Dynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis

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dc.authoridDil, Emre/0000-0002-9042-7694
dc.authoridkolay, erdinc/0000-0001-7436-3152
dc.contributor.authorDil, Emre
dc.contributor.authorKolay, Erdinc
dc.date.accessioned2025-03-23T19:30:59Z
dc.date.available2025-03-23T19:30:59Z
dc.date.issued2015
dc.departmentSinop Üniversitesi
dc.description.abstractWe consider a novel dark energy model to investigate whether it will provide an expanding universe phase. Here we propose a mixed dark energy domination which is constituted by tachyon, quintessence, and phantom scalar fields nonminimally coupled to gravity, in the absence of background dark matter and baryonic matter, in the framework of teleparallel gravity. We perform the phase-space analysis of the model by numerical methods and find the late-time accelerated attractor solutions implying the acceleration phase of universe.
dc.identifier.doi10.1155/2015/608252
dc.identifier.issn1687-7357
dc.identifier.issn1687-7365
dc.identifier.scopus2-s2.0-84956940797
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1155/2015/608252
dc.identifier.urihttps://hdl.handle.net/11486/5185
dc.identifier.volume2015
dc.identifier.wosWOS:000367926400001
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherHindawi Ltd
dc.relation.ispartofAdvances in High Energy Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WOS_20250323
dc.subjectProbe Wmap Observations
dc.subjectCosmological-Constant
dc.subjectQuintom Cosmologies
dc.subjectFixed-Points
dc.subjectModels
dc.subjectPhantom
dc.subjectEvolution
dc.subjectLambda
dc.subjectField
dc.subjectOmega
dc.titleDynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis
dc.typeArticle

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