Part Four of the Third Session of Course 14

From where I had left off last time, the differential series' that I had been just discussing are commutated after the course (no pun intended) of many iterations of instanton.  The said differential series' of such inter-related superstrings involve superstrings of discrete energy permittivity that are indistinguishably different from one another.  Such a genus of differential series' also involves substringular units that tend to be more kinematic than those of a steady state, and/or, such a genus of differential series' may sometimes involve alterior substringular units that are indistinguishably different. Sometimes, via the activity of a given arbitrary tense of kinematic differentiation over time, the directly related angles that I have been discussing in the last four sessions -- that the so mentioned isomorphic superstrings bear over a relatively brief period of time -- go into a state of perturbation, or alteration, that act in conjunction with the angling of both the corresponding Planck-related phenomena and their directly correlative-based counterstrings.  Yet, when a tense of isomorphism is maintained -- on account of what may here be the formation of a tense of static equilibrium in the directly related substringular region -- the angling between the multiplicit orbifolds that are again of the same universe, when in terms of the covariant wobbling of their directly associated Fadeev-Popov-Trace eigenstates that are both adjacent and are of two different orbifolds that are of the same universe, will form an angling between these that is of an identical degree.  That is, 1.104735878*10^(-81)I degrees.  So, the format of the chirality of the relative tense of norm, or, orphoganal, that exists between the corresponding Fadeev-Popov-Trace eigenstates, will alter in genus per the ensuing exterialization of adjacency that would here be among substringular units of energy that are of the same universe, yet, the angle of the wobbling that is covariant between such Fadeev-Popov-Trace eigenstates that are of the same given arbitrary universe will always be 1.104735878*10^(-81)I degrees -- as long as the corresponding discrete units of energy remain of the same universe.  To Be Continued!  Sam Roach.