Inflation and Singularity in Einstein–Cartan Theory
1 School of Science, Huaihai Institute of Technology, Lianyungang 222005
2 Department of Physics, Shanghai Normal University, Shanghai 200234
3 Department of Physics, Shanghai University, Shanghai 200444
4 The Shanghai Key Lab of Astrophysics, Shanghai Normal University, Shanghai 200234
Received Date:
October 07, 2010
Published Date:
January 31, 2011
Abstract
Within the framework of Einstein–Cartan theory, we obtain a general condition leading to singularity and inflation for all Bianchi cosmological models. If the spin energy is smaller than anisotropic energy density (i.e. S 2 −σ 2 ≤0), the Universe can not avoid singularity. If S 2 −σ 2 >-ρv /2 (ρv is vacuum energy density), the Universe can undergo an inflation phase. Examples of Bianchi type−IX, I and V cosmological models are discussed.
Article Text
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About This Article
Cite this article:
HUANG Zeng-Guang, FANG Wei, LU Hui-Qing. Inflation and Singularity in Einstein–Cartan Theory[J].
Chin. Phys. Lett. , 2011, 28(2): 029802.
DOI: 10.1088/0256-307X/28/2/029802
HUANG Zeng-Guang, FANG Wei, LU Hui-Qing. Inflation and Singularity in Einstein–Cartan Theory[J]. Chin. Phys. Lett. , 2011, 28(2): 029802. DOI: 10.1088/0256-307X/28/2/029802