New futures for cosmological models

L. Fernández-Jambrina, R. Lazkoz
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引用次数: 5

Abstract

The discovery of accelerated expansion of the Universe opened up the possibility of new scenarios for the doom of our space–time, besides eternal expansion and a final contraction. In this paper, we review the chances that may await our universe. In particular, there are new possible singular fates (sudden singularities, big rip, etc.), but there also other evolutions that cannot be considered as singular. In addition to this, some of the singular fates are not strong enough in the sense that the space–time can be extended beyond the singularity. For deriving our results, we make use of generalized power and asymptotic expansions of the scale factor of the Universe. This article is part of the theme issue ‘The future of mathematical cosmology, Volume 1’.
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宇宙学模型的新未来
宇宙加速膨胀的发现为我们时空的毁灭提供了新的可能性,除了永恒的膨胀和最终的收缩。在本文中,我们回顾了可能等待我们的宇宙的机会。特别是,有新的可能的奇异命运(突然奇点,大撕裂等),但也有其他不能被认为是奇异的进化。除此之外,从时空可以延伸到奇点之外的意义上说,一些奇异命运不够强大。为了得到我们的结果,我们利用了宇宙尺度因子的广义幂和渐近展开式。本文是主题问题“数学宇宙学的未来,第一卷”的一部分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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