Please read this whole thing carefully. The following is the case for an internal reference-frame that is relatively stationary in and of itself, that is here to be within an external reference-frame that is approaching light speed. The less partition-based discrepancies that the mass-bearing superstrings of discrete energy permittivity that are of an orbifold eigenset, are to bear -- the more contracted that such an orbifold eigenset will theoretically tend to appear at its relative length -- when this is taken by the theoretical reference-frame of a terrestrial observer, -- to where such an orbifold eigenset will then tend to not to seem to be contracted by the standpoint of one of whom is at the theoretical reference-frame of the moving orbifold eigenset that is of such a given case. The added partition-based discrepancies, that are of that kinetic energy -- that is of the kinematics of the Lagrangian that is most directly associated with the motion of such a said orbifold eigenset -- will then tend to make-up for any seeming loss in the conservation of homotopic residue, -- to where there will here tend to be no net loss nor gain of homotopic residue, at the substringular neighborhood that is proximal to the moving locus of such a said orbifold eigenset. Such a condition that helps to work at the conservation of homotopic residue -- is, in part, what is here to act in so as to tend to help to allow for such a perspective of no apparent contraction in length at the theoretical reference-frame of the said moving orbifold eigenset.
I will continue with the suspense later! To Be Continued! Sincerely, Samuel David Roach.
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