Rotating Cosmological Models of Bianchi Type V

Details Rotating Cosmological Models of Bianchi Type V Rotating Cosmological Models of Bianchi Type V

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1957b&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

Cosmological models of Bianchi type V are investigated using a tetrad approach based on Cartan's invariant description of spacetimes. The system can be reduced to an integrable system of five first order ordinary differential equations, suitable for perturbative and numerical calculations. The general solution is tilted and describes a fluid with shear and vorticity. We then solve the linearized equations around the open Friedmann universe. The full system is also studied numerically and the perturbative solutions agree well with the numerical ones in the appropriate domains.

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