Inflation and Singularity in Einstein-Cartan Theory
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摘要:
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.S2 -σ2 < 0), the Universe can not avoid singularity.If S2 - σ2 > -pv/2(pv is vacuum energy density), the Universe can undergo an inflation phase.Examples of Bianchi type-IX, I and V cosmological models are discussed.