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Bouncing scenario in Brans–Dicke theory

Sunil Kumar Tripathy

http://orcid.org/0000-0001-5154-2297

Department of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, India

E-mail Address: tripathy_sunil@rediffmail.com

Corresponding author.

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Subingya Pandey

Department of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, India

E-mail Address: subingya16@gmail.com

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Alaka Priyadarsini Sendha

Department of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, India

E-mail Address: alakapriyadarsini.2014@gmail.com

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, and

Dipanjali Behera

Department of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, India

E-mail Address: dipadolly@rediffmail.com

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https://doi.org/10.1142/S0219887820500565Cited by:7 (Source: Crossref)

Abstract

A bouncing scenario is studied in the framework of generalized Brans–Dicke theory. In order to have a dark energy (DE) driven late time cosmic acceleration, we have considered a unified dark fluid simulated by a linear equation of state (EoS). The evolutionary behavior of the DE equation of parameter derived from the unified dark fluid has been discussed. The effect of the bouncing scale factor on the Brans–Dicke parameter, self-interacting potential and the Brans–Dicke scalar field is investigated.

Keywords:

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