Global classical solutions of the three-dimensional relativistic Vlasov–Maxwell systemResearch Paper
Motivation
The relativistic Vlasov–Maxwell system is the basic kinetic model of a collisionless plasma: a cloud of charged particles, described by a phase-space density, moves under the electromagnetic field it generates, and the field evolves by Maxwell's equations with the particles as sources. Whether smooth, compactly supported data in three dimensions always produce a solution that stays smooth for all time has been the central question about the Cauchy problem for this system since the 1980s. Weak solutions exist globally, but they come without regularity or uniqueness, and every previous global classical result required smallness, a dimensional reduction, symmetry, or a nearby global reference solution.
This mission asks for a machine-checked proof of global existence and uniqueness of classical solutions for arbitrary smooth admissible data, as claimed in an OpenAI preprint dated September 23, 2026 (source). The preprint has not been peer reviewed and its claim has not been independently verified; on the platform the Lean goal below is open.
Timeline
- 1984 — Wollman proves local existence and uniqueness of classical solutions (CPAM 1984).
- 1986 — Glassey and Strauss show that a classical solution continues as long as the momentum support stays bounded (ARMA 1986); in 1987 they prove global existence for initially dilute plasmas (CMP 1987).
- 1985–1998 — Glassey and Schaeffer obtain global classical solutions for symmetric relativistic Vlasov–Poisson (CMP 1985) and for reduced Vlasov–Maxwell models in one and one-half, two and one-half, and two dimensions (1990, 1997, 1998).
- 1989 — DiPerna and Lions prove global existence of weak solutions for large data (CPAM 1989); Rein treats the relativistic case directly (CMS 2004).
- 1990 — Rein proves stability of global existence near suitable global solutions (CMP 1990).
- 2002–2003 — New proofs of the continuation criterion by Klainerman–Staffilani (CPAA 2002) and Bouchut–Golse–Pallard (ARMA 2003).
- 2004–2016 — Refined continuation criteria: Schaeffer's small-data theorem with momentum tails (IUMJ 2004), Pallard (IUMJ 2005), Luk and Strain's two-dimensional projection criterion (CMP 2014) and moment bounds (ARMA 2016).
- 2020–2025 — Small-particle global results with large fields: Bigorgne (CMP 2020; APDE 2025), Wei–Yang (CMP 2021).
- 2026 — Wang establishes large-data global existence under cylindrical symmetry (arXiv:2203.01199, arXiv:2607.14685).
- September 2026 — The OpenAI preprint claims the general large-data result without symmetry (Theorem 1.1, p. 3).
Setting
For momentum let and (the relativistic velocity, ). The unknowns are a particle density and fields , with charge and current densities and . In the one-species normalization the system is
A smooth admissible datum has , , smooth with every derivative bounded and , and satisfies , . A classical solution on is a triple solving the system pointwise, with continuous in time with values in , and with supported in a fixed compact set on each bounded time interval.
Formalization targets
Goal: Theorem 1.1 (p. 3)
Every smooth admissible datum generates a classical solution on with the given initial values; for every finite the solution is on (respectively for the fields) with compact phase-space support on ; and any other classical solution with the same datum agrees with it at every . This is OAI.RVM.global_classical_solution.
Significance
The result itself. It settles the large-data global classical regularity problem for three-dimensional relativistic Vlasov–Maxwell, with no size, symmetry or neutrality assumption; nonzero total charge with its Coulomb tail is allowed. Global well-posedness at this level is the starting point for questions about long-time behaviour, scattering and stability of plasma equilibria that previously could only be posed for small or symmetric data.
Formalizing it. The proof combines the Glassey–Strauss representation of fields along backward light cones, energy-flux estimates, a delicate signed bootstrap, and local well-posedness and continuation theory. None of this PDE infrastructure (wave-equation representation formulas, characteristics of transport equations in phase space, Sobolev local theory) is currently available in a proof assistant at the needed level, so each component is reusable.
Difficulty
By the Glassey–Strauss criterion it suffices to bound the momentum support on finite time intervals. The natural approach estimates the absolute value of the force along a characteristic using the retarded field representation and energy flux through light cones. At receiver energy this loses a factor relative to what is needed (Section 1.2, p. 4); the loss comes from sources whose velocity is much closer to the light ray than the receiver's. The preprint instead estimates the signed momentum increment , integrating the retarded force along source trajectories before taking norms (Proposition 2.1, p. 5; Lemma 6.1, p. 24), controls direction changes (Lemma 7.1, p. 29), and closes a bootstrap whose time-to-double lower bounds have a divergent sum (Section 9).
Formalization scope
- Space and momentum are
EuclideanSpace ℝ (Fin 3); derivatives are Fréchet derivatives in coordinate directions; the time derivative isderivWithinon , so is one-sided. Admissibleencodes with compact support and nonnegativity for ;ContDiff ℝ ∞with all iterated derivatives bounded andMemLp 2for ; and both Gauss constraints pointwise.Classicalrequires regularity on the closed half-spaces, , continuity of into on , compact phase support on each , all five equations pointwise for (including both constraints), and the initial values.- The conclusion asserts existence, smoothness on every finite horizon, and uniqueness within the same classical class; uniqueness is pointwise equality at all . The hypotheses are satisfiable (e.g. , ), so the statement is not vacuous.
- and are Bochner integrals in ; for compactly supported these are the genuine moments.
Selected references
- OpenAI, Global classical solutions of the three-dimensional relativistic Vlasov–Maxwell system, OpenAI Math Release preprint, September 23, 2026. https://github.com/openai/math/blob/adc7f1241b42e322a6451854ab7e4b4c146bf78a/preprints/Global-classical-solutions-of-the-three-dimensional-relativistic-Vlasov-Maxwell-system-September-23-2026/paper.pdf
- R. T. Glassey, W. A. Strauss, Singularity formation in a collisionless plasma could occur only at high velocities, Arch. Ration. Mech. Anal. 92 (1986). https://doi.org/10.1007/BF00250732
- R. T. Glassey, W. A. Strauss, Absence of shocks in an initially dilute collisionless plasma, Comm. Math. Phys. 113 (1987). https://doi.org/10.1007/BF01223511
- S. Wollman, An existence and uniqueness theorem for the Vlasov–Maxwell system, Comm. Pure Appl. Math. 37 (1984). https://doi.org/10.1002/cpa.3160370404
- R. J. DiPerna, P.-L. Lions, Global weak solutions of Vlasov–Maxwell systems, Comm. Pure Appl. Math. 42 (1989). https://doi.org/10.1002/cpa.3160420603
- J. Luk, R. M. Strain, A new continuation criterion for the relativistic Vlasov–Maxwell system, Comm. Math. Phys. 331 (2014). https://doi.org/10.1007/s00220-014-2108-8
- F. Bouchut, F. Golse, C. Pallard, Classical solutions and the Glassey–Strauss theorem for the 3D Vlasov–Maxwell system, Arch. Ration. Mech. Anal. 170 (2003). https://doi.org/10.1007/s00205-003-0265-6
- S. Klainerman, G. Staffilani, A new approach to study the Vlasov–Maxwell system, Commun. Pure Appl. Anal. 1 (2002). https://doi.org/10.3934/cpaa.2002.1.103
- X. Wang, Large data global solution of the 3D RVM system with cylindrical symmetry, arXiv:2203.01199 and arXiv:2607.14685 (2026). https://arxiv.org/abs/2607.14685v1