For the incompressible Euler equations on the periodic box , , global distributional weak solutions are known to exist for every divergence-free initial datum (the energy space of solenoidal zero-mean vector fields), but the known constructions force the kinetic energy to jump upward at . A weak solution is called admissible if its total kinetic energy never exceeds the initial energy for all . Admissible global weak solutions are currently constructed only for an -dense subset of initial data, and convex integration cannot plainly be extended to all data, since for smooth data any admissible solution must coincide with the classical solution by weak-strong uniqueness. As of 2026 the problem remains open in every dimension: does every admit a global admissible weak solution, and if not, which data do? Recent partial results (generic 2D well-posedness with energy balance, prescribed-energy-profile constructions, and topological smallness results for decaying solutions) sharpen the landscape on both sides without settling the core question.
Background
The incompressible Euler equations , model an ideal (inviscid, incompressible) fluid. On the periodic box , , the natural finite-energy phase space is : the space of -periodic, square-integrable, divergence-free vector fields with zero mean (the zero-mean condition is harmless because of Galilean invariance). A weak solution with initial datum is a map satisfying the equations in the sense of distributions against smooth periodic divergence-free test fields and attaining weakly in (such solutions are weakly continuous in time, so the initial condition is attained in the weak sense, the standard convention in the source paper). Its kinetic energy is , which for smooth solutions is conserved. For the viscous Navier–Stokes equations, global weak solutions satisfying the energy inequality have been known since the 1930s, but the inviscid case offers no parabolic smoothing and hence no comparable compactness argument. Following the terminology of De Lellis and Székelyhidi (2010), a weak solution of Euler is called admissible if for all ; admissibility is the minimal physical energy constraint, and it implies weak-strong uniqueness: any admissible solution whose initial datum admits a (Lipschitz) classical solution must coincide with that classical solution for as long as the latter exists. Modern existence theory for non-smooth data rests on convex integration, a flexible-construction technique in which one first builds a smooth subsolution — a triple solving the linear parts of the equations whose associated generalized energy strictly undershoots a prescribed energy profile — and then corrects it to infinitely many exact weak solutions; the solutions produced this way are often called wild solutions. De Lellis and Székelyhidi (2010) showed that admissibility criteria (energy conservation or dissipation) do not restore uniqueness of such wild solutions, and Buckmaster, De Lellis, Székelyhidi, and Vicol (2019) proved Onsager's conjecture for admissible weak solutions on the three-dimensional torus (Onsager's conjecture asserts that Hölder-continuous weak solutions with exponent above conserve energy while below dissipative solutions exist). Wiedemann (2011) proved that every admits infinitely many global weak solutions, but with a discontinuous energy increase at , so no energy inequality holds; and Székelyhidi and Wiedemann (2012) proved, via generation of admissible measure-valued solutions (solution concepts relaxed to Young measures carrying oscillation and concentration effects) by exact weak solutions, that an -dense set of initial data each admits infinitely many admissible weak solutions. Whether the dense set can be enlarged to all of is stated in both papers to be a delicate open issue: the initial-time energy jump is intrinsic to the subsolution construction for rough data, while for smooth data weak-strong uniqueness forces any admissible solution to be the classical one, so any all-data construction must be rigid exactly where data are smooth and flexible where they are rough.
Problem Statement
Let with , and let be the space of -periodic, square-integrable, divergence-free vector fields with zero mean. Consider the incompressible Euler equations , on , with weak solutions understood distributionally against smooth -periodic divergence-free test fields and kinetic energy . The problem, stated as open in the source paper and still open as of 2026, has one coherent objective — an admissible-existence theory over the whole energy space — with two facets: (i) does every initial datum admit a global weak solution with (attained weakly in ) and for all (an admissible solution)? (ii) if not, characterize the class of initial data in for which admissible global weak solutions exist. Any resolution must be consistent with weak-strong uniqueness (admissible solutions with data admitting a local classical solution coincide with that classical solution on its lifespan, so non-unique admissible solutions can occur only for highly irregular data) and must handle the initial time: the inequality is required from onward, which excludes the upward energy jumps at inherent in the known all-data weak-existence constructions. The question is open in every dimension on the periodic box, and analogously on smooth bounded domains with the corresponding energy space.
References
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