Conservation Of Higgs Field Density Eigenstates

 The mass-related density of the multiplicity of Higgs Boson eigenstates, is abnormally large. This works to help make the correlative Majorana-Weyl-Invariant-Mode that these work to express, abnormally great. In so long as such Higgs Boson eigenstates are not abruptly brought into perturbation, the directly associated attributable conservation of Higgs Field density eigenstates, works to prevent the facilitation of the formation of unwanted black holes. SAM. 

Increasing Relative Velocity And Rarita Structure Eigenstates

Let us initially consider an orbifold eigenset, that is here in this case to consist of at least in part -- the presence of mass-bearing superstrings of discrete energy permittivity.  Let us next say -- that the said orbifold eigenset, is to be accelerating up to nearly the rate of light speed.  As the said orbifold eigenset is to be increasing in its relative velocity, over an evenly-gauged Hamiltonian eigenmetric -- it is then to bear increasingly more mass, -- even though the overall specific Ward-Neumman constraints of the said eigenset's physical bounds are to if anything decrease.  This then works to indicate, that, as the so-eluded-to set of superstrings that are here to operate to perform a specific function, is to move at a relatively increasing rate, when this is in comparison to light that is here to go even faster -- that the density of the mass of the said orbifold eigenset is then to increase as well.  This will then work to indicate the physical conditions of an increased density, as to what are here to be the correlative centralized knotting of the proximal local Rarita Structure eigenstates.  It is the Rarita Structure, that works to convey both the vibrations of gravity, as well as the multivarious inflections in the conveyance of the ever changing forms of the four main physical forces of nature.
I will continue with the suspense later!  To Be Continued!  Sincerely Samuel David Roach.

Homotopic Residue And Dimensional Contraction

Although the quantitative-related net distribution of homotopic residue tends to be conserved, the spatial-related density of such a so-eluded-to  orbifold eigenset -- is to tend to be metrically increased -- as such an orbifold eigenset is to approach the speed of light.  When an orbifold eigenset moves faster -- its relative "length" is to contract.  This means, that the homotopic residue that is situated at the relative "length" of an orbifold eigenset -- is to tend to become denser, as the said orbifold eigenset is to move at a higher velocity.
I will continue with the suspense later!  To Be Continued!  Sincerely, Samuel David Roach.

Angle Of Light Scattering Strike

When any one given arbitrary photon is to strike the externalized core-field-density, that is of the first-order light-cone-gauge eigenstate of another discrete quantum of energy -- in an oblique manner that is of a Ward-based acute angling -- the spontaneously ensuing gravity waves that act as Schwinger-Indices that are thus consequently formed, will tend to be of more of a harmonic nature, than if the approach of the photon when in the process of such a so-eluded-to scattering, were instead of an oblique Ward-based obtuse angling.  Consequently, -- when any one given arbitrary photon is to strike the externalized core-field-density, that is of the first-order light-cone-gauge eigenstate of another discrete quantum of energy -- in an oblique manner that is of a Ward-based obtuse angling -- the spontaneously ensuing gravity waves that act as Schwinger-Indices that are thus consequently formed, will tend to be of more of an enhharmonic nature, than if the approach of the photon when in the process of such a so-eluded-to scattering, were instead of an oblique Ward-based acute angling.
I will continue with the suspense later!  To Be Continued!  Sincerely, Samuel David Roach.

Part One Of Session Seven Of Course 20

Light, or any other form of electromagnetic energy, can scatter upon either phenomenology of mass, phenomenology of plain kinetic energy, or upon phenomenology of other electromagnetic energy -- over time.  When electromagnetic energy is to scatter upon another phenomenology, it is to strike the externalized core-field-density of the light-cone-gauge eigenstate of the discrete energy quantum -- that it is to come into contact with in the so-inferred Gliosis-based manner.  Furthermore, any electromagnetic or electro-dynamic energy will tend to scatter upon any discrete quantum of mass, kinetic energy, and/or electromagnetic energy, in an initially Rayleigh-based manner -- when it is to strike the just inferred multiplicit externalized field of such a light-cone-gauge eigenstate, over any metric that may be gauged of as an even Hamiltonian operation, around the instance of contact, in which the so-eluded-to set of one or more photons are to make a direct Yukawa-based coupling upon the said phenomenology that may here be either as a quantum of a mass, a quantum of kinetic energy, and/or a quantum of electromagnetic energy, over time.  This is particularly the case, when the phenomenology that is to be struck is in the Lagrangian-based path -- as to the mappable-tracing of the electromagnetic energy that is in its venue of moving in the direction of least time, as a Hamiltonian operand -- in which the photon or the photons that are to be scattered, are here to be "toggled" as is as according to Snell's Law.  Mass-Bearing superstrings of discrete energy permittivity, that are in a state of superconformal invariance -- tend to be Yau-Exact.  This is why I term those substringular manifolds, that are to be comprised of here as  mass-bearing strings -- as Calabi-Yau manifolds.  Electromagnetic superstrings of discrete energy permittivity, that are in a state of superconformal invariance -- tend to be partially Yau-Exact.  This is why I term those substringular manifolds, that are to be comprised of here as electromagnetic strings -- as Calabi-Calabi manifolds.  Furthermore, -- kinetic energy-bearing superstrings of discrete energy permittivity, that are in a state of superconformal invariance,  tend to veer into a condition of bearing Chern-Simons singularities.  This is why I call those substringular manifolds, that are to be comprised of plain kinetic energy -- as Calabi-Wilson-Gordan manifolds. 
I will continue with the suspense later!  To Be Continued!  Sincerely, Samuel David Roach.

Schwinger-Indices and Gravitational Density

The higher that the scalar amplitude of the Hodge-based formation of Schwinger-Indices is, per density of overall dimensional parameterization, tends to be, given a dependent condition of a common duration of a group-related metric  --  then, the higher that the gravitational density will tend to be, of such  a so-eluded-to Ward-Caucy-based region.
I will continue with the suspense later!  To Be Continued!  Sincerely, Samuel David Roach.