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arXiv 1505.00007hep-thastro-ph.COhep-ph
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弱破缺的伽利略对称性

Weakly Broken Galileon Symmetry

David Pirtskhalava, Luca Santoni, Enrico Trincherini, Filippo Vernizzi

摘要:

标量$ϕ$不变量在内\textit{galileon symmetry} $ϕ\toϕ+b_μx^μ$下的有效理论由于其特殊的理论和唯象性质而得到了广泛的研究。在本文中,我们引入了\textit{weakly broken galileon invariance}的概念,它描述了这种理论与引力的唯一耦合类,这些理论最大限度地保持了它们的定义对称性。伽利略的量子特性的弯曲空间残余允许构建(准)德西特背景在很大程度上对环路校正不敏感。我们利用这一事实来建立新的宇宙学模型与有趣的现象,相关的通货膨胀和后期的宇宙加速。

英文摘要:

Effective theories of a scalar $ϕ$ invariant under the internal \textit{galileon symmetry} $ϕ\toϕ+b_μx^μ$ have been extensively studied due to their special theoretical and phenomenological properties. In this paper, we introduce the notion of \textit{weakly broken galileon invariance}, which characterizes the unique class of couplings of such theories to gravity that maximally retain their defining symmetry. The curved-space remnant of the galileon's quantum properties allows to construct (quasi) de Sitter backgrounds largely insensitive to loop corrections. We exploit this fact to build novel cosmological models with interesting phenomenology, relevant for both inflation and late-time acceleration of the universe.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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