Part Three of the Tenth Session of Course 17 About the Ricci Scalar

At the specific local cite where a Chern-Simmons singularity is happening -- to either a superstring, its effectual cohomological ghost-based index, an orbifold, or, an orbifold eigenset -- there is at least a partial break in the abelian-based effect of gravity upon the directly corresponding cohomology, to where the directly corresponding Ricci  Scalar eigenstates, that are here to act upon the said substringular phenomenon at the specific locus -- as to where such an eluded-to Chern-Simmons singularity is then here happening, bears less of a scalar amplitude of Hodge-based interaction -- as this may be extrapolated by the then here lessoned effect of the correlative Rarita Structure eigenstates upon the given arbitrary cohomological holonomic substrate, at the just-eluded-to specific locus of Laplacian-based perturbation.  At the just mentioned locus of Laplacian-based perturbation, at the Poincaire level of such an either Lagrangian-based or a metrical-based spike in the path integral -- as to the trajectory of the projection of the here given arbitrary substringular Hamiltonian operator -- the so-stated Chern-Simmons singularity does not integrate the "mers" of the additive gravitational pull, that would otherwise be ebbed into the translation of the kinematic translation of whatever the given arbitrary substringular-based cohomological-oriented holonomic substrate may be, in this given case scenario.  The result in the altered or perturbated Hodge-Index-based extrapolation of such a locus, that would here bear a certain genus of Chern-Simmons-based cohomology -- is that the so-eluded-to locant will then bear a lack of a mass-based attribution, in so long as such a cohomological-based index is spontaneous upon the said kinematic-based locant, over a sequential series of group related insantons.  This is in part due to the condition that a mass has Yau-Exact singularities, and, Yau-Exact singularities do not bear Chern-Simmons singularities that are exacted upon the directly corresponding superstrings, over the duration in which the consequential respective superstrings are acting in such a manner in so as to be discrete units of mass-based energy.  Even though gravity works, to some extent, upon all superstrings of discrete energy permittivity -- via the motion of  the correlative Rarita Structure eigenstates, over time -- gravity primarily acts most directly upon superstrings that are of Calabi-Yau-based manifolds.  This then means that the Ricci Scalar tends to interact most directly upon Calabi-Yau manifolds, via the just mentioned Rarita Structure eigenstates.  This is why the existence of anomalous Chern-Simmons singularities  work to decrease the effect of gravity upon the  respective superstrings, in which such an activity happens to it, and thus, the presence of Chern-Simmons singularities upon the holonomic substrate of any given arbitrary subs tringular phenomenon will tend to work at decreasing the correlative effect of both the activity of  local Rarita Structure eigenstates, as well as decreasing the correlative effect of the local Ricci Scalar eigenstates.  I will continue with the suspense later! Sincerely, Sam.