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Space of initial conditions for the full 3D system (1.1)

Ascertain whether it is possible to construct a space of initial conditions, in the sense of Definition 2.12, for the non-autonomous three-dimensional system (1.1) itself (i.e., without restricting to the invariant hypersurface), thereby providing a compactified phase space with a uniform foliation by solution leaves.

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Background

While the authors build spaces of initial conditions for the two restricted 2D systems and relate them to the standard Painlevé VI geometry, they emphasize that extending such a construction to the full 3D system is substantially harder due to higher-dimensional geometric complexities and the presence of different types of indeterminacies.

They indicate that the autonomous limit exhibits properties (e.g., elliptic fibration, multi-Hamiltonian structure) suggestive of Painlevé-type behavior, motivating the question of whether an appropriate higher-dimensional analogue of the Okamoto–Sakai construction exists for the full 3D system.

References

Another open problem, is whether the construction of a space of initial conditions for the general 3D system (1.1) is possible, see Conjecture 1.

The Painlevé equivalence problem for a constrained 3D system (2411.01657 - Filipuk et al., 3 Nov 2024) in Section 7 (Conclusions)