Nonlinear Spinor Fields and its role in Cosmology
arXiv:1103.2890 · doi:10.1007/s10773-011-1059-5
Abstract
Different characteristic of matter influencing the evolution of the Universe has been simulated by means of a nonlinear spinor field. Exploiting the spinor description of perfect fluid and dark energy evolution of the Universe given by an anisotropic Bianchi type-VI, VI, V, III, I or isotropic Friedmann-Robertson-Walker (FRW) one has been studied. It is shown that due to some restrictions on metric functions, initial anisotropy in the models Bianchi type-VI, VI, V and III does not die away, while the anisotropic Bianchi type-I models evolves into the isotropic one.
22 pages, 12 Figures
References in corpus (5)
Cited by in corpus (19)
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