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dc.contributor.authorMyrzakul, Aizhan
dc.contributor.authorGudekli, Ertan
dc.contributor.authorMYRZAKULOV, Ratbay
dc.date.accessioned2021-03-03T14:49:51Z
dc.date.available2021-03-03T14:49:51Z
dc.date.issued2015
dc.identifier.citationGudekli E., Myrzakul A., MYRZAKULOV R., "Teleparallelism by inhomogeneous dark fluid", ASTROPHYSICS AND SPACE SCIENCE, cilt.359, sa.2, 2015
dc.identifier.issn0004-640X
dc.identifier.otherav_3bb17833-c747-40b1-bcc5-c51436dd3e30
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/44079
dc.identifier.urihttps://doi.org/10.1007/s10509-015-2515-0
dc.description.abstractIn this paper, we investigate f (T) cosmology and find an exact solution for f which gives a Little Rip cosmology. Also, considering accelerating cosmology with dark matter, the time-dependent solution is found. For these cases, by using solutions obtained from f (T) gravity we find expressions for. and. defined as time functions via equivalent description in terms of inhomogeneous fluid. This puts the question: which theoretical model describes the observational cosmology?
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleTeleparallelism by inhomogeneous dark fluid
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.departmentL.N. Gumilyov Eurasian National University , ,
dc.identifier.volume359
dc.identifier.issue2
dc.contributor.firstauthorID64749


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