Λ

Depending on the magnitude of Λ, plasma properties can be characterized as following:See [http://farside.ph.utexas.edu/teaching/plasma/lectures/node8.html The plasma parameter] lecture notes from Richard Fitzpatrick

class="wikitable" style="text-align:center"
rowspan=2 | Description

! colspan=2 | Plasma parameter magnitude

{{math|Λ ≪ 1}} ({{math|Γ ≫ 1}}) || {{math|Λ ≫ 1}} ({{math|Γ ≪ 1}})
Coupling

| Strongly coupled plasma || Weakly coupled plasma

Debye sphere

| Sparsely populated || Densely populated

Electrostatic influence

| Almost continuously || Occasional

Typical characteristic

| Cold and dense || Hot and diffuse

style="vertical-align:top;"

! Examples

| Solid-density laser ablation plasmas
Very "cold" "high pressure" arc discharge
Inertial fusion experiments
Stellar interiors

| Ionospheric physics
Magnetic fusion devices
Space plasma physics
Plasma ball

References

{{reflist}}