Monday, October 1, 2012

A Little More As To Common "Wobble"

When a black-hole forms, the directly associated Planck phenomena that initially enter the said black-hole belong to the universe that inolve those Planck phenomena that are normal to the frayed stringular topology by a wobble of 1.104735878*(-81)Idegrees.  Next, Planck phenomena enter the said black-hole that are normal to the frayed superstrings related Planck phenomena that are normal when in consideration of a relative wobble that exists within a factor of 9.1*10^6* the most discrete adjacent-based covariant wobble that exists among two arbitrary given Planck phenomena that are of the same universe.  Next, the tendancy is toward the motion in the direction of Planck phenomena to enter the mentioned black-hole that are off of normalcy -- in terms of adjacent covariant wobble -- by up to 91*10^81.  (Black-Holes are to never get to that point of potential danger, if one may be able to ward them off by then.)  While some of our universe is being eaten up by any given arbitrary black-hole that has existed for any noticable period of time-based duration, some parts of paralllel universes are eaten up by black-holes as well.  A black-hole is elliminated when the whole black-hole sector is filled in a manner that I will not describe.  Black-Hole sectors "try" to eat up the universe.  That is why these are unwanted.  Black-Holes fray substringular material.  Black-Holes are formed by accumulative dilation build-up that interacts with normal substringlar Fourier-based differentiation.  Dilatons are the massless set quantum of gravitational-based angular momentum energy.  Excessive dilaon accumulation exists after a star has collapsed.  Dilatons accumulate when ghost anomalies are not efficiently annhilated by negative-norm-states.   When two-dimensional superstrings have anharmonically differentiated in a Fourier-based manner too much in a relatively limited region, the corresponding negative-norm-states do not have the adequate opportunity to orphoganate the related norm-conditions that are formed by the related positive-norm-states.  Masses that exist for a relatively long time tend to undergo more entropy.  Entropy produces annharmonics of the corresponding substringular fabric.  Annharmonic stringular Fourier-based differentiation produces multiple zero-norm ghost states, since the zero-norm states cannot form Jacobian-based spatial tangents with the active surface of the directly related ghost anomalic eigenbases.  This lack of multiplicit cohesive parity puts world-sheet paths in the way of each other, in terms of what should become their Laplcacian-mapped paths.  This works to breaksup the related topology, and thus form black-holes.

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