2026-10-30T02:13:05Zhttps://munzur-rdlopen.rawdatalibrary.net/oai/request

oai:munzur-rdlopen.rawdatalibrary.net:munzur/29102026-10-28T15:30:13Zopenairecom_munzur_1col_munzur_2com_munzur_11col_munzur_162

Kaniadakis holographic dark energy with scalar field in Bianchi type-V universeKorunur, SibelBianchi type-V universeKaniadakis holographic dark energyscalar fieldsIn this work, considering anisotropic and homogeneous Bianchi type-V universe we investigated Kaniadakis holographic dark energy (KHDE). It is demonstrated that the equation of state (EoS) parameter has a transition from the quintessence era to the phantom era for the chosen model. Additionally, in the late time of the universe, EoS parameter behaves like a cosmological constant (Λ) with an IR (Infrared) cut-off apparent horizon in case of a particular form of deceleration parameter. We reconstructed correspondence between the KHDE and tachyon, quintessence and k-essence scalar fields. Also, our numerical solutions have been shown in graphs for EoS parameter and scalar fields.World Scientific2022Articlehttps://rdlopen.rawdatalibrary.net/r/munzur/2910https://doi.org/10.1142/s0217751x225021410217-751XenInternational Journal of Modern Physics Ainfo:eu-repo/semantics/closedAccessinfo:eu-repo/semantics/articlehttps://munzur-rdlopen.rawdatalibrary.net/tr/items/munzur/2910