2026-10-29T21:50:15Zhttps://munzur-rdlopen.rawdatalibrary.net/oai/request

oai:munzur-rdlopen.rawdatalibrary.net:munzur/38152026-10-28T15:47:40Zopenairecom_munzur_1col_munzur_2com_munzur_11col_munzur_162

Tsallis holographic dark energy in Bianchi type-III spacetime with scalar fieldsKorunur, MuratBianchi type-III spacetimescalar fieldsTsallis holographic dark energyIn this paper, we study one of the new dark energy models named Tsallis holographic dark energy (THDE) model considering the Bianchi type-III spacetime model. Considering deceleration parameter, transition from deceleration to acceleration phase happens at z = 0.256. The equation of state (EoS) parameter has been found using the Granda-Oliveros (GO) scale. It is found that for > 2 values, EoS parameter behaves like the quintessence era; for < 2, EoS parameter behaves like the phantom dark energy and approaches CDM model at late-time cosmic acceleration phase. Also, we reconstructed a correspondence between THDE model and some well-known scalar fields, such as tachyon, quintessence and K-essence. In addition, we evaluated equation of state parameter, kinetic energy and scalar potential versus time.World Scientific Publishing Co. Pte Ltd2019Articlehttps://rdlopen.rawdatalibrary.net/r/munzur/3815https://doi.org/10.1142/s02177323195031030217-7323enModern Physics Letters Ainfo:eu-repo/semantics/closedAccessinfo:eu-repo/semantics/articlehttps://munzur-rdlopen.rawdatalibrary.net/tr/items/munzur/3815