Extended Ricci and holographic dark energy models in fractal cosmology

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dc.contributor.authorSalti, M.
dc.contributor.authorKorunur, M.
dc.contributor.authorAcikgoz, I.
dc.date.accessioned2024-04-24T17:12:01Z
dc.date.available2024-04-24T17:12:01Z
dc.date.issued2014
dc.departmentDicle Üniversitesien_US
dc.description.abstractWe consider the fractal Friedmann-Robertson-Walker universe filled with dark fluid. By making use of this assumption, we discuss two types of dark energy models: Generalized Ricci and generalized holographic dark energies. We calculate the equation-of-state parameters, investigate some special limits of the results and discuss the physical implications via graphs. Also, we reconstruct the potential and the dynamics of the quintessence and k-essence (kinetic-quintessence) according to the results obtained for the fractal dark energy.en_US
dc.identifier.doi10.1140/epjp/i2014-14095-1
dc.identifier.issn2190-5444
dc.identifier.issue5en_US
dc.identifier.scopus2-s2.0-84922575923
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjp/i2014-14095-1
dc.identifier.urihttps://hdl.handle.net/11468/17819
dc.identifier.volume129en_US
dc.identifier.wosWOS:000337272600001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoenen_US
dc.publisherSpringer Heidelbergen_US
dc.relation.ispartofEuropean Physical Journal Plus
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subject[No Keyword]en_US
dc.titleExtended Ricci and holographic dark energy models in fractal cosmologyen_US
dc.titleExtended Ricci and holographic dark energy models in fractal cosmology
dc.typeArticleen_US

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