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Spherical Domain Wall Collapse in a Dust Universe · Around

2014

Spherical Domain Wall Collapse in a Dust Universe

Tanahashi, Norihiro, Yoo, Chul-Moon

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To clarify observational consequence of bubble nucleations in inflationary era, we analyse dynamics of a spherical domain wall in an expanding universe.

We consider a spherical shell of the domain wall with tension $\sigma$ collapsing in a spherically-symmetric dust universe, which is initially separated into the open Friedmann-Lema\^itre-Robertson-Walker universe inside the shell and the Einstein-de Sitter universe outside.
The domain wall shell collapses due to the tension, and sweeps the dust fluid.
The universe after the collapse becomes inhomogeneous and is described by the Lema\^itre-Tolman-Bondi model.

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