Constricted Spin-Orbital Motion Of Fadeev-Popov-Trace Eigenstates

 In general, for Noether-Based discrete quanta of energy; The faster that a given arbitrary mass-bearing discrete quantum of energy is to be moving, in relation to the motion of electromagnetic energy, the more constrictive that the spin-orbital-related motion, of the directly associated respective Fadeev-Popov-Trace eigenstate, will therefore tend to be, to where it is to consequentially follow, that this will tend to result, in a general type of a Ward-Cauchy-Related situation, to where both the greater that the Lorentz-Four-Contraction will tend to be, and also, the lower that the scalar amplitude, of the directly corresponding Polyakov Action eigenstate, will therefore result in tending to be.Thereby and consequently, in general, for Noether-Based discrete quanta of energy; The slower that a given arbitrary mass-bearing discrete quantum of energy is to moving, in relation to the motion of electromagnetic energy, the less constrictive that the spin-orbital-related motion, of the directly associated respective Fadeev-Popov-Trace eigenstate, will therefore tend to be, to where it is to consequentially follow, that this will tend to result, in a general type of a Ward-Cauchy-Related situation, to where both the lesser that the Lorentz-Four-Contraction will tend to be, and also, the higher that the scalar amplitude, of the directly corresponding Polyakov Action eigenstate, will therefore result in tending to be. I WILL CONTINUE WITH THE SUSPENSE LATER! TO BE CONTINUED SOON! SAM ROACH.