Behavior of Tsallis holographic dark energy for Marder universe

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dc.authoridAktaş, Can / 0000-0002-0603-7862
dc.contributor.authorAktaş, Can
dc.date.accessioned2025-01-27T20:23:03Z
dc.date.available2025-01-27T20:23:03Z
dc.date.issued2024
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this study, Tsallis holographic dark energy (THDE) was discussed within the frame of f(R,T) gravitational theory and considering the homogeneous and anisotropic Marder universe. The Hubble horizon was taken into consideration as infrared cutoff of the system. To get the field equations, solutions were used for the THDE density and the anisotropy parameter. Furthermore, a variety of physical parameters such as deceleration parameter, anisotropy parameter and volume have been examined. They have been also been visually examined with the help of graphics. Different values of deceleration parameter consistent with different observational data were mentioned. In addition to this, cosmological parameters like jerk, lerk and snap parameters were analyzed. Statefinder diagnostics which are helpful tools for the separation of dark energy models have been examined. By the calculation and representation of the overall density parameter (Omega) it can be concluded that the anisotropic nature of model vanishes showing a tendency to isotropy in accordance with present universe. Finally, the physical and geometrical nature of the model was studied, collating with relevant studies and observations.
dc.identifier.doi10.1142/S0217732324501049
dc.identifier.issn0217-7323
dc.identifier.issn1793-6632
dc.identifier.issue19N20
dc.identifier.scopus2-s2.0-85199211749
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1142/S0217732324501049
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22108
dc.identifier.volume39
dc.identifier.wosWOS:001279591600004
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofModern Physics Letters A
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectf ( R,T) theory
dc.subjectTsallis holographic dark energy
dc.subjectstatefinder diagnostics
dc.titleBehavior of Tsallis holographic dark energy for Marder universe
dc.typeArticle

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