Numerical relativity and the early Universe
We consider numerical simulations in general relativity in ADM formalism with cosmological ansatz for the metric. This ansatz is convenient for investigations of the Universe creation in laboratory with Galileons. Here we consider toy model for the software: spherically symmetric scalar field minima...
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2016-01-01
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Online Access: | http://dx.doi.org/10.1051/epjconf/201612503015 |
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doaj-0422454da42649eb89ca48fe9df575012021-08-02T20:35:36ZengEDP SciencesEPJ Web of Conferences2100-014X2016-01-011250301510.1051/epjconf/201612503015epjconf_quark2016_03015Numerical relativity and the early UniverseMironov Sergey0Institute for Nuclear Research of the Russian Academy of SciencesWe consider numerical simulations in general relativity in ADM formalism with cosmological ansatz for the metric. This ansatz is convenient for investigations of the Universe creation in laboratory with Galileons. Here we consider toy model for the software: spherically symmetric scalar field minimally coupled to the gravity with asymmetric double well potential. We studied the dependence of radius of critical bubble on the parameters of the theory. It demonstrates the wide applicability of thin-wall approximation. We did not find any kind of stable bubble solution.http://dx.doi.org/10.1051/epjconf/201612503015 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Mironov Sergey |
spellingShingle |
Mironov Sergey Numerical relativity and the early Universe EPJ Web of Conferences |
author_facet |
Mironov Sergey |
author_sort |
Mironov Sergey |
title |
Numerical relativity and the early Universe |
title_short |
Numerical relativity and the early Universe |
title_full |
Numerical relativity and the early Universe |
title_fullStr |
Numerical relativity and the early Universe |
title_full_unstemmed |
Numerical relativity and the early Universe |
title_sort |
numerical relativity and the early universe |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2016-01-01 |
description |
We consider numerical simulations in general relativity in ADM formalism with cosmological ansatz for the metric. This ansatz is convenient for investigations of the Universe creation in laboratory with Galileons. Here we consider toy model for the software: spherically symmetric scalar field minimally coupled to the gravity with asymmetric double well potential. We studied the dependence of radius of critical bubble on the parameters of the theory. It demonstrates the wide applicability of thin-wall approximation. We did not find any kind of stable bubble solution. |
url |
http://dx.doi.org/10.1051/epjconf/201612503015 |
work_keys_str_mv |
AT mironovsergey numericalrelativityandtheearlyuniverse |
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