File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: Decelerating causal bulk viscous cosmological models

TitleDecelerating causal bulk viscous cosmological models
Authors
KeywordsBulk Viscosity
Causal Thermodynamics
Dissipative Cosmology
Issue Date2000
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, 2000, v. 9 n. 2, p. 97-110 How to Cite?
AbstractThe dynamics of a causal bulk viscous cosmological fluid filled flat constantly decelerating noninflationary Robertson-Walker spacetime is considered. 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 evolution of the relaxation time, temperature, bulk viscosity coefficient and comoving entropy of the dissipative cosmological fluid are obtained by assuming several bulk viscosity coefficient-relaxation time relations.
Persistent Identifierhttp://hdl.handle.net/10722/91838
ISSN
2015 Impact Factor: 1.963
2015 SCImago Journal Rankings: 0.718
References

 

DC FieldValueLanguage
dc.contributor.authorHarko, Ten_HK
dc.contributor.authorMak, MKen_HK
dc.date.accessioned2010-09-17T10:28:05Z-
dc.date.available2010-09-17T10:28:05Z-
dc.date.issued2000en_HK
dc.identifier.citationInternational Journal of Modern Physics D, 2000, v. 9 n. 2, p. 97-110en_HK
dc.identifier.issn0218-2718en_HK
dc.identifier.urihttp://hdl.handle.net/10722/91838-
dc.description.abstractThe dynamics of a causal bulk viscous cosmological fluid filled flat constantly decelerating noninflationary Robertson-Walker spacetime is considered. 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 evolution of the relaxation time, temperature, bulk viscosity coefficient and comoving entropy of the dissipative cosmological fluid are obtained by assuming several bulk viscosity coefficient-relaxation time relations.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.subjectBulk Viscosityen_HK
dc.subjectCausal Thermodynamicsen_HK
dc.subjectDissipative Cosmologyen_HK
dc.titleDecelerating causal bulk viscous cosmological modelsen_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-s2.0-0034404988en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0034404988&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume9en_HK
dc.identifier.issue2en_HK
dc.identifier.spage97en_HK
dc.identifier.epage110en_HK

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats