Using (4+1) split and energy conditions to study the induced matter in 5D Ricc-flat cosmology
Yongli Ping, Hongya Liu, Lixin Xu

TL;DR
This paper investigates 5D Ricci-flat cosmological models with bounces, using energy conditions to identify physically meaningful solutions, revealing diverse behaviors including acceleration, quintessence, and phantom matter.
Contribution
It introduces a method using (4+1) split and energy conditions to analyze induced matter in 5D Ricci-flat cosmology, highlighting the role of energy conditions in cosmic evolution.
Findings
Asymptotic approach to standard 4D FRW models
Decelerating universe with normal matter satisfying all energy conditions
Accelerating universe with abnormal quintessence and phantom matter
Abstract
We use split to derive the 4D induced energy density and pressure of the Ricci-flat cosmological solutions which are characterized by having a bounce instead of a bang. The solutions contain two arbitrary functions of time and, therefore, are mathematically rich in giving various cosmological models. By using four known energy conditions (null, weak, strong, and dominant) to pick out and study physically meaningful solutions, we find that the 4D part of the solutions asymptotically approach to the standard 4D FRW models and the expansion of the universe is decelerating for normal induced matter for which all the four energy conditions are satisfied. We also find that quintessence might be normal or abnormal, depending on the parameter of the equation of state. If , the expansion of the universe is accelerating and the…
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