Holographic scalar fields in Kaluza-Klein framework
dc.contributor.author | Erkan, Sevda | |
dc.contributor.author | Pirinccioglu, Nurettin | |
dc.contributor.author | Salti, Mustafa | |
dc.contributor.author | Aydogdu, Oktay | |
dc.date.accessioned | 2024-04-24T17:12:01Z | |
dc.date.available | 2024-04-24T17:12:01Z | |
dc.date.issued | 2017 | |
dc.department | Dicle Üniversitesi | en_US |
dc.description.abstract | Making use of the Friedmann-Robertson-Walker (FRW) type Kaluza-Klein universe (KKU), we discuss the holographic dark energy density (HDED) in order to develop its correspondence with some scalar field descriptions such as the tachyon, quintessence, DBI-essence, dilaton and the k-essence. It is concluded that the Kaluza-Klein-type HDED proposal becomes stable throughout the history of our universe and is consistent with the current status of the universe. Next, we obtain the exact solutions of self-interacting potential and scalar field function for the selected models. | en_US |
dc.identifier.doi | 10.1140/epjp/i2017-11795-x | |
dc.identifier.issn | 2190-5444 | |
dc.identifier.issue | 12 | en_US |
dc.identifier.scopus | 2-s2.0-85039044511 | |
dc.identifier.scopusquality | Q1 | |
dc.identifier.uri | https://doi.org/10.1140/epjp/i2017-11795-x | |
dc.identifier.uri | https://hdl.handle.net/11468/17821 | |
dc.identifier.volume | 132 | en_US |
dc.identifier.wos | WOS:000418613500001 | |
dc.identifier.wosquality | Q2 | |
dc.indekslendigikaynak | Web of Science | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | en_US |
dc.publisher | Springer Heidelberg | en_US |
dc.relation.ispartof | European Physical Journal Plus | |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/closedAccess | en_US |
dc.subject | [No Keyword] | en_US |
dc.title | Holographic scalar fields in Kaluza-Klein framework | en_US |
dc.title | Holographic scalar fields in Kaluza-Klein framework | |
dc.type | Article | en_US |