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dc.rights.licensehttp://creativecommons.org/licenses/by-nc-sa/3.0/ve/
dc.contributor.authorHerrera, L.es_VE
dc.contributor.authorBarreto Acevedo, Willianses_VE
dc.date2005-08-18es_VE
dc.date.accessioned2005-08-18T09:00:00Z
dc.date.available2005-08-18T09:00:00Z
dc.date.created2003-09-09es_VE
dc.date.issued2005-08-18T09:00:00Zes_VE
dc.identifier.otherT016300002250/0es_VE
dc.identifier.urihttp://www.saber.ula.ve/handle/123456789/16750
dc.description.abstractEvolution of relativistic polytropes in the post-quasi-static regime. (Herrera, L.; Barreto Acevedo, Willians.) Abstract A recently presented method for the study of evolving self-gravitating relativistic spheres is applied to the description of the evolution of rela- tivistic polytropes. Two different definitions of relativistic polytrope, yielding the same Newtonian limit, are considered. Some examples are explicitly worked out, describing collapsing polytropes and bring- ing out the differences between both types of polytropes.es_VE
dc.language.isoeses_VE
dc.publisherSABER ULAes_VE
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectGrupo de Física Teóricaes_VE
dc.titleEvolution of relativistic polytropes in the post-quasi-static regime.es_VE
dc.typeinfo:eu-repo/semantics/article
dc.description.emaillaherrera@telcel.net.vees_VE
dc.description.emailwbarreto@ula.vees_VE
dc.description.tiponivelNivel monográficoes_VE
dc.subject.departamentoDepartamento de Físicaes_VE
dc.subject.facultadFacultad de Ciencias.es_VE
dc.subject.institucionUniversidad Central de Venezuela (UCV)es_VE
dc.subject.keywordsRelativistic polytropeses_VE
dc.subject.keywordsPost-quasi-static regimees_VE
dc.subject.tipoArtículoses_VE


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