Cosmic evolutionary dynamics

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Definition

To explain what we see in the Universe, new hypotheses are needed. Here we propose a new vision: the Evolutionary Cosmological Model (ECM).

In this model, we can "easily" accommodate phenomena like the expansion of the cosmos and its acceleration in time (whatever they represent), the inconstancy of Hubble's Constant in space, as well as in time, the strange super homogeneity of CMB, the existence of well formed cosmic structures in the early Universe, just a few hundred millions years from the supposed birth date of the Universe. And it is not enough. There are rooms for a dark matter not made of particles, that does not need to reject or modify gravity, and the strange stuff we call dark energy, theoretically required to account for the acceleration of the cosmic expansion.

For the fundamental milestones of the Evolutionary Cosmological Model go to the page: Evolutionary Cosmological Model.

Common definition

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Description

See also

Links to the related sections of the TFNR Paper

Classification