Gravitational Stability for a Vacuum Cosmic Space Crystalline Model

J. A. Montemayor-Aldrete; J. R. Morones-Ibarra; A. Morales-Mori; A. Mendoza-Allende; A. Montemayor-Varela; M. del Castillo-Mussot; G. J. Vazquez

arXiv · physics/0603097

Gravitational Stability for a Vacuum Cosmic Space Crystalline Model

J. A. Montemayor-Aldrete·J. R. Morones-Ibarra·A. Morales-Mori·A. Mendoza-Allende·A. Montemayor-Varela·M. del Castillo-Mussot·G. J. Vazquez

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Abstract

Using Heisenberg's uncertainty principle it is shown that the gravitational stability condition for a crystalline vacuum cosmic space implies to obtain an equation formally equivalent to the relation first used by Gamow to predict the present temperature of the microwave background from the matter density. The compatibility condition between the quantum and the relativistic approaches has been obtained without infinities arising from the quantum analysis or singularities arising from the relativistic theory. The action which leads to our theory is the least action possible in a quantum scheme. The energy fluctuation involved in the gravitational stabilization of vacuum space is 10 to the power of (-40) times the energy of the crystalline structure of vacuum space inside the present Universe volume.

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J. A. Montemayor-Aldrete, J. R. Morones-Ibarra, A. Morales-Mori, A. Mendoza-Allende, A. Montemayor-Varela, M. del Castillo-Mussot, G. J. Vazquez. 2006-03-13. Gravitational Stability for a Vacuum Cosmic Space Crystalline Model. https://arxiv.org/abs/physics/0603097

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