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Self-accelerating solutions in the cascading DGP braneworld

机译:级联DGP braneworld中的自加速解决方案

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The self-accelerating branch of the Dvali–Gabadadze–Porrati (DGP) five-dimensional braneworld has provided a compelling model for the current cosmic acceleration. Recent observations, however, have not favored it so much. We discuss the solutions which contain a de Sitter 3-brane in the cascading DGP braneworld model, which is a kind of higher-dimensional generalizations of the DGP model, where ap-dimensional brane is placed on a(p+1)-dimensional one and thep-brane action contains the(p+1)-dimensional induced scalar curvature term. In the simplest six-dimensional model, we derive the solutions. Our solutions can be classified into two branches, which reduce to the self-accelerating and normal solutions in the limit of the original five-dimensional DGP model. In the presence of the six-dimensional bulk gravity, the ‘normal’ branch provides a new self-accelerating solution. The expansion rate of this new branch is generically lower than that of the original one, which may alleviate the fine-tuning problem.
机译:Dvali–Gabadadze–Porrati(DGP)五维Braneworld的自加速分支为当前的宇宙加速提供了引人注目的模型。但是,最近的观察并没有那么喜欢它。我们讨论了在级联DGP braneworld模型中包含de Sitter 3-brane的解决方案,这是DGP模型的一种高维概括,其中ap维骨架放在a(p + 1)维上p轴作用包含(p + 1)维诱导的标量曲率项。在最简单的六维模型中,我们得出解决方案。我们的解决方案可以分为两个分支,在原始的五维DGP模型的极限范围内,它们可以简化为自加速和常规解决方案。在存在六维体积重力的情况下,“常规”分支提供了新的自加速解决方案。新分支的扩展速率通常低于原始分支的扩展速率,这可以缓解微调问题。

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