Linear perturbations on the cosmological background in the relativistic theory of gravitation: II. Appendix

For the flat FLRW model of Universe evolution in RTG a new model of Dark Energy is proposed. It is a global scalar field Φ with the quadratic potential. It ensures cosmological acceleration at the present time and a bounce at the latе times. At the contraction stage Kazner-like growing anisotropy of Riemannian metrics will break a mass-of- the-graviton bounce mechanism near the Big Bang in FLRW case. There is also noncyclic option, when small enough graviton-mass-terms are significant only at the end of expansion. After bounce, during next contraction epoch, an anisotropy grows and the matter density finally reaches the Planck one.

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Linear perturbations on the cosmological background in the relativistic theory of gravitation: II. Appendix

Cited by 3 publications

References 7 publications

The Evolution of Homogeneous and Isotropic Universe in the Relativistic Theory of Gravitation

The Evolution of Homogeneous and Isotropic Universe in the Relativistic Theory of Gravitation

Is the Cyclic Model of the Universe Possible in the Relativistic Theory of Gravitation?

Is the Cyclic Model of the Universe Possible in the Relativistic Theory of Gravitation?

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