Tuesday, March 18, 2014

The Pauli rate in regions of high phase energy

One thing we can be sure of is that the vacuum, everywhere, quantizes phase energy.   The Plank rate is the Nyquist level, {-1,0,+2} sequences.  The {-1,0,+2} sequence then defines Plank, and the relative Pauli mass sizes, mass sizes are set by the fixed Pauli separability size. The Pauli rate defines the rate of quantization. The Higgs, then, defines the largest energy density in any region that is Pauli stable.  But we do not have a view of all the regions?


Compaction is not complete, fractional phase energy moves to the outer layer of compaction, which is Nyquist. At Nyquist it accumulated because Nyquist, like all quantization layers, is curved. So, the phase equalization is not done, and again, we do not have a view of the whole Nyquist. We have no proof that phase energy distribution matches the complete ordering down to Higgs.

The possibility of unequal, or fractional ordering, is measured as:
(density variation)/Pauli rate, Dv/Pr < 1 means that we get partial quantization, which I think happened with magnetism around these parts. Noise makes low SNR, the Pauli rate when phase is energy above the Nyquist (Plank) energy level.Phase is equalized along the Poly path, if there is no Nyquist equalization, or if there is mass density, the poly path is not existent, or tightly looped.

In a region the is ultimately destined for Star-dom, the Higgs form densely that phase variance accumulates and we get a squeeze, a partial ordering. Even today out Sun is minimizing phase energy at less than light speed. Atoms are a partial ordering, the nucleus is still trying to phase equalize.





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