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Article: Bianchi type I universes with causal bulk viscous cosmological fluid

TitleBianchi type I universes with causal bulk viscous cosmological fluid
Authors
Mak, MKHarko, T
Issue Date2002
PublisherWorld Scientific Publishing Co Pte Ltd. The Journal's web site is located at http://www.worldscinet.com/ijmpd/ijmpd.shtml
Citation
International Journal of Modern Physics D, 2002, v. 11 n. 3, p. 447-462 How to Cite?
DOI: http://dx.doi.org/10.1142/S0218271802001743
AbstractWe consider the dynamics of a causal bulk viscous cosmological fluid filled flat constantly decelerating Bianchi type I spacetime. The matter component of the Universe is assumed to satisfy a linear barotropic equation of state and the state equation of the small temperature Boltzmann gas. The resulting cosmological models satisfy the condition of smallness of the viscous stress. The time evolution of the relaxation time, temperature, bulk viscosity coefficient and comoving entropy of the dissipative cosmological fluid is also obtained.
Persistent Identifierhttp://hdl.handle.net/10722/91782
ISSN
0218-2718
2021 Impact Factor: 2.547
2020 SCImago Journal Rankings: 0.818
ISI Accession Number ID
WOS:000174774800013
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorMak, MKen_HK
dc.contributor.authorHarko, Ten_HK
dc.date.accessioned2010-09-17T10:26:28Z-
dc.date.available2010-09-17T10:26:28Z-
dc.date.issued2002en_HK
dc.identifier.citationInternational Journal of Modern Physics D, 2002, v. 11 n. 3, p. 447-462en_HK
dc.identifier.issn0218-2718en_HK
dc.identifier.urihttp://hdl.handle.net/10722/91782-
dc.description.abstractWe consider the dynamics of a causal bulk viscous cosmological fluid filled flat constantly decelerating Bianchi type I spacetime. The matter component of the Universe is assumed to satisfy a linear barotropic equation of state and the state equation of the small temperature Boltzmann gas. The resulting cosmological models satisfy the condition of smallness of the viscous stress. The time evolution of the relaxation time, temperature, bulk viscosity coefficient and comoving entropy of the dissipative cosmological fluid is also obtained.en_HK
dc.languageengen_HK
dc.publisherWorld Scientific Publishing Co Pte Ltd. The Journal's web site is located at http://www.worldscinet.com/ijmpd/ijmpd.shtmlen_HK
dc.relation.ispartofInternational Journal of Modern Physics Den_HK
dc.titleBianchi type I universes with causal bulk viscous cosmological fluiden_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.doi10.1142/S0218271802001743en_HK
dc.identifier.scopuseid_2-s2.0-0036004873en_HK
dc.identifier.hkuros77024-
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0036004873&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume11en_HK
dc.identifier.issue3en_HK
dc.identifier.spage447en_HK
dc.identifier.epage462en_HK
dc.identifier.isiWOS:000174774800013-
dc.identifier.citeulike3081424-
dc.identifier.issnl0218-2718-

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