TQNT-V5. 8 derives the Einstein field equations as the linearised, long-wavelength limit of the V5 conformal metric gᵢj = (1 + κg |Ψ|²) δᵢj. Newton's constant G inherits from κg previously fixed to 3. 13e-53 m at 0. 05% in V5. 7, so there is no free calibration in the gravitational sector. The emergent Einstein-Hilbert action is obtained at lowest order in (κg |Ψ|²) and the weak-field geodesic limit reproduces Newtonian gravity. This paper is the foundation document for the V5. 9-V5. 13 gravity and cosmology series. It complements the V5 monograph (10. 5281/zenodo. 19131538).
Lilian Cariou (Fri,) studied this question.