Propagation of Velocity Moments for the Magnetized Vlasov-Poisson System with Space-Time Dependent Magnetic Fields
Immanuel Ben Porat, Antoine Gagnebin, Mikaela Iacobelli, Jonathan Junné
TL;DR
This work analyzes the propagation of velocity moments for the 2D magnetized Vlasov-Poisson system and the 3D magnetized screened Vlasov-Poisson equation with a space-time dependent external magnetic field. It develops a moment-based framework combining Eulerian and velocity moments, kinetic interpolation inequalities, and the no-work property of magnetic forces to obtain global moment propagation in 2D and a two-stage strategy (short-time for $n=3,4$ and long-time via $L_4$) in 3D, along with propagation of regularity. It also improves stability estimates in the kinetic Wasserstein distance, achieving an optimal $\sqrt{\log}$ rate by leveraging the no-work identity, and thereby establishing global classical solutions under explicit decay and smallness conditions. The results bridge the non-magnetized theory and magnetized dynamics, providing rigorous control of moments, regularity, and stability for plasmas with non-uniform magnetic fields.
Abstract
We prove that polynomial velocity moments of solutions to the 2D magnetized Vlasov-Poisson system and the 3D magnetized screened Vlasov-Poisson equation remain finite for all times, provided they are finite initially, even when the external magnetic field $B=B(t,x)$ is space-time dependent. We deduce propagation of regularity, thereby implying the existence of global classical solutions. Moreover, we prove optimal stability estimates in the kinetic-Wasserstein distance on par with the unmagnetised case.
