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Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space

Author(s)
Bagchi, Arjun; Detournay, Stephane; Grumiller, Daniel; Simon, Joan
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.

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Abstract
Flat space cosmology spacetimes are exact time-dependent solutions of three-dimensional gravity theories, such as Einstein gravity or topologically massive gravity. We exhibit a novel kind of phase transition between these cosmological spacetimes and the Minkowski vacuum. At sufficiently high temperature, (rotating) hot flat space tunnels into a universe described by flat space cosmology.
Date issued
2013-10
URI
http://hdl.handle.net/1721.1/84956
Department
Massachusetts Institute of Technology. Center for Theoretical Physics
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
Bagchi, Arjun et al. “Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space.” Physical Review Letters 111.18 (2013): n. pag. © 2013 American Physical Society
Version: Final published version
ISSN
0031-9007
1079-7114

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