Inflation in Bianchi models and cosmic no-hair theorem in Einstein-Cartan theory

摘要

We have examined cosmic no-hair theorem for anisotropic Bianchi-models in Einstein-Cartan theory and it is possible to have inflationary solution with a scalar field. It has been noted that during the inflationary era, the evolution of the Universe does not depend on the form of the potential but the late time behaviour is dependent on the potential for the inflation field. [References: 14]