Ghost scalar field dark energy models from an extended Kaluza-Klein perspective

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Özet

Reconstruction process of scalar field models (quintessence, tachyon, dilaton and K-essence), which can be performed by making use of some dark energy density definitions such as holographic, Ricci, new agegraphic and ghost types proposals, has been an interesting and very attractive area to many physicists in literature. In this work, in a five-dimensional framework, we establish a correspondence between the quintessence, tachyon and the dilaton type scalar field definitions and the generalized ghost dark energy model by considering the extended form of the Kaluza-Klein (EKK) gravity. Accordingly, we numerically study the associated equation of state parameters, as well as their kinetic energy and scalar potential terms.

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https://doi.org/10.1088/1361-6382/abe31eYayıncı resmi DOI adresi
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dc.contributor.authorKorunur, Murat
dc.date.accessioned2026-10-28T14:55:57.058450453Z
dc.date.available2026-10-28T14:55:57.058450453Z
dc.date.issued2021
dc.description.abstractReconstruction process of scalar field models (quintessence, tachyon, dilaton and K-essence), which can be performed by making use of some dark energy density definitions such as holographic, Ricci, new agegraphic and ghost types proposals, has been an interesting and very attractive area to many physicists in literature. In this work, in a five-dimensional framework, we establish a correspondence between the quintessence, tachyon and the dilaton type scalar field definitions and the generalized ghost dark energy model by considering the extended form of the Kaluza-Klein (EKK) gravity. Accordingly, we numerically study the associated equation of state parameters, as well as their kinetic energy and scalar potential terms.
dc.identifier.articlenumber075004
dc.identifier.doi10.1088/1361-6382/abe31e
dc.identifier.eissn1361-6382
dc.identifier.issn0264-9381
dc.identifier.issue7
dc.identifier.scopus2-s2.0-85102415730
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/munzur/2900
dc.identifier.volume38
dc.identifier.wosWOS:000622300700001
dc.language.isoen
dc.publisherIOP Publishing Ltd
dc.relation.ispartofClassical and Quantum Gravity
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectgeneralized ghost dark energy
dc.subjectKaluza-Klein cosmology
dc.subjectscalar field
dc.subject.classificationAstronomy & Astrophysics
dc.subject.classificationQuantum Science & Technology
dc.subject.classificationPhysics, Multidisciplinary
dc.subject.classificationPhysics, Particles & Fields
dc.subject.classificationPhysics
dc.subject.otherGALAXY REDSHIFT SURVEY
dc.subject.otherCOSMOLOGICAL CONSTANT
dc.subject.otherCHAPLYGIN-GAS
dc.subject.otherRECONSTRUCTION
dc.subject.otherUNIVERSE
dc.subject.otherQUINTESSENCE
dc.subject.otherANISOTROPY
dc.subject.otherEXPANSION
dc.subject.otherCOMPONENT
dc.subject.otherDYNAMICS
dc.titleGhost scalar field dark energy models from an extended Kaluza-Klein perspective
dc.typeArticle
rdl.citation.openalex6
rdl.citation.scopus5
rdl.citation.wos5
rdl.oa.statusclosed
rdl.scopus.quartileQ1
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)