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

概要

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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 t_b increases, the interval of the contracting phase (t_e < t< t_b) decreases and, if anisotropy becomes dynamically effective, the models have no contracting phase.
理論物理学刊行会の論文
1978-08-25

著者

TOMITA Kenji
Research Institute for Theoretical Physics Hiroshima University
Nariai Hidekazu
Research Institute For Theoretical Physics Hiroshima Unicersity
Azuma Takahiro
Research Division Hokuriku Seiyaku Co. Ltd.
Azuma Takahiro
Research Institute For Theoretical Physics Hiroshima University
Nariai Hidekazu
Research Institute For Theorerical Physics Hiroshima University
AZUMA Takahiro
Department of Mathematics, King's College London

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

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