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Dusty plasma


Jan 16, 2022

A dusty plasma is a plasma containing micrometer (10−6) to nanometer (10−9) sized particles suspended in it. Dust particles are charged and the plasma and particles behave as a plasma.[1][2] Dust particles may form larger particles resulting in “grain plasmas”. Due to the additional complexity of studying plasmas with charged dust particles, dusty plasmas are also known as complex plasmas.[3]:2

A plasma containing millimeter to nanometer sized particles

Dusty plasmas are encountered in:

Dusty plasmas are interesting because the presence of particles significantly alters the charged particle equilibrium leading to different phenomena. It is a field of current research. Electrostatic coupling between the grains can vary over a wide range so that the states of the dusty plasma can change from weakly coupled (gaseous) to crystalline. Such plasmas are of interest as a non-Hamiltonian system of interacting particles and as a means to study generic fundamental physics of self-organization, pattern formation, phase transitions, and scaling.

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The temperature of dust in a plasma may be quite different from its environment. For example:

Dust plasma component Temperature
Dust temperature 10 K
Molecular temperature 100 K
Ion temperature 1,000 K
Electron temperature 10,000 K

The electric potential of dust particles is typically 1–10 V (positive or negative). The potential is usually negative because the electrons are more mobile than the ions. The physics is essentially that of a Langmuir probe that draws no net current, including formation of a Debye sheath with a thickness of a few times the Debye length. If the electrons charging the dust grains are relativistic, then the dust may charge to several kilovolts.[6]Field electron emission, which tends to reduce the negative potential, can be important due to the small size of the particles. The photoelectric effect and the impact of positive ions may actually result in a positive potential of the dust particles.

Interest in the dynamics of charged dust in plasmas was amplified by the detection of spokes in the rings of Saturn.[3]:85 The motion of solid particles in a plasma follows the following equation:

mdvdt=FL+FG+FP+FD+FT{displaystyle m{frac {dv}{dt}}=mathbf {F_{L}} +mathbf {F_{G}} +mathbf {F_{P}} +mathbf {F_{D}} +mathbf {F_{T}} }

where terms are for the Lorentz force, the gravitational forces, forces due to radiation pressure, the drag forces and the thermophoretic force respectively.[3]:70

The Lorentz force, the contributions from the electric and magnetic force, is given by:

FL=q(E+vc×B){displaystyle F_{L}=qleft(mathbf {E} +{frac {mathbf {v} }{c}}times mathbf {B} right)}

where E is the electric field, v is the velocity and B is the magnetic field.[3]:71

Fg{displaystyle mathbf {F_{g}} }

is the sum of all gravitational forces acting on the dust particle, whether it be from planets, satellites or other particles[3]:75,76 and

FP{displaystyle mathbf {F_{P}} }

is the force contribution from radiation pressure. This is given as:

FP=πrd2cIei^{displaystyle F_{P}={frac {pi r_{d}^{2}}{c}}Imathbf {hat {e_{i}}} }

The direction of the force vector,

ei^{displaystyle mathbf {hat {e_{i}}} }

is that of the incident radiation of photon flux

I{displaystyle I}

. The radius of the dust particle is

rd{displaystyle r_{d}}


For the drag force there are two major components of interest, those from positive ions-dust particle interactions, and neutral-dust particle interactions.[3]:76 Ion-dust interactions are further divided into three different interactions, through regular collisions, through Debye sheath modifications, and through coulomb collisions.[3]:77

The thermophoretic force is the force that arises from the net temperature gradient that may be present in a plasma, and the subsequent pressure imbalance; causing more net momentum to be imparted from collisions from a specific direction.[3]:80

Then depending in the size of the particle, there are four categories:

  1. Very small particles, where
    FL{displaystyle mathbf {F_{L}} }

    dominates over

    FG{displaystyle mathbf {F_{G}} }


  2. Small grains, where q/m ≈ G, and plasma still plays a major role in the dynamics.
  3. Large grains, where the electromagnetic term is negligible, and the particles are referred to as grains. Their motion is determined by gravity and viscosity.
  4. Large solid bodies. In centimeter and meter-sized bodies, viscosity may cause significant perturbations that can change an orbit. In kilometer-sized (or more) bodies, gravity and inertia dominate the motion.

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