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Astrophysics > Cosmology and Nongalactic Astrophysics

arXiv:1403.6688v2 (astro-ph)
[Submitted on 26 Mar 2014 (v1) , last revised 16 Oct 2014 (this version, v2)]

Title: How well do we understand the thermal history of the Universe? Implications of the recent BICEP2 data

Title: 我们对宇宙的热历史了解得多吗? 最近BICEP2数据的含义

Authors:Mairi Sakellariadou
Abstract: Applying Grand Unified Theories in the context of the early Universe, cosmic strings are an unavoidable partner of the inflaton field. To render such models compatible with the CMB temperature anisotropies, the inflationary scale has to be lower than the 2x10^{16} GeV value deduced from the tensor-to-scalar ratio announced from the BICEP2 collaboration. Some questions are consequently raised about our understanding of the thermal history of the Universe.
Abstract: 在早期宇宙的背景下应用大统一理论,宇宙弦是暴胀场不可避免的伴生物。 为了使这些模型与CMB温度各向异性相容,膨胀尺度必须低于从BICEP2合作组宣布的张量-标量比推导出的2x10^{16} GeV值。 因此,一些关于宇宙热历史的理解问题随之产生。
Comments: 4 pages; Slightly modified version to match publication
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO) ; General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th)
Cite as: arXiv:1403.6688 [astro-ph.CO]
  (or arXiv:1403.6688v2 [astro-ph.CO] for this version)
  https://doi.org/10.48550/arXiv.1403.6688
arXiv-issued DOI via DataCite
Journal reference: KCL-PH-TH/2014-9
Related DOI: https://doi.org/10.1103/PhysRevD.90.087301
DOI(s) linking to related resources

Submission history

From: Mairi Sakellariadou [view email]
[v1] Wed, 26 Mar 2014 14:29:17 UTC (9 KB)
[v2] Thu, 16 Oct 2014 13:27:19 UTC (10 KB)
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