Anisotropic Bianchi type-VI0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$VI_{0}$$\end{document} wet dark fluid cosmological models in Lyra’s manifoldAnisotropic Bianchi type-VI0H A Nimkar and M R Ugale

In this paper, we have Studied wet dark fluid cosmological model in the frame work of Lyra’s manifold in anisotropic Bianchi Type VI0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$VI_{0}$$\end{document} space time. To obtain the deterministic solution of field equation, we are using a power law, i.e. relation between metric potential A=Bn.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$A={B}^{n}.$$\end{document} Stability of the obtained model is discussed with the help of sound speed. Also, we have study some observational parameters such as deceleration parameter, jerk parameter and redshift of the obtaining model. Some physical and kinematical properties of the models are discussed.