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Bianchi Type-I Universe in Lyra Manifold with Quadratic Equation of State

机译:Bianchi Type-I Universe在Lyra歧管中具有二次方程的状态

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In this study, we have solved Einstein field equations for Bianchi type I universe model in Lyra manifold with quadratic equation of state (EoS) p = αρ(t)~2 - ρ(t). Where α ≠0 is an important constant. Cosmic pressure, density and displacement vector (β~2) are related with α constant. In this study β~2 is a decreasing function of time and behaves like a cosmological constant. These solutions agree with the studies of Halford, Pradhan and Singh, Aygun et al., Agarwal et al., Yadav and Haque as well as SN I_a observations.
机译:在这项研究中,我们在Lyra歧管中解决了Bianchi Iniverse模型的爱因斯坦野外方程,具有正状态(EOS)P =αρ(t)〜2 - ρ(t)的二次方程。其中α10是重要的常数。宇宙压力,密度和位移载体(β〜2)与α常数有关。在该研究中,β〜2是时间的降低,表现得像宇宙常数。这些解决方案与半月,Pradhan和Singh,Aygun等人,Agarwal等人的研究一致。,Yadav和Haque以及Sn I_a观察。

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