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The Solution of the Cosmological Constant Problem: The Cosmological Constant Exponential Decrease in the Super-Early Universe
Universe ( IF 2.9 ) Pub Date : 2020-12-04 , DOI: 10.3390/universe6120230
Ol’ga Babourova , Boris Frolov

The stage of a super-early (primordial) scale-invariant Universe is considered on the basis of the Poincaré–Weyl gauge theory of gravity in a Cartan–Weyl space-time. An approximate solution has been found that demonstrates an inflationary behavior of the scale factor and, at the same time, a sharp exponential decrease in the effective cosmological constant from a huge value at the beginning of the Big Bang to an extremely small (but not zero) value in the modern era, which solves the well-known “cosmological constant problem.”

中文翻译:

宇宙常数问题的解决方案:超早期宇宙中宇宙常数的指数减小

基于Cartan-Weyl时空的庞加莱-魏尔规范重力理论,考虑了一个超早期(原始)尺度不变的宇宙的阶段。发现了一个近似解,它证明了比例因子的膨胀行为,同时,有效宇宙学常数从大爆炸开始时的巨大值急剧减小到极小值(但不为零)急剧下降。 )的价值,解决了众所周知的“宇宙学常数问题”。
更新日期:2020-12-04
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