Up to date theories of the universe evolution
The first tree minutes of the Universe
Cosmology represents the science about the world (Pythagoras: cosmos=world; Logos=science). Its purpose is that of studying the entire material universe. In Aristotel cosmology was already categorized as a branch of physics. One of the possible theories about the origin of the universe is still found in the Greek philosophies in the principal of Platon’s “geouniverse”: “One created the world and the human”. After putting this principle to use, Platon was considered as one of the supporters of the biblical principle of determined genesis.
Science opposes, using the same principle (being the closest to the creator principle), the atrophic principle. This principle says that the Universe we live in didn’t appear after a creational act, but as a random result of some consequences initially arbitrary, randomly. Using this principle demonstrates that the apparition of life in a Universe depends on a small number of parameters and of real close variables of does parameters. This principle demonstrates that the chance of a universe that lets life appear is quite small. In the same time the intervals in which these parameters can vary make the number of possible universes (for life appearance) to be infinite. This demonstrates that there can be a infinity of universes that are the same, still different in their structure, which allow life apparel. The problem was treated a few centuries before, before Platen by a Greek philosopher, Anaximandrus. In such a multiuniverse, the creationist principle represents just one of the possibilities. Due to the limited speed of the speed of light, our initial universe (t>0), was formed of ~10**75 causal distinct zones. This indicates the fact that, walking towards its beginning, the universe loses its property of global causality. In present this science holds proof of an evolving process of the universe we live in. This process, looking back in time, is of a thermical type, starting from a initial state, with high temperatures and low reach, in which deterministic physics doesn’t act, it being replaced by the principles of cuantic relativist physics. At high temperatures, the forces tend to unify: first the electromagnetic one with the weak one, then with the strong one, and at last with he gravitational one. The universe, in it’s cuantic state, is small enough for it’s reach to become a huge black hole. The first 3 minutes of the universe Today the most accepted cosmonological theory is the universe in expansion one, starting from a primordial explosion, called Big Bang. We can consider our universe of being one of infinity of similar gigantic systems and that it has the following genesis. For a unimaginable small fraction of a second, matter was in a supradimentional shape, which had 3+1+N dimensions. With a topological faze transition, the N dimensions of matter take themselves apart from the space dimensions and time, eventually creating the apparition of a scalar field, wielded with a fantastic quantity of information, stocked under the shape of groups of mathematical symmetry. It is believed that the symmetry group SU(5) corresponds to the unification of all physical interactions possible. If the universe is a conservatory system, not only about substance and energy, but information, then all the diversity of actual information should come from the primordial symmetry SU(5) or, from a much larger group instead. It reaches the stage where big bang and here on, the universe, already formed, evolves in the relativist cosmological models. The mathematical formulation of the physical universe, having the actual composition, is done on the base of Einstein’s thinking. In a closed universe model, as so of a topological point of view, and energetico-informational, the quantity of substance, energy and information is constant. Global evolution is adiabatical, as so, if a region of the universe has proceses of degradation or vanishes, in other regions; there will be processes of organization and concentration. Dickens considered the physical universe a giant servo-system and some parameters that characterize evolution of a same ensemble. These parameters need to vary in a way of reciprocity conditioned to reassure the constant of