Research PaperNo Access

Çanakkale Onsekiz Mart University, School of Graduate Studies, Department of Mathematics, 17100 Çanakkale, Turkey

and

Sezgin Aygün

https://orcid.org/0000-0002-2969-4195

Çanakkale Onsekiz Mart University, Science Faculty, Department of Physics, 17100 Çanakkale, Turkey

E-mail Address: saygun@comu.edu.tr

Corresponding author.

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https://doi.org/10.1142/S0217732324500743Cited by:0 (Source: Crossref)

Abstract

In order to solve the mystery of the accelerating and expanding universe model first, various dark energy candidates, such as Quintessence, Tachyon, k-essence, Phantom and DBI-essence, were investigated in detail in the $f (Q)$ modified symmetric teleparallel gravitation theory for homogeneous and isotropic FRLW universe model. The $f (Q) = a Q^{n} + b$ model is used to obtain solutions in $f (Q)$ theory. Also, the physical behaviors of some cosmological parameters such as pressure and density were studied. Dark energy candidates were analyzed for different values of n with various graphs.

Keywords:

PACS: 04.50.+h, 04.20.Cv, 04.50.Kd

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