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arXiv physics/0603097physics.gen-ph
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真空宇宙空间晶体模型的引力稳定性

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

摘要:

利用海森堡的不确定原理,证明了晶体真空宇宙空间的引力稳定性条件意味着得到一个形式上等价于伽莫夫首先利用物质密度预言微波背景辐射温度的关系式的方程。量子方法和相对论方法之间的相容性条件已经得到,而没有量子分析所产生的无穷大或相对论理论所产生的奇点。导致我们理论的作用量是量子体系中可能的最小作用量。真空空间的引力稳定所涉及的能量波动是目前宇宙体积内真空空间晶体结构能量的10的(-40)次方。

英文摘要:

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.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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