Coupling q-Deformed Dark Energy to Dark Matter

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dc.authoridDil, Emre/0000-0002-9042-7694
dc.contributor.authorDil, Emre
dc.date.accessioned2025-03-23T19:30:51Z
dc.date.available2025-03-23T19:30:51Z
dc.date.issued2016
dc.departmentSinop Üniversitesi
dc.description.abstractWe propose a novel coupled dark energy model which is assumed to occur as a q-deformed scalar field and investigate whether it will provide an expanding universe phase. We consider the q-deformed dark energy as coupled to dark matter inhomogeneities. We performthe phase-space analysis of themodel by numericalmethods and find the late-time accelerated attractor solutions. The attractor solutions imply that the coupled q-deformed dark energy model is consistent with the conventional dark energy models satisfying an acceleration phase of universe. At the end, we compare the cosmological parameters of deformed and standard dark energy models and interpret the implications.
dc.identifier.doi10.1155/2016/9753208
dc.identifier.issn1687-7357
dc.identifier.issn1687-7365
dc.identifier.scopus2-s2.0-85003986548
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1155/2016/9753208
dc.identifier.urihttps://hdl.handle.net/11486/5179
dc.identifier.volume2016
dc.identifier.wosWOS:000389402500001
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.institutionauthorDil, Emre
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.subjectScalar Field
dc.subjectQuintom Cosmologies
dc.subjectParticle Creation
dc.subjectFixed-Points
dc.subjectDynamics
dc.subjectOscillators
dc.subjectModels
dc.subjectThermostatistics
dc.subjectStatistics
dc.titleCoupling q-Deformed Dark Energy to Dark Matter
dc.typeArticle

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