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开放宇宙中的宇宙微波背景异常。

Cosmic microwave background anomalies in an open universe.

机构信息

Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, United Kingdom.

出版信息

Phys Rev Lett. 2013 Sep 13;111(11):111302. doi: 10.1103/PhysRevLett.111.111302. Epub 2013 Sep 9.

Abstract

We argue that the observed large-scale cosmic microwave anomalies, discovered by WMAP and confirmed by the Planck satellite, are most naturally explained in the context of a marginally open universe. Particular focus is placed on the dipole power asymmetry, via an open universe implementation of the large-scale gradient mechanism of Erickcek et al. Open inflation models, which are motivated by the string landscape and which can excite "supercurvature" perturbation modes, can explain the presence of a very-large-scale perturbation that leads to a dipole modulation of the power spectrum measured by a typical observer. We provide a specific implementation of the scenario which appears compatible with all existing constraints.

摘要

我们认为,由 WMAP 发现并被 Planck 卫星证实的大尺度宇宙微波异常现象,最自然地可以用边缘开放宇宙的观点来解释。通过对 Erickcek 等人的大尺度梯度机制的开放宇宙实现,特别关注偶极功率不对称性。由弦景观激发的开放暴胀模型可以激发“超曲率”扰动模式,它们可以解释存在非常大尺度的扰动,从而导致典型观察者测量的功率谱的偶极调制。我们提供了一种与所有现有约束条件都相容的具体方案。

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