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首页> 外文期刊>Advances in high energy physics >From de Sitter to de Sitter: Decaying Vacuum Models as a Possible Solution to the Main Cosmological Problems
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From de Sitter to de Sitter: Decaying Vacuum Models as a Possible Solution to the Main Cosmological Problems

机译:从De Sitter到De Sitter:腐烂真空模型作为主要宇宙问题的可能解决方案

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摘要

Decaying vacuum cosmological models evolving smoothly between two extreme (very early and late time) de Sitter phases are able to solve or at least to alleviate some cosmological puzzles; among them we have (i) the singularity, (ii) horizon, (iii) gracefulexit from inflation, and (iv) the baryogenesis problem. Our basic aim here is to discuss how the coincidence problem based on a large class of running vacuum cosmologies evolving from de Sitter to de Sitter can also be mollified. It is also argued that even the cosmological constant problem becomes less severe provided that the characteristic scales of the two limiting de Sitter manifolds are predicted from first principles.
机译:腐烂的真空宇宙学模型在两个极端(非常早期和晚期)De Satter阶段之间顺畅地发展,能够解决或至少可以缓解一些宇宙学难题; 其中我们有(i)奇点,(ii)地平线,(iii)从通胀中的格栅,和(iv)重新发生问题。 我们的基本目标是讨论如何根据大类运行的真空宇宙从De Sitter演变为De Matter的巧合问题也可以覆盖。 还认为即使是宇宙学恒定的问题也变得不太严重,但是从第一原理预测了两个限制的DE设分歧管的特征尺度。

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