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Analytic integrability of the Bianchi class A cosmological models with O~ 1< < 1
dc.contributor.author | Ferragut, Antoni | |
dc.contributor.author | Llibre, Jaume | |
dc.contributor.author | Pantazi, Chara | |
dc.date.accessioned | 2014-02-27T08:31:17Z | |
dc.date.available | 2014-02-27T08:31:17Z | |
dc.date.issued | 2013-03 | |
dc.identifier.issn | 0960-0779 | |
dc.identifier.uri | http://hdl.handle.net/10234/84890 | |
dc.description.abstract | Many works study the integrability of the Bianchi class A cosmologies with k = 1, where k is the ratio between the pressure and the energy density of the matter. Here we characterize the analytic integrability of the Bianchi class A cosmological models when 0 ⩽ k < 1. We conclude that Bianchi types VI0, VII0, VIII and IX can exhibit chaos whereas Bianchi type I is not chaotic and Bianchi type II is at most partially chaotic. | ca_CA |
dc.format.extent | 10 p. | ca_CA |
dc.format.mimetype | application/pdf | ca_CA |
dc.language.iso | eng | ca_CA |
dc.publisher | Elsevier | ca_CA |
dc.relation.isFormatOf | Versió del document publicat a http://www.sciencedirect.com/science/article/pii/S0960077913000039# | ca_CA |
dc.relation.isPartOf | Chaos, Solitons & Fractals (2013), vol. 48 | ca_CA |
dc.rights | © 2013 Elsevier Ltd. All rights reserved | ca_CA |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | * |
dc.subject | Fractals | ca_CA |
dc.subject | Differential equations | ca_CA |
dc.subject | Geometry | ca_CA |
dc.subject | Dynamical systems | ca_CA |
dc.title | Analytic integrability of the Bianchi class A cosmological models with O~ 1< < 1 | ca_CA |
dc.type | info:eu-repo/semantics/article | ca_CA |
dc.identifier.doi | http://dx.doi.org/10.1016/j.chaos.2012.12.007 | |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | ca_CA |
dc.relation.publisherVersion | http://www.sciencedirect.com/science/article/pii/S0960077913000039# | ca_CA |
dc.type.version | info:eu-repo/semantics/publishedVersion |
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