# Two Fluid Scenario in Bianchi Type-I Universe

## TL;DR

This study analyzes a Bianchi type-I universe model with barotropic and dark energy fluids, estimating key cosmological parameters using observational data, and finds results consistent with Planck and recent studies.

## Contribution

It provides a statistical estimation of cosmological parameters in a Bianchi type-I universe with dark energy using multiple observational datasets, confirming consistency with established results.

## Key findings

- Results agree with Planck 2016 data
- Estimated cosmological parameters using H(z) and supernova data
- Investigated physical properties like universe age and deceleration parameter

## Abstract

In this paper, we study a Bianchi type -I model of universe filled with barotropic and dark energy(DE) type fluids. The present values of cosmological parameters such as Hubble constant $H_0$, barotropic, DE and anisotropy energy parameters $(\Omega_{m})_0$, $(\Omega_{de})_0$ and $(\Omega_{\sigma})_0 $ and Equation of State(EoS) parameter for DE ($\omega_{de}$) are statistically estimated in two ways by taking 38 point data set of Hubble parameter H(z) and 581 point data set of distance modulus of supernovae in the range $0\leq z \leq 1.414$. It is found that the results agree with the Planck result [P.A.R. Ade, et al., Astron. Astrophys. 594 A14 (2016)] and more latest result obtained by Amirhashchi and Amirhashchi [H. Amirhashchi and S. Amirhashchi, arXiv:1811.05400v4 (2019)]. Various physical properties such as age of the universe, deceleration parameter etc have also been investigated.