Difference between revisions of "Evolutionary Cosmological Model"

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== Definition ==
 
== Definition ==
 
{{Def-en|1={{PAGENAME}}}}
 
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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.
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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.  
  
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== Common definition  ==
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And it is not enough. There are rooms for a [[Dark matter]] not made of [[Particles]], that does not need to reject or modify [[Mass|gravity]], and the strange stuff we call [[Dark energy]], theoretically required to account for the acceleration of the cosmic expansion.
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Links to the Wikipedia page: [https://en.wikipedia.org/wiki/Cosmology Cosmology], [https://en.wikipedia.org/wiki/Physical_cosmology Physical cosmology], [https://en.wikipedia.org/wiki/Lambda-CDM_model Lambda-CDM model]
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== Description ==
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The '''fundamental milestones of the Evolutionary Cosmological Model''' are the following:
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The '''fundamental milestones of the Evolutionary Cosmological Model''' are:
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*The Universe is the section of Reality we call the present
 
*The Universe is the section of Reality we call the present
 
*The Universe is older, larger and more complex than we think
 
*The Universe is older, larger and more complex than we think
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*Cosmic expansion as an effect of the rising complexity of Reality
 
*Cosmic expansion as an effect of the rising complexity of Reality
 
*The Hubble constant is not constant, neither in space nor in time
 
*The Hubble constant is not constant, neither in space nor in time
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== Common definition  ==
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{{WpPages}}
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*[https://en.wikipedia.org/wiki/Cosmology Cosmology]
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*[https://en.wikipedia.org/wiki/Physical_cosmology Physical cosmology]
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*[https://en.wikipedia.org/wiki/Lambda-CDM_model Lambda-CDM model]
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== Description ==
  
 
=== Origin ===
 
=== Origin ===
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== See also ==
 
== See also ==
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*[[Dynamics of Physical Forms]]
 
*[[Universe]]
 
*[[Universe]]
 
*[[Physical Universe]]
 
*[[Physical Universe]]
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*[[Cosmological vision]]
 
*[[Cosmological vision]]
 
*[[Cosmic evolutionary dynamics]]
 
*[[Cosmic evolutionary dynamics]]
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*[[Evolutionary Cosmological Model]]
 
  
 
{{Template:LinksToTFNR}}
 
{{Template:LinksToTFNR}}
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*[[TFNR - 1.4 Very important hypotheses about Reality]]
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*[[TFNR - The cosmic evolution]]
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*[[TFNR - Some astrophysical and cosmological phenomena]]
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*[[TFNR - The dynamics of the cosmic feedback]]
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*[[TFNR - What doesn’t work in the Standard Model of Cosmology]]
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*[[TFNR - Who needs a Big Bang?]]
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*[[TFNR - Who needs a Cosmic Inflation?]]
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*[[TFNR - No Big Bang and Inflation: an incessant creation and evolution]]
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*[[TFNR - The beginning of the Universe]]
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*[[TFNR - The formation and the evolution of the Universe]]
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*[[TFNR - The Forms and the Universe]]
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*[[TFNR - The Universe of the Forms]]
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*[[TFNR - The origin and evolution of the Universe]]
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*[[TFNR - Dynamics of the cosmos]]
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*[[TFNR - Objects and structures in the cosmos]]
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*[[TFNR - A brief history of the Universe]]
 
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Latest revision as of 21:03, 8 December 2021

Definition

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.

The fundamental milestones of the Evolutionary Cosmological Model are the following:

  • The Universe is the section of Reality we call the present
  • The Universe is older, larger and more complex than we think
  • The Universe is unlimited: no limits in cause, space and time. No limits at all
  • Only one Universe is needed, not many or an infinite number
  • The Universe as a whole is inherently flat
  • No singularities: neither in the case of the Big Bang, nor in Black Holes
  • At the largest scales, the cosmos is substantially homogeneous
  • Inhomogeneity and anisotropies "are" the cosmic structures (especially dark structures) that give shape to the Universe and determine its evolution
  • The dark side of the Universe is a causal and variational (spatial and temporal) precursor of the visible side
  • Dark matter is not made of particles
  • Dark energy as anti-mass (or positive mass density)
  • Mass can be positive and negative (dark/ordinary matter and dark energy create an actraction and repulsion gravitational cosmic dance)
  • Ordinary matter (and antimatter) forms from the dynamics of dark matter/dark energy structures (galaxies and clusters/super clusters dark halos)
  • The cosmos has a gravitational, kinetic, electric and magnetic structure (hardly visible, if not completely invisible)
  • The Cosmic Web is the 3D structure of the Universe
  • Cosmic expansion as an effect of the rising complexity of Reality
  • The Hubble constant is not constant, neither in space nor in time

Common definition

Links to Wikipedia pages:

Description

Origin

Evolution

Shape

Structures

See also

Links to the related sections of the TFNR Paper

Classification

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