Inter-Binding(s) Between Linked Cohomology-Related World-Sheets

 When the inter-binding(s) between linked cohomology-related world-sheets is (are) hermitian, the inferred net flow of curvature, of which is here to interdependently exist from amongst the proximal local presence of such world-sheets, is thence to often tend to work to bear a relatively smooth homotopy. SAMUEL ROACH. 

When Perturbative Gravitational Forces Counterbalance Each Other

 When perturbative gravitational forces counterbalance each other, this tends to work to allow for a flat Ricci Curvature, of which tends to work to allow for a smooth Ricci Flow. SAMUEL ROACH. 

Hermitian Motion Of Hamiltonian Operator -- Lack Of Perturbation Due To Externalized Distortive Influences

 When the motion of a Hamiltonian Operator is of a hermitian nature, the inferred  tense of a smooth respective Lagrangian-Based motion, may often tend to work, to not bear a perturbative flow that is due to externalized distortive influences. TO BE CONTINUED! SINCERELY, SAMUEL DAVID ROACH.

Hermitian Deformation Of Ricci Flow

 A smooth Ricci Flow will tend to work to bear a directly associated tense, of a hermitian deformation. SAMUEL DAVID ROACH. 

Balance Between Euclidean Expansion And Clifford Expansion

 A double-helix (such as with a DNA molecule), works to bear a heuristic example, of the Laplacian-Based exhibition of a smooth covariant balance, that is here to be displayed, between the general workings of a Euclidean Expansion -- when in conjunction with the general workings of a Clifford Expansion. SAM.

Heteromorphic Gravitational Field

 The more heteromorphic that a gravitational field is to be, the less smooth that its directly associated Ricci Flow will consequently tend to be. TO BE CONTINUED! SINCERELY, SAMUEL ROACH. (1989).

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.

Quickly Reiterated Recursively Smooth Ricci Flow

 A relatively tight braided cohomology, that is here to help form a set of conditions, that is directly attributable to a relatively quickly reiterated recursively smooth Ricci Flow, may often work to help in the facilitation, of "cutting through" the potentially hazardous conditions of atmospheric abrasion (such as the potential dangers of both atmospheric heat and atmospheric friction.) SAMUEL DAVID ROACH. (1989).

Hermitian Ricci Flow -- Recursively Smooth Ricci Flow

 When any given arbitrary hermitian Ricci Flow, that is here to be directly appertaining to the eminent physical conditions, of the Lagrangian-based flow -- of a mass-bearing cohesive set of discrete energy quanta, of which is here to be constantly altering in its direction while yet moving at a constant speed, -- is to continually reiterate its "Stoke's-based path," via a Ward-Cauchy-related tense of physical circuitry, then, the motion of such a described mass-bearing cohesive set of discrete energy quanta, will consequently here, in such a general type of a case, often tend to work to bear a Recursively Smooth Ricci Flow. Sincerely, Sam Roach.