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arXiv 0905.2552hep-th
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第一量子弦宇宙学中作为α ' -非微扰解的速子-膨胀子驱动的暴胀

Tachyon - Dilaton driven Inflation as an alpha' - non-perturbative solution in First Quantized String Cosmology

Anna Kostouki

摘要:

将一种新的非微扰泛函方法框架应用于具有快子、介子和引力子背景的二维玻色子西格玛模型,构造了与世界面Weyl不变性一致的精确(Regge斜率为非微扰)暴胀解.暴胀的机制需要一个(部分)的“对齐”之间的快子和快子背景的解决方案空间。一些宇宙学解,其中包含暴胀时代的一个短的时期和插入之间的平坦宇宙在遥远的过去和遥远的未来进行了讨论。这些解的特点是没有宇宙视界,因此具有明确的散射振幅。这使得它们与微扰弦框架相容,因此我们认为这些解在我们的方法中是自洽的。在插值解的范围内,也可以研究膨胀(预热)结束时的串产生。我们的方法的优点是,解决方案是有效的,直接在四个目标空间的时间维,由于非平凡的的介子配置。

英文摘要:

Applying a novel non-perturbative functional method framework to a two-dimensional bosonic sigma model with tachyon, dilaton and graviton backgrounds we construct exact (non perturbative in the Regge slope) inflationary solutions, consistent with world-sheet Weyl Invariance. The mechanism for inflation entails a (partial) "alignment" between tachyon and dilaton backgrounds in the solution space. Some cosmological solutions which contain inflationary eras for a short period and interpolate between flat universes in the far past and far future are also discussed. These solutions are characterized by the absence of cosmological horizons, and therefore have well-defined scattering amplitudes. This makes them compatible with a perturbative string framework, and therefore it is these solutions that we consider as self-consistent in our approach. Within the context of the interpolating solutions, string production at the end of inflation (preheating) may also be studied. The advantage of our method is that the solutions are valid directly in four target-space-time dimensions, as a result of the non trivial dilaton configurations.

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