摘要
首先讨论一个具有状态方程ρ=Kp的理想流体内部高维非均匀时空的演化,然后对流体的自旋及角速度作一些假定,讨论各种情况下的高维宇宙暴涨解.
The evolution of the inhomogeneous spacetime inside an ideal fluid with the state equation ρ=Kp is reviewed. Some special assumptions about the spin and angular velocity of the fluid are made and various inflational solutions for higher-dimensional universe with spinning matter are discussed.
出处
《华中理工大学学报》
CSCD
北大核心
1993年第5期152-154,共3页
Journal of Huazhong University of Science and Technology
关键词
宇宙暴涨
非均匀时空
高维
inflation of higher-dimensional universe
inhomogeneous spacetime
Szekeres-Ⅱ type metric