Let us consider the condition -- that the particles known of as gluons, are the phenomenology that is preeminent where the Rarita Structure eigenstates work to bear what I term of as the multivarious loci of the condition of a centralized knotting. Remember, that the multivarious light-cone-gauge eigenstates act as the initiation-based source of the Rarita Structure, and, the multivarious gauge-boson eigenstates act as the ending-based source of the Rarita Structure. Let us now consider the condition -- that those genre of the tenses of conformal invariance, that would here directly appertain to the activity of the Rarita Structure eigenstates of phenomenology that exists on a star or a planet, will tend to bear more torsional-affiliated external inter-play -- than those genre of the tenses of conformal invariance that would, instead, directly appertain here to the activity of the Rarita Structure eigenstates of phenomenology that would tend to exist in an isolated region that is deep into outer space. Stars and planets are phenomenology that bear a large quanta of mass. Mass is put together, basically, due to the activity of gluons -- in the process of acting as the operators of the strong force. At least partially on account of the condition that any respective given arbitrary star or planet is a physical phenomenological-based entity, that works to bear a significant external inter-play of the directly corresponding Rarita Structure eigenstates -- that would be correlative to the existence of both their Laplacian-based and their Fourier-based activity -- there is then the predominant need for a much higher Hodge-Index of the quantity of eigenstates of the centralized knotting of the Rarita Structure for the so-stated respective stars and planets. This would then work to explain, in part, the basis for the existence of the high quantities of mass -- of which would here bear a high quantity of gluons -- for both stars and planets. To Be Continued!
Sam Roach.
No comments:
Post a Comment