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arXiv · hep-ph/9303250

Domain Wall Formation In The Post-Inflationary Universe

Z. Lalak·S. Thomas
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Abstract

We consider the evolution of the probability distribution $\pp (χ,\chib, \t)$, associated with an inhomogeneous light scalar field $χ$ in the Robertson-Walker Universe, where the inhomogeneities are produced by quantum fluctuations during an earlier inflationary epoch. For a specific choice of scalar potential which occurs in models of so called late-time phase transitions in which domain walls are produced, $\pp$ is shown to evolve from a Gaussian to a non-Gaussian distribution. The structure of the latter justifies the recent use of 3-dimensional percolation theory to describe the initial distribution of domain walls in these models.

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Z. Lalak, S. Thomas. 1993-03-12. Domain Wall Formation In The Post-Inflationary Universe. https://doi.org/10.1016/0370-2693(93)91130-f

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