Friday, June 21, 2013

Dimensionality and Gravitational Pull

When a phenomenon is traveling with more spatial dimensions that are directly associated with the immediate field of the said phenomenon, when compared to the condition of the same phenomenon when it is traveling in fewer spatial dimensions, the degree of the relative scalar amplitude of gravity in general that is applied to the initially mentioned phenomenon is dependent upon whether or not the said immediate field -- that the said phenomenon that is traveling in additional spatial dimensions is traveling through per time -- has more of an abelian geometry applied to it, or, whether it has more of a non-abelian geometry applied to it. So, when a phenomenon is traveling in more dimensions than it usually is traveling through over an analogous timeframe -- these timeframes of which act through the same duration and through the same general format of terrestrial-based path -- if the initially mentioned phenomenon has more of an abelian-based differentially geometric field applied to it, then, the gravitational force that will act upon it will be greater than if it traveled in fewer spatial dimensions over the given arbitrary duration in the given arbitrary general format of projection. Yet, if the initially mentioned phenomenon has more of a non-abelian-based differentially geometric field applied to it, then, the gravitational force that will act upon it will be less than if it had traveled in fewer spatial dimensions over the given arbitrary duration in the given arbitrary general format of projection. This is because extraneous wave-tug and/or wave-pull that is abrasive upon a phenomenon under such an eluded to substringular scenario will add extraneous impedance upon the Rarita Structure-based eigenindices that are applied to a given phenomenon over a respective common duration in a respective common format of projection, while, a lowering of wave-tug and/or wave-pull that would otherwise be abrasive upon a phenomenon under such an eluded to substringular scenario will work to decrease the extraneous impedance upon the Rarita Structure-based eigenindices that are applied to a given phenomenon over a respective common duration in a respective common format of projection.  Less extraneous impedance acting upon a phenomenon means a both an added potential for permittivity and propagation of the immediate field of a given arbitrary phenomenon, and, such an added potential for permittivity and propagation is shown when there is less of a gravitational limitation that is imposed upon the same  stated given arbitrary phenomenon.  Sincerely, Samuel David Roach.                                          

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