When there are added spatial dimensions to the Ward-Caucy bounds of a physical phenomenon that bears an overall Yang-Mills or non-abelian light-cone-gauge topology, then, the wave-tug/wave-pull that the directly corresponding Rarita Structure eigenstates will operate with, via the scalar amplitude of the directly corresponding Ricci Scalar eigenstates, will here, have a gravitational index that has a higher elastic modulus over the course of the duration in which the said given arbitrary physical phenomenon is going through the so stated added spatial dimensions. Yet, when there are added spatial dimensions to the Ward-Caucy bounds of a physical phenomenon that bears an overall Kaluza-Klein or abelian light-cone-gauge topology, then, the wave-tug/wave-pull that the directly corresponding Rarita Structure eigenstates will operate with, via the scalar amplitude of the directly corresponding Ricci Scalar eigenstates, will have a gravitational index that, instead,will have a lower elastic modulus over the course of the duration in which the said given arbitrary physical phenomenon is going through the so stated added spatial dimensions. This is, in a nutshell, why a phenomenon that is Yang-Mills is more free to move -- with less of a burden in regards to graviational impedance -- when traveling in added spatial dimensions, than a physical phenomenon that is Kaluza-Klein.
I hope that this relatively small bit of knowledge may be adequately helpfull. To Be Continued. Sam Roach.
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