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Kaluza-Klein dark energy cosmological model in scale Co-variant Theory of Gravitation

机译:尺度协变引力理论中的Kaluza-Klein暗能量宇宙学模型

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A five dimensional Kaluza-Klein dark energy model with variable EoS parameter is investigated in the scale co-variant theory of gravitation proposed by Canuto et al. (in Phys. Rev. 39:429, 1977) in a five dimensional Kaluza-Klein space-time in the presence of perfect fluid source. Using the special law of variation for Hubble's parameter proposed by Berman (in Nuovo Cimento B 74:183, 1983), we have obtained a determinate solution which represents a dark energy cosmological model in the theory. We have also used the result that the scalar expansion is proportional to shear scalar of the space-time. It is observed that the EoS parameter, skewness parameter in the model turn out to be functions of cosmic time. Some physical and Kinematical properties of the model are also discussed.
机译:利用Canuto等人提出的尺度共变引力理论研究了具有可变EoS参数的五维Kaluza-Klein暗能量模型。 (在Phys。Rev. 39:429,1977)中,在存在完美流体源的五维Kaluza-Klein时空中。使用Berman提出的哈勃参数的特殊变化定律(在Nuovo Cimento B 74:183,1983),我们获得了一个确定的解,该解表示理论中的暗能量宇宙学模型。我们还使用了标量扩展与时空的剪切标量成比例的结果。可以看出,模型中的EoS参数,偏度参数是宇宙时间的函数。还讨论了模型的一些物理和运动学特性。

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