Abstract
The main purpose of this paper is to construct interacting and non-interacting Tsallis holographic dark energy models in an anisotropic and homogeneous Bianchi type-VI0 space time within the framework of a scalar tensor theory proposed by Saez and Ballester (1986). For this purpose, we use the relationship between metric potentials of the model and varying deceleration parameter to solve the Saez–Ballester field equations. In order to study the physical behavior of the models, we obtain some well-known cosmological parameters like deceleration, equation of state, statefinder, Om diagnostic parameters, and ωT - ωT′ planes of the models. Also, we observe that in our non-interacting and interacting models deceleration and equation of state parameters support the recent observational data.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
