Slowdown of interpenetration of two counterpropagating plasma slabs due to collective effects

The nonlinear evolution of electromagnetic instabilities driven by the interpenetration of two e(-), e(+) plasma clouds is explored using ab initio kinetic plasma simulations. We show that the plasma clouds slow down due to both oblique and Weibel generated electromagnetic fields, which deflect the particle trajectories, transferring bulk forward momentum into transverse momentum and thermal velocity spread. This process causes the flow velocity v inst to decrease approximately by a factor of root 1/3 in a time interval Delta t(alpha B)omega(p) similar to c/(v(fl)root alpha B), where alpha(B) is the magnetic equipartition parameter determined by the nonlinear saturation of the instabilities, v(fl) is the initial flow speed, and omega(p) is the plasma frequency. For the alpha(B) measured in our simulations, Delta t(alpha B) is close to 10 times the instability growth time. We show that as long as the plasma slab length L > v(fl)Delta t(alpha B), the plasma flow is expected to slow down by a factor close to root 1/3.

Automated summary

This research investigates the nonlinear evolution of electromagnetic instabilities driven by the interpenetration of electron and positron plasma clouds using ab initio kinetic plasma simulations. The study shows that the plasma clouds slow down due to electromagnetic fields generated by oblique and Weibel effects, with the plasma flow expected to decrease by a factor close to root 1/3, providing important insights into the fluid dynamics of plasmas.