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Article: Exact causal viscous cosmologies

TitleExact causal viscous cosmologies
Authors
KeywordsCausal Viscous Cosmologies
Issue Date1998
PublisherSpringer New York LLC. The Journal's web site is located at http://springerlink.metapress.com/openurl.asp?genre=journal&issn=0001-7701
Citation
General Relativity and Gravitation, 1998, v. 30 n. 8, p. 1171-1186 How to Cite?
AbstractThe general exact solution of the gravitational field equations for a homogeneous flat Friedmann-Robertson-Walker universe filled with a causal bulk viscous fluid with bulk viscosity coefficient proportional to the Hubble function is obtained in the framework of the full causal Israel-Stewart-Hiscock theory. The general solution of the field equations is represented in an exact closed parametric form and corresponds to a transition between two Minkowskian space-times connected by an inflationary period. The evolution of the temperature, entropy, deceleration parameter and bulk viscosity coefficient are considered in the general case. Particular solutions corresponding to a particular choice of parameters and leading to a non-inflationary evolution of the universe are presented too.
Persistent Identifierhttp://hdl.handle.net/10722/91774
ISSN
2023 Impact Factor: 2.1
2023 SCImago Journal Rankings: 0.794
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorMak, MKen_HK
dc.contributor.authorHarko, Ten_HK
dc.date.accessioned2010-09-17T10:26:13Z-
dc.date.available2010-09-17T10:26:13Z-
dc.date.issued1998en_HK
dc.identifier.citationGeneral Relativity and Gravitation, 1998, v. 30 n. 8, p. 1171-1186en_HK
dc.identifier.issn0001-7701en_HK
dc.identifier.urihttp://hdl.handle.net/10722/91774-
dc.description.abstractThe general exact solution of the gravitational field equations for a homogeneous flat Friedmann-Robertson-Walker universe filled with a causal bulk viscous fluid with bulk viscosity coefficient proportional to the Hubble function is obtained in the framework of the full causal Israel-Stewart-Hiscock theory. The general solution of the field equations is represented in an exact closed parametric form and corresponds to a transition between two Minkowskian space-times connected by an inflationary period. The evolution of the temperature, entropy, deceleration parameter and bulk viscosity coefficient are considered in the general case. Particular solutions corresponding to a particular choice of parameters and leading to a non-inflationary evolution of the universe are presented too.en_HK
dc.languageengen_HK
dc.publisherSpringer New York LLC. The Journal's web site is located at http://springerlink.metapress.com/openurl.asp?genre=journal&issn=0001-7701en_HK
dc.relation.ispartofGeneral Relativity and Gravitationen_HK
dc.subjectCausal Viscous Cosmologiesen_HK
dc.titleExact causal viscous cosmologiesen_HK
dc.typeArticleen_HK
dc.identifier.emailHarko, TC:harko@hkucc.hku.hken_HK
dc.identifier.authorityHarko, TC=rp1333en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.scopuseid_2-s2.0-0032219728en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0032219728&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume30en_HK
dc.identifier.issue8en_HK
dc.identifier.spage1171en_HK
dc.identifier.epage1186en_HK
dc.identifier.isiWOS:000075157200002-
dc.identifier.issnl0001-7701-

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