The Fine-Tuning Question Rewritten: Admissibility geometry, coupling conditions, and why isolated parameter windows do not define a universe

La Profilée is a universal structural law of persistence under transformation. It determines no physical value, and it does not predict the constants. But it corrects two category errors in the standard fine-tuning argument, using actual cosmological and stellar physics, and it makes one prediction that is already confirmed against the published data. Window-based fine-tuning arguments commonly make two category errors. First — the measure: an admissible window is treated as though it determined a probability; it does not, for any window and any target probability there is a normalized measure realizing it. Second — the reference scale: magnitudes are compared with an arbitrary ultraviolet scale rather than with the physical conditions under which determinate, persisting systems exist. Correcting both requires separating four kinds of constraint — Frame, Module, overload, and, crucially, Coupling (whether the parts are actually one integrated thing). La Profilée predicts, from the representational resources of the standard fine-tuning corpus, that it can contain Frame, Module, and overload conditions but no coupling condition; audited against rules fixed in advance, the published tables contain exactly zero, and asking the coupling question supplies four physical conditions absent from every table. The cosmological constant is bounded by the structure-formation turnaround, , which the measured value respects — a bound kept strictly distinct from the quantum-field-theoretic radiative problem, which is not solved here. Every number is domain-imported; every contribution of La Profilée is a structural condition.