科研之友
微信
新浪微博
Facebook
分享链接
摘要
We have studied the Hoyle-Narlikar C-field cosmology with N-dimensional Kaluza-Klein space-time. Using methods of Narlikar and Padmanabham (1985), the solutions have been studied when the Hoyle-Narlikar creation field C is a function of time t (non-static case) only. The geometrical and physical aspects for models are also studied. Further, we have shown that our model admits a solution with a decelerating phase in the early era followed by an accelerated expansion. This is in conformity with the present day observational status for dark energy.
- 出版日期2010-12
