Vacuum shell in the Schwarzschild-de Sitter world
General Relativity and Quantum Cosmology
2008-11-26 v1 High Energy Physics - Phenomenology
Abstract
We construct the classification scheme for all possible evolution scenarios and find the corresponding global geometries for dynamics of a thin spherical vacuum shell in the Schwarzschild-de Sitter metric. This configuration is suitable for the modelling of vacuum bubbles arising during cosmological phase transitions in the early Universe. The distinctive final types of evolution from the local point of view of a rather distant observer are either the unlimited expansion of the shell or its contraction with a formation of black hole (with a central singularity) or wormhole (with a baby universe in interior).
Cite
@article{arxiv.0709.0616,
title = {Vacuum shell in the Schwarzschild-de Sitter world},
author = {S. V. Chernov and V. I. Dokuchaev},
journal= {arXiv preprint arXiv:0709.0616},
year = {2008}
}
Comments
15 pages, 8 figures