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Evolution of perturbations in bouncing cosmological models

机译:弹跳宇宙学模型中扰动的演变

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The singularity theorems [1] show that, under reasonable physical assumptions, the Universe originated from an initialsingularity, and will develop future singularities in the form of black holes and, perhaps, of a big crunch. Until now,singularities are out of the scope of any physical theory. If we assume that a physical theory can describe the wholeUniverse at every instant, even at its possible moment of creation, which is the best attitude because it is the onlyway to seek the limits of physical science (in the words of Wheeler about singularities [2], ‘physics stops, but physicsmust go on’), then it is necessary that the ‘reasonable physical assumptions’ of the theorems be not valid under extreme situations of very high energy density and curvature.We may say that General Relativity (GR), and/or nongravitational field theory, must be changed under these extreme conditions. In fact, one must view such theorems as indications of the limits of GR and/or intervention of new types of matter.
机译:奇点定理表明,在合理的物理假设下,宇宙起源于初始性,并且将以黑洞的形式发展未来的奇点,也许是一个大皱纹。到目前为止,奇点超出了任何物理理论的范围。如果我们假设物理理论可以在每个瞬间描述整个局部,即使在可能的创作时刻,这是最好的态度,因为它是迄今为止探索物理科学的局限性(以惠特派团的惠特派团的话说[2 ],'物理停止,但物理士继续'),那么定理的“合理的物理假设”是必要的,在非常高的能量密度和曲率的极端情况下无效。我们可以说一般相对性(GR)和/或非投资场理论必须在这些极端条件下更改。事实上,必须将这样的定理视为遗留条目的迹象和/或新类型的干预。

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