Primordial Bubbles within Primordial Bubbles

F. Occhionero, L. Amendola, Pier Stefano Corasaniti
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Abstract

Two consecutive, distinct episodes of phase transition occurring during inflation may nucleate two generations of bubbles, one inside the other. We design a model of inflation that realizes this sequence and yields bubble spectra that are bimodal and tunable functions of phenomelogical parameters in turn combinations of microphysical parameters. We argue in favor of a tuning of the parameters such that the outer and earlier generation of bubbles becomes hundreds of Mpc/h in diameter (like the local Hubble bubbles of the literature) whereas the inner and later generation becomes tens of Mpc/h in diameter (like the observed large scale voids).
原始气泡中的原始气泡
在暴胀期间发生的两个连续的、不同的相变可能形成两代气泡的核,一个在另一个里面。我们设计了一个实现这一序列的膨胀模型,并产生了双峰气泡光谱,这些气泡光谱是物象参数的可调函数,而微物理参数又是组合的。我们主张调整参数,使外层和早期气泡的直径达到数百Mpc/h(就像文献中局部的哈勃气泡),而内部和后期气泡的直径达到数十Mpc/h(就像观察到的大尺度空洞)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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