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Extended Holographic Ricci Dark Energy in Chameleon Brans-Dicke Cosmology
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In the present work, we have studied some features of the generalized Brans-Dicke (BD) model in which the scalar field is allowed to couple nonminimally with the matter sector. Extended holographic Ricci dark energy (EHRDE) has been considered in the above framework
of BD cosmology. Some restrictions have been derived for the BD parameter ω, and a stronger matter-chameleon coupling has been observed with the expansion of the universe. In this framework, the equation of the state parameter of EHRDE has behaved like quintom. Also, we have reconstructed the potential and coupling function for BD model for the EHRDE. It has been observed that the potential function is increasing as the matter-chameleon coupling is getting stronger.
Title: Extended Holographic Ricci Dark Energy in Chameleon Brans-Dicke Cosmology
Description:
In the present work, we have studied some features of the generalized Brans-Dicke (BD) model in which the scalar field is allowed to couple nonminimally with the matter sector.
Extended holographic Ricci dark energy (EHRDE) has been considered in the above framework
of BD cosmology.
Some restrictions have been derived for the BD parameter ω, and a stronger matter-chameleon coupling has been observed with the expansion of the universe.
In this framework, the equation of the state parameter of EHRDE has behaved like quintom.
Also, we have reconstructed the potential and coupling function for BD model for the EHRDE.
It has been observed that the potential function is increasing as the matter-chameleon coupling is getting stronger.
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