Gravitational Warp -- Perturbative Ricci Flow

 When a Ward-Cauchy-Related cohomology-based topological structure, that is here to be proximal local, to the core-field-density, of a directly corresponding kinematically propagated Hamiltonian Operator in time and space, is thence to be spatially transferred through a region in space and time, in which the gravitational force is here to be of a warped nature, this general characteristic, will thereby tend to spontaneously work, to induce the consequential physical attribute, to where the earlier stated Hamiltonian Operator, will thereupon tend to work to exhibit a perturbative Ricci Flow, from within the Ward-Neumann bounds, of such an earlier inferred region of gravitational warping. TO BE CONTINUED! SAMUEL ROACH.