Wavelength Of Gravitational Perturbation

 When the given arbitrary Noether-Based wavelength of gravitational perturbation is zero, the directly corresponding  Ricci Curvature, is thence to be flat, and, the correlative Ricci Flow, will thereby tend to be smooth. When the given arbitrary Noether-Based wavelength of gravitational perturbation is less than zero, the directly corresponding Ricci Curvature, is thence to have a general tendency, of being eminently associated with a fractional value, and, the correlative Ricci Flow, will thereby tend to not be smooth. Furthermore; When the given arbitrary Noether-Based wavelength of gravitational perturbation is more than zero, the directly corresponding Ricci Curvature is thence to have a general tendency, of being eminently associated, with a value that is more than one, and, the correlative Ricci Flow, will thereby tend to not be smooth. I WILL CONTINUE WITH THE SUSPENSE LATER! TO BE CONTINUED! SAM ROACH.

Inverted Gravitational Wavelengths -- Fraction-Related Ricci Curvature

 The proximal local covariant kinematic presence, of a cohesive set of one or more inverted gravitational wavelengths, often tends to be associated, with the respective proximal local presence, of the general genus of a Ricci Curvature, that is to work to bear a scalar magnitude, that is to be heuristically described of as a fractional value. I will continue with the suspense later! To Be Continued! Sincerely, SAMUEL ROACH. (1989).