Determine the critical stability and collapse couplings
Determine the critical couplings separating stability from collapse for the Pauli and relativistic spinless non-Abelian gauge-field models, and likewise clarify the corresponding critical couplings in the abelian case.
References
The critical couplings are not known, here or in the abelian case.
— Stability of Matter Interacting with Classical Non-Abelian Gauge Fields
(2610.08313 - Reuvers et al., 6 Oct 2026) in Section 'Open problems', item 3; see also Remark 'Thresholds'