The Simplest Parametrization of the Equation of State Parameter in the Scalar Field Universe

Author:

Shrivastava Preeti12,Khan Abdul Junaid1,Kumar Mukesh3,Goswami Gopikant4,Singh Jainendra Kumar5ORCID,Yadav Anil Kumar6ORCID

Affiliation:

1. Department of Mathematics, MATS University, Raipur 490006, India

2. Department of Mathematics, Shri Shankaracharya, Mahavidyalaya, Bhilai 490006, India

3. Department of Mathematics, GLA University, Mathura 281406, India

4. Department of Mathematics, Kalyan P. G. College, Bhilai 490006, India

5. Department of Mathematics, Netaji Subhas University of Technology, Delhi 110078, India

6. Department of Physics, United College of Engineering and Research, Greater Noida 201306, India

Abstract

In this paper, we investigate a scalar field cosmological model of accelerating Universe with the simplest parametrization of the equation of state parameter of the scalar field. We use H(z) data, pantheon compilation of SN Ia data and BAO data to constrain the model parameters using the χ2 minimization technique. We obtain the present values of Hubble constant H0 as 66.2−1.34+1.42, 70.7−0.31+0.32 and 67.74−1.04+1.24 for H(z), H(z) + Pantheon and H(z) + BAO respectively. In addition, we estimate the present age of the Universe in a derived model t0=14.38−0.64+0.63 for joint H(z) and pantheon compilation of SN Ia data which has only 0.88σ tension with its empirical value obtained in Plank collaboration. Moreover, the present values of the deceleration parameter q0 come out to be −0.55−0.038+0.031, −0.61−0.021+0.030 and −0.627−0.025+0.022 by bounding the Universe in the derived model with H(z), H(z) + Pantheon compilation of SN Ia and H(z) + BAO data sets, respectively. We also have performed the state-finder diagnostics to discover the nature of dark energy.

Publisher

MDPI AG

Subject

Astronomy and Astrophysics

Reference112 articles.

1. Some Bianchi type V models of accelerating universe with dark energy;Kumar;Mod. Phys. Lett. A,2011

2. Some anisotropic dark energy models in Bianchi type-V space-time;Yadav;Astrophys. Space Sc.,2011

3. A transitioning universe with anisotropic dark energy;Yadav;Astrophys. Space Sc.,2016

4. Probing kinematics and fate of Bianchi type V Universe;Goswami;Mod. Phys. Lett. A,2020

5. Interacting Dark Sectors in Anisotropic Universe: Observational Constraints and H0 Tension;Amirhashchi;Phys. Dark Uni.,2022

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