Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space
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 temper...
| Main Authors: | , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
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American Physical Society
2014
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| Online Access: | http://hdl.handle.net/1721.1/84956 |
| _version_ | 1826213321234186240 |
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| author | Bagchi, Arjun Detournay, Stephane Grumiller, Daniel Simon, Joan |
| author2 | Massachusetts Institute of Technology. Center for Theoretical Physics |
| author_facet | Massachusetts Institute of Technology. Center for Theoretical Physics Bagchi, Arjun Detournay, Stephane Grumiller, Daniel Simon, Joan |
| author_sort | Bagchi, Arjun |
| collection | MIT |
| description | 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. |
| first_indexed | 2024-09-23T15:47:12Z |
| format | Article |
| id | mit-1721.1/84956 |
| institution | Massachusetts Institute of Technology |
| language | en_US |
| last_indexed | 2024-09-23T15:47:12Z |
| publishDate | 2014 |
| publisher | American Physical Society |
| record_format | dspace |
| spelling | mit-1721.1/849562022-10-02T04:04:06Z Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space Bagchi, Arjun Detournay, Stephane Grumiller, Daniel Simon, Joan Massachusetts Institute of Technology. Center for Theoretical Physics Bagchi, Arjun 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. 2014-02-14T17:20:12Z 2014-02-14T17:20:12Z 2013-10 2013-05 Article http://purl.org/eprint/type/JournalArticle 0031-9007 1079-7114 http://hdl.handle.net/1721.1/84956 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 en_US http://dx.doi.org/10.1103/PhysRevLett.111.181301 Physical Review Letters 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. application/pdf American Physical Society American Physical Society |
| spellingShingle | Bagchi, Arjun Detournay, Stephane Grumiller, Daniel Simon, Joan Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space |
| title | Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space |
| title_full | Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space |
| title_fullStr | Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space |
| title_full_unstemmed | Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space |
| title_short | Cosmic Evolution from Phase Transition of Three-Dimensional Flat Space |
| title_sort | cosmic evolution from phase transition of three dimensional flat space |
| url | http://hdl.handle.net/1721.1/84956 |
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