On classical solutions to the 3D relativistic Vlasov-Maxwell system: Glassey-Strauss' theorem revisited
Francois Bouchut, Francois Golse, Christophe Pallard

TL;DR
This paper revisits and simplifies Glassey and Strauss's 1986 proof that classical solutions to the 3D relativistic Vlasov-Maxwell system remain regular as long as the momentum support stays bounded.
Contribution
The paper provides a simplified proof of a key theorem ensuring the global regularity of solutions to the 3D relativistic Vlasov-Maxwell system.
Findings
Classical solutions do not develop singularities if momentum support remains bounded.
Simplified proof enhances understanding of the conditions for solution regularity.
Revisits foundational results in relativistic plasma physics.
Abstract
R. Glassey and W. Strauss have proved in [Arch. Rational Mech. Anal. 92 (1986), 59--90] that classical solutions to the relativistic Vlasov-Maxwell system in three space dimensions do not develop singularities as long as the support of the distribution function in the momentum variable remains bounded. The present paper simplifies their proof.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGas Dynamics and Kinetic Theory · Fluid Dynamics and Turbulent Flows · Computational Fluid Dynamics and Aerodynamics
