On Anisotropic and Homogeneous Cosmological Models in the Renormalized Theory of Gravitation

Details On Anisotropic and Homogeneous Cosmological Models in the Renormalized Theory of Gravitation On Anisotropic and Homogeneous Cosmological Models in the Renormalized Theory of Gravitation

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pthph..60..403t&link_type=abstract

Progress of Theoretical Physics, Vol. 60, No. 2, pp. 403-413

Physics

14

Scientific paper

The evolution of anisotropic cosmological models of Bianchi type I in the renormalized theory of gravitation is investigated. Only the models which tend in the last expanding phase to those in the Einstein theory are considered. It is shown that the models with the bouncing point tb have always another extremal point te before tb and that, as the relative degree of anisotropy at tb increases, the interval of the contracting phase (te < t < tb) decreases and, if anisotropy becomes dynamically effective, the models have no contracting phase.

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