Vlasov–Maxwell regularity
Establish global regularity, or exhibit breakdown, for solutions of the Vlasov–Maxwell equations from appropriate smooth initial data.
References
Primary source
Progress summary
The general three-dimensional problem remains open: known results cover restricted data, while a reader-submitted 2026 claim of a complete solution has no independent verification.
The problem asks whether smooth admissible data for the three-dimensional relativistic Vlasov–Maxwell system always produce global regular solutions, or whether breakdown can occur. Published sources continue to describe the unrestricted question as open.
Known results
- Glassey–Strauss and Schaeffer proved global existence in small-data regimes, with later work removing some support assumptions.
- Global existence is known for sufficiently small smooth data with decay, including scattering results.
- Arbitrarily large global solutions are known under spherical symmetry and for some cylindrically symmetric data.
- Continuation criteria give conditional global regularity when suitable momentum-integrability or support bounds persist.
Community submission (unverified), 2026-10-07
A submitted claim alleges that an attached manuscript proves global existence and uniqueness for arbitrary smooth admissible data in the one-species relativistic system. No independently retrieved source assesses this claim, so it does not establish a solution.
Current status (as of October 2026): Restricted-data and symmetry results are established, but global regularity or breakdown for general smooth three-dimensional data remains open; the submitted complete-solution claim is unverified.
Solutions 1
Claimed by OpenAI: global classical solutions of the three-dimensional relativistic Vlasov–Maxwell system.See full solution
Claimed by OpenAI. The attached preprint claims global existence and uniqueness for arbitrary smooth admissible initial data in the three-dimensional, one-species relativistic Vlasov–Maxwell system, with initially compactly supported particle density and finite-energy electromagnetic fields whose derivatives of all orders are bounded.
GitHub repository: https://github.com/openai/math
- 362.pdfOpen