Thursday, April 8, 2010

Course 3 on Lorentz-Four-Contractions, Last Test Solutions, Part 1

1) At .5c, the superstrings of the given object closest region along the given axis would contract lengthwise according to l = ((1-v^2/c^2)^.5). The superstrings of the given object that surrounded the prior mentioned region would contract moderately. The superstrings that did not define the length of the given object, and thus were furthest from the center of the specific axis given, would not contract at all, since the superstrings here would not define the length of the given object.

2) Matter and kinetic energy that are of a Kaluza-Klein light-cone-gauge topology contract relative to light because, since light is the result of the recycling of differential geometries, and all motion that involves mass that is of an abelian light-cone-gauge topology moves relative to the basis of such recycling, the physical parameters associated with such phenomena of mass must alter when such phenomena change in kinematic differentiation relative to light.

3) l = ((1-v^2/c^2)^.5, m = (1/(1-v^2/c^2)^.5), and relative to one traveling just under light speed, t = (1-v^2/c^2)^.5, or the proportion of more time noticed by a stander by as compared to one traveling just under light speed would obey t = (1/(1-v^2/c^2)^.5).

4) Its length would contract by .6, its mass would increase by (1/.6), and, the amount of time noticed by the one going at .8c would be .6 of the time of a stander by.

5) A mass with a Kaluza-Klein light-cone-gauge topology can not travel at light speed or else it would have all of the mass in space and time. This is because a Kaluza-Klein light-cone-gauge topology is abelian, and such topology bears a maximum fractal modulae in terms of its Gliossi field generation as encountered with just under light speed, and you can not increase such a fractal stress and expect it to obey the properties of a non-abelian light-cone-gauge topology.

6) Since the center of such strings specifically travels at .8c, this central region would contract according to (1-v^2/c^2)^.5 and (1/(1-v^2/c^2)^.5), and, the Lorentz-Four-Contractions would ease homeomorphically as one examines the further regions of the kinematic strings involved here.

7) The strings that are directly in the path of the directoralizations that moves at the given "quick" speed would contract in their given directoralizations according to Einstein's equations. Yet, since the two phenomena moving at the "quick" speed are differentiating in a multiplicit directoralization, the observation of such contractions would form a radial covariance that would be non-trivially isomorphic. The superstrings that are slower would also obey Einstein's equations would contract less.

8) A spherical object consisting of many superstrings that is moving in a unitary direction and is not spinning, orbiting, nor otherwise radially differentiating kinematically will only contract lengthwise toward the center of its directoralization, and would thus not contract uniformally.

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