Thursday, September 4, 2014
Part Four of the Tenth Session of Course 17 About The Ricci Scalar
Also, when there are Chern-Simmons singularities in-between two different relatively conformally invariant orbifolds, that work to comprise an cohomological eigenbasis in such a manner in so as to form one overall respective given arbitrary orbifold eigenset -- the existence of the so-stated Chern-Simmons singularities, whether the specific nature of such Chern-Simmons singularities is of a Lagrangian-based genus or of a metrical-based genus, works to where the so-eluded-to discontinuities may work to impede the overall degree of the correlative Ricci-Scalar scalar magnitude, that would otherwise be affectual towards the respective given arbitrary substringular cite -- at which, the directly corresponding Rarita Structure eigenstates are then to here utilize Hamiltonian-based kinematic operation upon such a cite in less of a warp-like manner. So, even the existence of Chern-Simmons singularities of any kind, that would here be exacted upon an interconnective Hamiltonian-based operation -- that works to connect two or more orbifolds of an orbifold eigenset, at any given arbitrary relative respective locus in the substringular, will work to impede the scalar magnitude of the effect of gravity upon the so-eluded-to local cite. This is due to the condition that any discrete lack of hermicity upon the topological holonomic substrate of any initially Calabi-Yau-based substringular locus will work to impede the Hodge-based scalar amplitude of the so-stated Calabi-Yau-based genus -- that is of the so-eluded-to substringular neighborhood that is in question here. Any lack of Calabi-Yau-based conditions upon an otherwise Calabi-Yau-based manifold will work at decreasing the relative respective scalar magnitude of that mass -- that would here work to describe the correlative warping-based genus of the directly associated space-time-fabric of the correlative substringular region. Such Chern-Simmons singularities work to cause the directly associated Ricci Scalar eigenstates to lack, to some degree, the otherwise existent scalar magnitude of correlative gravitational pull. This would thus work to decrease the affectual mass of the so-stated substringular cite, from what it would otherwise be. I will continue with the suspense later! To Be Continued! Sam!
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