Thursday, October 17, 2013
An Elaboration As To Reverse-Gravity Versus Antigravity
Here is some of an explanation as to what is the difference between a given case of reverse gravity versus a given case of antigravity.: A substringular scenario begins at an arbitrary case-point in time. The directly associate gravitational-based particles are differentiating kinematically here in a tense of static equilibrium, or, in other words, in a condition of superconformal invariance. Also, the directly associated indices of the corresponding Rarita Structure eigenstates are here bearing a multiplicit general format of wave-tug/wave-pull that corresponds to a multidirectoral integrable tense of angular momentum, in a specific genus of a related Hamiltonian operation. We will here call the general wave-tug/wave-pull that is here associated with the multiplicit directoralization of the resultant motion of the corresponding activity -- of the related gravitational-based particles -- as the basis of what my be relatively described of as the initial given arbitrary forward-moving gravitational pull. The permittivity of such a genus of what would here be the angular momentum of such a gravitational pull --- by the directly associated gravitational particles -- is the motion that we will here use to describe of as the forward-holomorphic gravitational Hamiltonian operation. When the given arbitrary angular momentum of the corresponding gravitational-based particles reverses in terms of the directoralization of its holomorphic-based permittivity, then, the substringular region -- that would here correspond to the activity of the said given gravitational-based pariticles, would be said to be undergoing a situation of a relative reversal of gravity. This is a case of reverse gravity. Yet, if instead, the directly corresponding indices of the eigenstates of the directly associated local Rarita Structure -- in the form of second-ordered Schwinger-Indices -- multiplicitly, as a group, simultaneously reverses in the directoralizaton of the permittvity of their angular momentum-based Hamiltonian operation, by reversing the holomorphicity of the kinematic delineation of the said second-ordered Schwinger-Indices, then, the corresponding substringular region of this scenario is said to be undergoing antigravity.
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samsphysicsworld
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12:43 PM
Labels:
Hamiltonian,
holomorphic,
permittivity,
Rarita Structure,
Schwinger-Indices
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