What makes a plasma collisionless?

Click For Summary
SUMMARY

Collisionless plasmas are characterized by weak coupling among particles, where collisions are negligible compared to long-range collective interactions. A large mean free path and low particle density are critical factors that determine whether a plasma is collisionless. The electromagnetic perspective emphasizes that charged particles are primarily influenced by net charge distribution and magnetic fields. For further insights, refer to the discussions in "The Sun as a Guide to Stellar Physics" by E.R. Priest, 2019.

PREREQUISITES
  • Understanding of plasma physics concepts
  • Familiarity with mean free path and particle density
  • Knowledge of electromagnetic interactions in plasmas
  • Basic principles of magnetohydrodynamics
NEXT STEPS
  • Research the role of mean free path in plasma behavior
  • Study electromagnetic interactions in collisionless plasmas
  • Explore magnetohydrodynamics and its applications
  • Read "The Sun as a Guide to Stellar Physics" by E.R. Priest for advanced insights
USEFUL FOR

Researchers, physicists, and students interested in plasma physics, particularly those focusing on the dynamics of collisionless plasmas and their electromagnetic properties.

Jd1431
Messages
2
Reaction score
0
Hi, I'm trying to understand what determines whether a plasma will be collisionless or collisional. I understand that a diffuse plasma with large mean free path will be collisionless but I don't really understand it from an electromagnetic point of view
 
Physics news on Phys.org
Jd1431 said:
Hi, I'm trying to understand what determines whether a plasma will be collisionless or collisional. I understand that a diffuse plasma with large mean free path will be collisionless but I don't really understand it from an electromagnetic point of view
Succinctly put, "Collisionless plasmas are weakly coupled, i.e., the coupling between the particles due to collisions is generally negligible, and instead, the long-range collective interactions bind particles together." In other words, the charged particles are mainly affected by the net charge distribution and the magnetic field.

So a relatively large mean free path, or low particle density, would be a key factor.

Some good discussions here - https://www.sciencedirect.com/topics/earth-and-planetary-sciences/collisionless-plasmas

See the discussion under

Magnetohydrodynamics and Solar Dynamo Action

E.R. Priest, in The Sun as a Guide to Stellar Physics, 2019
 
  • Like
  • Informative
Likes   Reactions: artis, malawi_glenn, Lord Jestocost and 1 other person

Similar threads

  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 15 ·
Replies
15
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
4
Views
2K
  • · Replies 5 ·
Replies
5
Views
5K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 2 ·
Replies
2
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K