Erkan, SevdaPirinccioglu, NurettinSalti, MustafaAydogdu, Oktay2024-04-242024-04-2420172190-5444https://doi.org/10.1140/epjp/i2017-11795-xhttps://hdl.handle.net/11468/17821Making 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.eninfo:eu-repo/semantics/closedAccess[No Keyword]Article13212WOS:0004186135000012-s2.0-8503904451110.1140/epjp/i2017-11795-xQ1Q2