Bianchi type VI0 cosmological model in self-creation theory in general relativity and Lyra geometry

被引:0
|
作者
Hegazy, E. A. [1 ]
Rahaman, F. [2 ]
机构
[1] Menia Univ, Fac Sci, Math Dept, El Minia 61519, Egypt
[2] Jadavpur Univ, Dept Math, Kolkata 700032, W Bengal, India
关键词
Lyra geometry; Einstein field equations; Bianchi type VI0 cosmological models; Self-creation theory; Scalar expansion; Entropy; ISOTROPY;
D O I
10.1007/s12648-019-01424-8
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this paper, we show that no solutions exist for Bianchi type VI0 cosmological model in the modified gravity theories, namely in self-creation theory and in gravity theory based on Lyra geometry under the two physical conditions: The pressure p and the density rho of the fluid are related by the equation of state p=lambda rho,0 <=lambda <= 1,and the scalar expansion Theta of the cosmological model is proportional to the eigenvalue sigma 33 of the shear tensor. In self-creation theory, only the possible solutions are found for dust and radiation cases. Physical and geometrical properties of the obtained models are discussed for different cases of matter distribution. Also, we study the effect of the scalar field phi on the entropy S of our universe with an expression for the entropy for all different cases of matter distribution. Also we have proved that the Lyra term has no effect on the entropy of the universe.
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页码:1643 / 1650
页数:8
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