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dc.contributor.authorAKDENIZ, KG
dc.contributor.authorRIZAOGLU, E
dc.contributor.authorARIK, M
dc.date.accessioned2021-03-04T07:58:18Z
dc.date.available2021-03-04T07:58:18Z
dc.date.issued1994
dc.identifier.citationAKDENIZ K., ARIK M., RIZAOGLU E., "COASTING BIG-BANG", PHYSICS LETTERS B, cilt.321, sa.4, ss.329-332, 1994
dc.identifier.issn0370-2693
dc.identifier.otherav_60d7ed4b-533f-4551-a57b-2270f0bda390
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/67562
dc.identifier.urihttps://doi.org/10.1016/0370-2693(94)90251-8
dc.description.abstractWe consider a cosmological model in which the early universe is dominated by the equation of state p = -rho/3 corresponding to a coasting cosmology. This equation of state was first obtained in the context of cosmic string theories whereas its one-parameter generalization describing a coasting early universe followed by a radiation-dominated universe was first derived from Kaluza-Klein theories based on Euler form actions. We show that in such a model the temperature is almost absolute zero at the beginning and the universe quickly heats up to maximum temperature.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectAstronomi ve Astrofizik
dc.subjectFİZİK, NÜKLEER
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleCOASTING BIG-BANG
dc.typeMakale
dc.relation.journalPHYSICS LETTERS B
dc.contributor.department, ,
dc.identifier.volume321
dc.identifier.issue4
dc.identifier.startpage329
dc.identifier.endpage332
dc.contributor.firstauthorID115054


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