Stability of the Einstein static Universe in the scalar-tensor theory of gravity
Stability of the Einstein static Universe in the scalar-tensor theory of gravity
复制标题
引力标量张量理论中爱因斯坦静态宇宙的稳定性
DOI:
10.1088/0264-9381/33/21/215011
复制
发表时间:
2016
影响因子:
3.5
通讯作者:
Yu Hongwei
中科院分区:
文献类型:
--
作者:
Miao Haitao;Wu Puxun;Yu Hongwei
In this paper, we study the viability of a singularity-free emergent scenario in the scalar–tensor theory of gravity by analyzing the stability of the Einstein static (ES) Universe. In order to obtain analytical results, we assume the perfect fluid which fills our Universe to be radiation or pressureless matter. We find that there are no stable ES solutions when scalar perturbations and tensor ones are considered together. Thus, in the scalar–tensor theory of gravity with a normal perfect fluid, such as radiation or pressureless matter, the emergent mechanism cannot be used to avoid the big bang singularity as the Universe cannot stay at the ES state past-eternally.