Difference between revisions of "Cosmic evolutionary dynamics"
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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. | 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]]. | |
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== Common definition == | == Common definition == | ||
Revision as of 20:55, 8 December 2021
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
Links to Wikipedia pages:
Description
See also
- TFNR - 2.13 The cosmic evolution
- TFNR - 2.13 Some astrophysical and cosmological phenomena
- TFNR - 2.13 The dynamics of the cosmic feedback
- TFNR - 2.13 What doesn’t work in the Standard Model of Cosmology
- TFNR - 2.13 Who needs a Big Bang?
- TFNR - 2.13 Who needs a Cosmic Inflation?
- TFNR - 2.13 No Big Bang and Inflation: an incessant creation and evolution
- TFNR - 2.13 The beginning of the Universe
- TFNR - 2.13 The formation and the evolution of the Universe
- TFNR - 10. The Forms and the Universe
- TFNR - 10.2 The Universe of the Forms
- TFNR - 10.2.1 The origin and evolution of the Universe
- TFNR - 10.2.2 Dynamics of the cosmos
- TFNR - 10.2.3 Objects and structures in the cosmos
- TFNR - 10.3 A brief history of the Universe
Classification
- Topic id: t_cosmo_ev_dyna
- Belongs to the class: Dynamics of the Forms
- Has as instances:
- Belongs to the groups:
- Semantic Map: ekm|map=m_ph_dynamics&topic=t_cosmo_ev_dyna
- Semantic Map Test Version: ekmt|map=m_ph_dynamics&topic=t_cosmo_ev_dyna
