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arXiv 1709.09016hep-th
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再访德西特超光速子膜世界

A de Sitter tachyonic braneworld revisited

Nandinii Barbosa-Cendejas, Roberto Cartas-Fuentevilla, Alfredo Herrera-Aguilar, Refugio Rigel Mora-Luna, Roldão da Rocha

摘要:

在膜世界的框架内,几个有趣的物理效应可以在广泛的能量尺度上描述,从高能物理到宇宙学和低能物理。生成厚膜世界模型的一个常用方法是将体标量场耦合到更高维的扭曲引力。最近,一个新的膜世界是在快子体标量场的帮助下产生的,它具有几个显著的性质。它包括一个正规和稳定的解决方案,其中包含一个相关的3-膜与德西特诱导度规,产生作为一个精确的解决方案的5D场方程,描述我们的宇宙的暴胀时代。此外,它是{ \it渐近平坦},尽管存在负的5D宇宙学常数,这是一个有趣的功能,与大多数已知的,渐近的dS或AdS模型。此外,它包含了一个引力子谱与一个单一的无质量的束缚态,占四维引力局域在膜上,从卡鲁扎-克莱因大质量引力子模式的连续分开的质量间隙,使5D修正牛顿定律指数衰减。最后,规范,标量和费米子领域也被证明是本地化在这个braneworld。在这项工作中,我们表明,这种快子braneworld允许一个非平凡的解决方案与消失的5D宇宙学常数,保留了所有上述显着的属性与较少的参数,构成了一个现实的宇宙braneworld模型的建设的重要贡献。

英文摘要:

Within the framework of braneworlds, several interesting physical effects can be described in a wide range of energy scales, starting from high-energy physics to cosmology and low-energy physics. An usual way to generate a thick braneworld model relies in coupling a bulk scalar field to higher dimensional warped gravity. Quite recently, a novel braneworld was generated with the aid of a tachyonic bulk scalar field, having several remarkable properties. It comprises a regular and stable solution that contains a relevant 3--brane with de Sitter induced metric, arising as an exact solution to the 5D field equations, describing the inflationary eras of our Universe. Besides, it is {\it asymptotically flat}, despite of the presence of a negative 5D cosmological constant, which is an interesting feature that contrasts with most of the known, asymptotically either dS or AdS models. Moreover, it encompasses a graviton spectrum with a single massless bound state, accounting for 4D gravity localized on the brane, separated from the continuum of Kaluza-Klein massive graviton modes by a mass gap that makes the 5D corrections to Newton's law to decay exponentially. Finally, gauge, scalar and fermion fields are also shown to be localized on this braneworld. In this work, we show that this tachyonic braneworld allows for a nontrivial solution with a vanishing 5D cosmological constant that preserves all the above mentioned remarkable properties with a less amount of parameters, constituting an important contribution to the construction of a realistic cosmological braneworld model.

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