SUMMARY
This discussion centers on the paradox of highly collisional plasmas exhibiting low resistivity within the framework of ideal Magnetohydrodynamics (MHD). It highlights that while frequent collisions among electrons should theoretically increase resistivity, the energy loss during these collisions is minimal, leading to negligible impedance in MHD scenarios. The conversation references the momentum loss rate and energy loss calculations, emphasizing the importance of electron density and kinetic energy in understanding plasma behavior. The discussion also questions the applicability of ideal MHD to extreme conditions such as solar winds and neutron star magnetospheres.
PREREQUISITES
- Understanding of ideal Magnetohydrodynamics (MHD)
- Knowledge of plasma physics, particularly electron-electron collisions
- Familiarity with momentum and energy loss rates in plasmas
- Basic principles of Maxwellian velocity distribution in plasmas
NEXT STEPS
- Research the relationship between electron density and resistivity in plasmas
- Study the implications of momentum loss rates in high-energy plasma environments
- Examine the conditions under which ideal MHD applies to astrophysical phenomena
- Explore the microscopic models of plasma interactions to understand energy transfer during collisions
USEFUL FOR
Physicists, plasma researchers, and engineers working in fields related to astrophysics, fusion energy, and plasma technology will benefit from this discussion.