Homeomorphic Gravitational Push

When the net directoral-based push of those Schwinger-Indices  -- that act as gravity waves -- are to interact upon one respective given arbitrary orbifold eigenset, to where the case scenario works to bear, that the Ward-Caucy-based  conditions are in such a manner, to where it is to here be that basically just the gravitational-based push that is proximal local to the directly correlative orbifold eigenset, is to be basically the sole source of the resultant wave-tug that is to here be delineated upon the said eigenset -- are to exist as both one general homeomorphic and as one homeogenous manner upon the so-stated orbifold eigenset, over time, then, this general condition will then work to cause the tendency of then working to make the said orbifold eigenset to then exist in a relative Majorana-Weyl-Invariant-based manner, -- over the so-eluded-to group-metric, in which the so-stated net gravitational push is to work to bear both such a homeomorphic and such a homeogenous wave--tug, upon the so-eluded-to metrical-gauge-based Hamiltonian operator.  Such a tense of a homeomorphic gravitational push, is to here be in terms of both the angling of the correlative directoral-based push of the directly corresponding Schwinger-Indices, the scalar amplitude of the wave modulae of the said Schwinger-Indices, &, the overall genus of the Noether-based current -- that is to here be Yukawa to those gravitational waves, that are to here be effectual upon the so-stated orbifold eigenset.  I will continue with the suspense later!  To Be Continued!  Sincerely, Samuel David Roach.