Homotopy And Rate Of Cohomological Formation

The faster that any orbifold eigenset of mass-bearing superstrings, that are of discrete energy permittivity, is to travel through space, over an evenly-gauged Hamiltonian eigenmetric -- the more uneven that its homotopic residue will then tend to be distributed, from within the Ward-Cauchy confines of the proximal locus -- that is Poincare to the motion of the said eigenset.  The more uneven that an orbifold eigenset's homotopic residue will be distributed, from within the Ward-Cauchy confines of the proximal locus -- that is Poincare to the motion of any given arbitrary orbifold eigenset, -- the higher that the scalar amplitude will then tend to be, of that cohomology, that  will then tend to be produced -- by the Fourier-related kinematic motion of the said eigenset, over the so-eluded-to constraints of terrestrial time.  This would here be relativistic to a terrestrial observer's reference-frame.  This is even though the overall net scalar amplitude, of the homotopic residue of the said orbifold eigenset -- as a whole -- is to be conserved.
I will continue with the suspense later! To Be Continued!  Sincerely, Samuel David Roach.