English

A Non-Linear Type Equation of State and Cosmic Fluid Dynamics

General Relativity and Quantum Cosmology 2023-04-14 v1

Abstract

In this chapter we have introduced a special type of non-linear equation of state to discuss the cosmological evolution mechanism. The new equation of state is a four parameters model which can be represented as p=Aρ+Bρ2Cραp=A\rho+B\rho^2-\frac{C}{\rho^{\alpha}} where B=AβγB=A\beta-\gamma. The evolution of universe have been interpreted by fluid dynamics. The reconstruction of Chaplygin gas and Van-Der-Waals (VDW) fluid equation of states have been done from the parametric analysis of this new non-linear model. Different cosmological phases like Quintom, Quintessence and warm universe have been discussed here. Finally, we have provided a comparative studies of this model with other non-linear fluid solutions.

Keywords

Cite

@article{arxiv.2304.06481,
  title  = {A Non-Linear Type Equation of State and Cosmic Fluid Dynamics},
  author = {Shouvik Sadhukhan and Alokananda Kar and Surajit Chattopadhyay},
  journal= {arXiv preprint arXiv:2304.06481},
  year   = {2023}
}