9) If a spherical object containing many superstrings spin-orbits, rolls, and moves transversely at the same speed in a constant mutiplicitly unitized direction, that spherical object will contract uniformally.
10) Yes. It may if its fastest speed just under light speed is along a one-dimensional axial. If the center of an object that is traveling at the given object's maximum speed is in one direction along the center of a superstring's topological field that is propagating straight in that given directoralization, this will happen.
11) Phenomena relatively much larger than a superstring bear interial tensorisms of conformal invariance that result in a kinematic operation that causes the vectors and tensors of the given Fourier Transformation of that given object to differentiate as a whole at under light speed if it is not traveling in a worm-hole. If its volume is radially dependant, its Lorentz-Four-Contractions are effected by the transversel (rho), radial (phi), and spin-orbital (theta) Fourier Transformations that effect the kinematic differentiation of the given object.
12) If the tensoric and/or Njenhuis dimensions of an object are intrinsic to the Fourier Transformation of that object, then its Lorentz-Four-Contractions happen according to their Ward velocities and accelerations that exist metrically within the Ward spacial parameters of the given object.
13) Yes.
14) As a superstring keeps reiterating, the Gliossi-Shirk-Olive field that the given superstring maps out will cause it to be detected as larger than its primal essence and of a different shape than its primal essence.
15) The unitized field bearing to the center of the propagation of the field of the given oscillatory path is Lorentz-Four-Contracted according to Einstein's equations.
Thursday, April 8, 2010
Course 3 on Lorentz-Four-Contractions, Last Test Solutions, Part 2
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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.
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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Wednesday, April 7, 2010
Course 3 on Lorentz-Four-Contractions, Last Test, Part 2
9) How may one get a spherical object to Lorentz-Four-Contract uniformally?
10) May a material object contract as in one dimension in the globally distinguishable? Why? At what level could such a contraction happen?
11) Describe in general the directoralization of phenomena much larger than a string. What if its volume is radial?
12) If an object is in 3-D, how may its other dimensions happen?
13) Do strings vibrate?
14) Describe how the reiteration of a string in its neighborhood effects how it is detected.
15) Describe how an oscillating path is Lorentz-Four-Contracted by the transversel motion of its velocity in a given directoralization.
10) May a material object contract as in one dimension in the globally distinguishable? Why? At what level could such a contraction happen?
11) Describe in general the directoralization of phenomena much larger than a string. What if its volume is radial?
12) If an object is in 3-D, how may its other dimensions happen?
13) Do strings vibrate?
14) Describe how the reiteration of a string in its neighborhood effects how it is detected.
15) Describe how an oscillating path is Lorentz-Four-Contracted by the transversel motion of its velocity in a given directoralization.
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Course 3 of Session 3 on Lorentz-Four-Contractions,
direcoralization,
globally distinguishable,
Lorentz-Four-Contract uniformally,
radial metric,
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