Perturbative Gravitational Force -- Lack Of Isomorphic Cohomological Deformation

 When the gravitational force, that is here to be incurred upon a given arbitrary proximal local cohesive mass-bearing Hamiltonian Operator, is to be perturbative; Both the Ricci Curvature will not be flat, the Ricci Flow will not be smooth, and, the cohomological deformation, that is here to be eminently associated, with the Lagrangian-Based flow of the kinematic modulus, that is here to directly appertain to the inferred Fourier-Related-Progression, of such a stated Hamiltonian Operator, will consequently tend to not bear the likings of an isomorphic nature -- as this is here to be taken, over the respectively inferred duration, in which such an inferred "team" of mass-bearing energy, is here to be under the proximal local influence, of such a stated perturbative gravitational force. TO BE CONTINUED! SINCERELY, SAMUEL DAVID ROACH.