The cyclical reversible transitions of the universe's evolution

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Locality, Globality, Hubble Parameters, Matter-Energy Density, Oscillating Universe Models

Scientific paper

In this work we propose cyclical reversible transitions as the scenario in which the universe evolves, through a series consisting of reversible expansion, temporary stability, and contraction. Our model is based on the comparison between local and global time-dependent densities { ρ 0( τ 0), ρ( τ)} instead of the critical density ρ c, local and global time-dependent Hubble parameters { H 0( τ 0), H( τ)}, and the variations {Δ ρ( τ),Δ H( τ)} due to cosmological chaotic fluctuations, which are generally ignored in certain oscillating models. By taking into account all these factors, a rate equation in the form of ( H 0/ H)2 ∝( ρ 0/ ρ) has been established, and from it we derive some others, to provide a mechanism that is responsible for the cyclical reversible transitions. Also, the problems of singularities, black hole overproduction, and the second law of thermodynamics arising in oscillating universe models are conceptually resolved.

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