International Journal of Theoretical Physics

, Volume 52, Issue 3, pp 765–778

Multi-Component Einstein–Cartan Cosmologies


DOI: 10.1007/s10773-012-1385-2

Cite this article as:
Galiakhmetov, A.M. Int J Theor Phys (2013) 52: 765. doi:10.1007/s10773-012-1385-2


Flat Friedmann universes filled by radiation, stiff fluid and a nonminimally coupled ghost scalar field with polynomial potentials of the fourth degree V(Φ) are investigated in the framework of the Einstein–Cartan theory. Exact solutions are obtained and analyzed for an arbitrary coupling constant ξ. It is shown that both singular and bouncing models with the late-time accelerated expansion are possible. A comparative analysis of the cosmological models with and without stiff fluid is carried out. The role of sources in the evolution of models is elucidated. Some conclusions from comparison of the presented results with other approaches in literature for accelerated expansion are made.


Einstein–Cartan theory Ghost scalar field Polynomial potentials of the fourth degree Radiation Stiff fluid Cosmology 

Copyright information

© Springer Science+Business Media New York 2012

Authors and Affiliations

  1. 1.Department of PhysicsDonetsk National Technical UniversityGorlovkaUkraine

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