An analytic model for the transition from decelerated to accelerated cosmic expansion
J. Ponce de Leon

TL;DR
This paper presents an analytical five-dimensional cosmological model where the universe transitions from decelerated to accelerated expansion as a first-order phase transition, aligning with observational data.
Contribution
It introduces a novel five-dimensional hypersurface model that describes the universe's transition as a phase change, providing new insights into cosmic acceleration.
Findings
Transition from deceleration to acceleration at redshift z ~ 1-1.5
Deceleration parameter jumps from +1.5 to -0.4 at z ~ 1.17
Current deceleration parameter q = -0.55, equation of state w ~ -0.7
Abstract
We consider the scenario where our observable universe is devised as a dynamical four-dimensional hypersurface embedded in a five-dimensional bulk spacetime, with a large extra dimension, which is the {\it generalization of the flat FRW cosmological metric to five dimensions}. This scenario generates a simple analytical model where different stages of the evolution of the universe are approximated by distinct parameterizations of the {\it same} spacetime. In this model the evolution from decelerated to accelerated expansion can be interpreted as a "first-order" phase transition between two successive stages. The dominant energy condition allows different parts of the universe to evolve, from deceleration to acceleration, at different redshifts within a narrow era. This picture corresponds to the creation of bubbles of new phase, in the middle of the old one, typical of first-order phase…
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