Let us initially consider one given arbitrary orbifold eigenset -- of which is here to be Yukawa to a certain respective given arbitrary scalar amplitude of Schwinger-Indices. The higher that the scalar amplitude of the Schwinger-Indices, that are here to be directly associated with the Fourier Transformation of an orbifold eigenset, is to be, then, the higher that the scalar amplitude of the gravitational force -- that is to be directly associated with the said orbifold eigenset, will then tend to be as well. Therefore, if the initially so-stated orbifold eigenset is then to work to increase in the condition as to how Yukawa that it is to Schwinger-Indices over a proscribed group-related metric, that is to here be related to the same constraint of relative limited time, then, the said orbifold eigenset will here tend to increase in its covariant gravitational pull.
I will continue with the suspense later! To Be Continued! Sincerely, Samuel David Roach.
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