在封闭宇宙中相互作用的暗能量

Eleonora Di Valentino, A. Melchiorri, O. Mena, S. Pan, Weiqiang Yang
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引用次数: 29

摘要

最近由普朗克卫星测量的宇宙微波各向异性功率谱的测量表明,在超过99%的置信水平上,对封闭宇宙的偏好。然而,这种情况与一些低红移观测值不一致,包括Ia型超新星的光度距离。在这里,我们表明相互作用暗能量(IDE)模型可以缓解普朗克和超新星Ia数据在封闭宇宙中的差异。因此,IDE宇宙论仍然是非常吸引人的场景,因为它们可以为不同基准宇宙论中的许多观测张力提供解决方案。这里提出的结果强烈支持对宇宙数据进行更广泛的分析,并表明放宽通常的平坦性和真空能量假设可以使理论和观测之间更好地一致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Interacting dark energy in a closed universe
Recent measurements of the Cosmic Microwave Anisotropies power spectra measured by the Planck satellite show a preference for a closed universe at more than $99 \%$ Confidence Level. Such a scenario is however in disagreement with several low redshift observables, including luminosity distances of Type Ia Supernovae. Here we show that Interacting Dark Energy (IDE) models can ease the discrepancies between Planck and Supernovae Ia data in a closed Universe. Therefore IDE cosmologies remain as very appealing scenarios, as they can provide the solution to a number of observational tensions in different fiducial cosmologies. The results presented here strongly favour broader analyses of cosmological data, and suggest that relaxing the usual flatness and vacuum energy assumptions can lead to a much better agreement among theory and observations.
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