Analytic integrability of the Bianchi class A cosmological models with O~ 1< < 1
![Thumbnail](/xmlui/bitstream/handle/10234/84890/61040.pdf.jpg?sequence=5&isAllowed=y)
View/ Open
Metadata
Show full item recordcomunitat-uji-handle:10234/9
comunitat-uji-handle2:10234/7037
comunitat-uji-handle3:10234/8635
comunitat-uji-handle4:
INVESTIGACIONMetadata
Title
Analytic integrability of the Bianchi class A cosmological models with O~ 1< < 1Date
2013-03Publisher
ElsevierISSN
0960-0779Type
info:eu-repo/semantics/articlePublisher version
http://www.sciencedirect.com/science/article/pii/S0960077913000039#Version
info:eu-repo/semantics/publishedVersionSubject
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 ... [+]
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. [-]
Is part of
Chaos, Solitons & Fractals (2013), vol. 48Rights
© 2013 Elsevier Ltd. All rights reserved
http://rightsstatements.org/vocab/InC/1.0/
info:eu-repo/semantics/openAccess
http://rightsstatements.org/vocab/InC/1.0/
info:eu-repo/semantics/openAccess
This item appears in the folowing collection(s)
- MAT_Articles [766]