Axially Symmetric Cosmological Mesonic Stiff Fluid Models in Lyra's Geometry

Abstract

In this paper, we obtained a new class of axially symmetric cosmological mesonic stiff fluid models in the context of Lyra's geometry. Expressions for the energy, pressure and the massless scalar field are derived by considering the time dependent displacement field. We found that the mesonic scalar field depends on only $t$ coordinate. Some physical properties of the obtained models are discussed.

13 pages, no figures, typos corrected

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