一个生长和旋转的普朗克宇宙的轮廓图,其中出现了黑暗泡沫

U. Seshavatharam, S. Lakshminarayana
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引用次数: 3

摘要

参考普朗克尺度、马赫关系,增加对大尺度宇宙各向异性和优选方向的支持,从普朗克尺度开始,引入两个新的参数Gamma和Beta,我们试图估计普通物质密度比、暗物质密度比、质量、半径、温度、年龄和宇宙各方向的膨胀速度(来自和关于宇宙各方向)。我们认为,从普朗克尺度开始,暗物质就可以被认为是一种宇宙泡沫,负责星系的形成。宇宙角速度与宇宙温度的平方成正比。3)宇宙膨胀速度随总物质密度比的减小而增大。4)为了理解宇宙加速,没有必要考虑暗能量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
An Outline Picture of a Growing and Rotating Planck Universe with Emerging Dark Foam
With reference to Planck scale, Mach’s relation, increasing support for large scale cosmic anisotropy and preferred directions and by introducing two new parameters Gamma and Beta, right from the beginning of Planck scale, we make an attempt to estimate ordinary matter density ratio, dark matter density ratio, mass, radius, temperature, age and expansion velocity (from and about the bay universe in all directions). We would like suggest that, from the beginning of Planck scale, 1) Dark matter can be considered as a kind of cosmic foam responsible for formation of galaxies.  2) Cosmic angular velocity is directly proportional to squared cosmic temperature. 3) Cosmic expansion velocity increases with decreasing total matter density ratio. 4) There is no need to consider dark energy for understanding cosmic acceleration.
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