File Download
  Links for fulltext
     (May Require Subscription)
Supplementary

Article: Bianchi type I cosmology in N=2, D=5 supergravity

TitleBianchi type I cosmology in N=2, D=5 supergravity
Authors
KeywordsPhysics - nuclear physics
Issue Date2000
PublisherAmerican Physical Society. The Journal's web site is located at http://prd.aps.org
Citation
Physical Review D (Particles and Fields), 2000, v. 61 n. 10, p. 104017:1-6 How to Cite?
AbstractThe dynamics and evolution of Bianchi type I space-times are considered in the framework of the four-dimensional truncation of a reduced theory obtained from N=2, D=5 supergravity. The general solution of the gravitational field equations can be represented in an exact parametric form. All solutions have a singular behavior at the initial or final moment, except when the space-time geometry reduces to the isotropic flat case. Generically the obtained cosmological models describe an anisotropic, expanding or collapsing, singular universe with a noninflationary evolution for all times.
Persistent Identifierhttp://hdl.handle.net/10722/43320
ISSN
2004 Impact Factor: 5.156

 

DC FieldValueLanguage
dc.contributor.authorChen, CMen_HK
dc.contributor.authorHarko, TCen_HK
dc.contributor.authorMak, MKen_HK
dc.date.accessioned2007-03-23T04:43:31Z-
dc.date.available2007-03-23T04:43:31Z-
dc.date.issued2000en_HK
dc.identifier.citationPhysical Review D (Particles and Fields), 2000, v. 61 n. 10, p. 104017:1-6en_HK
dc.identifier.issn0556-2821en_HK
dc.identifier.urihttp://hdl.handle.net/10722/43320-
dc.description.abstractThe dynamics and evolution of Bianchi type I space-times are considered in the framework of the four-dimensional truncation of a reduced theory obtained from N=2, D=5 supergravity. The general solution of the gravitational field equations can be represented in an exact parametric form. All solutions have a singular behavior at the initial or final moment, except when the space-time geometry reduces to the isotropic flat case. Generically the obtained cosmological models describe an anisotropic, expanding or collapsing, singular universe with a noninflationary evolution for all times.en_HK
dc.format.extent88691 bytes-
dc.format.extent122136 bytes-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.languageengen_HK
dc.publisherAmerican Physical Society. The Journal's web site is located at http://prd.aps.orgen_HK
dc.rightsCreative Commons: Attribution 3.0 Hong Kong License-
dc.rightsPhysical Review D (Particles and Fields). Copyright © American Physical Society.en_HK
dc.subjectPhysics - nuclear physicsen_HK
dc.titleBianchi type I cosmology in N=2, D=5 supergravityen_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0556-2821&volume=61&issue=10&spage=104017:1&epage=6&date=2000&atitle=Bianchi+type+I+cosmology+in+N=2,+D=5+supergravityen_HK
dc.description.naturepublished_or_final_versionen_HK
dc.identifier.doi10.1103/PhysRevD.61.104017en_HK
dc.identifier.hkuros63702-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats